Astronomy & Astrophysics manuscript no. AA201528048_astroph_lores_wrk1 c ESO 2018 March 7, 2018

NIBLES – an HI census of stellar mass selected SDSS galaxies: I. The Nançay HI survey

W. van Driel1, 2, Z. Butcher3, S. Schneider3, M.D. Lehnert4, R. Minchin5, S-L. Blyth6, L. Chemin1, 7, 8, N. Hallet1, T. Joseph6, P. Kotze6, 9, R.C. Kraan-Korteweg6, A.O.H. Olofsson1, 2, 10, and M. Ramatsoku6, 11, 12

1 GEPI, Observatoire de Paris, CNRS, Université Paris Diderot, 5 place Jules Janssen, 92190 Meudon, France e-mail: [email protected] 2 Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU USR 704, Université d’Orléans OSUC, route de Souesmes, 18330 Nançay, France 3 University of Massachusetts, Astronomy Program, 536 LGRC, Amherst, MA 01003, U.S.A. 4 Institut d’Astrophysique de Paris, UMR 7095, CNRS Université Pierre et Marie Curie, 98 bis boulevard Arago, 75014 Paris, France 5 Arecibo Observatory, National Astronomy and Ionosphere Center, Arecibo, PR 00612, USA 6 Astrophysics, Cosmology and Gravity Centre (ACGC), Department of Astronomy, University of Cape Town, Private Bag X3, Rondebosch 7701, South Africa 7 Université de Bordeaux, Observatoire Aquitain des Sciences de l’Univers, BP 89, 33271 Floirac Cedex, France 8 CNRS, Laboratoire d’Astrophysique de Bordeaux-UMR 5804, BP 89, 33271 Floirac Cedex, France 9 Southern African Large Telescope Foundation, PO Box 9, Observatory 7935, Cape Town, South Africa 10 Onsala Space Observatory, Dept. of Radio and Space Science, Chalmers University of Technology, 43992 Onsala, Sweden 11 Kapteyn Astronomical Institute, University of Groningen, Landleven 12, 9747 AV Groningen, The Netherlands 12 ASTRON, Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA Dwingeloo, The Netherlands

Received 27/12/2015 ; Accepted 01/07/2016

ABSTRACT

To investigate galaxy properties as a function of their total stellar mass, we obtained 21cm HI line observations at the 100-m class Nançay Radio Telescope of 2839 galaxies from the Sloan Digital Sky Survey (SDSS) in the Local Volume (900redshifts – galaxies: general – galaxies: ISM – galaxies: photometry – radio lines: galaxies

1. Introduction did not drive significant outflows during that period (Snaith et al. 2014; Lehnert et al. 2014). Understanding the gas cycle in galaxies – how galaxies acquire, This is over a time span during which the cosmological ac- arXiv:1607.02787v1 [astro-ph.GA] 10 Jul 2016 process, and expel their gas – is the central goal of most studies of galaxy evolution. Our current understanding is that this cycle cretion of dark matter was thought to decline by an order-of- is a balance between the accretion of gas onto the galaxy, the magnitude (Neistein & Dekel 2008; Dekel et al. 2009, 2013). To efficiency of turning the accreted and “recycled” gas into stars, accommodate the high accretion rates onto galaxies relative to and ejecting gas through a coupling of the gas to the luminous their star formation rates, studies often focus on ways of having and mechanical energy output of stars and active galactic nuclei galaxies drive vigorous massive outflows many times their star (Bouché et al. 2010; Lilly et al. 2013). However, well-studied formation rates (Mitra et al. 2015). While this is logical, perhaps galaxies, such as our own Milky Way, point to a very different it is also important to search for processes that slow down the ac- picture (Haywood et al. 2013). The Milky Way’s star formation cretion timescale and the growth of the gas content of galaxies. rate has been roughly constant over the last 9 Gyrs and likely One plausible way, which is certainly not unique, is to consider the growing angular momentum of accreted gas with decreasing Send offprint requests to: W. van Driel redshift, which has the natural effect of increasing the timescale

Article number, page 1 of 71 A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 over which gas is made available for star formation (e.g., Lehnert of galaxies based on total stellar mass, is aimed to complement et al. 2015). other recent and/or ongoing large HI surveys in the local vol- The role of HI in galaxy formation and evolution is not yet ume. These surveys are, in order of the time at which they were completely clear. The reservoir of HI gas in galaxies must ulti- started: mately feed their star formation (Vollmer & Leroy 2011), after cooling and forming molecular clouds. These gaseous disks are 1. HIPASS: blind survey at the Parkes 64 m telescope very extended, typically beyond the optically bright region of the (Barnes et al. 2001). Beam FWHM 140, rms noise level galaxy (Bigiel & Blitz 2012). Since rotation curves are approxi- 13 mJy beam−1 at a velocity resolution of 18 km s−1, mately flat out across these outer extended HI disks (van Albada −90◦<δ<25◦, search range −1280 to 12,700 km s−1, data et al. 1985), they dominate the specific angular momentum bud- taken in 1997-2002 (Barnes et al. 2001). A total of ∼5300 get of the galaxy, i.e., the angular momentum per unit mass. This galaxies were detected. The major galaxy catalogs are Meyer is an important clue to their formation and their longevity. How- et al. (2004); Wong et al. (2006); ever, to interpret this important clue requires us to have a com- 2. ALFALFA: blind survey at the Arecibo 305 m telescope. plete census of the HI content of galaxies. To interpret spatially HPBW 40, rms 2.4 mJy beam−1 at a velocity resolution resolved observations of HI disks, we need to place them into of 10 km s−1, 0◦<δ<36◦, search range −2000 to 18,000 the general context of galaxies. Moreover, although integrated km s−1, data taken in 2005-2012, not counting single-horn detections of galaxies (at any wavelength) provide only limited receiver follow-up observations (Giovanelli et al. 2005). constraints on models of galaxy evolution, general demographics A total of ∼30,000 galaxies are expected to be detected. of galaxies and gas-phase distributions as a function of mass, en- The first galaxy catalogs are Giovanelli et al. (2007); Sain- vironment, and morphological type, are at the moment the only tonge et al. (2008); Kent et al. (2008); Martin et al. characteristics that models are able to reliably predict. This is (2009); Stierwalt et al. (2009), the subsequent α.40 cata- simply due to our rudimentary understanding of the physics un- log (Haynes et al. 2011) contains 15,855 detections over derpinning galaxy evolution (Silk & Mamon 2012). 40% of the final survey area; the recently uploaded online There are two basic approaches to large HI surveys of galax- α.70 catalog (http://egg.astro.cornell.edu/alfalfa/data/) con- ies: blind surveys where the sky is scanned to search for detec- tains 25,534 detections over 70% of the final survey area; tions, and pointed surveys targeting a high number of individual 3. AGES: blind survey at the Arecibo 305 m telescope of galaxies. Both approaches have their strengths and weaknesses. selected small (∼5◦×5◦) areas sampling different kinds of − Blind surveys are best for unbiased detection of HI-bearing galaxy environments. HPBW 3.05, rms 0.6 mJy beam 1 at galaxies, even discovering galaxies not previously known (Gio- a velocity resolution of 10 km s−1, search range −2000 to vanelli et al. 2013), and for determining the unbiased comoving 20,000 km s−1, data taking started in 2005. A total of 927 ob- density of HI in the local universe (e.g., Zwaan et al. 2005; Mar- jects were detected so far. The galaxy catalogs are Auld et al. tin et al. 2010). The disadvantages are that most of the sky is (2006); Cortese et al. (2008); Irwin et al. (2009); Minchin free of HI emission from galaxies, making the surveys time con- et al. (2010); Davies et al. (2011); Taylor et al. (2012, 2013, suming and enabling them to reach only modest depths, and that 2014a,b); Minchin et al. (2016); Keenan et al. (2016); a sample of HI-selected galaxies will under-represent popula- 4. GASS: pointed survey at the Arecibo 305 m telescope tions of galaxies that have low HI content. Moreover, determin- (Catinella et al. 2012) of 666 galaxies with stellar masses 10 ing detection limits can be tricky and, almost by definition, the greater than 10 M selected from the SDSS spectroscopic upper limits for undetected galaxies lie at similar HI masses as and the Galaxy Evolution Explorer (GALEX) ultraviolet the detections (e.g., Papastergis et al. 2012). Thus the upper lim- imaging surveys. HPBW 3.03, mean rms 0.74 mJy beam−1 −1 its do not add significantly to the analysis of global properties at a velocity resolution of 10-21 km s , 6750

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(2008); Hong et al. (2013); Masters et al. (2014). These were ob- tained with the Green Bank Telescope (GBT) and at Parkes with HIPASS; see Sect. 4 for a comparison between results obtained with these telescopes and the NRT and NIBLES. Here, we present the HI survey undertaken at Nançay, and limit ourselves to a short discussion of the results. In future papers in this series, we will present the results of our deeper Arecibo HI observations (Butcher et al. 2016a, Paper II, sub- mitted to A&A), the bivariate luminosity function and HI mass function (Butcher et al., in prep.), stacking of HI spectra of un- detected sources (Healy et al., in prep.) and further analyses of the sample. The NIBLES HI data are also used for a comparison with local galaxies with extremely high specific Star Formation Rates (Lehnert et al. 2016 and Lehnert et al., in prep.) In Sect. 2 we describe the selection of the observed sam- ple of galaxies, in Sect. 3 the observations and data reduction, in Sect. 4 the results, including a summary of the problems encoun- tered with various SDSS Data Releases (DRs), and in Sect. 5 we present a first, brief discussion. Fig. 1. Distribution on the sky of the SDSS galaxies observed for NIBLES. The radial velocities of the galaxies have been divided into bins and color-coded accordingly, see the legend. The shaded areas in- 2. Sample selection dicate zones that we aimed to avoid, when possible: the pink area in- dicates the Virgo Cluster volume which only extends out to V = 2000 The original sample of about 3000 target galaxies, aimed to be as km s−1, and the gray areas indicate the zones to be covered by the AL- uniformly distributed over the entire stellar mass range of local FALFA blind HI survey: the lighter shade shows the total area, and the galaxies as possible, was selected in 2007 from the SDSS DR5. darker shade those areas for which results were included in the α.40 It should be noted that all SDSS data published here are from the catalog (Haynes et al. 2011). DR9, which was released in 2012, except when explicitly men- tioned otherwise (see also Sect. 4). Our selection criteria were as follows: 3. Observations and data reduction 1. SDSS data: must have both SDSS magnitudes and optical Throughout this paper, all radial velocities given are heliocen- spectra in the DR5; tric, and all HI-line related parameters are calculated according 2. Redshift limits: must lie within the local volume (recession to the conventional optical definition (V=c(λ – λ )/λ ). A Hub- −1 0 0 velocity 900

Article number, page 3 of 71 A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 ing on source redshift. Data were recorded in the radio conven- dure adequate for the purpose of NIBLES. Our HI spectra will tion, in a heliocentric reference frame. The data were taken in be made available online in flux density-velocity table format, position-switching mode, with an elementary integration time through CDS, in case other authors wish to carry out their own of 4+4 seconds per ON-OFF pair. Each observation consists of parametrization procedures. “cycles” of 10/10 pairs of ON/OFF integrations, plus three two- Our observing strategy was to first obtain a relatively short second-long calibrations. For each cycle, the OFF position ob- observation of each galaxy, using about 40 min of telescope time servation is made along exactly the same portion of the track as (resulting in an rms noise level of ∼3 mJy at 18 km s−1 velocity the ON position. The observations were made in the period Jan- resolution), which was repeated in case of weak detections or uary 2007–December 2010, using a total of about 3450 hours of non-detections, time permitting (see Sect. 4 and Fig. 6). On av- telescope time. erage, about 70 minutes of telescope time was used per source. We used the standard NRT NAPS software package to iden- We obtained higher-sensitivity follow-up HI observations at tify, flag, and mitigate strong Radio Frequency Interference Arecibo of 90 galaxies not, or only marginally, detected with the (RFI), see Monnier Ragaigne et al. (2003) for details. The RFI NRT and detected 72 of them, with an rms on average about four that affects our observations are narrow terrestrial radars in the times lower than the NRT levels (see Sect. 4). These results will range 8500-9500 km s−1 and broader, intermittent RFI L3 trans- be described in detail in Paper II. missions around 8300 km s−1 – for illustrations, see Fig. 3 in On visual inspection, spectra of 83 sources appeared affected van Driel (2011). The RFI-flagging trigger level we use is ten by a well-known instrumental baseline ripple (e.g., Wilson et al. times the rms noise level at full velocity resolution per 40/40 sec 2009) which can significantly increase the rms noise level. The ON/OFF cycle of integrations. In practice, the radar signals are ripple, related to the presence of a strong continuum source, is too strong to mitigate and reliably measure a galaxy HI profile caused by radiation reflected between telescope structures which that crosses them. In the case of strong intermittent GPS L3 sig- forms a standing wave with a wavelength corresponding to about nals, we exclude the affected integrations from further analysis 115 km s−1 in the case of NRT HI line spectra. As it is a well- if they disturb the velocity range of the target. We used the stan- defined standing wave, in an FFT deconvolution of a spectrum dard NRT SIR software package to average the two receiver po- it is characterized by a narrow peak at always the same position, larizations, perform the declination-dependent conversion from which can therefore be effectively identified and removed; an in- system temperature to flux density in mJy, fit polynomial base- verse FFT then results in a de-rippled line spectrum. We wrote a lines (usually third-order, of low amplitude), smooth the data to Python routine to perform this derippling, and will illustrate the a velocity resolution of 18 km s−1 and ultimately convert the ve- derippling process on one of our Arecibo follow-up HI spectra in locities measured according to the radio convention to the opti- Paper II. The 12 cases for which the derippling significantly im- cal system. All HI spectra shown have a heliocentric, optical (cz) proved the rms noise level and removed the systematic baseline radial velocity scale. wave pattern have been flagged with a D in Tables A.1-A.3. The HI spectra were reduced using the traditional approach, i.e., by visual inspection of waterfall displays (van Driel 2011) to verify the quality of the data and the automated RFI flagging 4. Results with the NAPS package, followed by averaging, baseline fitting, Color SDSS images and NRT HI spectra of all our clear HI de- and profile parametrization with the SIR package. Our approach tections are shown in Fig. 2, marginal detections are shown in to profile parametrization has been used at the NRT for numer- Fig. 3 and the non-detections in Fig. 4. ous previous surveys, such as KLUN and KLUN+ (e.g., Bot- For the classification of HI spectra as detection, marginal or tinelli et al. 1992; Theureau et al. 1998, 2007, and references non-detection, we also considered two signal-to-noise ratios (the therein). peak ratio, SNR, and the line-width dependent ratio, S/N – see We first inspected the entire averaged spectrum, covering a hereafter) but the adjudication was made independently by three − velocity range of about 12,000 km s 1, for the presence of what of us (ZB, WvD, SES) through visual inspection, after which looks like a galaxy HI profile, irrespective of the SDSS redshift. differently classified sources were discussed in detail, and the fi- In the rare cases where we found an HI detection at a redshift nal adjudication was made by ZB. Some of the marginal sources quite different from the SDSS value we determined its line pa- would be classified as non-detections in a blind survey, as the rameters. We then extracted a velocity range of about ±2000 median peak signal-to-noise ratio and its standard deviation is − km s 1 around the SDSS redshift and performed our further anal- 3.0±0.5 for the sources in this category – their mean S/N is ysis of the target’s HI line properties within that range. 3.2±1.1. However, given we know the optical velocities for all To measure the integrated HI line flux a range of velocities our sources, if a peak is coincident with the SDSS velocity, it was selected that we are confident encompassed the full range of gives greater credibility to the likelihood of a real signal than if the HI profile. To measure the W50 profile width we moved in- we were searching through velocity space. wards along the profile slopes from the outer edges till the 50% The results from the HI observations and other relevant level of the peak flux density was reached, whereas for the W20 galaxy properties are listed in Tables A.1-A.3. width we measured outwards from the inside (e.g., Lewis 1983). Certain physical parameters of the galaxies (MEDIAN total The center velocity of the profile, VHI, was taken to be the mid- stellar masses and star-formation rates) were taken from the pub- point of the velocity width measured at the 50% level of the peak licly available SDSS “added-value" MPA/JHU catalogs (Brinch- flux density. mann et al. 2004; Kauffmann et al. 2003; Salim et al. 2007; The NIBLES data reduction was performed before pack- Tremonti et al. 2004), and the remaining optical data are from ages for the reliable, completely automated processing of much the SDSS DR9. larger HI data sets were readily available (e.g., Westmeier et al. Listed throughout Tables A.1-A.3 are the following proper- 2014; Flöer et al. 2014b). These publications show that the re- ties of the target galaxies: sults of classical data reduction are consistent within the quoted uncertainties with the automated results, for profiles with a peak – Source + flags: internal NRT target number, which we use SNR>5. We consider our non-automated data reduction proce- for quick object identification throughout the paper. Also in-

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Fig. 2. a. Color images from the SDSS and 21-cm HI line spectra of the galaxies clearly detected at Nançay. The size of each image is 3.05×3.05 (i.e., the E-W HPBW of the Nançay Radio Telescope). Each image is centered on the position of the selected photometric source whose properties are listed in Table A.1, the white + sign indicates the pointing center of the Nançay Radio Telescope, the magenta cross indicates the position of the selected SDSS spectroscopic source whose properties are listed in Table A.1, and the crosses of various other colors indicate the positions of the other SDSS spectroscopic positions within the boundaries of the image. Indicated along the top of each image are (from left to right) the NIBLES catalog number of the target galaxy (see Table A.1, only available online at CDS), its absolute magnitude in the z band, Mz, and the logarithm of its total HI mass, log(MHI) (in M ), while indicated in the lower left are the color-coded optical velocities of the SDSS spectroscopic sources in the image. The scale along the horizontal axes of the HI spectra is heliocentric radial velocity (cz) in km s−1, and the vertical scale is flux density in mJy. Indicated in each spectrum are the central HI velocity (blue triangle) and the W50 width of the profile (blue horizonal line), and the SDSS velocity of the selected spectroscopic source (dashed magenta vertical line) and the other sources in the image (dashed vertical lines in colors corresponding to those of the crosses in the image). The velocity resolution is 18 km s−1.(Note: only the first page is shown here ) Article number, page 5 of 71 A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1

Fig. 3. a. SDSS color images and 21-cm HI line spectra of the galaxies marginally detected at Nançay. See Fig. 2a for further details. The properties of the photometric and spectroscopic sources of these galaxies are listed in Table A.2 (only available online at CDS). (Note: only the first page is shown here )

dicated are the various flags regarding the SDSS and NRT have changed between Data Releases and various databases data (see Sect. 4.1-4.5); recognize only older source names; – RA & Dec: Right Ascension and Declination in epoch – Name: common catalog name, other than the SDSS; J2000.0 coordinates, as used for the observations. We do not – Vopt: heliocentric radial velocity measured in the optical give the latest SDSS catalog name, as its precise coordinates wavelength domain (in km s−1). In case more than one value

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Fig. 4. a. SDSS color images and 21-cm HI line spectra of the galaxies not detected at Nançay. See Fig. 2a for further details. The properties of the photometric and spectroscopic sources of these galaxies are listed in Table A.3 (only available online at CDS). (Note: only the first page is shown here )

was listed in the SDSS, the one with the smallest uncertainty – Mz: absolute z-band magnitude, corrected for Galactic ex- and closest match to the HI velocity was chosen; tinction following Schlegel et al. (1998);

– g-z: g-z band color, corrected for Galactic extinction, follow- – M?: MEDIAN total stellar mass estimates, from the ing Schlegel et al. (1998) (in mag); MPA/JHU added-value catalogs (in M );

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– sSFR: specific Star Formation Rate, or SFR/M?, based on SFR and M? from the MPA/JHU added-value catalogs (in yr−1); – rms: rms noise level values of the HI spectra (in mJy); – VHI: heliocentric radial HI velocity of the center of the HI spectra, taken to be the midpoint of the W50 profile width; – W50, W20: velocity widths measured at 50% and 20% of the HI profile peak level, respectively, uncorrected for galaxy in- clination (in km s−1); −1 – FHI: integrated measured HI line flux (in Jy km s ); – SNR: peak signal-to-noise ratio, which we define as the peak flux density divided by the rms noise level. For non- detections, the SNR listed is the maximum found in the ex- pected velocity range of the HI profile; – S/N: signal-to-noise ratio determined taking into ac- count the line width, following the ALFALFA HI survey formulation from Saintonge (2007), S/N = 0.5 1000(FHI/Wfifty)·(W50/2·R) )/rms, where R is the ve- Fig. 5. NIBLES W20 HI line widths as a function of r-band luminos- locity resolution, 18 km/s; ity, Lr, for all clear, non-confused detections. The red line indicates the 5 2 – MHI: total HI mass (in M ), MHI = 2.36·10 ·D ·FHI, where upper envelope used in estimating the upper limits to total HI masses −1 of our non-detections (see Table A.3) as a function of L , log(W ) = the galaxy’s distance D = V/H0 (in Mpc) and H0 = 70 km s r 20 Mpc−1. In the cases of non-detections, 3σ upper limits are 0.62 + 0.21 log(Lr). The two sources (0117 and 2167; i.e., SHOC 30 listed for a flat-topped profile with a width depending on the and NGC 5675) which lie well above the line have exceptionally broad widths as they are either a merger or a possibly confused detection (see target’s r-band luminosity, Lr, according to the upper enve- Appendix). lope in the W20-Lr relationship of our clear, non-confused detections (see Fig. 5); – MHI/M?: ratio of the total HI and stellar masses. The deeper observations permitted us to better constrain the line flux and width for the weak marginal detections and to set lower Our method of determining upper limits to M appears to be HI limits on total HI masses for non-detections. a fair estimate of the amount of HI flux that could escape detec- tion, as we will show in Paper II using our four times more sen- For a description of the flags used in the tables to point out sitive Arecibo follow-up observations of Nançay non-detections. various issues with the SDSS data, see Sect. 4.5. For a descrip- tion of the 240 cases that were not used for further analysis for Estimated uncertainties are given after the values in the ta- various reasons, see Sect. 4.8. bles. Uncertainties in the central HI line velocity, VHI, and in the integrated HI line flux, FHI, were determined following Schnei- der et al. (1986, 1990) as, respectively 4.1. Photometry update to SDSS DR9 −1 −1 σvHI = 1.5(W20 − W50)SNR (km s ) (1) Using the SDSS DR5 data upon which the initial galaxy se- lection was based, as our HI data started accumulating we dis- covered (Joseph 2008) that a fairly large subset of the detected galaxies showed unprecedentedly high M /L ratios, together σ = 2(1.2W R)0.5rms (km s−1) (2) HI z FHI 20 with very low luminosities. These values for gas content and lu- where R is the instrumental resolution, 18 km s−1, SNR is the minosity did not appear physical, and they were mainly found peak signal-to-noise ratio of a spectrum and rms is the rms noise among the seemingly least-luminous targets: all galaxies with a level (in Jy). Following Schneider et al., the uncertainty in the listed DR5 g-band absolute magnitude Mg>-13 mag had MHI/Lg between 10 and 10,000, with a linear increase between M and W50 and W20 line widths is expected to be 2 and 3.1 times the g log(M /L ), the apparently less luminous sources being the uncertainty in VHI, respectively. HI g These formulae give just the expected rms of a signal inte- most gas-rich. grated across a number of channels with uncorrelated Gaussian All this made us suspect that the associated magnitudes were noise, so this is the minimum expected uncertainty. Fluctuations in fact severely misunderestimated (a term that captures the com- due to uncertainties in the baseline fit are difficult to quantify, plexities involved), which also lead to unrealistically low lumi- but as the baseline variations are generally rather mild with an nosities of galaxies. Having only the DR5 products at our dis- amplitude small compared to the peak in the HI signal, we be- posal, it turned out to be infeasible to pinpoint the technical prob- lieve the fits are well constrained. In the past, we also tried the lem(s) involved, to find other measured parameters that would more complicated NRT-based formulae of Fouqué et al. (1990) enable the identification of sources with unusable photometry, but they yield similar results. or how to select the correct magnitudes from the DR5, if those The distribution of the rms noise levels for our clear detec- existed. Measuring Petrosian magnitudes ourselves from DR5 tions, marginals, and non-detections is shown in Fig. 6 at 18 FITS images using SourceExtractor (Bertin & Arnouts 1996) we km s−1 velocity resolution, together with that of the homoge- found much brighter magnitudes for suspect sources, which led neous, blind ALFALFA survey with its symmetric peak (mean to normal MHI/Lz ratios (Joseph 2008). rms 2.3 mJy, at 10 km s−1 resolution). The effect of our flexi- Since the start of NIBLES, several more SDSS data releases ble observing time strategy is reflected in the peaks around 2.6 were made public during the observation and data reduction pro- mJy (mainly for clear detections after the first run of 40 min) cess phase. In particular, data releases 8-12 use an updated pho- and the lower peaks around ∼1.6 mJy of the deeper integrations. tometric processing pipeline (v5_6_3) which re-calibrated and

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In 25 other cases, both the DR7 and DR9 photometry obvi- ously missed a significant amount of the total flux of the galaxy, or is unreliable due to a bright foreground star (flag U).

4.2. Radial velocity update to SDSS DR9 Using the SDSS DR9 radial velocities instead of the DR5 values used for the original source selection exposed a number of issues for individual sources, which could not be resolved in all cases; see also the Appendix for details on specific cases. There are 20 DR9 objects with an unconstrained redshift (er- ror message “zerr=-1”, nominal V = 1245 km s−1). For these we searched the online HyperLeda database and the NASA Extra- galactic Database (NED) for independent (i.e., non-SDSS) ve- locities, and inspected their SDSS spectra and the fits made to the lines. For the five cases with HI velocities we adopted those val- ues instead: three from this paper (sources 1355, 1371, and 1698; Fig. 6. Comparison between peak-normalized distributions of rms noise −1 i.e., MCG +09-19-160, CGCG 292-024, and IC 3612, respec- level values below 5 mJy: NIBLES (at 18 km s velocity resolution), tively) and two from Paper II (sources 0828 and 2140; i.e., ASK all observations (black line, N = 2606), clear detections (blue line, N = 261057 and ASK 082514). For the four HI non-detections with 1727), marginal detections (yellow line, N = 176) and non-detections (red line, N = 703), and (dark gray line) all 15,598 ALFALFA α.40 independent optical velocities from the literature we adopted the catalog detections, at 10 km s−1 velocity resolution (Haynes et al. 2011) latter values instead (sources 0998, 1654, 1723, and 2265; i.e., . NGC 3156, PGC 40315, ASK 77777, and PGC 3350778, respec- tively). We removed the remaining 11 cases (see Table A.6) from our sample as inspection confirmed that no credible velocity can re-resolved all the imaging data. In order to take advantage of be derived for them. the new data available, and to address the abovementioned prob- There are 44 cases where the difference between the DR9 lem with the DR5 SDSS photometry, we updated all the NIBLES and DR5 velocity exceeds 100 km s−1 (and for 22 of these photometry to the then current DR9. it is much larger – at least 300 km s−1). For the 16 galaxies In addition to the updated photometric processing, DR9 has a with NIBLES HI-detections we used our HI velocity instead, flux based association between the spectroscopic and photomet- which is supported by literature HI values for five cases and ric information. In the data releases prior to DR8, the only as- optical redshifts for four. In all cases these values are consis- sociation available was position based, that is, the spectrum was tent with the DR9 velocities, not the DR5 values: 13 sources only associated with the nearest photometric source. DR9 incor- 0006, 0255, 1217, 1619, 1871, 1894, 2081, 2161, 2333, 2414, porates two matches, one based on position and another based 2427, 2562, and 2565; i.e., PGC 4567836, PGC 1146688, NGC on flux. This new matching method provided a much better asso- 3633, VCC 423, UGC 08517, CGCG 017-048, PGC 140287, ciation between spectroscopic sources and photometric sources PGC 4553986, SHOC 513, 2MASX J21231841+0115175, ASK with a Petrosian radius large enough to capture most of the flux 139251, 2MASXi J2340427-092336, and 2MASX J23411334- from a galaxy. However, this did not entirely solve the problem. 1059310, respectively) from this paper and three sources (0645, The DR9 photometric information that we decided to use for 1807, and 2316; i.e., ASK 522849, PGC 1958740, and ASK a galaxy was not always associated with the spectroscopic infor- 421256, respectively) from Paper II. For nine cases we used the mation via the normally used fluxObjID in the SDSS database. (average) independent, non-SDSS optical velocity listed in the In two cases, the photometric source associated with the spectro- online HyperLeda database: Sources 0609, 0718, 0824, 1598, scopic source was instead selected using bestObjID, because the 1715, 1717, 1771, 2155, and 2356 (i.e., KUG 0814+251, CGCG standard procedure using fluxObjID returned no result (flag B in 263-080, KUG 0910+433, VCC 315, IC 3665, NGC 4649, PGC the tables). 1132599, NGC 5644, and CGCG 137-019, respectively). For In another 312 cases, the selection of a photometric source the 19 cases where no independent literature redshifts could be associated with the spectroscopic source using either bestObjID found, we adopted the DR9 velocities in the six cases where the or fluxObjID returned no result or one that was obviously miss- line fits seemed reliable to us (sources 0995, 1712, 2056, 2249, ing a significant amount of flux. Here, we queried the photo- 2397, and 2585; i.e., ASK 209206, ASK 1622, ASK 400932, metric database around the NRT HI pointing position (towards CGCG 221-008, PGC 3104052, and ASK 124704, respectively), the spectroscopic source) and manually selected the photometric whereas the remaining 13 cases (see Table A.6) were removed source which was centered on the galaxy and had a sufficiently from further analysis as their DR9 velocities are too uncertain. large Petrosian radius to encompass the target galaxy (flag N). Twenty-three of the observed DR5 sources are not included 4.3. Confused sources in the DR9. For these objects, photometric and spectroscopic in- formation from DR7 was used (flag P). There are also 20 cases As the HPBW of the telescope used for our HI survey is 3.05 in 0 0 where the DR7 redshift more closely agrees with the HI velocity α and 23 − 30 in δ, we need to examine a large area on the sky (flag Z). These are frequently low surface brightness (LSB) ob- surrounding the target object for the presence of other galaxies jects, whose spectra only show weak line features. There are also whose HI emission might cause confusion with that originating 18 cases where the DR7 photometry more adequately captured from the intended target. the galaxy’s total flux than the DR9 photometry, which have been In the pre-SDSS era, this would usually involve a great deal flagged as P in the tables. of guesswork, as velocity data for large numbers of galaxies was

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the 25% beam sensitivity contour, it was flagged, regardless of whether or not it was deemed to be a significant contributor of HI flux. Selected galaxies outside this contour were also flagged, but only when they were (at least) comparable in angular size to the target source and considered potential HI contamination sources. We also queried HyperLeda for published HI data on all flagged secondary galaxies. For all potentially confused target galaxies, we estimated the probability of HI profile contamina- tion and flagged them accordingly. We use three flags to indicate the potential contamination level: – C1: target detection is definitely confused with a secondary galaxy containing comparable or higher HI mass than the tar- get; – C2: target detection is probably confused, but unable to as- certain how much of the detected flux is likely due to a sec- ondary galaxy; – C3: target detection may be slightly confused, but the con- tribution to the detected flux from one or more secondary galaxies is likely insignificant or non-existent. These three confusion flags are listed in Tables A.1-A.3 for all NIBLES sources, whether detected or undetected.

4.4. Spatially resolved sources Fig. 7. Comparison between NIBLES and literature values for central HI line velocities, VHI, and W50 line widths. Only sources matched in Some of the target galaxies are of sufficiently large apparent size HI velocity and in line width are plotted (see Sect. 4.6). Top panels: that some HI flux will likely be missed by the NRT beam; these comparison with data from the α.40 ALFALFA catalog (Haynes et al. have been flagged as R in the tables. In assessing galaxy sizes 2011); lower panels: comparison with HIPASS data ((Meyer et al. 2004; and comparing them to the telescope beam, one has to take into Wong et al. 2006). Left-hand panels: W50 line widths. Literature val- account several factors: the telescope is also sensitive to emis- ues as a function of NIBLES widths (in km s−1). The solid line marked with “1:1” indicates equality between both scales and was only added sion outside its HPBW, which is not a “hard” beam edge, using to guide the eye. Right-hand panels: central HI line velocity. Difference isophotal optical diameters such as D25 (de Vaucouleurs et al. −1 between VHI (in km s ) measured at the NRT for NIBLES and literature 1991, HyperLeda) as a selection criterion does not take into ac- values as a function of NIBLES line velocity (in km s−1). The horizontal count low surface brightness (LSB) disks which usually are rel- lines indicates the mean velocity differences. atively HI-rich, and there is considerable variation in the ratio of HI and optical disk sizes (for various definitions of these two). We therefore adopted the working definition that a galaxy is unavailable. However, since this is a targeted survey of SDSS spatially resolved if it is larger than the NRT HPBW on an SDSS galaxies, we can make use of the redshift information provided color image. The SDSS images are not very deep, so this should for nearby galaxies to help ascertain whether or not a particu- identify objects that have a significant amount of HI flux that will lar object is a likely source of confusion. As the SDSS does not be missed by the NRT. This applies to 85 objects (flag R). contain redshift information for every neighboring galaxy, par- As we intend to keep these in our NIBLES sample for further ticularly in the case of ellipticals and dwarfs, we also used NED analysis, we searched the literature for HI observations that can to query for nearby galaxies. be confidently expected to include their entire HI content (see For each NIBLES source, we first queried NED for all galax- Butcher et al., in prep.). ies within a 200 radius and with a recession velocity of less than 12,500 km s−1. We then selected galaxies that lay within a box of dimensions 100 in RA and 400 in DEC, centered on the target, 4.5. Cases flagged in the tables and with a systemic velocity located within the W20 width of the In summary, the following types of cases have been flagged in HI profile window. the tables. It should be noted that most of these merely serve to The latter galaxies constitute our working database of po- flag technical problems which were ultimately resolved. Only a tentially confusing “secondary” sources with known redshifts. few indicate sources whose SDSS or HI data have issues which However, estimating the likeliness of a particular galaxy being make them unsuitable for use in, e.g., further analysis of rele- a confusion source requires a certain amount of educated guess- vant global properties of the NIBLES sample, such as HI source work. For example, a small dwarf galaxy near a large targeted confusion (C1, C2) and resolution (R) or unreliable or underesti- blue spiral will contribute only a negligible amount of flux to the mated SDSS flux (U) – these flags concern a total of 275 (11%) integrated observed HI flux, whereas a large gas-rich spiral lo- out of the 2600 sources in the final NIBLES sample (for the 240 cated just outside the telescope’s HPBW is bound to contribute observed sources not included in the final sample, see Sect. 4.8). a significant amount of contaminating flux to the observation. Next, we extracted an SDSS image of size 140×400 (α×δ) – A1, A2 (124 and 20 cases, respectively): follow-up HI obser- centered on each targeted source and superimposed telescope vations with four times higher sensitivity were obtained by beam contours at levels corresponding to 90%, 75%, 50%, 25%, us at Arecibo (see Paper II). Arecibo detections are denoted and 10% of the peak sensitivity. We also extracted SDSS im- by A1 and non-detections by A2. Here, only their NRT fluxes ages of each secondary source. If a galaxy was contained within are listed.;

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– C1, C2, C3 (231,19,185 cases, respectively): HI detection of the target galaxy is confused to a certain degree by another galaxy in the telescope beam. Three different levels are in- dicated (see Sect. 4.3): definitely confused (C1), probably confused (C2) and only a slight chance of confusion (C3); – D (12 cases): baseline ripple removed from HI spectrum (see Sect. 3); – F (175 cases): significant offset between the galaxy center and the SDSS spectral fiber position closest to it. This will usually result in a significant discrepancy between the SDSS velocity and the center velocity derived from the HI profile; – N (465 cases): the selection of a photometric source associ- ated with the spectroscopic source using either bestObjID or fluxObjID returned no result or one that was obviously miss- ing a significant amount of flux. Therefore we queried the photometric database around the NRT pointing position and selected the brightest source encompassing the NRT pointing position within its Petrosian radius; – P (25 cases): SDSS DR7 photometry used instead of DR9; – R (78 cases): extended source whose integrated HI flux is likely to be underestimated at the NRT (see Sect. 4.4); – U (25 cases): SDSS photometry from DR7 and DR9 almost certainly missed a significant amount of the total flux of the galaxy due to either an obviously too small Petrosian radius or a bright foreground star (see Sect. 4.1); – Z (53 cases): SDSS DR7 spectroscopy used instead of DR9.

4.6. Comparison with other H I surveys To compare HI line parameters between NIBLES, ALFALFA and HIPASS we matched the coordinates of each NIBLES galaxy to the corresponding galaxy positions in the other sur- veys using a 3000 and 20 radius respectively, i.e., about one sixth of the telescope HPBW. On comparing our sources to the α.40 ALFALFA catalog (Haynes et al. 2011), we find five ALFALFA sources, observed with a noise level comparable to NIBLES, which were not de- tected in our data. Of these, three were undetectable at the NRT due to an OFF-beam detection (AGC 180485, AGC 181493, and AGC 182461) and one due to RFI (AGC 320479). The remain- ing object, source 0023 (KUG 0007+140), has an ALFALFA mean line flux density at a level (3.6σ) which should make it faintly detectable in NIBLES, but our four times deeper Arecibo follow-up observation (Paper II) shows a much weaker detection than ALFALFA, at a level undetectable at Nançay. The mean difference between NIBLES HI central velocities and data from other large surveys is −0.5±9.8 km s−1 for AL- Fig. 8. Comparison between NIBLES and literature HI line fluxes, in Jy FALFA α.40 and -1.8±8.4 km s−1 for HIPASS, when excluding − km s 1. Black dots indicate the sources matched in HI velocity and in the Nançay beam-confused cases (see Fig. 7). line width that were used for the survey flux scale comparisons, whereas The six objects with the greatest difference in W50 in the gray dots indicate the other common sources (see also Sect. 4.6 and NIBLES compared to ALFALFA (Fig. 7) are discussed in the Table A.7). In each panel, the solid line indicates the mean relationship between both flux scales, whereas the dotted “1:1” line indicates equal- Appendix (sources 0784, 0793, 0958, 1319, 1970, and 2183, i.e., ity between both scales and was only added to guide the eye. Top pan- UGC 4722, NGC 2743, PGC 4571034, PGC 1275866, NGC nel: For line flux calibrator galaxies only, as measured with single-feed 5356, and LSBC D723-05, respectively). In three cases (0784, receivers at the Nançay Radio Telescope (NRT) for NIBLES and at the 0793, and 1970) the W20 widths are comparable, and the differ- Green Bank Telescope (GBT), both compared to Arecibo single-feed ence in profile shape only occurs at higher flux density levels. receiver fluxes (Arecibo and GBT data are from O’Neil 2004); middle In two cases (0958 and 1319) the NIBLES W50 is considerably pannel: Fluxes from the α.40 ALFALFA catalog (Haynes et al. 2011) larger, whereas in one other (2183) it is much smaller. For the as a function of NIBLES values; lower pannel: Fluxes from HIPASS latter three discrepant W50 cases no potentially confusing other catalogs (Meyer et al. 2004; Wong et al. 2006) as a function of NIBLES source could be identified in the vicinity, nor was any RFI iden- values. tified in the data. In order to check the routine NRT flux calibration scale – B (2 cases): the photometric source associated with the spec- (which is based on continuum sources - see Sect. 3), over the troscopic source was selected using bestObjID, because the period May 2009 - December 2010 we obtained a total of 64 standard procedure using fluxObjID returned no result; Article number, page 11 of 71 A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1

The resulting flux ratios are α.40/NRT = 1.45±0.17 and HIPASS/NRT = 1.34±0.28, where the uncertainty given is the standard deviation of the weighted mean. This indicates that the multi-beam survey fluxes are considerably higher than those from single-receiver NIBLES.

Fig. 9. Total number of galaxies observed (black line) and detected (blue line) in HI, either clearly or marginally, per 0.5 wide bin in absolute z- band magnitude, Mz, together with the overall detection percentage per bin (green line). We observed 130-165 objects per half-magnitude bin in Mz over the range of −23 < Mz < −16.5 mag (the target number was 150), and observed all objects known from the DR5 in the least-filled bins. −1 Fig. 10. Integrated HI line flux, FHI (in Jy km s ), as a function of −1 W50 line width (in km s ). Black dots represent clear NIBLES detec- observations of 12 HI flux calibrator galaxies with very precise tions and gray dots marginal detections, whereas green squares are high- New Reference Galaxy Standards for HI Emission Observations quality (their Category 1) α.40 catalog ALFALFA detections (Haynes from O’Neil (2004), who made observations with two different et al. 2011, from), and light blue ones their marginal (Category 2) de- single-horn instruments – the L-narrow receiver at Arecibo and tections. The ALFALFA galaxies shown cover the same velocity range −1 the 100-m Green Bank Telescope (see Table A.7 for the mea- as NIBLES, 900-12,000 km s . The red line indicates the expected line sured line fluxes). These NRT data were obtained and reduced flux as a function of line width for a flat-topped 3σ HI profile and a 2 mJy rms noise level. in the same manner as the NIBLES spectra. We found that these line flux scales are consistent (see Table A.4 and Fig. 8): the Arecibo values are on average 1.13±0.12 (mean and σ) times However, we noted that the α.40 catalog ALFALFA flux the NRT values – we would like to point out that we did not use scale is also higher (though less so than in the case of NIBLES) this ratio to rescale our NIBLES line fluxes. The NRT fluxes than the Arecibo and GBT HI single-receiver measurements are also stable over long periods of time: using similar mea- of O’Neil (2004) (1.25±0.16 and 1.14±0.09, respectively), and surements made during the last year we found exactly the same those of the deeper AGES survey (see Introduction) carried NRT/Arecibo ratio (Kraan-Korteweg et al., in prep.). The other out at Arecibo with the same multi-beam ALFA instrument flux ratios are 0.93±0.24 for GBT/NRT (for two sources only) (1.20±0.06). Haynes et al. (2011) mention that “some earlier and 0.99±0.18 for Arecibo/GBT. The small differences between measurements tended to underestimate fluxes for the brightest the flux calibration scales are illustrated in Fig. 8. and more extended sources, a systematic effect for which a cor- We also cross-checked the fluxes of NIBLES sources with rection was applied”; comparing the results for 2704 sources in those measured by the HIPASS and ALFALFA surveys (see In- the α.40 catalog included in earlier ALFALFA catalogs (see In- troduction for catalog references). troduction), we noted a systematic difference for all sources be- To reduce noise contamination we only used high peak tween the published line fluxes which increased with the flux signal-to-noise ratio NIBLES detections of at least SNR = 12 value. This had the effect of aligning the α.40 ALFALFA flux for the α.40 ALFALFA matches and at least 20 for HIPASS. We scale with that of Springob et al. (2005), which includes theoret- also excluded all NIBLES detections that are definitely or prob- ical corrections for HI self absorption and source extension, at ably confused, or resolved. To further mitigate effects of beam the expense of agreement with other HI catalogs. offsets or confusion sources within the telescope beams in the By fitting the ratio between the α.40 line fluxes and comparison (we control for confusion in NIBLES, but cannot in those in earlier ALFALFA catalogs, we find a best fit of the other surveys), we only use galaxies whose difference in cen- log(FHI,ALFALFAα.40) = (log(FHI,ALFALFAprevious) − 0.0283)/1.04). −1 tral line velocity and W50 line width is 20 km s or less between Using this, we corrected the α.40 values back to the older AL- NIBLES and the α.40 and HIPASS surveys. This helps ensure FALFA flux scale. We find that the older flux scale is signifi- we are only measuring differences in flux calibration without cantly closer to that of NIBLES, with a flux ratio of 1.25±0.14. contamination by differing velocity offsets. These matching cri- It should be pointed out that the perceived differences in flux teria yield 82 flux comparison sources with α.40 and 51 with scale between multi-beam and single-receiver observations is not HIPASS (the black dots in Fig. 8). necessarily due to flux calibration differences alone. Compared Our HI line fluxes were compared using a weighted mean to measuring total line fluxes with single-horn receivers, recon- of the ratios of α.40/NRT and HIPASS/NRT. Each source was structing total fluxes from multi-beam receiver data is a rather weighted using the inverse of the square of its relative uncer- complex process (Barnes et al. 2001) involving choices on re- tainty in order to give more weight to low uncertainty sources. gridding, flux conservation, etc.

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Fig. 11. Total HI mass, MHI (in M ), as a function of radial velocity Fig. 12. Total HI mass, MHI (in M ), as a function of radial velocity −1 −1 (in km s ), i.e., VHI for the detections and SDSS optical values for the (in km s ) – as in Fig. 11. Shown besides the NIBLES detections and non-detections. Black dots represent clear NIBLES detections, gray dia- marginals are the ALFALFA data from Haynes et al. (2011), where monds marginal detections, and open red triangles estimated upper limit green squares represent high-quality (Category 1) detections, and blue for non-detections. Excluded were all NIBLES detections which are ei- ones the weaker (Category 2) ones. The HI masses of the ALFALFA ther resolved (flag R in the tables), or definitely or probably confused detections were calculated in the same way as for the NIBLES sources, by another galaxy within the telescope beam (flags C1 and C2). The using simply a distance of D = V/H0, where the adopted Hubble con- −1 −1 relatively high estimated upper limits for non-detections are quite con- stant is H0 = 70 km s Mpc . For clarity, the velocity range plotted is −1 servative, as they are based on the largest W20 line widths measured as limited to the NIBLES search range limit of 12,000 km s , whereas the a function of r-band luminosity (see Sect. 4). ALFALFA search range continues till 18,000 km s−1. The green vertical arrow left of the legend of 0.16 dex in log(MHI) indicates the difference between the on average 1.45 higher ALFALFA α.40 catalog fluxes and the NIBLES values (see Sect. 4.6).

We explored this using data from the publicly-available 4.8. Sources not included in the final NIBLES sample AGES NGC 7332 data cube (Minchin et al. 2010). For sources chosen to be at a high enough redshift to ensure they are point- Data were obtained for a total of 240 sources among the 2840 like, we measure the sources using two algorithms implemented observed that are not part of the final NIBLES sample of 2600 in the mbspect routine in miriad. One (which is that used by the objects. They are not listed in the tables as their data will not AGES survey) fits the position of the source and uses this to be used for further analysis of the results of our surveys. They reconstruct the flux of a point source at that position using a were excluded for the following reasons, listed in order of the Gaussian beam model that applies lower weights to pixels fur- frequency of occurrence: ther from the position. The second is simply to sum the flux – OFF-beam detection (95 cases): the HI line profile of a and correct it for the beam size. We carried out this analysis galaxy detected in the OFF-beam, which appears as a neg- 0 0 0 0 0 0 0 0 over 5 × 5 , 7 × 7 , 9 × 9 , and 11 × 11 sized regions, cen- ative signal in the reduced spectrum, lies (partly) in the ve- tered on the cataloged positions of the sources. We found that locity range where HI emission from the target is expected the two methods, which should give essentially identical an- to occur, or is in fact observed; swers for point sources, have markedly different results, with – High velocity, out of HI search range (28 cases): these fluxes in the sum-and-correct method increasing with box size sources have radial velocities in DR9 which are significantly well beyond that predicted by a Gaussian beam model. The ra- higher than their DR5 values, and which consequently lie tio between the beam-corrected sum over the 90 × 90 region and outside our velocity search range; curiously, 17 of these the beam-weighted reconstruction over the 50 × 50 region was have reported redshifts in the narrow range 23,100 to 23,700 1.19 on average. Although this is exploratory only, it does indi- km s−1; cate that changing the way in which total line fluxes are recon- – Telescope problem (20 cases): telescope malfunction which structed from images obtained with single-dish telescopes can makes the data unusable (mainly pointing and receiver prob- significantly change the result. lems); – Not a galaxy (18 cases): originally classified as galaxies in DR5, but in DR9 17 were reclassified as stars, and one ap- pears to be a cosmic ray; 4.7. CRUMBS: stacking of NIBLES non-detections – Unreliable redshift (14 cases): conflicting redshift informa- tion between DR7 and DR9. Only some have warnings of unreliable line fits. These sources were also all undetected in The NIBLES sub-project named CRUMBS (Characterizing HI so there is no independent measure of their redshift (see Radio-Undetected Masses in Baryonic Surveys), includes an in- Table A.6 and Sect. 4.2); vestigation of all NIBLES non-detections using the spectrum – Unconstrained redshift (12 cases): these sources have a listed stacking technique. Preliminary results are presented in Blyth uncertainty of z±1 in their SDSS redshift, and they also all et al. (2009) and further results will be published as part of this have the same reported radial velocity of 1245 km s−1. They series (Healy et al., in prep.). are listed in Table A.6 (see also Sect. 4.2);

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As noted in Sect. 3, the rms noise level is not constant for the entire NIBLES sample (see Fig. 6), with more observing time spent on weak marginal detections and non-detections, tele- scope time permitting; the mean rms for the sample is 2.1 mJy. The comparable overall rms noise level of the NIBLES and AL- FALFA surveys is reflected in their similar FHI-W50 distribution (Fig. 10), where also the effect of longer integrations for weak NIBLES marginal detections can be noted. The higher veloc- ity resolution of the ALFALFA data, 10 km s−1 compared to 18 km s−1 for NIBLES, has resulted in a number of very narrow ALFALFA detections, more extreme than found by us. The distribution of the total HI masses as a function of ra- dial velocity is shown in Figs. 11 and 12. The former shows both the clear and the marginal NIBLES detections as well as the estimated upper limits of the non-detections, whereas the latter shows the clear and the marginal detections of both NIBLES and ALFALFA. Excluded in both figures were the NIBLES sources which are definitely or probably confused by another galaxy Fig. 13. Integrated g-z color, in mag, as a function of absolute z-band within the telescope beam (flags C1 and C2 in the tables). For the magnitude, M . All data were corrected for Galactic extinction follow- z sake of clarity, the velocity range is only plotted to the NIBLES ing Schlegel et al. (1998). Black dots represent clear NIBLES detec- −1 tions, gray dots marginal detections, and red triangles estimated non- limit of 12,000 km s , whereas ALFALFA detections continue −1 detections. out to 18,000 km s . Figure 11 shows that the estimated upper limits to the HI masses of NIBLES non-detections are quite conservative, as they – RFI (10 cases): Radio Frequency Interference (RFI) is are based on the upper envelope of the W20 line widths measured present in the velocity range around the SDSS velocity; as a function of r-band luminosity (see Sect. 4). At the highest – Baselines bad (9 cases): unstable baselines which made it velocities (V>8000 km s−1), where in general the most luminous impossible to verify if an HI line signal was present; sources are located with the greatest expected line widths, the – Low velocity (6 cases): radial velocity in SDSS DR9 <850 upper limits even tend to be higher than the NIBLES detections −1 −1 km s , well below the 900 km s lower velocity limit of our at the same redshift. sample (see Table A.5). As can be seen in 12, the NIBLES SDSS sources were se- – Incorrect velocity search range selected (3 cases): these lected at the lowest velocities in their Mz bins, as far as prac- sources had an observed HI velocity search range between ticable, whereas ALFALFA is a blind HI survey, bound to de- −1 0 and 10,000 km s whereas their current SDSS redshifts tect high numbers of relatively high HI mass objects at larger −1 are over 10,000 km s . distances than the SDSS sources selected for NIBLES. The AL- FALFA line fluxes from the α.40 catalog are on average 1.45 times higher than our Nançay values due to a flux calibration 5. Discussion difference (see Sect. 4.6), which corresponds to a difference of Further discussion and analysis of the data presented here will 0.16 dex in log(MHI) – see the vertical arrow in the plot. be given in future papers in this series (e.g., Paper II; Butcher et The integrated g-z color as a function of absolute z- al., in prep.; Healy et al., in prep.). band magnitude is shown in 13 with different symbols Our goal was to observe a total of 3000 galaxies in the local for NIBLES clear detections, marginal detections, and non- Universe, distributed as uniformly as possible over the full range detections. NIBLES sources were selected on Mz, irrespective in absolute z-band magnitude detected in the SDSS, without se- of color. The distribution shows the well-known “red sequence” lection on color. The final Mz distribution is shown in Fig. 9, and “blue cloud” loci, with a mixture of detections and non- which contains all sources observed and detected, both clearly detections in both. The highest concentration of non-detections and marginally. For some galaxies the redshift and/or photom- occurs among the most luminous red systems, but these are not etry changed as a result of moving from the SDSS DR5 data all elliptical systems and HI detections do occur. Among the low- used to select them to the DR9 data used for further analysis luminosity systems (at log(Lr) 7.8-8.5) the non-detected dwarfs (see Sect. 4). are predominantly red. We will study the underlying HI prop- We observed 130-165 sources per half-magnitude bin over erties of undetected galaxies using four times higher sensitivity the absolute magnitude range −23 < Mz < −16.5 mag (the target Arecibo observations in Paper II. number was 150), and observed all objects known from the DR5 in the least-filled bins (see Fig. 9). For Mz> −21 mag the overall 5.1. The MHI/M? – M? relationship, including H I detection rate is high, at about the 75% level, and rather con- non-detections stant, but it starts to decline steadily for more luminous galaxies, towards the 30% level at −23 mag (see also Fig. 13). The ratio of HI and stellar masses, MHI/M?, as a function of Shown in Fig. 10 is the integrated HI line flux, FHI, as a total stellar mass is shown in Fig. 14 for NIBLES detections, function of W50 line width for the 1733 clear detections and 137 marginals, and estimated upper limits for non-detections. We did marginal detections, together with the line indicating the flux ex- not use those sources we flagged as either C1/C2 (confused by pected for a flat-topped 3σ detection with a 2 mJy rms noise another galaxy in the NRT beam), R (resolved by the NRT beam) level. For comparison, the same data are shown for the 11,941 or U (significant SDSS flux missing), as their MHI/M? ratios ALFALFA high-quality detections (their Category 1) and 3100 will be either under- or overestimated by unknown amounts (see marginal detections (their Category 2) from Haynes et al. (2011). Sect. 4). Overlaid on this plot are high-quality ALFALFA de-

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−1 tections, and the mean relationship for four literature reference was applied for VCMB<6000 km s (see Haynes et al. 2011 for samples of local HI-detected galaxies (pink line) from Papaster- details). The ALFALFA HI masses shown in Fig. 14 were all gis et al. (2012). We first explore the differences between the calculated by us using the same method as for NIBLES. plotted properties for the various samples and their uncertain- For the four reference samples used in Papastergis et al. ties, both relative and systematic. (2012), no individual distances are given, nor in the paper that Like for the NIBLES data, the total stellar masses used here comprises the bulk of those data, Zhang et al. (2009). From the for the ALFALFA detections were taken by us from the SDSS fact that the latter are all SDSS galaxies with pre-ALFALFA HI “added-value" MPA/JHU catalogs (see Sect. 4). To estimate the detections listed in HyperLeda, we deduce they are relatively the uncertainty in the stellar masses of individual galaxies we nearby objects with a mean velocity of a few thousand km s−1. examined the +1 σ, -1 σ and median mass estimates, and found At such velocities, the ALFALFA distances are only about 7% a typical (mean) relative uncertainty of about 20%. Matching higher than the NIBLES values, corresponding to +0.03 dex in positions with those of the 15,598 α.40 catalog HI detections log(MHI) – small compared to the other typical uncertainties of resulted in 2500 matches. individual galaxy data as shown in Fig. 14. A caveat in the comparison between our MPA/JHU catalogs’ A linear regression fit made only to the NIBLES detections total stellar masses for NIBLES and ALFALFA galaxies and (excluding resolved and confused sources) results in a mean re- those used for the reference samples in Papastergis et al. (2012) lationship (dark green line in Fig. 14) of log(MHI/M?) = −0.54 is that the latter used a somewhat different way to estimate stel- log(M?) + 4.70. lar masses, see Huang et al. (2012) for details. We do not have We now want to examine the impact of HI non-detections, of a simple way of estimating the systematic uncertainties between which the estimated upper limits to their total HI masses are rou- the two stellar mass estimate methods as stellar masses for indi- tinely ignored, in the study of this relationship for our optically- vidual galaxies are not given in Papastergis et al. (2012). We will selected NIBLES sample. To this purpose, we fitted our data, in- therefore ignore this uncertainty, but we note that in our experi- cluding MHI upper limits, with three estimators of the slope and ence different mass estimates usually agree within about 0.3 dex intercept, from the STSDAS statistics package 1. These were the (e.g., Drory et al. 2004; Moustakas et al. 2013; Sorba & Sawicki Buckley-James, expectation-maximization (EM) algorithm, and 2015). Schmitt binning methods of linear regression. It is beyond the For the NIBLES HI masses, we estimate a typical relative un- scope of the paper to discuss the differing nature of these meth- certainty, due to variations within the telescope system, of about ods (see Feigelson & Nelson 1985; Isobe et al. 1986, for details). 15% and a systematic uncertainty of about 10%, after compar- At low stellar masses, log(M ) < 7.5, the relationship be- ison with flux scales of other telescopes (see Sect. 4.6). Even ? ∼ tween M /M and M apparently becomes non-linear, and we when correcting the log(M ) of the ALFALFA α.40 catalog de- HI ? ? HI therefore excluded galaxies below this limit from these linear tections by −0.16 dex, they lie on, and above, the upper envelope fits. It is sufficient to say here, that all three methods gave similar of the NIBLES detections. slopes and intercepts within 0.1 dex in log(M /M ). Using the The mean relationship found by Papastergis et al. for the en- HI ? Buckley-James method, we find log(M /M ) = −0.59 log(M ) semble of four literature samples they use to evaluate the gas-to- HI ? ? + 5.05. stellar mass ratio of galaxies as a function of M? (pink line) is Since we were concerned that our estimated 3σ MHI upper log(MHI/M?) = −0.43 log(M?) + 3.75. The latter reference samples only contain objects selected limits might be overly conservative owing to our choice of the largest observed W line widths as a function of L (see Fig. 5), based on previously known HI detections, and do not include 20 r we also explored how adjusting our upper limit estimates would any HI non-detections. Among the total of about 1000 galaxies, influence the fits. To this end, we subtracted 0.25 dex from the the largest sample used (Zhang et al. 2009) is based on 721 HI detections from HyperLeda, two others are based on Westerbork upper envelope line shown in Fig. 5, which corresponds to the radio synthesis observations (Swaters et al. 2002; Noordermeer mean relationship between W20 and Lr. In this case, we found log(M /M ) = −0.62 log(M ) + 5.20. et al. 2005) of 239 galaxies selected to have a strong enough HI HI ? ? line to enable imaging and the smallest (Garnett 2002) contains We show these two fits, dark blue when using our conser- 42 HI-detected objects. Their HI masses as used by Papastergis vative upper envelope limits and light blue based on the mean et al. are based on the originally published values, and are inde- W20-Lr relationship, in Fig. 14. The uncertainties in our fits are pendent of subsequent ALFALFA measurements. 0.03 in the slope and 0.3 in the zero-point. Although Papastergis Papastergis et al. also estimated maximum upper limits to et al. (2012) do not provide an estimate of the uncertainties in their fit, the spread of the data points in their Fig. 19 indicates a MHI/M? ratios for galaxies in their selected sky regions covered by ALFALFA which were not detected by ALFALFA, using HI standard deviation of order ±0.2 dex in log(MHI/M?) around the mass upper limits based on the 25% completeness limit of the mean relationship. α.40 catalog as a function of HI line width. These ratios also Overall, our regression fits to all NIBLES data are not very lie systematically above the relationship for the four literature dependent on the choice of line widths for HI mass upper samples. limit estimates based on our Nançay data, which on average In order to keep Fig. 14 readable, we did not plot the un- causes a difference of 0.25 dex in log(MHI); the difference in certainties for all individual galaxies but instead indicated the log(MHI/M?) between using the conservative, upper envelope typical uncertainty for both the stellar mass and the HI-to-stellar widths and the mean widths amounts to only 0.03 dex at log(M?) mass ratio of the NIBLES detections. For the HI mass, we added = 7.5 and goes up to 0.12 dex at 11.5. About one quarter of the the typical relative and systematic uncertainties in quadrature. NIBLES galaxies were not detected in HI, and most of these have A second, though minor, caveat in comparing samples shown the highest stellar masses. Therefore, the effect of using lower in Fig. 14 concerns the distance scales used. For NIBLES we MHI estimates for non-detections will have the greatest effect at used a pure Hubble-flow method and heliocentric velocities, the high mass end. whereas for published ALFALFA detections (including those used in Papastergis et al. 2012) a correction for peculiar motions 1 http://stsdas.stsci.edu/cgi-bin/gethelp.cgi?statistics

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Fig. 14. The ratio of total HI and stellar masses, MHI/M?, as a function of total stellar mass, M? (in M ). Black dots represent clear NIBLES detections, gray dots marginal detections, and red open triangles estimated upper limits for non-detections, whereas green dots represent the clear ALFALFA detections from Haynes et al. (2011). All total stellar masses used for the NIBLES and ALFALFA galaxies were taken from the SDSS “added-value" MPA/JHU catalogs (see Sect. 4). The HI masses of the ALFALFA detections were calculated in the same way as for the NIBLES −1 −1 sources, using simply a distance of D = V/H0, where the adopted Hubble constant is H0 = 70 km s Mpc . The green vertical arrow on the right indicates the mean flux scale difference of 0.16 dex in log(MHI) between the higher ALFALFA α.40 catalog HI line fluxes and the NIBLES values (see Sect. 4.6). For all fits made to the NIBLES data, we excluded sources that are either resolved, confused or missing significant SDSS flux. The dark green line shows a linear regression fit made only to the NIBLES detections. The dark blue line shows a linear regression fit to all NIBLES data including our rather conservative estimates for HI mass upper limits based on the upper envelope in the W20-Lr relationship (Fig. 5), whereas the light blue line shows a fit using low upper limit estimates based on the mean W20-Lr relationship (see text). The pink line shows the mean relationship derived for four literature reference samples of HI-detected local galaxies from Papastergis et al. (2012), which is based on a stellar mass estimation method different from the one used in the MPA/JHU catalogs (see Sect. ). For the NIBLES detections, we indicate the typical uncertainty in both quantities by the black cross on the right hand side of the plot (see text for details).

On the other hand, the difference between the Papastergis thank Eric Gérard, and Laurence Alsac and other Nançay Radio Telescope staff et al. HI-detected reference samples and the NIBLES fit using members for their technical advice and assistance. TJ and RM are grateful for the conservative upper limits amounts to −0.08 dex at log(M ) = bursary provided by the South African SKA Project Office; SB, TJ, RCKK, MR ? & PS were supported by the South African National Research Foundation. The 7.5 and goes up to 0.57 dex at log(M?) = 11.5. However, keep Nançay Radio Astronomy Station is operated as part of the Paris Observatory, in mind there may be a systematic difference of up to 0.3 dex in association with the Centre National de la Recherche Scientifique (CNRS) between the two methods used for total stellar mass estimates. and partially supported by the Région Centre in France. This research has made use of the HyperLeda database (http://leda.univ-lyon1.fr), the NASA/IPAC Ex- Our follow-up Arecibo detections of 72 Nançay non- tragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, detections show that they lie mainly among the lower envelope California Institute of Technology, under contract with the National Aeronautics of the Nançay detections and marginals in Fig. 14, indicating and Space Administration and the Sloan Digital Sky Survey which is managed that HI observations sufficiently sensitive to detect all our targets by the Astrophysical Research Consortium for the Participating Institutions. would significantly lower the mean MHI/M? ratio over the entire range of M? for our NIBLES sample of optically selected local galaxies. We will discuss this in further detail in future papers in References this series. Augarde, R., Chalabaev, A., Comte, G., Kunth, D., & Maehara, H. 1994, A&AS, Acknowledgements. We wish to thank the anonymous referee for carefully read- 104, 259 ing our manuscript and making a number of very useful comments. We wish to Auld, R., Minchin, R. F., Davies, J. I., et al. 2006, MNRAS, 371, 1617

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Appendix A: Notes on individual galaxies mean independent optical value of 1266 km s−1 (Sandage 1978; Tonry & Davis 1981; Vennik & Kaazik 1982; Falco – Source 0023 (KUG 0007+140): Detected in ALFALFA, but ◦ et al. 1999). It has no HI detection, either from NIBLES or not in NIBLES. Small, blueish galaxy of about 60 inclina- in the literature. tion, without clear spiral arms. The ALFALFA detection has – Source 1319 (PGC 1275866): The W line width is much a W of 205 km s−1 and a 7 mJy peak flux density (peak SNR 50 50 larger in NIBLES than in ALFALFA (69 and 37 km s−1, re- = 2.8, S/N = 6.8, rms = 2.5 mJy). The NRT rms is lower, 1.8 spectively). The peak in the NIBLES profile which is cen- mJy, but the NIBLES spectrum only shows a narrow, 6 mJy tered on the optical velocity has about the same width as the peak at the optical velocity. The mean ALFALFA flux den- ALFALFA profile, but in addition it has a noise peak cen- sity of 5.4 mJy is merely at the 3.0 σ level for the NIBLES tered on a ∼100 km s−1 lower velocity which rises up to 35% spectrum. However, our four times deeper Arecibo observa- of the main peak level. The latter can explain the measured tions (see Paper II) show a clear detection (S/N 15) at a mean width difference. We could not identify a potentially confus- level of 3.5 mJy, which is considerably lower than the AL- ing other galaxy within the NRT beam. FALFA value, and too low to expect a NIBLES detection. – Source 0117 W I −1 – Source 1355 (MCG +09-19-160): Its SDSS DR9 redshift is (SHOC 30):Its 20 H line width of 390 km s −1 is significantly higher than for the other detections of similar unconstrained (nominally at 1245 km s ), and we adopted the value of 1233 km s−1 of the marginal NIBLES HI detec- luminosity, log(Lr) = 8.25 (see Fig. 5), but it is a relatively W tion, which is marginally lower than the independent optical weak detection and its estimated uncertainty in 20 is of or- −1 der 30 km s−1, which could move it below the upper envelope velocity of 1322±50 km s (Falco et al. 1999). plotted in Fig. 5. Also, the detection could be confused, as – Source 1371 (CGCG 292-024): Its SDSS DR9 radial ve- − there are two other blue compact objects in the NRT beam, locity is unconstrained (nominally 1245 km s 1), and we − without known redshifts. adopted the NIBLES HI value of 1294 km s 1 which agrees – Source 0609 (KUG 0814+251): Its DR9 and DR6 velocities with the independent optical literature value of 1265 km s−1 are significantly different (2075 and 1496 km s−1, respec- (Sandage 1978; Tonry & Davis 1981; Vennik & Kaazik tively), and we used the mean independent optical velocity 1982; Falco et al. 1999) and the previous Nançay detection −1 of 1888 km s−1 (Augarde et al. 1994). It has no HI detection, at 1282 km s (Garcia et al. 1994). either from NIBLES or in the literature. – Source 1598 (VCC 0315): Its DR9 and DR6 velocities are – Source 0718 (CGCG 263-080): Its DR9 and DR6 veloci- significantly different (1589 and 1461 km s−1, respectively), ties are very different (7602 and 2340 km s−1, respectively), and we used the independent optical velocity of 1575 km s−1 and we used the independent optical velocity of 7669 km s−1 (Grogin et al. 1998; Falco et al. 1999). It has no HI detection, (Falco et al. 1999). It has no HI detection, either from either from NIBLES or in the literature. NIBLES or in the literature. – Source 1654 (PGC 40315): Its SDSS DR9 radial velocity − – Source 0784 (UGC 4722): The W50 line width is much is unconstrained (nominally 1245 km s 1), and we adopted − smaller in NIBLES than in ALFALFA (57 and 137 km s 1, its mean independent optical value of 1370 km s−1 (Prugniel respectively) but the ALFALFA spectrum could not be found 2001, private comm.; see HyperLeda). It has no HI detection, in the survey’s online database. The NRT profile becomes either from NIBLES nor in the literature. much broader just below the 50% level, and its W20 = 152 – Source 1715 −1 (IC 3665): Its DR9 and DR6 velocities are very km s . different (7 and 1200 km s−1, respectively), and we used the – Source 0793 (NGC 2743): The NIBLES profile is as broad independent optical velocity of 1227 km s−1 (Binggeli et al. as the ALFALFA detection at the W20 level, but at the 1985). It has no HI detection, either from NIBLES or in the 50% level the lower-velocity half of the line is considerable literature. weaker in the NIBLES profile, hence the difference in W 50 – Source 1717 (NGC 4649): Its DR9 and DR6 velocities are (74 and 178 km s−1, respectively). The NRT spectrum slop- different (1169 and 1018 km s−1, respectively) and based on ing off could in principle be due to a superimposed, narrow two spectroscopic targets on either side of the galaxy center. OFF-beam detection. Instead, we used the mean independent optical velocity of – Source 0824 (KUG 0910+433): Its DR9 and DR6 veloci- 1117 km s−1 (from a dozen references, see HyperLeda for ties are very different (4232 and 2641 km s−1, respectively), details). It has no HI detection, either from NIBLES or in the and we used the mean independent optical velocity of 4221 literature. km s−1 (Saunders et al. 2000; Falco et al. 1999). It has no HI detection, either from NIBLES or in the literature. – Source 1723 (ASK 77777): Its SDSS DR9 radial velocity is unconstrained (nominally 1245 km s−1), and we adopted – Source 0828 (ASK 261057): Its DR9 radial velocity is un- −1 constrained (nominally 1245 km s−1), and we adopted our the independent optical value of 1169 km s (Colless et al. Arecibo NIBLES HI value of 1370 km s−1 (Paper II). There 2003). It has no HI detection, either from NIBLES or in the are no independent literature values. literature. – Source 0958 (PGC 4571034): The W50 line width is much – Source 1771 (PGC 1132599): Its DR9 and DR6 veloci- − larger in NIBLES than in ALFALFA (116 and 32 km s−1, ties are significantly different (1235 and 982 km s 1, respec- respectively). The peak in the NIBLES profile which is cen- tively), and we used the independent optical velocity of 1229 − tered on the optical velocity has about the same width as the km s 1 (Colless et al. 2003). It has no HI detection, either ALFALFA profile, but in addition it has a noise peak cen- from NIBLES or in the literature. tered on a ∼80 km s−1 higher velocity which rises up to 60% – Source 1970 (NGC 5356): The NIBLES and ALFALFA pro- of the main peak level. The latter can explain the measured files are as broad at the W20 level, but the NIBLES profile −1 width difference. We could not identify a potentially confus- is much narrower at the W50 level (127 vs. 278 km s , re- ing other galaxy within the NRT beam. spectively), which appears to be due to a narrow OFF-beam – Source 0998 (NGC 3156): Its SDSS DR9 radial velocity is detection centered on ∼1320 km s−1 and cutting through the unconstrained (nominally 1245 km s−1), and we adopted the lower-velocity half of the line profile.

Article number, page 18 of 71 van Driel et al.: NIBLES – the Nançay HI survey

– Source 2140 (ASK 082514): Its DR9 radial velocity is un- constrained (nominally 1245 km s−1), and we adopted our Arecibo NIBLES HI value of 1728 km s−1 (Paper II). There are no independent literature values. – Source 2155 (NGC 5644): Its DR9 and DR6 velocities are very different (7650 and 64 km s−1, respectively), and we used the mean independent optical velocity of 7649 km s−1 (Huchra et al. 1983; Falco et al. 1999). It has no HI detection, either from NIBLES or in the literature. – Source 2167 (NGC 5675): Its W20 HI line width of ∼1030 km s−1 is significantly higher than for the other detections of similar luminosity, log(Lr) = 10.4 (see Fig. 5), but the SDSS image clearly shows it is an ongoing major merger, so we can expect unsettled gas at extreme velocities. – Source 2183 (LSBC D723-05): Although the NIBLES and ALFALFA HI profiles look similar, the fitted W50 width is much smaller in NIBLES compared to ALFALFA (62 and 121 km s−1, respectively). This may be due to the bumpy slope of the low-velocity edge of the profile, the presence of noise spikes and differences in the line width measurement algorithms. – Source 2265 (PGC 3350778): Its SDSS DR9 radial velocity is unconstrained (nominally 1245 km s−1), and we adopted the independent optical value of 1312 km s−1 (Mahdavi et al. 2005). It has no HI detection, either from NIBLES or in the literature. – Source 2356 (CGCG 137-019): Its DR9 and DR6 veloci- ties are very different (4508 and 12 km s−1, respectively), and we used the mean independent optical velocity of 4555 km s−1 (Falco et al. 1999). It has no HI detection, either from NIBLES or in the literature. – Source 2555 (KUG 2335+148): Detected in ALFALFA, but only marginally in NIBLES. Very small blue, roundish galaxy with an arc of star formation clumps; it looks like a late-stage merger. The ALFALFA detection has a W50 of 106 km s−1 and peak flux density of 10 mJy (peak SNR = 5, S/N = 8.0, rms = 2.1 mJy). The NIBLES rms noise level is lower, 1.7 mJy, but nothing is visible in the NRT spectrum although the mean Arecibo flux density is at the 4.3σ level for the NIBLES spectrum.

Article number, page 19 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.190.42 3.40.11 5.00.36 4.20.31 5.4 10.0 6.10.28 6.1 9.06 4.30.45 9.82 5.7 9.30.50 -0.67 12.1 10.5 7.56 -0.36 0.37 13.2 9.53 4.00.23 35.5 9.41 0.80 10.19 4.70.39 -0.03 5.0 8.73 0.74 6.90.35 -1.12 3.8 7.20.31 8.73 9.86 5.3 9.40.25 14.4 9.53 4.30.21 -1.27 10.3 9.26 9.60.12 23.9 -0.31 9.18 3.00.09 13.8 10.26 0.15 9.46 3.60.31 -0.40 5.0 -0.63 8.55 3.60.30 18.9 1.99 2.80.46 8.55 8.82 9.0 4.10.45 31.5 20.0 8.160.14 -0.30 10.1 14.4 7.53 8.990.22 45.8 0.31 4.00.28 20.2 8.69 0.26 10.01 8.99 4.60.13 5.5 9.69 5.10.39 8.69 0.11 3.7 6.30.08 3.04 8.58 4.0 8.30.18 9.03 4.40.30 4.0 0.32 9.20 3.00.27 6.0 -0.14 10.5 8.630.33 2.7 0.41 9.47 5.70.15 4.7 18.4 -0.68 23.7 8.020.26 -1.13 8.81 2.9 9.670.31 9.1 44.6 -0.08 9.30.35 -0.06 10.09 0.13 4.8 9.290.39 3.7 14.1 4.00.17 0.16 -0.03 11.6 8.43 8.30.29 9.48 3.6 6.70.12 23.1 -0.02 9.50 -0.47 5.00.23 9.30 9.62 3.5 4.20.46 -0.16 5.5 7.00.26 -0.11 0.26 8.59 8.1 3.80.45 9.03 6.5 8.30.43 0.27 16.3 8.34 6.50.44 22.2 0.64 13.0 8.900.42 9.45 13.7 2.12 12.3 44.8 -0.32 0.72 9.37 13.9 -0.99 31.40.51 9.67 -0.47 9.85 7.1 27.10.19 18.7 -0.34 9.700.20 3.20 16.5 9.60 4.40.23 42.8 1.64 4.5 9.45 11.3 1.82 9.85 6.7 6.5 1.74 18.0 1.25 8.52 8.55 9.23 0.82 0.74 0.26 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 7 2146 2327 407 0.67 1783 58 700 209 466 0.26 9 7296 2.02 492 2298 2.55 180 10.05 261 2092 2023 1.70 231 1166 1.35 8 1.06 96 143 1054 1173 41 4.56 1172 40 2.02 1 80 0.48 61 1313 55 294 129 0.18 147 312 0.20 313 4.96 5 2.70 338 13.58 7 1763 5.82 5 55 196 3112 33 1.45 74 322 2781 0.31 1.55 51 298 1422 0.11 4 3.56 170 136 2382 8.98 1559 254 243 2.27 1216 1.66 259 1443 5.74 86 0.43 332 10184 350 0.28 2718 2338 4.79 311 278 300 232 3.42 9 353 11.26 313 246 8.08 3 6.42 365 11.93 93 123 2.37 / HI 21 23317 308 117 2.50 19332 1.75 184 27610 1.92 199 237 2.06 1127 114 128 146 214 0.41 21 0.73 12210 167 11718 0.50 159 8411 1.42 121 162 0.31 11 19415 66 1.44 10823 75 1.07 217 132 324 0.95 1.85 36 1132010 293 67 111 4.89 129 142 0.59 0.74 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 34 0.971 1.11 -19.392 -0.18 -20.20 0.80 -14.79 9.743 10.18 -19.613 6.76 -9.96 -10.15 1.672 9.57 2.00 -21.623 -8.37 1.38 2.65 1.46 -19.102 11.31 -9.75 1.04 1.57 -23.22 7397 6 6009 -12.02 0.87 -19.362 2.84 11.14 — 0.87 -18.01 1705 4 1.17 -11.57 0.30 9.84 6365 -19.18 1.37 9.11 -18.72 11228 —2 3.33 -9.99 9.57 -22.622 -9.92 0.88 7.47 2.18 -10.682 8860 2.54 10.89 0.40 -18.862 1.74 -12.30 0.33 2.78 1049 -16.395 6401 — 0.64 9.12 -14.284 2.85 5281 7.85 0.37 5425 -18.142 2.49 -9.95 7.27 1.04 -15.332 -9.44 9110 1.16 5400 -20.562 2.12 — -9.40 0.54 -20.085 1.69 — 0.63 9.91 -16.942 1.27 5391 0.77 6.65 -17.88 -10.37 —1 4030 0.91 8.26 -17.553 — 1870 -7.97 1.62 9.17 2.84 2.91 -18.342 -9.37 0.60 8.79 2.71 -21.525 2.67 0.71 9.31 3956 2018 -16.342 1.23 10.60 — -9.87 1.05 -17.354 1939 4202 -9.51 0.70 8.10 -19.102 4390 -9.96 1.67 2.15 0.81 8.68 -18.333 1.69 -9.34 0.17 9.73 2.40 -20.34 5541 4 4790 -9.82 1.01 9.32 -18.32 -10.31 1.18 5352 0.98 9.93 -19.764 6263 1.56 -9.68 8.45 1.90 -19.781 -9.91 4370 0.77 9.953 5205 2.37 -8.81 0.54 9.66 -19.68 5228 -10.271 2.76 0.64 -17.39 -10.10 5314 2 1.48 9.37 0.38 2.26 -16.704 5309 8.31 0.64 2.12 -10.09 4276 -17.502 1.37 8.38 5277 -18.785 -9.50 1.04 2.62 6.22 6301 -21.462 -9.61 0.96 9.22 -20.45 1.541 10.45 -8.85 0.99 3891 -21.00 3.063 -9.79 -11.32 9.85 0.46 -20.61 1.332 10.01 4316 0.33 4541 -16.89 2.19 2.653 -9.71 -10.15 6.64 0.60 -15.892 4000 8.06 1.37 4156 1.58 -16.694 2.76 3515 -8.25 7.78 0.06 -20.774 -9.37 0.49 5145 7.71 -15.68 2.71 5357 -9.45 8.60 -16.18 2.55 — -9.08 7.70 2.56 3589 -19.17 7.81 4.58 3570 — -9.14 3571 8.97 -9.36 3546 2.92 1.78 -9.91 1.78 3389 3525 2.24 3155 3853 / 10 0.72 -17.24 8.67 -9.77 2.37 5142 11 0.84 -18.38 9.41 -11.96 2.75 5347 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± 539 -0.18 -14.37 — — 2.48 1913 V ± ± km ± 1413283 5344 + 156 6000 134 5378 001 4151 + + + (J2000.0) [log] [log] [log] [log] 00 03 11.3000 03 15.00 1500 57 03 56.50 32.10 16 08 44.70 IC -10 5381 44 40.70 NGC 7814 NGC 780800 07 11.6000 13 08 46 48.79 06.80 KUG 0004 14 02 01.30 PGC00 4018118 13 02.7600 13 11218 38.62 1059 14 24 34.80 8865 00 15 15 40 50.73 28.00 UGC 0119 FGC 5A 16 05 20.70 UGC 1888 00 0148 20 48.60 14 13 27.80 2MASX J00204857 2009 1961 4154 00 28 03.9000 29 16.80 14 18 06.40 -01 00 25.30 PGC 2816194 KUG 0026-01200 30 29.8000 31 13.30 -08 4600 59.80 31 21.90 -10 2900 01.40 31 2MASX 22.30 J00302984-0847002 -10 2400 25.50 31 2MASX 27.50 J00311327-1028518 -10 2200 42.70 31 ASK 35.97 126658 -10 5388 40 33.10 ASK 4543 126660 -10 4000 3500 30 17.30 SHOC 02000 32 48.96 2MASX J00313571-1030228 -10 00 43.70 3583 2MASX J00255246-0939427 3660 3859 3524 3522 Basic optical and HI data – clearly detected galaxies F F 3 2 1 3 1 1 1 3 1 N NZF N N F A N N F R C C C C C C C C Table A.1. 00020004000500060007 00 00 12.800008 00 01 03.590010 00 01 01 07 33.95 12.700011 00 14 02 34 14.77 48.600013 CGCG 382-016 15 04 53.600016 ASK 146570 14 29 15.99 CGCG0017 433-016 PGC0019 4567836 00 03 44.320020 00 06 02.380021 00 16 07 11 01.59 12.700022 14 25 02.900029 CGCG 00 456-027 14 7396 08 06 34.29 23.600030 UGC 0043 -10 UGC0031 56 0056 00 1714 6352 57.50 09 40.230035 00 09 5131 50.40 2MASX J00083428-1056579 -100039 25 00 02.70 12 14.68 -000041 55 04.00 2MASX J00094023-10250270042 15 9099 15 26.70 ASK 275890044 00 6418 14 31.90 ASK0047 147670 5415 0049 -00 44 00 15.20 19 11.000050 5274 00 19 20.60 UGC0051 0139 5421 00 15 20 06 09.30 22.700052 15 58 40.600053 ASK 00 147806 14 21 17 51.20 28.700055 ASK 00 147996 21 58.700056 -09 ASK 29 00 147978 32.10 22 4029 20.300057 00 15 1879 22 58 57.10 51.80 2MASX0060 J00215111-0929321 00 15 23 56 14.90 30.300062 ASK 00 16 148034 23 15 59.40 11.200063 ASK 00 148040 14 24 6269 48 25.90 34.300064 3946 UGC 00 0219 15 24 46 42.69 13.500065 PGC 00 1467720 14 25 04 4363 28.86 10.300066 NGC 00 0099 14 26 49 5485 24.97 28.400068 -08 ASK 48 00 147870 26.60 27 4803 49.700070 UGC 00 0233 01 27 01 53.80 12.00 2MASX0071 J00252890-0848260 -01 11 59.90 -000072 UGC 58 0252 00.50 4388 UGC 02720073 00 6313 29 5213 PGC 38.40 31079050074 00 30 07.300075 5300 00 00 5245 30 24 09.00 37.40 -110076 06 49.10 -09 KUG 570077 0027 5308 11.80 4269 2MASX J00300730-11064910079 Mrk 09510080 5276 0081 3527 5350 4345 3898 00 31 40.70 00 32 31.30 -09 34 34.30 -10 41 22.10 ASK 126851 ASK 126629 5129 3395 3156 Source0001 RA 00 00 02.10 15 52 54.10 Dec KUG 2357 Name

Article number, page 20 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.320.54 40.20.21 19.10.27 68.7 4.60.44 46.5 2.9 9.400.53 10.04 5.2 6.20.16 1.14 -1.04 6.4 4.10.36 10.0 9.27 8.60.47 11.9 10.8 8.740.40 -1.47 9.66 15.8 5.00.24 25.7 9.61 0.02 -1.08 4.90.22 9.20 9.87 4.2 2.12 7.40.43 15.2 -0.38 6.50.21 9.87 9.27 8.5 7.10.34 30.6 10.00 6.70.24 -1.63 18.7 -0.95 9.17 3.1 9.590.16 10.8 3.90.39 9.72 -0.74 1.63 8.9 4.50.34 9.26 -0.77 4.0 5.60.36 11.8 -0.95 9.08 6.30.51 9.05 5.4 6.30.32 -0.53 8.86 12.6 4.50.40 -0.37 9.08 9.6 0.24 9.90.13 9.31 7.4 7.90.23 -0.07 16.7 -1.63 9.46 5.10.17 13.7 9.33 4.10.24 9.50 0.40 6.60.33 5.1 9.69 9.33 -1.12 8.6 4.20.22 10.0 -0.19 8.84 3.20.43 15.2 8.67 4.00.61 8.92 8.84 4.1 5.60.13 9.57 19.6 0.52 6.0 0.63 0.47 8.94 -0.59 6.7 7.50.17 37.4 8.93 6.90.33 1.34 9.37 9.06 3.5 9.90.35 0.05 12.9 4.10.15 -1.52 29.5 0.82 8.870.21 3.5 9.57 6.8 6.90.38 53.7 2.01 -0.14 7.4 8.540.36 29.4 9.28 9.18 8.80.19 -0.45 25.6 17.30.23 65.8 -0.93 0.65 8.09 4.80.13 51.5 9.55 10.39 4.90.28 -0.21 10.26 -1.02 4.3 -0.59 7.60.28 5.7 4.20.33 2.45 9.12 9.6 3.90.45 10.9 8.15 7.30.24 -0.49 13.1 16.0 8.550.21 21.6 0.58 9.29 4.10.22 29.1 9.57 0.37 5.3 9.730.25 -1.28 3.9 9.78 6.7 0.07 -0.85 10.1 3.3 -0.72 8.90 5.4 9.09 5.4 -0.32 -1.21 8.85 8.83 0.55 0.23 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 11 1437 4606 169 133 478 176 13.37 158 16.32 1904 0.81 8 0.70 1778 342 214 3194 370 5.65 349 225 2.19 8 1.72 2747 2636 4.14 259 2818 59 278 0.97 5566 0.85 983 591 290 0.95 6 2024 2.72 310 2329 2283 60 2.58 266 79 3.35 1319 3.38 78 106 149 378 0.40 0.56 2 1.03 3994 133 1.18 108 167 127 13.18 13 0.79 1779 1041 194 3141 121 206 11.83 6 363 1995 0.81 233 1865 2.31 229 15.91 7 86 208 11.68 3 77 346 105 0.92 157 92 375 0.57 4 182 0.30 1.33 1968 2.73 209 108 1.02 129 0.71 / HI 1273 31914 225 365 93 551 2.76 17921 2.43 1.20 1311610 194 215 264 0.92 312 31210 4.49 1.40 55720 586 267 1.60 346 2.09 11 1601860 227 188 190 2.06 23814 36113 0.78 26651 1.55 136 334 287 169 3.59 435 0.35 1.23 1017 145 14817 227 307 20330 3.83 6.00 269 142 1.22 212 0.74 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 33 1.734 1.37 -22.792 0.75 -22.191 11.08 1.35 -18.051 10.75 -11.74 0.44 -22.31 -11.85 8.72 0.57 -17.553 2.69 10.75 -20.253 1.83 -9.86 -10.75 7.48 1.621 3744 9.58 1.60 -20.69 2.123 2.52 6960 -9.95 0.09 -22.502 10.90 -9.28 1.04 5895 -18.424 2.46 4068 10.94 -10.70 1.51 -20.683 1.29 -10.54 1.71 7.54 6022 -21.871 10.32 2.64 1.33 5228 -18.536 10.49 2.36 -10.35 0.82 -17.98 10.21 — 4217 -10.21 0.80 -18.81 10941 2 1.48 -10.39 9.61 -18.23 1.862 2.68 9.42 1.62 -10.523 1.31 4382 8.62 0.61 5761 4916 -22.594 -9.83 2.18 1.20 5225 -10.60 -18.465 10.94 1.25 -21.461 1.55 -12.78 0.95 1.71 9.06 5059 -21.132 0.48 -19.792 10.62 5245 1.51 — -9.66 0.51 3982 -17.765 -10.39 0.51 9.87 -16.421 2.13 3944 1.11 -17.21 -10.342 — 2.31 — 0.30 8.15 -21.06 5350 2 0.72 8.29 2.65 3.13 -16.092 10.16 -9.53 4450 1.74 -18.26 —2 -9.55 -10.54 7.60 0.43 5454 4161 -22.184 2.46 8.89 0.14 1.66 -17.442 1.48 1.75 10.89 -8.95 1.52 -17.094 4173 -9.88 -11.57 8.25 0.68 5993 -18.21 6103 1 1.80 4096 1.55 6.86 -18.933 1.57 2.45 -9.54 0.73 9.71 -20.663 3893 0.70 8.99 4764 -17.96 5655 3 5.07 10.21 — 1.45 -16.609 — -9.69 -10.50 1.48 8.53 -21.723 1.26 1345 -0.02 8.30 -22.714 2.80 10.57 1.40 1.72 -9.87 0.99 -16.85 -10.182 10.98 4398 -10.39 0.41 4631 4526 -19.26 5673 2 2.74 7.81 -12.57 0.60 1.49 -15.535 1.23 1.35 9.61 -10.30 -16.413 2.75 1621 0.74 7.57 1774 -20.41 -10.064 5675 2.63 8.18 1.51 -19.513 10.56 -9.10 5656 1.38 1.45 -21.792 -9.64 -11.80 0.70 5657 9.49 -21.732 2.40 10.58 1.37 5462 -19.47 -10.553 1.45 10.49 1.60 -11.92 0.38 -21.10 2269 -10.89 0.69 9.22 2.23 -17.19 10.30 4933 2.40 5496 -16.97 2.78 -9.66 -10.45 8.29 5288 5414 8.60 4548 1.79 1.39 -9.37 -9.80 4590 2.09 4006 1.89 4520 4356 4 0.78 -17.11 8.27 -10.37 2.69 1986 / 45 0.91 -21.60 — — 2.7011 0.89 5243 -18.39 9.15 -11.95 1.76 3949 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± km 1439509 5219 + . (J2000.0) [log] [log] [log] [log] continued 00 34 57.90 -09 2000 31.90 36 28.9000 36 2MASX 38.40 J00345797-0920323 -10 06 22.10 -10 0800 44.20 37 NGC 55.89 016500 6942 39 ASK 13.75 126563 -09 15 11.2000 00 39 51 2MASX 22.90 42.40 J00375747-0915092 -08 NGC 49 0192 24.40 5317 ASK 12722300 41 11.6000 41 16.20 15 03 09.70 5889 6032 00 15 41 13 29.50 01.50 FGC 007700 41 33.90 -10 CGCG 00 434-03000 47.50 41 38.00 -10 01 17.10 ASK 127634 4177 00 15 NGC 27.40 0217 5755 ASK00 30093 43 55.30 -09 13 47.50 5269 ASK 127769 5059 00 46 47.06 4035 00 47 46.43 -00 42 02.90 3932 -09 5000 06.10 49 ASK 17.00 5416 30486 2MASX J00474641-0950063 -08 4600 22.60 50 27.50 PGC 1002925 -08 6002 43 5729 06.60 2MASX J00502753-084306700 56 42.7000 4525 56 44.90 -09 54 49.90 4749 -09 48 17.70 NGC 0309 4389 ASK 12836900 59 40.1001 15 00 19 04.10 51.50 -11 UGC 04 0615 57.30 2MASX J01000412-110457701 01 43.60 5648 -09 5691 19 5408 00.70 PGC 992557 5483 4519 – 1 1 1 1 3 3 3 1 1 3 1 3 3 N NC NZF N NC NP N N N N C C C C C C C C C C C Table A.1. 00830085 00860088 0089 00 34 02.800090 -090091 42 00 19.20 35 26.300093 NGC 0151 -090094 45 37.100095 00 37 PGC 10.60 9867760096 -090097 27 25.100098 00 39 Mrk 20.10 09540101 -100102 28 00 55.40 39 34.800103 00 39 35.80 2MASX J00392015-10285490104 00 00 39 51 38.30 35.80 3732 -090105 11 40.30 10895 NGC 4078 0107 0201 14 39 51.20 NGC 01950109 00 41 23.90 2MASX0110 J00393835 -000111 03 53.900112 5229 ASK 300110113 00 43 27.800114 00 43 32.400115 -00 07 00 41.10 43 51.870117 14 20 33.20 NGC0118 0237 4380 00 00 44 48 23.30 07.00 4894 0119 NGC 00 0234 45 34.700120 UGC 00 0466 14 45 17 51.92 15.70 -100121 59 00 14.00 46 08.80 -090122 PGC 19 1454298 41.50 3989 ASK 127560 -100123 24 31.00 2MASX J00455191-09194090125 00 47 SHOC 47.50 3001270128 -09 53 00 6108 58.30 49 52.980130 4172 UGCA 140132 4445 00 00 51 57 18.50 38.900133 5437 00 51 59.600134 -09 CGCG 4192 01 00 384-011 12.40 52 52.800135 -00 4103 29 00 12.10 53 29.92 2MASX0136 J00511854-0901125 01 12 50.40 2MASX J00515961-0029114 -080137 46 04.000138 CGCG 384-019 3910 00 5696 57 NGC 41.90 02910139 00 1627 57 56.600140 00 15 58 04 55.50 04.900141 1344 00 4600 52 08.900142 CGCG 00 13 435-026 59 43 42.10 15.000143 ASK 310330144 PGC 3126941 01 00 00 54 45.80 59.70 01 1774 01 16.60 -09 UGC 11 01 0618 08.50 01 19.50 -10 37 40.80 NGC 5689 0341 -09 50 01 42.90 02 00.40 2MASX J01011685-1037394 5464 2MASX J01011945-0950434 15 34 57.70 4023 2281 4942 PGC 3128241 4591 5287 4538 4354 Source0082 RA 00 33 22.10 -01 07 16.70 Dec UGC 0328 Name 1989

Article number, page 21 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.170.15 3.80.47 4.00.19 6.1 5.60.16 4.6 2.40.49 12.9 8.75 6.80.32 8.41 10.38 3.7 6.90.45 0.72 3.7 6.6 -0.53 0.23 -1.02 8.94 6.3 4.50.18 7.60 4.00.35 5.0 -1.79 12.2 9.97 4.90.26 0.57 9.78 4.9 6.40.13 -1.40 9.89 9.3 7.50.38 -1.25 8.96 -0.26 7.0 9.50.28 44.7 12.3 8.740.46 -0.47 13.1 9.47 9.70.37 86.1 8.02 0.20 8.40.24 -1.02 22.1 8.91 7.1 9.46 0.27 0.18 11.9 3.8 8.830.16 -0.92 13.3 0.21 5.00.19 9.41 0.92 6.40.28 5.6 9.81 3.80.28 6.8 0.33 9.05 7.0 -0.57 0.35 8.9 5.3 8.040.20 5.9 -0.61 10.8 8.6 8.830.37 1.98 8.82 4.2 9.10.86 -0.34 8.43 46.6 18.30.27 -0.03 104.6 9.30 5.8 7.4 0.07 0.17 9.43 6.70.36 -0.14 9.80 12.7 13.4 8.89 0.22 0.38 5.3 10.38 9.30.32 -1.03 9.80 18.7 5.40.34 -1.01 13.0 9.09 8.56 6.80.30 6.9 9.00.23 24.0 0.96 8.56 9.04 8.70.31 12.0 10.01 13.6 9.420.16 -0.22 16.8 3.9 -0.83 0.12 18.1 9.52 17.2 0.70 0.21 8.69 7.6 8.57 7.40.51 0.78 26.3 3.3 0.28 0.43 0.96 9.27 7.0 9.39 9.80.25 9.7 3.60.26 -0.59 10.7 0.27 8.06 3.50.17 17.6 8.87 3.30.22 8.97 0.84 5.90.37 5.5 -2.03 9.66 4.1 1.07 5.00.20 8.48 8.4 8.2 9.66 0.43 9.06 3.8 6.00.26 10.2 8.48 16.5 8.700.41 -1.96 8.94 5.2 7.40.50 20.7 9.15 11.7 0.75 -1.15 -0.14 8.92 5.4 9.78 7.0 33.4 -0.89 -0.66 10.17 9.14 9.6 -0.58 0.28 9.60 -0.94 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 76 82 31 1023 47 0.57 42 0.20 5 565 189 0.61 1525 2053 1711 85 0.92 2 0.82 90 167 1184 122 109 197 1.77 1257 145 0.79 19.48 151 2683 3.65 7 3.27 2873 84 1445 0.85 127 1006 164 173 144 195 0.85 1 0.71 1947 1.85 234 2656 1.58 5312 3.84 299 112 561 23.91 1124 1395 7.60 135 189 1.51 4547 1.88 2045 503 118 2.17 2 70 4.93 1644 104 117 2.80 5 61 134 2.11 3 120 2.53 86 137 146 0.66 1616 3.24 3 4.67 294 2085 312 228 3783 0.85 9 3.86 413 388 344 5.70 417 380 8.82 3.07 / HI 3023 49123 71 62324 500 14517 3.73 201 564 0.62 243 26712 1.46 318 0.98 249 3.21 291 2.04 14 17114 243 66 2.83 117 0.61 19 241 29810 0.91 11411 154 145 1.43 23 198 172 2.67 12 235 326 1.33 10 35430 10915 0.50 448 134 68 51922 0.83 130 0.81 12010 0.67 180 51 0.80 91 0.93 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 23 0.782 1.42 -18.632 1.45 -21.393 8.95 0.05 -20.613 11.40 1.57 -14.544 10.72 -9.76 -10.94 1.47 -21.924 -12.15 7.03 1.01 2.37 -21.252 2.10 11.37 1.03 -21.403 1.74 11.03 -8.78 11520 -12.40 0.66 -18.364 5224 10.16 -11.61 1.44 -17.80 5371 5 2.34 2.31 -10.10 0.40 9.43 -21.453 2.20 11548 8.54 1.05 -14.25 -10.122 10.48 1167 2.75 11350 0.70 -19.48 -9.66 -12.17 7.75 0.42 1.72 -19.51 7112 4 9.84 -16.625 1.46 2.22 1.03 9.25 4538 -11.141 — 1.14 7.90 5456 -20.812 -10.21 3725 -2.29 1.41 -19.57 2.58 10.38 -9.31 0.61 -12.25 2.899 -10.27 9.66 4632 -19.074 2.48 1108 6.06 0.366 1757 -10.48 2.64 0.79 9.17 -17.134 -8.30 1949 0.72 1.52 -19.104 6879 -9.43 1.21 8.36 -18.82 1.843 0.70 9.45 -19.06 5242 -10.024 1.71 9.21 1.64 1933 -19.85 -10.093 9.92 0.43 2.53 -10.20 -23.274 4093 0.55 2.17 -10.33 -16.423 11.39 — 0.84 2.46 1737 -17.262 -13.12 0.71 1.29 8.13 5131 -19.253 1.66 3796 -17.53 —2 4.00 — 4203 -9.39 0.52 9.26 -20.491 0.61 8.73 2.32 -17.87 -11.422 2.53 10.84 8127 0.12 -15.87 -10.557 — -11.20 1.14 8.74 3.20 2334 -16.61 4122 0.57 8.41 2.89 1.57 -20.302 1.57 -9.66 3981 7.61 -17.002 1.51 9.86 5040 1997 2.67 — -8.66 6562 0.43 9.12 -22.476 -9.94 5107 -15.843 2.53 2.29 10.90 0.752 2.24 — -12.32 7.91 1.75 -16.892 1917 1913 0.36 5364 -22.454 1.55 1.25 -9.71 1.15 -16.503 11.02 — 0.85 -20.96 5555 4 4.57 4506 -12.02 1.24 7.95 -18.251 10.09 1.54 -20.24 —3 2453 1.26 -9.86 -10.26 9.29 0.45 -21.331 9.80 1.46 2.37 -10.37 -18.88 5424 1.61 1.35 10.44 1.38 -22.22 2747 -10.71 2.67 8.85 3962 -20.43 10.75 — 4623 10.54 2.33 -9.20 -11.47 2761 1.63 -10.28 3.03 2.19 4660 4635 2.82 5513 5879 5154 4 0.40 -16.68 8.03 -9.41 1.82 4525 / 13 0.67 -18.30 9.0811 -11.00 0.54 4.05 -16.95 8.85 4065 — 1.65 4397 18 0.48 -14.8317 7.22 1.06 -20.10 -9.42 1.41 — 1909 — 3.71 4486 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± ± km 0027460 4549 + 00-04-049 1107 + . (J2000.0) [log] [log] [log] [log] continued 01 06 50.9901 07 14.20 -00 3401 13.70 07 22.60 1301 57 09 PGC 18.40 07.90 1140108 0001 55 09 33.40 21.99 IC 1620 0101 07 09 15.70 28.80 NGC 0391 14 20 32.20 SHOC 053 14 21 47.20 UGC 0717 UGC 071901 14 20.4001 14 5211 36.80 0001 55 15 01.90 30.40 01 10 46.90 MCG -00 5101 39.50 17 11436 48.39 UGC 5345 0790 NGC 450 -08 1167 36 27.10 11505 11250 MCG -02-04-02001 4630 4081 22 10.2001 1756 22 23.80 00 56 57.70 -00 5201 30.70 23 14.50 NGC 0493 NGC 0497 -00 42 04.8001 25 22.10 UGC 0931 14 50 19.30 IC01 1698 27 09.40 -09 18 08.10 2363 2MASX 8131 J01270941-091808001 30 15.4001 31 26.90 1985 1401 5336 40 31 39.10 36.05 14 17 05.00 LSBC F612-01 13 19 52.70 UGC 1087 PGC 6554 9384401 33 35.2001 34 02.50 -01 05 31.00 -01 0401 32.70 35 UGC 51.10 1116 2454 UGC 1120 -10 00 10.60 4567 NGC 0624 2744 4741 4638 5870 – 2 1 3 1 1 3 3 1 2 3 3 N NC N N N N N NF N N R C C C C C C C C C C Table A.1. 0157 0159 0160 0161 0162 0163 01650166016701680173 01 10 20.800174 01 11 35.50 -090177 01 34 12 10.30 07.750179 01 00 12 27 08.63 39.70 2MASX -01 J01102076-09341040180 00 02.40 -00 2MASX0182 24 J01113551 36.70 2MASX J01120777-01000220183 7111 IC 16430184 01 17 30.500186 3726 0187 -09 17 01 48.30 18 45.900188 01 19 04.40 PGC0190 4647 01 14 19 59 14.30 35.600191 -00 08 01 18.80 19 32.900192 -09 UGC 01 35 0838 19 46.40 58.70 UGC0193 0847 01 14 20 52 06.80 19.00 SHOC0194 061 01 00 21 43 09.30 20.300196 -00 NGC 01 12 0469 21 19.60 21.30 5455 0197 LSBC 01 F827-05 15 21 41 30.66 40.90 UGC 08660198 00 05 25.400201 CGCG 436-032 14 30 18.00 IC0202 1942 1681 01 23 03.30 CGCG0204 436-0340205 01 15 6872 24 12 44.40 41.800208 5240 01 25 04.60 1912 0212 -08 ASK 50 42584 4399 36.700213 4103 01 14 25 23 39.40 58.80 2MASX0216 J01244434-0850365 01 5130 26 04.90 1741 0217 ASK 01 42415 00 26 07 46.60 49.300220 00 4207 3974 18 56.00 -000224 UGC 38 01 0998 46.00 27 13.10 UGC0225 3795 01 1011 28 38.60 UM 3230226 01 13 28 36 58.63 08.30 -000227 40 30.40 4133 -000228 UGC 56 1026 56.30 ASK 326100229 NGC 05700230 01 31 42.11 5047 0232 01 32 22.300235 -00 55 01 59.00 33 01.98 -080236 5119 38 01 02.40 33 17.70 NGC 0585 -000237 1904 41 23.30 ASK 130362 13 19 55.20 IC 1930 0138 01 34 49.90 UGC 1901 4508 1110 -09 28 01 17.40 36 00.15 5526 PGC 990633 00 39 48.70 NGC 0622 5413 3956 4635 2769 5471 5158 Source0145 RA 01 02 39.20 -09 08 37.10 Dec PGC 4010442 Name 4543

Article number, page 22 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.140.23 4.00.32 5.20.31 4.40.30 4.2 4.30.18 8.2 8.4 8.010.16 6.2 7.3 8.650.11 7.9 16.4 0.30 8.28 5.40.48 0.58 3.2 9.210.24 7.0 -0.21 9.58 7.1 9.50.32 -0.10 8.07 9.7 4.00.17 0.73 14.5 8.61 3.60.17 -0.24 19.6 8.31 6.00.28 9.50 0.93 6.8 3.70.42 -0.88 9.62 -0.21 4.3 9.70.55 33.2 10.8 -0.99 9.000.19 14.7 9.110.15 6.5 64.3 9.10 9.00 3.60.24 35.3 -0.08 8.06 6.8 -0.06 9.500.41 4.9 9.260.45 5.3 -0.62 0.31 8.2 9.50.15 31.7 -1.13 8.83 6.80.29 13.1 8.16 3.80.39 64.1 -1.22 8.11 6.50.68 9.65 1.46 9.47 4.5 4.60.21 0.67 10.5 -0.43 6.20.46 -0.45 8.68 6.6 6.80.30 9.28 12.9 15.10.21 -1.86 -0.65 9.21 9.1 9.40.19 29.9 9.79 3.20.42 9.21 16.1 9.03 5.9 9.91 0.86 0.47 37.8 4.80.42 9.58 0.30 0.36 6.8 8.5 81.90.35 8.45 3.4 0.37 0.46 13.5 8.99 9.44 4.60.21 0.26 6.3 5.20.27 9.95 0.39 3.34 3.0 8.80.22 14.9 -0.61 9.64 4.00.45 9.29 4.3 4.1 -1.36 0.34 9.75 12.1 6.80.27 -1.61 8.77 -1.03 4.9 6.2 22.80.39 9.23 4.5 -0.17 0.23 8.29 9.55 4.2 6.7 -1.05 0.44 4.8 6.10.23 -1.06 1.86 12.7 9.02 7.30.39 8.19 4.4 6.90.53 18.9 2.78 9.49 3.60.26 27.9 1.01 8.53 8.75 7.30.46 -1.56 56.1 4.00.32 63.3 14.0 0.52 8.75 8.380.21 84.5 66.0 9.26 9.20 30.9 21.6 0.74 107.1 9.15 -0.67 9.20 8.79 31.1 -0.16 9.27 8.79 -0.15 8.43 -0.55 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 4 1213 1348 56 1.22 8 88 72 237 1087 0.74 278 0.27 171 4.24 1 2042 179 0.99 3795 203 403 16.50 4 77 12.19 1 280 103 2599 306 0.81 282 100 3.47 18.12 1443 1.71 17331 194 1305 226 3.02 146 3888 251 1.02 416 21.35 2139 4.13 240 1507 1.92 170 1026 0.54 125 2458 0.81 2651 125 1.46 3306 1546 345 2011 0.93 1433 5.29 2171 78 269 2042 1.01 101 15.97 100 235 12.63 48 122 8.59 20.68 87 3.12 / HI 1310 79 11822 11412 155 220 129 0.32 15 1.09 289 202 116 1.40 10 2.65 17510 400 0.81 17 85 47020 128 112 2.85 101 212 0.69 12 161 0.98 24418 0.95 274 9115 0.65 15220 51 0.83 20 10917 90 39112 171 132 0.35 477 19739 1.43 210 6.16 312 1.05 61 7.34 14710 0.43 54512 570 32319 1.45 380 12722 4.22 181 1442331 1.02 327 79 170 4.53 15234 260 0.79 72 1.54 175 0.71 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 5 0.632 -16.771 0.752 -0.40 8.07 -18.912 0.50 -17.913 -9.57 0.18 9.31 -15.762 8.85 0.84 -15.663 2.02 -9.84 0.83 8.31 -19.078 -9.48 1.40 7.68 -20.533 2915 1.96 0.38 9.18 -20.43 2.323 — -9.13 0.83 9.71 -17.66 4922 6 10.61 -9.86 0.72 5450 -19.212 2.34 1.29 -9.83 -11.27 0.95 -18.413 1.17 — 0.58 9.19 3251 -17.794 3.12 1.19 1821 1.83 9.17 -18.80 3935 -9.73 1.27 8.67 -21.084 5508 — 3917 -9.88 9.19 -19.243 -10.35 1.28 10.39 0.58 3.284 10.04 1.30 -9.98 1.21 -11.76 2.42 -15.143 5194 -10.40 1.19 5509 -19.644 5218 3.17 2.94 1591 1.54 7.44 -20.912 10.08 1.29 1.06 -21.76 -10.102 1987 -10.43 1754 9.92 0.37 -19.82 4617 2 10.54 1.57 2.13 -11.41 -17.892 2.58 -12.15 9.94 0.51 -20.334 1797 2.91 0.65 -10.86 -17.762 1.73 — 5196 8.93 0.82 -20.182 2.67 8.74 0.52 1831 5377 -18.124 0.58 9.55 — -17.234 — -9.56 0.82 9.21 4827 -17.453 -9.57 2.69 3.28 8.19 -19.81 3.39 1.603 -9.96 8.60 1.61 -21.312 2.86 4846 -9.55 6.10 1.62 4525 4626 -21.003 2.33 10.56 -9.62 1.35 4796 -20.674 1.90 11.01 -11.58 0.77 -21.85 1.734 10.90 5087 — -12.26 1.16 3632 -17.722 2.53 10.78 -11.68 0.59 -21.50 2.87 4438 1.94 -10.64 8.94 1.38 -15.80 10.27 2.45 6700 -10.05 7916 -21.692 1637 2.57 -10.37 6.432 10.61 4601 1.74 1.44 5288 -10.292 2.19 -12.10 0.55 -21.451 2.11 1.48 4777 5857 -16.092 2.71 11.05 0.29 -20.732 -12.42 1.02 8.01 2242 -16.21 4017 6 0.78 -20.734 2.64 — -9.67 0.86 7.65 -20.334 1.49 9.93 -19.52 6435 4 2.00 -9.07 1.24 -19.83 — — -9.86 9.32 0.96 -19.10 1.91 2760 2.55 -12.06 -18.49 2.89 — 9.42 2669 — 2.79 8.98 1480 -12.29 6121 3.50 — -11.49 3.17 1528 3.23 2.40 1438 1368 1216 1350 1 0.57 -15.25 7.72 -9.55 1.38 2619 / 10 0.79 -17.35 8.49 -10.12 2.98 1802 11 0.51 -16.48 6.70 -10.82 1.61 1918 1212 3.20 0.44 -17.21 -14.74 6.25 7.18 -9.96 -9.23 2.29 2.40 3863 2014 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± ± km 0015156 4435 + 005 2755 + . (J2000.0) [log] [log] [log] [log] continued 01 47 49.90 -00 1801 14.20 47 55.16 PGC 1146688 12 41 31.20 ASK 4415801 51 27.10 5510 -08 3001 19.30 51 39.1801 52 NGC 58.99 0707 5249 14 55 43.0001 12 54 42 00.50 28.40 ASK 4473101 54 03.70 -00 NGC 45 0716 09.50 14 54 UGC 34.30 136501 56 23.10 UGC 1364 -09 0301 36.00 57 09.8001 59 NGC 34.70 5377 0755 14 32 59.50 14 00 4853 29.50 IC 175502 02 11.80 NGC 4392 077402 02 46.90 -00 0702 49.50 08 58.70 4842 -08 2702 27.30 09 NGC 19.30 0800 -07 5097 46 00.50 ASK 132208 -09 5202 02.10 17 NGC 04.80 0830 1652 PGC 401994402 01 30 14 33.00 39.10 -01 NGC 06 0867 40.20 7912 4594 02 35 33.90 NGC 0955 -09 21 47.40 5958 2248 02 40 23.90 2MASX J02352867-0921306 3847 02 40 32.80 3856 -08 26 00.70 -08 08 1377 51.60 NGC 1042 NGC 1047 6418 1546 1370 1421 – 1 1 1 1 1 1 1 1 1 1 N N F N NF N NF NRUF R C C C C C C C C C C Table A.1. 02390241024202460247 01 37 08.100249 01 37 30.800250 -00 33 01 53.50 37 37.100252 -08 53 01 07.70 41 19.30 ASK0254 33073 01 00 41 02 39.70 24.90 MCG0255 -02-05-026 -09 13 01 31.90 42 59.300256 -09 UGC 13 01 1159 03.90 44 35.80 MCG0257 -02-05-036 01 00 46 21 25.05 36.20 PGC0258 993763 -08 15 01 05.90 46 59.170262 -08 ASK 38 33838 11.80 2MASXi0263 J0144358-081506 01 13 47 07 50.50 30.40 IC0267 0159 1803 0270 -10 NGC 00 0671 01 22.50 48 36.40 2912 0273 3941 01 49 5458 10.40 2MASX0274 J01475058-1000228 -10 19 01 34.30 49 10.800275 -10 03 01 4916 40.40 49 24.80 2MASX0276 J01483634-1019329 -10 25 01 1821 5199 35.30 49 54.30 UGCA0277 21 01 13 50 22 54.40 08.20 NGC0278 3235 0681 -09 01 13 51 41.70 1588 02.00 -100281 UGC 22 01 1279 10.40 51 04.00 ASK 1316360283 13 17 47.50 ASK 130977 -09 3917 0284 42 01 5505 08.30 51 29.90 UGC0285 1312 NGC 07010290 13 07 54.100291 01 53 29.30 UGC0292 13220293 1992 12 49 43.10 1745 0294 01 55 1918 59.80 PGC0295 4615 138476 01 56 10.60 -000296 1811 11 08.000298 01 00 57 15 05.90 16.10 PGC 31119710299 5183 1863 -00 2MASX0300 28 J01561055 26.300301 01 59 IC 44.50 1756 4835 0302 02 00 43.90 -070304 50 20.900305 14 4658 12 37.90 2MASX J01594449-07502090306 PGC0310 1452135 3637 0312 02 5289 16 19.400314 -090317 28 02 12.30 18 08.100318 ASK 1328330319 02 00 31 45 6730 32.20 30.100320 02 31 37.70 -00 KUG0321 43 0215 39.50 4788 -00 08 02 24.90 35 32.70 SHOC 123 02 39 29.10 IC 0234 -07 09 15.90 -08 08 01.10 NGC 0991 2012 NGC 1035 2667 6120 1528 1288 Source0238 RA 01 36 40.92 15 05 12.00 Dec ASK 43236 Name 2625

Article number, page 23 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.240.10 3.40.72 2.40.35 42.4 3.80.43 109.7 7.7 2.90.30 35.3 9.580.36 9.37 10.4 7.15 8.90.12 83.5 -1.79 47.60.12 -0.51 9.37 8.89 13.6 6.6 9.380.09 97.1 8.30.56 0.25 8.91 -0.63 5.5 9.27 7.80.31 6.3 2.76 7.60.19 3.14 7.76 3.9 4.60.40 13.1 7.61 4.40.30 11.4 0.53 7.89 6.00.31 9.77 18.0 7.61 4.80.14 17.9 1.77 9.13 -0.47 8.30.36 31.0 8.24 4.2 9.250.44 -1.50 18.6 14.7 9.270.28 0.12 0.53 6.1 3.70.33 35.9 9.34 0.94 4.50.42 11.0 12.9 7.61 9.61 9.34 0.27 12.1 10.14 4.60.23 23.3 0.07 9.61 7.60.48 21.6 -0.85 9.51 3.1 9.500.64 13.8 4.9 9.590.48 9.51 0.98 3.7 5.20.43 9.50 10.7 4.20.25 — 8.73 8.0 0.17 3.50.21 9.62 4.1 5.2 -0.33 0.32 18.0 -0.79 9.65 3.30.29 9.50 4.2 7.70.24 -1.45 9.74 6.7 5.3 -1.11 0.41 23.6 9.18 0.96 6.50.29 16.5 10.6 8.70 43.5 -0.83 0.31 9.42 7.7 -0.54 32.60.26 8.54 16.0 9.100.22 0.81 10.05 14.4 -0.14 5.00.29 29.6 0.45 -0.66 4.50.39 9.78 10.3 10.1 9.860.33 -1.08 5.1 5.2 23.20.41 9.46 0.38 6.00.27 18.7 10.3 -0.86 8.16 9.010.11 11.7 5.30.37 -0.60 42.4 -0.25 9.74 4.40.37 9.72 6.9 9.44 9.74 6.80.73 10.1 -1.10 5.40.49 12.8 9.44 8.37 7.70.31 20.4 8.64 8.30.22 9.02 10.00 0.37 16.3 4.9 -0.18 16.5 -0.96 4.5 10.08 -0.37 10.40 8.6 -1.20 9.6 -0.65 9.34 9.44 0.09 -0.62 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 66 20416 84 220 3661 1145 0.60 95 404 2251 145 48.92 5 0.18 99 253 1733 2.10 21.86 1337 42 1949 41 2.34 21.74 39 65 310 63 0.49 2 67 3512 0.46 202 0.21 4.58 1097 2191 1384 55 4.58 1928 5.47 4376 76 214 1542 458 235 0.29 6 8.09 180 223 3.78 285 214 0.82 2466 4.70 2465 5.76 501 2.35 294 518 309 1.50 9 1.63 1 1033 1335 148 2814 154 323 1.67 319 258 6.31 3 3513 8.44 312 2.67 95 198 5.51 1052 221 0.71 234 4.18 4 2719 159 10.57 4 217 180 6135 2821 2.96 636 215 4.46 324 7.83 232 329 1.72 1.40 / HI 7311 378 56 57321 1.03 89 405 0.48 528 2.68 2212 124 404 17119 44550 0.67 22118 3.27 38316 327 183 525 126 4.25 225 1.10 174 0.66 1.18 27 30142 39439 226 1.52 24220 37911 408 2.11 82 48 2.02 15510 82 0.88 390 0.31 454 5.14 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 34 1.714 0.88 -23.272 2.10 -15.352 11.37 0.44 -18.11 -12.83 0.93 7.66 -16.931 -20.921 1.79 — -9.98 0.43 8.641 10.02 0.10 -17.60 11462 1 1.12 -9.63 -10.05 0.38 -14.605 — 0.23 6.13 -14.822 3.11 2.89 1289 1.22 7.24 3.87 -15.223 -8.75 1.33 -21.385 2773 — -9.16 1518 0.18 6.12 -22.062 2.82 10.25 991 0.55 -15.422 1.58 10.64 -9.45 -10.66 0.35 -17.88 —1 1330 -12.09 8.12 1.07 -17.892 1.22 3.24 1571 0.42 8.72 1.58 -20.063 1.43 1.45 8.33 -15.76 -10.422 2760 — 5184 1.51 1352 -21.97 5253 2 — -9.42 0.54 7.54 2.96 -22.79 2.215 0.79 -18.614 2.79 10.99 — -9.26 0.86 2752 2841 -17.56 —2 -10.72 0.86 -19.892 1.78 2647 — 0.97 8.52 1.49 — -19.434 2.27 1.45 9.58 -18.592 1697 -9.82 4112 2.68 9.33 1.57 — -21.28 -10.314 8708 9.05 1.29 -10.08 -22.93 2.163 10.41 2.29 0.51 2.94 3212 -20.742 11.10 -9.96 -11.55 1.91 1.37 -18.431 10.61 3747 -11.24 0.86 9110 3730 -20.29 1.913 2.49 -10.62 8.78 0.43 5269 -19.216 3.12 10.01 0.62 4086 5133 -18.143 2.97 -9.62 -11.51 9.24 0.86 -17.102 7865 8.61 1.20 -17.93 2.603 1.19 6368 -9.94 8.68 1.49 -22.553 -9.31 8.65 1.19 5211 5410 -22.56 1.522 10.71 1.64 -10.08 -19.38 2.633 10.86 — -10.09 3940 0.74 -20.722 -11.66 2.07 9.48 0.97 6808 2.56 -17.592 2.53 10.32 0.92 -19.462 1.68 -9.95 -10.44 8.77 2038 1.38 -20.24 2095 2 5235 9.26 0.94 -10.08 -20.91 1.906 1.42 6833 0.55 -20.364 10.82 — -9.96 0.81 2.31 6277 -16.484 5239 -11.84 1.16 -18.322 2.11 — 1.11 8.00 2063 -20.73 —3 1.80 1.64 8.81 -20.724 2253 -9.63 9.98 1.30 2.21 -23.10 7330 6 — 10.38 -9.85 0.79 -10.66 -23.16 2.37 11.28 7341 -12.01 1.28 2.69 -19.38 1.36 11.05 -12.67 3.03 2344 -19.18 2.41 -10.30 9.25 5395 2330 10.07 3.16 2710 2.53 -9.84 6860 -11.84 5667 10121 2.23 1.32 5166 6416 / 12 0.24 -16.58 6.15 -9.06 2.85 2678 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± km . (J2000.0) [log] [log] [log] [log] continued 02 40 37.90 -08 32 00.00 NGC 1048 11606 02 41 44.70 00 26 34.70 NGC02 1055 49 10.80 -07 4902 24.50 53 46.70 SHOC 138a -07 23 44.00 SHOC14202 59 14.5003 00 40.20 00 33 59.7003 00 03 01 957 41.20 13.30 ASK 37367 -01 UGC 04 2479 24.80 1296 2MASX J03034116-010424903 09 33.9003 09 35.22 1347 -07 4103 4187 32.70 09 39.10 -07 57 26.00 ASK 55399 -07 50 46.20 ASK 5540203 13 24.20 NGC 2754 123403 13 45.20 -08 2842 12 44.60 -00 1403 29.10 14 2MASX 06.70 J03132426-081244803 14 IC 40.90 0307 -07 16 34.30 -06 46 5110 03 34.40 16 ASK 06.30 5553303 9093 17 2MASX 02.80 J03144089-0646348 -00 26 3811 18.00 -06 1203 20.40 17 KUG 53.40 3742 0313-00603 5535 17 ASK 57.10 55587 -07 1703 52.10 18 00.20 -00 1003 08.60 18 NGC 02.80 1285 -07 1703 48.00 18 NGC 29.10 1280 -00 32 20.30 7788 2MASX J03180013-0717477 -07 53 5318 03 30.70 19 CGCG 43.00 390-05203 19 ASK 47.00 55287 6815 5125 0003 33 20 55.60 09.00 00 35 04.40 Mrk -06 1076 15 2096 49.10 CGCG 390-059 NGC 129903 22 5250 47.20 6832 6307 03 00 25 08 11.60 57.50 -06 UGC 10 2705 51.40 2079 KUG 0322-063A 7248 7300 2252 10093 6851 – 1 3 1 1 3 3 3 1 1 3 3 3 1 3 1 1 3 3 1 NRF NF A N N N NF NF C C C C C C C C C C C C C C C C C C Table A.1. Source0322 RA Dec Name 03230324 032503260327 02 41 29.400328 0331 -07 20 02 45.80 44 21.100332 02 46 25.20 PGC 10205210334 02 00 48 40 52.60 31.400335 -00 29 55.100336 -00 UGC 21 02 2216 03.90 52 16.80 NGC 10870337 UGCA 420338 02 00 56 17 28.40 41.300339 02 57 04.40 ASK0343 02 37020 00 57 36 33.60 28.10 -070344 41 08.30 1292 -070348 ASK 45 37325 31.70 NGC 11480351 03 01 NGC 03.30 11520352 -000353 2773 44 03 36.50 04 34.80 1523 0354 03 06 2659 52.40 UGC 2482 -000355 28 03 30.90 08 48.30 -000358 47 40.10 SHOC149 1576 -070360 02 26.20 NGC 12110361 2MASX 2754 J03084835-07022610362 03 11 03.97 5187 0363 03 12 06.70 5258 -070364 22 8666 02.20 -080365 13 57.30 2MASX J03110395-07220260366 03 13 2MASX 47.80 2644 J03120670-08135740368 0370 00 5268 41 39.70 1682 0372 4090 03 15 38.60 3209 CGCG0373 390-029 -070374 04 43.800375 03 17 KUG 29.70 0313-0720376 -080377 08 42.800378 2MASX J03172972-08084310379 0380 6355 0381 2040 03 19 26.100383 -06 3947 0386 07 16.000387 Mrk 10750388 03 20 32.800389 03 21 06.100392 -06 03 07 22 07.60 17.500394 -07 16 56.20 ASK -07 55782 05 03 26.40 25 01.70 ASK 55716 KUG 0319-072 -05 44 03 44.80 33 29.46 03 34 44.66 NGC 1324 -07 33 08.40 2269 00 17 49.50 ASK 55983 FGC 059A 2337 2710 5396 5667 5169 6434

Article number, page 24 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.250.38 3.40.28 12.60.19 3.8 4.20.53 21.4 3.80.35 8.92 7.0 9.35 4.80.27 7.0 4.10.43 12.7 0.48 11.9 0.56 8.770.21 13.8 8.96 5.00.39 22.7 -0.15 9.94 3.90.39 9.78 0.72 10.8 -0.90 5.6 9.860.29 13.50.54 5.3 1.02 9.34 -0.32 4.60.34 9.3 25.7 8.73 3.4 -0.73 0.43 7.4 9.57 9.94 4.20.45 0.50 3.7 5.10.23 -0.56 -0.35 10.7 9.29 3.50.34 18.1 9.550.39 5.0 -1.17 9.48 5.30.15 7.3 31.9 -1.11 9.69 4.80.13 0.53 10.12 4.3 9.640.21 9.1 -1.09 2.8 -0.45 0.19 8.0 -0.83 9.15 4.60.22 5.5 5.8 9.31 3.20.26 0.25 8.61 8.2 7.20.21 -0.45 8.44 4.7 7.30.25 0.46 14.8 9.02 3.80.38 -1.61 9.26 3.7 6.90.21 8.72 13.9 0.92 6.10.40 0.60 9.55 5.1 0.23 6.30.21 28.9 9.40 5.20.33 10.33 0.01 9.33 3.5 7.20.22 0.70 8.3 -0.50 8.80.30 0.67 8.68 4.1 3.10.47 10.6 9.140.12 9.9 0.13 8.85 6.40.33 6.6 17.6 0.24 3.9 8.940.51 -0.36 11.4 9.33 3.9 9.290.25 11.1 1.10 0.17 5.6 -0.98 9.90 0.72 3.90.21 7.2 20.3 8.37 3.6 -0.49 0.35 10.05 4.1 9.95 5.30.31 0.36 2.9 -0.23 4.00.80 -1.17 8.63 3.4 7.30.35 8.31 7.1 5.50.13 0.62 9.48 4.00.33 3.8 0.49 13.4 9.59 4.50.28 -0.27 8.0 9.05 5.30.44 -0.78 9.87 4.4 5.20.55 -0.37 14.3 8.68 -1.08 4.60.33 8.07 3.5 6.5 9.34 0.05 6.3 7.9 0.22 8.68 0.75 6.1 9.39 9.4 8.68 9.58 0.16 9.29 0.27 -0.28 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 2 12976 155 127 3652 4.86 148 397 235 0.48 4.11 2551 3.98 27875 293 324 188 6.53 3416 215 1.82 1037 2.27 5 184 214 119 3.83 238 1348 1.99 0.51 140 1847 1.89 232 3082 6.54 12414 139 141 2947 2.00 1555 314 383 3.27 3434 3.49 4039 383 123 1.62 158 6.58 1333 184 0.43 4815 0.98 8 500 50 135 7.01 66 1839 0.40 2.68 174 215 1.83 / HI 32 22615 302 11213 0.60 154 21627 0.75 13 284 29328 125 2.87 386 19916 160 2.70 310 331 0.64 10 1.98 38313 280 0.78 36512 306 399 134 1.40 11 2.14 1821711 63 1.74 13118 80 86 18625 201 12524 0.24 0.83 221 262 0.76 12711 28911 1.08 190 19743 0.77 160 0.87 23615 44 201 0.90 323 152 2.10 13 368 0.23 92 0.93 22 128 88 0.39 19 14714 369 0.67 15717 409 191 118 1.26 10 0.71 1661314 99 1.04 235 212 130 276 246 1.06 2.16 2.08 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 14 0.563 0.63 -18.573 0.35 -18.621 1.34 8.79 -17.514 0.29 8.91 -21.944 -9.75 1.01 8.24 -19.004 10.84 -9.83 1.31 -21.294 3.29 -9.22 -10.69 0.67 8.76 -20.684 2.42 10.18 1.27 -17.162 1.68 10.07 2.94 3091 -8.96 1.09 -11.14 -20.792 4015 1.42 -10.42 8.23 -21.536 2.31 10.13 1.87 6297 6657 1.46 -19.953 -11.49 10.29 2.41 0.67 -10.38 -22.043 6603 10.46 -11.28 6136 1.45 1.77 -18.615 4104 10.66 2.46 -11.92 1.31 -22.123 2.50 4169 -11.87 1.14 8.95 -21.645 6262 10.78 1.64 0.62 -22.205 10.47 3.22 -9.81 5248 -12.23 1.10 -18.623 7185 10.57 0.57 -11.17 -20.121 2.54 2.73 6349 1.22 -10.40 8.90 -16.874 2.49 0.27 9.75 -20.631 -10.01 8489 1.91 5229 0.62 8.15 -17.213 -10.30 6477 10.05 0.73 2.71 -18.022 -9.54 -10.07 8433 0.87 8.10 2.79 -17.646 4092 8.65 0.55 -18.863 1.40 1.55 -9.21 8.49 0.66 4599 -17.854 -9.61 1.21 9.54 -17.36 4822 2 1.65 4060 0.79 8.70 -21.26 -10.034 1.89 — 0.60 8.66 5139 -16.754 10.83 -9.46 0.72 1.78 7000 -18.26 1.784 -1.78 -9.50 -11.86 8.55 -18.514 1.38 8281 1.50 -15.39 8.904 -10.10 1.98 2398 2.40 0.21 9.21 8244 -19.442 7.84 -9.61 1.22 1.47 7190 -17.513 -10.00 10.31 8283 0.34 -20.324 -9.52 3.10 3351 -10.49 1.42 8.57 1.84 -16.522 10.39 1.43 -21.78 3.003 3702 -10.77 1.28 7978 0.40 -10.95 8.01 -19.792 11.12 0.56 2.58 -16.594 6923 3009 10.28 2.92 -9.33 0.77 -11.48 -15.68 -10.60 1.65 8.01 -19.81 3534 2 1.18 1.85 6914 7.82 -19.162 2.86 -9.12 9.75 1.63 3546 10706 10.37 -9.74 0.66 -20.803 2.22 -9.84 5963 -10.99 -17.422 1.60 10.95 0.10 3659 2 1.74 1.93 -11.09 0.65 8.63 -17.794 3154 0.68 -15.839 8039 7987 3.92 -9.59 8.59 1.52 -18.78 0.98 -10.61 -13.75 2.99 — 4667 9.23 -18.80 2.65 9.31 3098 -9.67 9.58 -10.87 — 4137 -10.68 2.91 3.84 2.69 2.44 4857 6180 3059 4708 1 0.50 -17.65 8.44 -9.49 1.55 5370 / 34 0.93 -18.4314 0.54 9.42 -15.73 — 7.85 2.45 -9.45 5702 1.77 2492 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± km 0103238 7186 4108483 8291 4210499 6911 314621842230503157476 7978 8095 5698 4802407 6178 + + + + + + + 407 3696 420332 3099 4855 + + + . (J2000.0) [log] [log] [log] [log] continued 03 36 21.33 -06 42 53.10 UGCA 8003 38 12.96 -05 32 25.50 SHOC16903 3086 45 32.20 -07 23 47.20 2MASX J03453226-0723476 6640 8490 07 19 15.1207 19 23.61 41 08 48.40 41 09 18.50 2MASX J07191508 07 24 56.10 ASK 475438 37 46 20.6007 27 14.03 ASK 424790 42 12 14.30 ASK 475626 8165 3416 07 33 58.9907 34 58.80 42 23 3007 04.50 31 57 47.60 2MASX J07335904 2MASX J07345882 07 36 31.7007 41 37 26 14.90 23.90 ASK 425441 48 02 40.70 2MASX J07371494 3028 – 1 1 3 1 1 1 F N NUZP NF U C C C C C C Table A.1. 0396 0398040004010404 0406 03 37 26.400407 03 37 49.830410 -05 32 03 10.80 37 58.900412 -05 50 58.10 2MASX0413 J03372647-0532115 -06 16 03 14.20 38 33.00 ASK0414 56553 03 38 39.20 2MASX0418 J03375889-0616148 -05 03 28 4011 39 02.00 13.900420 -05 20 03 50.40 39 37.20 2MASX0421 -06 J03383303-0528022 38 03 6623 44.80 40 42.98 2MASX0422 J03383910-0520505 -05 03 37 40 58.50 44.41 ASK0424 56463 -06 24 03 54.50 42 6135 40.10 2MASX0425 J03393720-0537581 03 01 45 4133 03 23.40 23.50 2MASX0426 J03404296-0624544 -06 22 54.500430 -06 2MASX 27 03 J03404444 32.80 6269 45 45.20 6279 NGC0431 1423 03 5242 46 26.96 ASK0432 56905 -07 03 15 50 26.80 40.170434 -06 31 03 52.50 51 33.93 2MASX0436 -05 J03454517-0715266 33 04 13.60 04 36.32 2MASX0438 J03462695-0631521 -00 04 28 06 03.70 14.72 4171 ASK0439 57022 -06 32 04 47.20 06 6496 38.26 CGCG0446 -05 391-040 39 04 06.70 10 8431 49.32 ASK0448 57729 -04 29 04 04.80 11 06.49 IC 2031 -060451 34 30.90 ASK 57785 -050454 6347 42 13.00 5228 ASK 575950455 07 22 PGC 10.80 10414400458 07 23 33.200461 40 55 30.200462 4611 07 41 25 26 4102 55.40 05.500463 ASK 07 475459 26 20.000465 UGC 3825 40 41 4065 58.900466 07 42 27 02 45.10 46.200467 KUG 07 0722 28 5137 54.900468 4823 ASK 07 475860 42 29 10 7004 16.60 2392 50.500469 07 40 29 12 53.60 21.700471 2MASX 07 J07274518 42 29 16 54.30 46.600472 UGC 07 3868 40 30 05 54.70 44.300473 UGC 07 3871 37 32 27 7198 55.00 06.300474 PGC 07 2160491 39 33 01 19.00 10.100476 IC 07 39 2190 8280 33 18 38.10 21.100477 UGC 3888 42 32 43.100479 PGC 2147389 31 46 7994 21.700481 ASK 425621 07 35 02.300483 2MASX J07333803 07 35 35.600485 07 32 35 49 52.10 19.500486 07 41 3538 36 57 11.40 48.80 NGC 3539 2410 29 6915 54 10.90 KUG 07 0732 32 36 30 45.60 54.70 ASK 148333 10681 ASK 3662 84991 5956 07 33 37 07 31.50 21.90 3144 KUG 0733 28 50 15.30 CGCG 147-044 4636 2493 4150 4695 Source0395 RA 03 35 34.50 -05 44 30.50 Dec ASK 56318 Name 5398

Article number, page 25 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.590.65 8.40.37 9.50.44 14.1 4.00.23 11.5 18.50.31 9.96 3.2 10.560.47 6.9 21.5 -0.70 5.70.33 -0.29 3.5 9.32 9.640.30 4.5 5.40.44 9.2 -0.29 0.22 8.86 6.80.38 5.0 4.7 9.100.44 6.9 10.00 0.30 9.0 9.30.33 0.52 9.64 4.5 -1.13 9.00.52 15.8 8.96 3.40.45 -0.11 9.70 9.1 8.00.45 9.84 0.91 4.9 6.00.59 -0.58 18.8 9.68 -0.50 8.50.35 11.3 9.38 9.60.30 9.56 0.73 17.4 5.10.25 -1.06 27.3 9.30 3.8 0.63 0.98 9.65 5.4 9.74 7.70.30 0.10 3.4 5.6 9.65 0.58 -1.01 8.91 6.1 6.70.53 8.52 4.7 5.20.40 0.10 8.37 8.1 9.80.14 1.33 9.13 6.1 8.30.30 0.01 14.6 9.09 4.70.47 0.08 10.0 9.69 5.30.54 9.89 0.64 3.7 3.70.36 -1.21 8.98 13.2 -1.09 6.80.39 8.97 6.1 5.60.51 8.98 34.4 8.33 4.70.35 14.7 1.87 9.08 9.86 8.00.39 1.00 9.0 6.0 25.50.51 -0.54 9.86 9.19 5.70.45 15.3 9.05 9.90 9.10.32 -0.82 10.9 9.40.35 9.54 0.14 9.90 21.2 4.40.34 9.34 22.4 21.4 0.22 0.33 9.80 -0.66 7.10.33 7.3 40.9 9.74 -0.35 5.30.32 13.2 4.2 9.06 9.290.23 1.10 10.0 7.70.19 9.49 -0.06 2.46 4.2 5.20.43 9.26 14.1 5.8 9.49 0.22 8.89 6.3 4.8 2.27 0.32 8.80 5.6 6.30.40 1.51 8.74 -0.36 5.1 9.40.57 8.86 3.2 8.90.50 8.74 9.24 5.30.22 9.1 8.86 9.39 8.3 3.7 25.0 9.24 8.63 8.2 2.98 17.3 8.98 36.5 -0.50 9.49 -0.95 9.70 9.10 -1.07 0.38 0.61 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 34 357 3352 3796 364 2825 5.45 244 7.99 304 1258 258 5.96 146 152 0.67 6 1.71 184 121 1.41 15989 3.54 2463 1757 275 435 228 1346 2.68 4636 4.56 162 10.23 6 86 1546 1.64 154 1116 170 396 181 0.96 3613 3.23 418 1.82 3959 3.15 68 5.00 214 817 2382 0.33 1484 1.68 343 172 2102 3654 1.44 239 332 8.38 3321 3.34 3464 360 2446 7.09 1907 6.10 263 1643 211 1607 9.05 188 1738 2.85 1814 78 2.07 1906 87 1.07 179 101 2.85 168 121 198 0.65 195 0.69 2.52 1 1.24 95 117 4.76 / HI 31 145 23211 1.33 1741024 202 110 25314 1.53 15816 334 19029 1.55 279 2.32 236 172 319 2.13 355 1.25 14 4.55 70 108 0.90 13 11614 17223 4716 2.16 278 100 176 493 0.90 24519 9.32 1.61 20127 276 2.41 70 153 1.07 1431 13610 20615 185 426 274 232 1.62 465 0.84 318 2.99 4.95 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 33 1.382 1.54 -20.794 0.68 -20.652 10.66 1.05 -18.604 10.85 -11.38 0.62 -19.504 -11.26 0.49 9.10 -17.215 3.34 1.40 9.93 -17.611 3.81 -9.63 1.05 8.56 -21.773 -10.33 5899 0.39 8.58 -19.194 11.13 2.63 -9.62 9657 1.14 2.72 -16.504 -9.96 -10.78 1.18 9.75 -20.163 5736 1.56 0.38 8.05 -20.26 -10.42 3893 2 10.28 2.75 3.71 1.46 -17.953 10.34 4748 -9.23 -10.14 11665 0.69 2.69 -19.782 3905 -10.67 8.95 0.77 -17.842 2.61 10.44 2.63 0.63 8006 -18.622 3.32 -9.92 -12.28 8.92 1.79 3501 6667 -19.841 9.20 0.79 -19.90 3.151 2.03 6380 -9.78 -0.24 -10.04 -17.352 10.75 — 0.50 -15.95 6831 6279 1 3.03 -11.28 0.51 2.94 8.81 -16.822 7.19 0.52 4057 -18.17 —2 2.96 -9.74 8.36 1.47 3933 -17.15 -8.386 9.05 1.52 3.25 -20.913 3.02 -9.83 3351 8.45 0.67 3.16 -20.83 10.89 -9.72 0.52 4517 -15.884 2.54 10.98 3204 -9.43 -12.43 2762 -18.145 8.16 -13.31 0.965 2.46 2252 3.12 — 1.41 7.10 -18.594 2948 2.94 1.08 -19.702 3735 5672 -9.47 0.68 9.62 -19.883 — 5681 1.68 -17.92 -10.472 1.75 10.01 — 0.53 3.30 -19.354 -10.07 8.91 1.35 3.35 -19.096 7707 3019 0.83 -11.09 -19.08 —2 2.49 — 9.32 0.58 3849 -19.485 10.00 3.22 0.41 2.67 -10.22 4486 -17.573 10.15 -11.77 1.09 — -17.161 4020 -10.34 0.64 2.47 8.64 4050 -17.914 2.56 0.49 2.92 6.60 -19.336 3.01 -9.70 0.72 9.35 4631 -18.345 4339 -10.48 0.86 4413 -17.274 -10.78 2.57 — 4310 0.71 6.99 2.85 -17.845 0.59 7.38 2.34 -16.652 4309 -8.93 4708 9.16 0.60 -16.81 -10.93 —2 0.34 -10.21 2116 -19.013 2.64 — 2.67 0.68 2.57 -17.343 — 2.55 1.28 -18.512 4270 — 1.44 6.41 3878 4745 — -19.087 0.69 9.13 2138 — -20.07 -9.07 0.70 2.51 9.93 -19.07 — 10.56 -9.59 1.93 -16.24 -10.40 1.75 -12.40 9.32 3.29 4215 2.52 8.49 2.62 4662 2.90 6386 -9.64 3780 2337 -10.69 4841 4640 3.09 2.21 4579 2342 / 10 0.64 -14.03 7.33 -9.27 3.19 2222 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± km 27213874921219 8012 6666 4907036 6228 2352188 2269 + + + + 323323394 4058 493 3921 3252 2974 + + + + . (J2000.0) [log] [log] [log] [log] continued 07 37 37.10 41 56 49.40 UGC 3933 5899 07 37 49.40 46 23 51.50 UGC 393507 39 55.2007 40 10.30 4907 9631 07 40 03.40 16.30 3207 12 40 23.10 33.60 2MASX J07395516 32 15 30.00 KUG 0736 07 34 40 13 57.90 48.20 KUG 0737 IC 2203 39 22 45.2007 42 32.40 KUG 0737 07 49 43 11 36.40 27.9007 43 50.30 KUG 0738 4907 40 44 03.20 37.60 49 36 51.00 IC 0471 40 52 59.50 IC 0472 ASK07 04554 46 53.10 4532 39 00 52.4007 48 21.10 NGC 244507 34 49 20 59.99 06.8007 50 09.20 UGC 4029 3007 44 50 48.80 10.50 5493 30 43 56.50 3032 CGCG 5654 148-041 30 41 06.30 UGC 4047 UGC 4046 4114 07 54 42.10 4278 07 4360 55 05.90 2607 38 55 33.50 40.60 4307 29 57 14.10 10.44 PGC 4009437 4253 28 44 30.10 UGC 4087 4434 23 46 47.30 FGC 0684 NGC 2480 4713 3778 6410 2344 – RF 3 3 3 1 1 3 1 1 3 1 1 1 3 N N N NC NF N NP F C C C C C C C C C C C C Table A.1. Source0487 RA Dec Name 0488 04910494049504960497 07 38 00.200498 07 38 36.500499 07 31 38 14 40.90 57.300500 07 37 39 38 01.93 00.600501 PGC 07 30 1938511 39 35 06.00 52.200502 UGC 07 3944 33 39 54 20.60 58.500503 ASK 07 148341 29 39 09 34.50 36.200504 UGC 07 27 3947 39 21 34.70 38.500505 CGCG 07 147-050 38 39 01 45.30 41.40 2MASX0508 07 J07392058 49 39 21 46.40 22.40 ASK0509 45739 48 44 31.10 2MASX0511 J07393469 30 04 11.60 UGC0512 5750 3949 ASK0514 1483820516 3898 07 4809 40 39.30 11664 05170518 3916 07 39 41 13 05.30 59.900519 07 41 54.20 NGC0521 2424 39 09 52.40 3500 0522 07 23 43 52 32.90 18.20 PGC0523 3129299 2MASX0525 6375 J07415401 6836 31 32 06.900528 UGC0530 3986 07 44 44.200531 07 44 45.200532 07 39 46 25 18.80 36.700534 18 34 08.200535 ASK 3344 07 39 45249 47 04 09.20 00.70 2760 ASK0536 07 362856 48 14.70 CGCG0537 206-022 30 29 19.600539 07 39 49 02 51.20 44.80 IC0540 0475 ASK0541 3735 45842 18 49 44.3005430546 UGC 4044 07 50 49.400547 07 50 56.00 7722 0549 2236 07 27 3840 51 42 08.03 23.500550 07 23 51 53 43.10 45.200551 ASK 07 34 179855 53 03 45.26 22.900552 UGC 07 4054 30 53 26 45.30 55.00 UGC0553 07 4055 39 54 46 25.90 57.30 4055 CGCG0554 4475 21 148-049 02 57.90 FGC0555 0675 35 04 23.80 CGCG0556 4647 118-019 ASK0557 149072 07 57 47.50 07 4708 57 56.50 07 16 58 01 04.99 48.80 2125 07 25 4269 58 09 12.40 39.10 CGCG 4742 088-008 26 34 14.30 NGC 2486 11 2136 01 14.10 CGCG 148-074 3867 ASK 607239 4242 4824 4569 4633 2348

Article number, page 26 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.350.38 4.30.38 10.30.52 4.1 7.00.17 20.7 7.60.25 9.03 4.8 9.75 6.00.32 20.7 3.10.61 -0.07 -1.08 8.79 5.0 6.60.42 9.96 4.8 4.50.30 0.11 8.78 -0.86 5.6 8.50.23 12.0 8.77 7.00.23 0.08 11.2 9.23 6.7 10.190.21 -1.37 11.6 4.60.62 -1.27 9.56 -0.99 3.5 6.70.40 8.63 -1.00 4.1 8.50.41 11.7 7.44 4.7 1.27 0.25 9.08 5.8 6.90.31 20.6 1.00 8.08 7.90.29 -1.80 10.29 11.5 9.37 7.70.11 12.0 8.08 10.29 8.90.47 21.8 0.30 9.39 6.40.44 13.0 9.12 8.3 9.450.30 -0.53 3.8 8.750.61 7.5 -0.69 9.12 15.0 5.20.50 1.33 7.68 4.6 6.50.64 9.30 20.8 8.40.81 0.75 8.52 4.2 9.30.27 0.33 49.8 8.75 8.00.24 30.6 0.53 9.83 9.66 4.70.18 0.84 19.3 3.40.63 30.1 -0.67 -0.66 9.18 4.1 10.170.38 9.02 5.6 5.70.27 -0.84 2.54 5.6 5.90.49 12.6 0.95 8.89 9.10.21 10.0 9.28 8.9 -0.96 0.54 20.9 47.7 9.500.45 8.71 2.89 18.4 8.88 8.5 -1.19 93.40.36 29.2 -0.24 0.39 9.02 21.2 0.57 18.9 9.31 62.40.31 11.1 1.91 47.20.23 9.47 2.17 9.54 8.3 29.80.55 9.33 0.28 2.80.47 9.54 13.6 11.3 9.050.16 0.91 11.6 3.20.43 26.2 8.68 1.31 5.90.50 23.4 10.05 8.70 9.5 0.39 0.44 6.4 -0.75 9.64 8.30.34 -2.18 12.3 14.70.33 19.7 12.1 0.65 8.530.45 29.0 9.51 10.09 3.10.16 36.0 20.0 0.77 -0.26 9.81 -0.94 4.1 9.20 4.7 38.7 -0.50 9.20 8.08 9.90 5.4 -0.16 0.52 8.04 0.82 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 43 1675 2657 180 1485 289 529 1.54 165 122 5.01 571 1.43 139 6.91 6 0.71 6 1496 31 1773 91 2.10 583 197 106 0.72 4 2935 226 0.59 3 50 308 1154 5.12 6 47 2.03 74 157 59 196 1.24 3.80 73 77 2332 2.00 7 0.45 4.22 3073 1831 337 5904 204 15.45 3 31 610 280 1.89 160 10.21 4 56 2913 171 187 3.98 0.89 1442 0.70 2055 176 1341 2.40 2322 3.40 216 204 266 10.10 2033 237 6.28 234 17.03 2 68 10.49 2 4053 90 4173 431 2.03 6 84 434 2244 9.40 515 1001 7.15 250 259 545 0.82 2101 3.93 3016 4.03 232 245 7.79 134 7.56 267 152 10.95 0.54 / HI 3621 13966 35718 217 529 432 225 0.60 75218 1.66 298 4.22 24413 2.70 304 670 1.18 709 2.94 1126 12511 94 156 331 188 1.67 369 1.16 3.59 14 39023 446 3.55 97 23819 3.81 12322 268 134 5.23 177 0.43 34 41 115 0.61 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 24 1.453 0.70 -20.843 1.66 -17.392 10.83 0.61 -20.501 -12.73 1.40 8.69 -17.633 10.82 1.77 -19.19 -10.273 2.43 -10.47 1.44 8.70 -19.841 10.13 1.44 3.20 -21.272 10.51 2.38 -9.72 4837 -12.01 0.48 -20.142 11.19 -11.36 0.23 3007 -16.284 1.61 10.56 1.86 5222 1.55 -11.75 -13.301 1.69 -10.50 0.54 7.36 -20.54 4460 3 2.48 4183 6.44 0.41 -14.98 4632 3 10.87 2.63 -9.89 0.65 -18.52 8747 7 -8.88 -12.69 1.30 -18.26 5260 3 2.46 — 0.45 -18.945 3.22 1.46 — 0.85 9.07 -16.522 2047 -2.37 9.92 -20.72 4585 —3 -9.82 -14.51 0.35 893 -10.442 — 10.14 — 0.72 2.16 -13.672 2.91 7.41 -10.01 0.51 2.53 2.62 -17.993 0.45 6.93 2073 -15.974 — 11722 -9.50 2.66 3081 1.33 8.97 5021 -16.013 -9.43 1.56 7.99 3.20 3.69 -21.097 -9.96 3925 0.71 7.91 -19.564 1.31 10.50 -9.39 1.99 -17.597 4677 2407 3.32 10.32 -9.50 0.50 -19.75 -9.843 3.81 1484 1.54 -10.49 6.64 -16.343 2.35 11.01 3124 0.35 3.47 -18.30 2005 -10.533 2.93 -10.88 8.07 1.78 3159 -17.711 6284 9.86 0.76 4.90 -10.81 -19.712 3.57 2472 6.40 0.13 -11.79 -17.733 10.69 3.90 1.75 4075 -17.142 -8.66 5460 -0.25 -11.38 1.52 8.95 -18.402 8.31 0.89 -14.52 2346 1.542 3.26 -9.80 7.11 0.45 4266 -18.165 -9.39 7.14 0.58 4291 -17.54 2.90 7550 2 -9.00 9.19 0.56 -16.99 2.24 -8.982 0.45 -10.02 -15.32 3.48 2096 2 — 8.42 1.53 1.54 -17.07 2155 2 3.60 7.74 2400 1.45 -20.762 -9.52 8.29 0.68 — 2058 -11.26 -20.693 10.88 3107 0.48 2.58 -18.053 10.80 -9.43 -12.26 3.16 2.61 0.86 -15.552 -12.41 1.62 9.00 -19.67 3.584 2063 1.90 2109 1.44 2064 7.75 -21.042 2.92 -9.71 9.78 0.68 -19.69 4868 3 11.04 2224 -0.44 -9.46 -17.732 2.46 10.31 -9.93 4992 -11.95 -13.65 1.09 1.78 -10.04 0.37 -19.90 2.93 2.38 3578 — 7.56 -14.59 2.74 10.06 2916 -9.62 4141 7978 -11.79 7.22 — 4126 3.28 2.98 -9.02 2.40 2004 1.43 3872 2080 2062 2 0.74 -18.28 9.10 -9.79 2.80 3798 / opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V km 1326003 4474 1731269 2048 4040427 3087 2211349 2007 + + + + 221A228 3462 4141 + + . (J2000.0) [log] [log] [log] [log] continued 07 59 13.10 32 54 52.80 UGC07 4132 59 53.50 23 23 24.20 CGCG 118-03608 01 58.9008 02 38.60 21 22 19.10 30 10 35.70 ASK 363290 5192 08 05 53.10 ASK 180641 23 8736 34 47.0008 10 30.65 ASK 280521 18 37 04.20 ASK 48323808 2089 12 57.90 11861 36 15 16.60 NGC 2543 4678 08 15 40.7008 15 59.10 27 00 1486 29.4008 23 17 11 25.40 58.60 ASK 26541908 17 36.90 IC 2247 2108 09 17 47.90 53.93 35 26 48.80 CGCG 119-02808 24 18 41 01.60 12.00 UGC 2469 430608 18 06.60 ASK 363797 2408 44 18 07.10 08.30 2408 47 18 47.20 19.70 IC 2267 2408 30 19 06.30 10.70 IC 7550 2268 2408 31 19 36.90 12.76 ASK 363805 2108 26 19 08.80 41.26 IC 2166 2271 20 30 38.60 4294 NGC 2557 22 02 30.80 NGC 2558 2420 KUG 2065 08 0816 22 10.7008 22 19.50 03 16 04.9008 19 22 24 44.95 57.50 2083 IC 0503 2104 1985 IC 2329 24 17 48.90 2213 NGC 4834 2575 4978 4124 2082 3873 – 1 A 1 1 3 1 3 1 A 3 1 1 3 1 1 3 3 3 1 3 NA NC N N NC N F NC NC NPF NF C C C C C C C C C C C Table A.1. 055905600561 05630566 07 58 20.500567 07 58 43.700568 25 08 57.100570 07 32 59 44 23.10 19.700571 NGC 07 2487 59 37.800573 ASK 07 189652 39 59 24 40.10 48.500574 13 26 00.700576 PGC 07 15 2149346 59 23 57.20 12.500577 2MASX 08 J07593778 00 23.900578 UGC 08 4145 35 00 48 57.90 51.400583 08 17 01 31 23.10 21.300585 CGCG 178-015 54 13 55.100588 2MASX J08002396 15 22 09.300589 ASK 478418 4827 08 3018 02 42.90 UGC0591 4170 08 05 05.390592 4164 40 40 42.900593 08 25 07 03 24.83 45.200594 2MASX 08 J08024287 07 48.500595 UGC 4651 4210 39 5236 11 40.000597 08 50 10 54 47.80 46.600598 NGC 08 2528 11 47.600599 ASK 08 443347 46 12 54 00.90 44.10 894 0600 08 22 12 11 46.40 34.400601 UGC 4661 4258 20 39 38.500603 2MASX 08 J08114758 26 13 21 25.30 53.400604 ASK 08 483292 13 57.240605 NGC 08 2540 31 14 56 27.00 44.300610 08 5032 52 15 38 21.30 54.40 CGCG0612 149-005 50 34 36.60 UGC0613 21 4277 3914 33 2420 29.40 ASK0614 48913 08 16 54.40 LSBC0615 F561-020616 3124 24 10 36.500617 3157 IC 22560619 08 18 01.40 6277 0620 4072 0621 47 51 09.300625 UGC 5457 43070629 4281 2348 063206330634 0636 08 20 29.200638 08 20 49.30 2103 0639 08 03 21 29 24.60 34.900640 22 39 27.90 ASK 257965 19 08 52.00 3106 KUG 0817 08 22 41.40 NGC 2572 08 16 22 28 46.20 51.20 PGC 4163150 19 22 29.10 ASK 522650 2921 7964 1997 2033 Source0558 RA 07 58 16.60 39 50 00.20 Dec UGC 4120 Name 3820

Article number, page 27 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.340.21 4.90.35 17.70.32 15.0 11.7 30.80.31 5.1 26.90.23 9.90 9.19 4.00.37 -1.28 9.03 3.4 9.40.39 9.19 4.9 5.60.56 37.9 3.01 9.32 5.00.14 8.32 8.00.54 9.8 67.5 0.88 8.82 5.70.19 14.0 0.63 17.3 8.72 9.520.10 -1.69 3.4 8.70.22 25.5 -0.72 9.97 0.39 5.30.18 8.07 -0.87 9.90 8.0 4.20.30 10.5 8.40.28 -0.24 -0.72 12.4 8.82 7.30.30 20.7 19.6 8.010.37 8.31 14.3 8.82 14.5 8.64 30.20.35 -0.05 33.4 -0.10 29.50.20 8.69 -0.55 17.1 8.930.40 61.6 10.53 4.5 0.40 0.28 27.8 8.93 -0.06 9.44 8.60.24 8.4 9.02 4.90.55 33.1 0.29 15.60.36 14.2 1.80 8.13 5.2 46.10.36 8.85 4.10.40 8.76 1.07 9.57 4.6 7.4 2.73 0.35 -0.12 5.8 7.30.44 0.01 9.02 5.4 7.20.15 10.9 9.69 5.6 -0.24 0.44 10.2 8.51 3.80.80 8.78 9.69 12.0 7.00.47 9.45 0.01 3.9 8.78 3.10.28 9.57 19.2 11.9 -1.02 0.54 11.2 8.41 -0.76 6.50.25 43.9 9.24 4.0 10.250.68 -1.46 10.4 -0.76 6.5 9.890.29 -0.92 5.30.39 6.5 8.55 -0.80 15.7 9.00.18 11.8 10.10 6.80.46 0.54 32.0 8.42 -1.14 4.00.42 21.7 9.55 4.4 9.010.28 0.94 4.0 9.54 5.10.44 -1.11 10.8 0.88 8.30.41 -0.86 8.76 3.5 6.70.64 9.47 5.7 9.50.32 20.9 2.56 8.86 -0.95 6.90.25 59.1 9.35 8.3 -0.09 0.52 38.4 9.14 7.50.75 97.9 9.35 8.66 9.50 5.9 -1.50 10.6 9.7 9.53 -0.31 9.50 8.8 9.11 19.6 9.53 9.28 9.11 9.29 0.01 -0.80 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 22 1194 153 146 4829 1795 3.75 497 1741 5.75 2459 2.00 195 116 264 4521 0.70 1478 2.30 507 332 15.46 6 94 6.12 3498 84 113 8.87 178 1081 0.50 3 237 0.48 1271 2805 2.09 147 1296 3179 5.14 80 1646 5.71 61 13.14 145 1371 1697 80 203 4.91 65 209 200 0.56 3.49 6 2.38 92 2279 208 6.26 2.52 2194 2353 254 1226 2.70 3451 2.21 132 6513 359 3877 0.30 668 1265 3.39 412 6134 6.04 143 107 13.21 2 634 3762 1.82 129 159 2.38 392 2556 1.35 182 3.01 272 3472 5.63 5.44 3669 831 3.21 177 1001 276 212 1.64 1136 2973 2.04 137 15.49 249 351 18.52 276 373 2.89 9.37 / HI 10 474 51022 2.61 121 18313 0.93 111 16512 0.64 16 98 147 163 228 1.38 2.28 1624 176 285 22435 362 1.61 224 1.49 362 2.81 3013 52 147 13916 185 0.37 477 1.64 51710 1.90 117 173 1.43 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 22 0.922 0.38 -16.844 1.77 -18.302 0.69 -20.483 — 6.02 1.40 -16.443 8.44 1.16 -20.232 -9.03 7.69 0.55 -11.39 — -18.122 10.51 1.62 -19.023 2.86 -9.32 -11.76 0.87 1.59 1.84 9.44 -20.522 1.42 9.14 -15.89 -10.256 2.51 1965 10.84 1.76 0.46 4643 2916 -20.442 -9.46 -12.06 8.31 0.62 2.49 2162 -16.684 10.63 4418 0.36 -10.19 -15.654 3.52 2.72 -10.74 0.89 2183 -17.092 — 0.59 1.15 8.07 -18.423 3.13 2118 5645 0.47 8.40 -16.482 1958 -9.74 1.20 9.19 -16.28 —1 4329 -9.44 8.29 0.68 -21.012 1.02 -9.99 0.45 2.00 -18.632 1.85 10.59 — -9.71 0.05 -16.943 1.25 2121 -11.67 9.15 0.26 1755 5210 -14.563 2.15 0.69 7.23 — -16.606 1.86 2083 -9.60 0.90 7.06 2127 -17.862 -8.80 0.95 2.50 6.11 -19.16 11162 3 3.11 -8.96 0.73 8.87 -18.11 -10.202 3.26 9.57 0.79 1849 -19.95 2.384 2087 -9.76 9.26 1.45 3.06 -10.17 -16.674 2110 1.30 -10.20 -19.22 2.132 2229 — 2.76 8.50 1.56 2064 -20.344 3.98 1.40 -19.393 2234 10.47 — -9.84 1.46 3524 — -18.552 10.34 -10.69 1.75 2920 -18.882 2.04 -10.56 2.69 1.49 9.87 — -21.033 10.00 2.40 0.43 2115 -20.59 -11.913 11.17 2.55 7980 -11.11 1.56 2.84 -16.233 10.68 5118 -12.49 0.50 1.45 -21.661 5249 2.52 -12.13 1.46 8.01 2154 -15.032 11.25 3.42 0.64 4225 -20.412 2.52 -9.62 3242 1.49 -12.25 7.47 -16.334 10.67 7847 0.32 -19.873 2.58 2.40 -9.37 3474 -12.63 1.59 8.13 -17.935 10.39 0.71 -19.502 10522 2.40 3.74 2001 -1.42 -9.46 -10.67 6.20 -18.092 10.42 1.60 -16.79 -10.494 2.31 2.59 1998 4966 -10.46 8.95 0.83 -20.08 1.62 1.65 -17.74 —2 10.64 2.62 1938 -9.73 3623 -17.696 5651 -11.62 8.97 0.94 3.353 4373 — 0.77 -17.35 2.08 — -9.56 1.65 3030 -18.01 3.08 3898 -18.31 3.04 — 9.27 — 10.09 5348 -11.98 2153 -11.70 4.02 — 3.42 4.22 2.04 2067 3709 2082 4329 2 1.55 -21.40 11.18 -12.60 1.67 7984 / 30 0.82 -17.58 — — 2.94 1956 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± km 0445257 4212 0748303 2001 4925310 3044 + + + 388278438 2059 2230 7893 306 5657 + + + + . (J2000.0) [log] [log] [log] [log] continued 08 23 34.8008 03 24 13 01.60 15.6008 24 17.99 CGCG 032-017 2108 01 25 37.80 12.10 2008 30 25 49.40 44.49 UGC 4386 20 20 05.10 ASK 522889 27 52 28.40 NGC 2582 IC 236108 27 51.3008 2929 29 21.64 36 20 04.50 25 53 08.80 ASK 167246 ASK 4631 08 363933 2166 31 21.64 4411 08 07 33 00 23.10 00.1008 33 36.32 CGCG 2074 032-035 29 32 19.7008 29 33 30 40.71 07.20 NGC 2604 NGC 2604B 38 5222 38 59.00 2117 KUG08 0830 34 47.5008 35 13.83 4308 1864 43 35 40.30 15.48 2808 45 35 11.90 24.70 KUG 0831 2808 28 35 30.40 29.17 UGC 4482 23 31 30.50 NGC 2082 2608 25 2118 01 39.00 CGCG 119-12608 37 28.20 NGC 2611 24 56 48.1008 38 44.50 NGC 2620 43 32 51.00 UGC 2052 4507 5112 2177 08 40 45.20 5241 30 28 42.9008 41 32.80 KUG 0837 7822 08 52 42 29 48.20 20.8008 43 15.90 UGC 4515 1408 15 43 54.90 21.80 10509 1308 05 43 08.90 27.00 CGCG 060-036 45 44 09.60 UGC 4550 04 25 59.40 UGC 4543 CGCG 032-055 5357 2126 2072 4308 1990 – F 1 1 3 F 3 3 1 3 3 1 3 1 3 3 1 1 N A N N N NC NC NC N NF N NZ N C C C C C C C C C C C Table A.1. 0644 06460647 0648 0649 0651 08 23 51.9906520655 14 45 06.100658 UGC0659 43850660 08 26 04.400661 08 26 32.900662 08 45 27 58 11.00 03.500663 08 23 27 11 42.00 33.900664 UGC 4393 25 14 35.200665 UGC 4405 21 28 44.700667 ASK 363925 08 29 38.74 NGC0670 2595 08 30 01.690672 1955 08 52 30 04 25.50 34.800673 17 15 35.40 UGCA0674 08 140 31 31 11 57.00 22.80 UGC0675 4444 CGCG0677 149-040 19 12 41.000678 2137 08 33 35.64 UGC0680 5640 4457 1951 0682 08 25 33 08 42.56 47.100683 4323 08 33 56.60 ASK0684 08 485610 27 34 42 04.00 43.400685 26 58 21.50 1753 KUG0686 0830 52 2121 00 07.60 NGC0687 2086 2607 CGCG0691 263-0510692 11145 0693 08 35 38.780696 08 36 11.670699 2228 04 45 25.300700 08 50 37 25 32.70 08.400701 2MASX 08 J08353875 37 35.480702 UGC 4505 2917 28 42 18.700703 3522 08 07 40 48 04.40 31.000704 NGC 08 2619 40 09.500705 2MASX 08 J08373545 23 40 22 14.20 04.200706 08 52 40 27 22.70 21.700707 ASK 486031 05 38 01.600709 UGC 08 23 4515 40 32 53.78 22.80 UGC0710 08 4524 41 02.60 NGC0711 2628 19 21 17.600712 3242 08 49 42 25 25.80 30.70 UGC0713 4526 2MASX0714 J08410259 3469 37 13 15.60 NGC 2638 1997 08 43 40.76 4966 08 44 07.60 1954 22 05 38.80 3614 30 07 08.90 UGC 4554 UGC 4369 4559 3852 3726 2070 Source0643 RA 08 23 30.10 18 44 57.90 Dec IC 2340 Name 7970

Article number, page 28 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.430.32 7.20.34 4.50.18 10.6 5.70.37 4.0 7.20.16 9.40 3.7 8.60.21 -1.01 9.06 8.8 6.60.38 8.61 5.30.25 5.2 1.51 10.4 8.18 5.40.21 0.77 8.78 5.2 3.60.49 -0.04 8.19 5.4 9.30.19 0.14 8.45 6.0 8.30.28 0.29 9.21 5.5 8.90.18 -1.72 63.9 8.520.47 8.4 2.38 117.1 8.71 4.80.46 7.6 0.70 9.96 8.60.11 9.61 0.29 8.81 4.5 6.90.48 -1.11 14.8 6.5 -0.00 0.23 0.86 8.04 4.7 7.80.44 9.66 4.2 8.00.14 0.43 9.63 -0.85 5.5 6.00.24 7.85 3.6 4.60.25 -0.82 31.5 9.17 9.70.23 1.81 8.73 8.50.33 3.5 42.7 9.17 8.84 4.00.27 -1.34 15.5 13.9 7.76 9.130.55 -1.03 25.7 6.60.57 26.8 -2.20 8.90 2.98 4.30.59 47.6 8.23 -1.01 7.3 9.580.12 9.39 6.3 7.70.24 -0.94 13.2 0.39 4.50.26 0.58 16.3 9.81 3.50.53 9.56 3.4 4.10.20 -1.08 9.67 -0.64 3.3 6.10.28 7.84 -1.53 8.3 4.30.53 37.9 8.71 5.00.32 -0.52 11.6 8.05 6.30.62 63.3 -2.09 9.06 5.30.34 8.57 12.0 0.62 12.3 9.870.32 -0.92 11.2 9.8 2.52 0.26 25.6 -0.63 9.68 9.00.75 9.07 19.4 4.9 9.49 2.58 0.26 19.7 4.0 0.31 0.29 9.41 3.37 3.8 6.20.59 9.21 49.8 -0.51 9.80.32 8.19 7.1 0.46 5.7 92.50.54 10.27 9.70.33 8.19 12.6 -1.17 9.41 9.24 3.40.46 18.1 7.30.44 9.75 13.3 3.05 1.14 4.30.41 9.35 14.0 11.6 -1.22 26.5 8.84 -0.20 8.1 30.6 9.20 9.52 -1.15 11.2 -0.93 9.57 -0.69 9.11 -0.75 -0.48 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 47 2336 294 253 135 3183 2.87 1596 1.47 48 1.78 6 31 70 180 554 0.92 2041 0.37 104 1.26 1317 1215 159 3486 0.87 413 19.74 395 47 4305 4.34 8 2.34 76 2451 126 0.47 8 266 59 146 1512 2.70 1 0.30 82 201 136 1525 5.73 2.03 1585 177 2955 5.37 625 7.96 3227 37 647 4.79 6 6.29 75 541 0.27 3 75 92 119 216 109 0.65 2 144 233 1.29 10.50 265 4.17 286 10.00 92 232 59 257 1532 0.94 6 10.83 1145 2222 128 231 282 228 2.37 285 7.10 244 8.03 2.96 / HI 1714 130 216 17710 254 0.68 15213 1.18 14 190 104 398 2.08 15316 460 1.02 64 2.64 1181419 0.60 93 211 141 266 1.57 36 0.62 21914 318 340 0.83 38349 2.68 21715 335 274 0.78 30811 1.65 1851013 226 21319 22319 2.17 286 111 308 539 3.80 17423 3.51 59410 0.84 49312 4.79 126 608 303 195 4.52 331 3.07 1.45 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 16 0.552 0.50 -16.802 0.72 -15.636 7.55 0.63 -16.132 0.60 7.84 -17.413 -8.64 1.20 8.21 -15.741 -9.55 0.27 8.64 -19.872 1.96 -9.77 0.41 7.90 -17.002 2.95 10.17 -9.64 0.08 -15.743 1.48 4036 -9.90 -10.42 1.60 6.84 -17.972 2.54 2193 0.48 7.82 2121 -21.022 -11.17 2.11 3.02 1.26 8.42 -15.814 3273 11.07 -9.35 0.49 2.97 -18.223 -8.97 1865 3931 -12.48 1.31 7.95 -15.116 1.86 4050 1.49 9.61 -20.41 -10.48 1.85 2.55 0.84 7.61 -19.74 -11.652 10.51 2335 1.84 -15.18 3204 3 8478 10.45 -9.40 -10.44 1.34 2.432 -10.75 6.03 1.49 3917 -19.216 1.80 2.58 1.33 2067 -18.594 2.41 10.07 -8.61 0.45 1946 -18.893 4680 -11.82 1.05 9.87 -17.253 1.41 6171 1.18 9.97 -19.503 -10.84 1.52 0.77 6.15 -17.243 -12.17 1756 0.47 9.92 2.92 -18.385 -10.21 4227 1.45 9.17 1.27 -17.87 -10.212 1.28 9.18 2.87 2296 -21.09 -10.062 8.80 1.78 1.95 -19.66 1994 -10.002 10.89 0.58 1.40 -10.53 2200 -21.321 10.21 -12.19 1.60 2.82 2877 -16.942 11.20 2050 -10.52 2.23 0.34 -20.793 3.08 -11.98 8.36 1.39 3813 -15.133 3.48 10.80 0.06 2516 7115 -18.701 2.54 -9.49 -10.77 1.29 7.43 -15.772 3973 0.67 9.98 -20.55 1.793 1.41 3915 -9.19 0.68 6.06 -18.72 -10.603 10.50 1.04 -17.66 3721 3 2.90 2277 -8.84 -10.16 1.39 7.10 3.31 -19.322 0.87 8.77 -18.892 2.12 2.49 1890 -9.50 3812 0.84 6.12 -17.082 -9.66 9.93 1.60 -17.685 3.79 2450 3842 -8.20 8.75 0.77 -10.65 -22.06 2.342 0.44 -10.00 -18.47 3.963 11.44 4870 — 2.21 1.85 3380 -16.892 -12.48 1.97 6.36 0.64 -20.212 2526 3756 8.10 1.56 — -10.31 -18.842 3.41 10.96 3093 1.43 -10.60 -18.492 -10.45 2.15 1.36 1.76 9.55 -19.15 9025 4 2.51 9.99 1.32 -19.40 10.13 2.64 1961 -9.85 0.99 7541 -10.69 -19.49 10.21 -12.35 1829 -18.93 5072 2.48 10.32 -12.10 3.21 3.15 -10.37 9.58 3899 2.97 3142 -10.23 2.85 3735 3109 2.87 3104 3004 4 1.10 -20.67 10.41 -10.74 2.92 4240 / opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± 412 0.75 -17.24 — — 4.39 4425 V km ± 5014095 3363 3112417 2032 2746052 2295 5152429 3804 0023295 3413 2109055 3095 + + + + + + 307 2127 479 3127 + + 09-15-069 7547 + . (J2000.0) [log] [log] [log] [log] continued 08 44 28.5008 44 28.60 09 20 53.6008 31 45 21 20.00 23.40 ASK 435554 ASK 282097 50 14 10.40 2MASX J08451995 08 46 43.96 02 32 14.70 3929 IC 0521 2200 08 49 01.5008 50 01.30 -00 20 54.9008 19 51 00 PGC 32.90 35.10 4086883 NGC 2677 30 51 55.20 NGC 8416 267908 56 47.70 4417 08 39 57 22 20.50 55.90 NGC 270408 02 57 55 35.90 16.70 4216 08 58 00.60 NGC 2713 0308 05 58 24.80 37.30 2034 25 41 52.40 NGC 2716 51 52 42.60 ASK 48693408 59 07.40 2MASX J08583725 08 53 59 37 49.80 59.80 SHOC231 7120 55 41 58.6009 00 13.10 NGC 3894 271009 00 20.20 3109 59 00 58.30 22.70 3614 52 1897 29 39.20 CGCG 150-05609 53 00 56 38.20 41.50 UGC 471309 00 41.90 MCG 50 40 42.10 17 37 18.40 UGC 4826 471909 03 59.70 UGC 472909 04 00.40 2582 21 54 23.60 1987 21 58 03.40 NGC 2737 NGC 2738 9029 5071 3899 3144 3099 – 1 1 1 1 3 2 3 1 3 3 3 1 1 1 1 1 A NZF NA F NF NF R C C C C C C C C C C C C C C Table A.1. 0716 0717 07200721 072207250727 08 45 00.3007280729 08 30 45 32 22.50 27.300731 08 45 37.900734 KUG 08 0841 02 46 11 12.20 24.200736 08 36 46 56 19.14 04.700739 ASK 08 35 58108 46 41 34.40 36.900740 UGC 4572 35 18 58.200741 UGC 08 4579 36 47 26 19.64 20.800742 ASK 08 205841 47 41.690745 Mrk 08 0627 05 48 53 03.54 52.500749 08 13 48 25 04.60 08.800750 ASK 08 259622 25 48 20 09.15 01.500752 UGC 08 4599 17 48 42 18.70 08.500755 PGC 2807195 17 36 41.300757 1874 IC 01 2406 15 52.500758 IC 2407 08 3920 50 11.800759 PGC 1189545 4054 2328 0761 08 35 54 04 24.02 35.000762 08 54 3188 54.040764 UGC 08 4621 34 55 3909 33 33.20 21.700765 08 49 55 09 52.30 37.400766 1951 UGC 08 2058 31 4660 56 12 40.70 42.000767 NGC 2684 02 31 27.40 2MASX0769 08 J08553314 00 57 22 01.10 30.00 1756 UGC0772 4680 4673 UGC0773 6176 4684 08 13 57 11 35.30 56.800774 UGC0776 4685 27 46 05.100777 2296 2MASX0778 J08573529 08 58 41.000779 2192 08 58 50.460780 2883 02 11 35.400781 08 06 59 17 15.70 34.70 ASK0782 3813 58734 NGC 2517 0783 2718 08 00 59 23 49.00 29.800784 08 59 53.90 2MASX 3991 0785 J08591570 05 03 39.000786 21 09 05.10 Ark1890787 2MASX0789 J08595397 09 00 24.100790 0791 25 36 53.00 2468 0792 09 00 58.50 UGC 3832 4722 09 03 39.90 47 47 43.30 03 22 11.20 KUG 0857 09 04 22.80 CGCG 033-053 3737 27 57 10.80 IC 2430 1828 3715 2997 Source0715 RA 08 44 08.30 34 43 02.00 Dec NGC 2649 Name 4228

Article number, page 29 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.370.28 6.90.32 5.90.34 14.0 6.70.41 8.6 6.90.43 8.95 12.1 13.60.30 15.1 8.95 -0.76 6.50.62 23.2 8.66 4.20.24 8.77 1.81 8.5 9.07 1.06 9.40.56 4.1 5.4 8.77 0.51 10.21 25.6 18.1 0.29 0.18 8.87 -1.13 7.5 5.70.39 68.9 9.30 14.70.28 -0.59 16.6 7.83 9.5 9.64 0.04 0.46 22.4 3.5 10.100.46 0.50 16.8 9.64 8.59 9.20.66 -0.82 5.8 4.40.46 9.45 1.11 11.4 7.60.50 10.5 -0.19 7.70 7.80.37 8.46 10.9 14.80.35 9.60 0.81 10.9 5.20.48 8.46 18.5 8.74 18.8 -1.23 0.61 8.59 38.6 9.12 7.00.26 0.22 30.9 4.9 0.68 80.30.44 -0.16 8.30 2.8 9.030.55 9.89 4.0 5.30.41 1.17 9.03 8.2 2.80.19 -0.45 16.0 9.82 8.40.42 15.7 7.83 3.8 -1.48 26.80.60 18.4 9.64 -0.29 0.75 9.16 8.92 8.6 5.0 -1.25 38.00.44 4.9 9.16 0.50 8.92 27.8 9.33 9.11 7.90.51 10.8 5.80.41 -1.91 9.17 18.1 3.07 13.40.47 9.10 3.6 9.17 9.90.67 37.5 8.90 16.4 -1.15 0.27 8.92 3.2 9.36 4.4 2.81 0.26 30.8 7.30.17 10.2 0.04 0.41 7.84 9.36 3.40.36 10.6 3.20.35 17.9 -0.78 0.65 8.89 8.60.29 8.61 17.2 8.39 2.50.49 0.44 11.8 6.4 2.53 0.39 31.3 0.21 7.37 5.20.30 8.88 10.1 13.9 8.860.73 0.13 -0.38 8.7 8.30.57 16.8 8.93 8.86 9.70.50 15.2 -0.83 8.82 8.2 8.790.37 23.0 4.80.33 9.55 -0.42 10.9 8.82 24.0 9.48 -1.03 5.0 7.5 16.3 9.85 -0.45 -0.99 9.08 8.68 8.3 -0.11 2.64 8.92 2.84 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 36 1245 1693 139 1179 199 1844 1.21 146 2754 2.64 209 1377 3.02 320 2511 5.87 1505 90 2.64 274 3335 1.03 366 1116 7.06 3646 65 393 0.80 127 24.16 4 1193 89 5.51 172 401 1.99 236 1048 3.76 4313 251 0.75 58 3.30 2422 3.16 1051 266 1034 2.45 1778 5.78 131 604 210 76 6.29 618 23.43 3 2.20 4 926 94 0.43 8 94 238 127 306 1057 319 6.17 3 355 0.63 1 9.07 91 10.07 1848 238 1312 196 99 261 3.21 3706 3.11 12.03 1202 3944 61 1.08 1433 9.24 2 48 93 161 2277 317 1.55 2.89 59 245 2802 345 0.26 3 2.70 311 215 6.80 1525 2.50 2303 171 5852 4.10 174 2.86 617 132 186 8.80 147 2.41 3.71 / HI 29 75 215 2.02 12 11713 179 56 5.12 10526 1.26 15 361 135 433 219 2.29 13 4.42 366 413 4.99 29 212 277 1.30 15 12724 183 220 2.22 38144 8.44 45 196 0.88 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 1 0.232 -16.302 0.534 7.60 1.37 -17.854 0.88 -22.442 -8.77 0.95 8.79 -18.723 11.34 0.49 -18.35 -10.733 2.48 -11.62 1.54 9.45 -14.469 9.27 1.50 3.09 -18.90 -10.415 1895 2.70 7.33 0.13 -10.21 -20.556 0.97 2.68 2047 -15.44 11241 10.92 — -9.45 0.06 4.07 -19.382 -12.72 7.48 3864 -11.87 2.453 9.63 1.47 2433 —2 2.83 -9.18 6.89 0.38 -10.83 -20.705 1325 0.36 3.18 -17.692 1.80 10.82 -9.53 6885 0.89 3.26 -16.112 -12.68 0.53 8.51 1943 -18.313 2.97 2017 0.48 7.91 3932 -15.514 3.20 -9.34 1.31 9.29 -16.703 1173 -9.18 1.68 7.13 -20.25 -11.353 5.31 5101 0.59 -21.51 -10.149 4.87 10.34 — 1.29 3.32 1484 -16.252 11.30 -11.48 3.93 0.40 -21.553 1816 -11.92 8.12 0.63 2186 — -15.604 3.62 10.89 1819 1.40 -17.76 2.732 -9.49 -11.12 3.32 0.70 -21.892 — 2625 1.42 -17.34 2.952 2.33 11.24 7932 — 1.57 1878 -19.043 -12.39 6.04 0.40 6320 — -19.22 1817 8 0.77 — -10.27 -16.742 2.08 10.25 — 3.99 0.25 -17.563 -10.68 3.93 0.43 2.56 6.09 -17.552 2616 8420 1.78 8.88 -14.13 —1 4.00 -8.01 0.49 8.95 1682 1721 -18.423 -10.12 -0.25 7.19 3.43 -17.32 2267 -11.853 4.15 10.14 0.28 -16.98 3.846 -9.48 -11.22 0.65 8.45 3.44 1758 -15.998 2275 6.08 1.27 2358 -13.924 4.07 2.58 -9.24 8.18 1.49 1991 -17.322 -8.13 1.23 7.24 -18.145 4.37 1156 -9.91 2261 9.26 0.61 3.09 -18.762 -9.62 1.29 3543 -10.47 -17.61 2.234 — 9.76 1.21 -17.43 2325 2 2.45 2.51 1.27 -10.34 -20.793 1330 — 1.68 9.22 — -19.38 10.58 1357 1.77 0.03 2409 -20.47 -10.172 -11.64 2.02 9.93 — -16.91 10.84 0.66 2.75 2659 2.50 -11.90 3.90 6.44 1485 -17.58 — 1772 -10.42 2.49 5085 2476 6.08 4.07 4.00 -10.33 4095 2732 2.58 3216 4395 4 0.95 -19.49 9.71 -10.25 2.75 2997 / 19 0.75 -16.76 7.13 -10.54 2.59 3890 69 1.47 -20.30 — — 2.41 1352 10 0.87 -16.40 8.80 -12.09 3.28 1645 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± 159 0.13 -15.06 — — 3.06 2010 V ± ± ± km ± 3733490 1894 3301148 1819 + + 356 1819 543 3559 + + . (J2000.0) [log] [log] [log] [log] continued 09 05 36.9009 45 07 19 11.10 20.60 UGC 4762 50 42 45.80 UGC09 4778 09 33.7009 09 41.80 33 07 24.70 37 36 05.70 NGC 277009 10 18.20 IC 052709 10 19.50 58 1684 09 36 10 02.30 39.70 07 01 41.10 ASK 62242 50 22 11241 47.40 NGC 2775 NGC 277109 12 09.50 1934 35 31 36.1009 14 48.80 UGC 6867 483709 14 59.70 3309 01 16 15.30 23.80 1186 2909 43 16 48.80 1468 46.70 2MASX J09144880 4309 11 17 19.50 06.90 NGC 5098 2789 3409 26 17 12.00 21.60 ASK 264086 2009 04 17 10.90 22.70 NGC 2793 41 54 39.50 NGC 280909 41 17 59 47.30 54.10 UGC 490409 17 59.30 1851 NGC 2798 53 17 37.40 52 44 33.50 SHOC249 UGC09 4913 20 07.50 6343 2644 54 04 24.70 1679 09 21 14.99 SBS 8345 0916 1667 09 09 21 43 47.80 52.20 1828 ASK 29325509 40 23 09 11.30 00.60 2280 09 23 17.30 NGC 2352 2844 26 49 02.6009 40 24 12 02.90 00.10 CGCG 151-073 NGC 285309 49 25 12 13.27 14.90 NGC 2854 58 57 30.80 1383 ASK 62388 1422 2470 1783 2789 3223 – F F RZPF 3 1 1 3 F 3 3 3 3 1 1 3 1 3 1 1 1 NZ N NC NPF A NC NF NC NC A NF NF F U C C C C C C C C C C Table A.1. 079407950796 07970798 09 05 12.500800 09 05 33.600803 05 52 05.200804 09 37 06 33 40.50 47.500805 ASK 260160 2MASX0806 J09053367 09 34 08 37 51.01 08.600807 09 09 19.400808 UGC 09 4777 03 09 26 20.20 54.000810 54 54 43.00 CGCG0811 01 034-004 36 51.50 UGC0813 4800 09 10 01.70 PGC0814 1200328 09 10 05.50 3868 0815 32 56 59.800816 54 34 49.100818 ASK 282881 UGC0819 4807 09 10 41.800820 2034 09 3844 11 08.400822 09 07 11 12 33.80 24.100827 09 42 11 39 45.30 22.10 1321 0829 NGC 2440 51 2777 15 15.90 ASK0832 09 264072 35 12 24 14.50 18.50 UGC0834 09 4824 13 31.40 KUG0837 0908 44 2019 57 17.400838 28 57 06.30 NGC 3929 27760839 IC 244608400841 0842 1475 0843 1815 0845 09 17 39.90 2177 08470851 52 59 34.500852 09 18 36.50 2619 0853 UGC 4906 09 18 58.600854 09 47 19 52 58.02 20.70 7950 0855 58 14 07.700856 UGC 09 37 4922 20 11 56.10 28.500859 ASK 09 62006 20 59.60 IC0860 2461 52 34 04.200861 09 11 21 03 45.60 33.20 Mrk0862 1416 CGCG0863 062-024 09 39 23 31 03.09 29.300865 2274 UGC0866 4970 44 33 17.700867 09 23 36.50 UGC0870 1998 4982 1167 09 02 24 08 55.10 11.20 NGC 2257 2861 09 26 1330 25 46 47.99 28.80 09 2314 28 33.13 NGC 2862 34 16 37.50 41 23 30.10 UGC 2411 5015 ASK 207866 2658 5070 4079 1629 4392 Source0793 RA 09 04 54.10 25 00 14.10 Dec NGC 2743 Name 2991

Article number, page 30 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.520.23 6.90.30 6.60.30 12.7 9.30.47 5.1 9.20.17 9.16 16.8 4.00.36 7.94 -0.62 4.5 8.20.39 8.58 5.9 5.20.20 0.23 8.42 5.5 4.1 1.17 0.55 13.6 9.75 6.9 -1.36 0.47 7.64 5.8 8.50.30 -1.11 9.05 19.1 15.70.37 0.70 18.4 11.1 8.97 -1.99 0.64 29.7 8.95 7.60.28 -0.77 31.2 9.03 -1.42 3.4 9.770.66 12.4 3.1 9.06 9.03 0.38 -0.86 6.7 6.70.22 8.47 0.63 4.7 4.60.53 17.4 13.7 9.940.46 0.13 7.91 6.5 10.20 8.00.28 18.3 -1.09 27.90.39 -0.62 -0.96 14.0 9.23 3.7 8.430.30 55.9 5.80.58 -0.78 9.58 11.8 8.43 9.94 3.30.50 10.9 -0.71 7.20.31 17.9 -0.32 16.8 7.920.32 8.58 8.79 7.4 9.4 38.40.29 0.38 -0.29 6.90.40 10.05 62.3 8.79 12.3 9.620.19 12.0 12.0 107.4 -0.18 -1.15 0.34 8.24 3.50.26 21.8 8.57 9.50 28.1 8.24 0.32 9.03 4.2 8.57 3.9 9.50 0.58 68.3 36.20.60 9.03 8.89 9.08 9.4 5.30.14 55.3 3.70.35 8.89 9.08 25.1 8.20 9.04 4.10.30 8.2 6.30.45 8.73 20.3 1.75 9.04 3.70.53 21.9 11.3 8.15 -2.16 0.27 34.1 7.44 9.50.40 48.9 9.18 10.3 0.24 8.640.39 26.3 7.44 28.0 9.37 3.08 0.47 14.8 1.03 10.21 6.40.35 61.8 25.1 3.16 8.380.17 -0.64 9.36 7.5 9.00.31 47.4 0.51 4.10.72 82.8 9.36 10.5 9.13 9.370.19 15.8 183.7 5.00.30 8.39 2.15 0.63 5.40.21 31.1 57.4 9.62 7.60 19.4 10.20 — 119.2 8.3 9.62 0.59 -0.39 28.3 9.35 8.14 8.49 -1.08 0.76 0.64 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 86 2954 91 334 123 1207 4.07 149 1.21 6 59 3.01 2169 833 238 320 0.39 1 3576 2.10 359 174 400 96 3.75 192 8.70 130 5.89 1 2.56 31 41 3103 3435 62 327 1063 372 1676 2.19 4.78 115 16.21 3 79 188 379 0.59 250 1095 2.62 4130 285 2.96 151 3.50 4 11.93 1316 174 2452 160 1404 2.34 279 18.23 2910 156 5.31 99 332 132 0.46 14.28 1116 1533 0.85 10.69 1 411 81 1219 58 268 1022 145 468 0.28 1 288 2.35 1009 6.08 529 13.98 2161 121 1374 9.36 239 210 2.35 179 15.20 1 92 2362 2.03 13.85 228 1176 3871 180 2.11 2 73 411 211 41.33 14.38 70 49 232 22.46 108 1.28 3.10 / HI 3316 279 39867 395 443 31415 1.33 1.59 585 296 2.35 36729 1.86 42 42114 12212 492 509 212 237 2.70 575 0.63 277 5.72 1.85 10 110 162 2.04 4457 218 105 501 246 6.25 1.61 21 53 112 0.38 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 25 0.703 0.08 -14.912 1.50 -14.752 1.56 7.71 -18.092 0.28 7.41 -20.763 -9.78 9.79 1.73 -13.992 10.86 -9.49 1.17 -11.47 -20.462 2.27 -10.06 6.94 1.48 -19.28 2.672 11.04 1.61 1.23 -19.802 2.46 1228 -9.08 -13.08 9.75 1.36 -19.42 10.37 1619 2036 0.58 -10.47 8627 -20.342 2.05 1.60 -11.87 -17.152 10.63 — 1.60 2.78 3142 2 1509 1.14 -10.54 0.74 8.43 -21.133 1.46 3054 -16.97 3153 — 11.03 2.55 -9.68 1.12 -21.591 -11.08 8.53 3.12 -19.613 2.37 11.15 3722 1.376 10.01 3.20 -9.68 -12.58 1.53 2428 -19.894 -0.14 2006 -10.05 -19.84 8161 2.07 10.29 3.01 0.87 -13.302 10.26 2.47 -12.01 1638 -17.47 7541 4 7.54 -10.91 1.43 4357 2 3.19 8.87 1.10 -10.38 -20.796 2.58 0.57 -10.16 -20.233 10.77 2.83 4060 0.36 -16.412 10.23 3335 -10.38 3.06 1.04 -15.415 -11.27 1716 1.53 -19.72 3.133 — 0.76 1726 -18.52 3.23 — 1.53 -18.285 4985 — — -18.893 4415 — 1.34 —3 — 2.63 2.15 — -16.99 — 2.61 0.54 — -19.102 1328 2.45 — -15.621 10.90 — 2.57 0.59 1831 —1 -13.56 0.28 1.64 7.91 1886 -18.073 0.89 2.03 2033 -15.60 —3 2.79 -9.70 6.10 1.63 5894 -18.801 7.61 0.78 2.78 1314 -20.49 1406 4.115 -8.71 6.21 0.80 -15.322 10.84 -9.55 1.42 1353 1462 -17.63 3.792 -8.64 -10.62 7.87 0.76 -15.76 2.681 0.47 -18.01 2.892 3665 2.52 — -9.40 0.32 6.98 -17.323 1222 8.74 1.00 -14.06 -11.115 2.63 1869 5982 1.13 8.39 -10.04 — -18.553 1.16 7.01 3.16 -21.022 1454 -9.10 0.49 3.34 2.77 -17.59 10.59 -0.04 — -9.37 3712 -18.22 3.45 -11.49 -16.07 9.22 1875 1775 1.73 8.59 -10.49 — 3.86 1550 7.86 1470 -9.47 2.98 2.47 -9.11 4778 2.15 2.16 1502 1454 1438 1445 3 1.56 -18.14 9.78 -10.63 3.08 2718 / 22 0.74 -16.02 8.3462 -11.79 0.19 3.47 -14.50 1541 13 — 0.58 -12.13 — 3.06 — 1593 —13 3.08 0.29 2074 -14.5739 6.45 0.54 -10.96 -14.24 2.66 — 1966 — 1.92 1438 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± ± ± km 293277 1661 1440 587 1344 282 1451 + + + + 10-14-027 1708 + . (J2000.0) [log] [log] [log] [log] continued 09 30 28.0009 16 33 21 46.10 43.00 CGCG 091-10109 10 34 09 02.80 09.0009 34 46.40 NGC 2911 1009 06 34 31.30 57.60 10 17 29.90 NGC 2914 21 42 18.90 NGC 2919 NGC 291609 8637 37 15.2009 23 37 35 47.70 26.10 NGC 3231 2927 27 33 57.70 KUG 3144 0934 2565 09 38 57.10 3713 09 00 39 41 07.90 33.5009 40 43.20 ASK 60823 3409 00 40 22.70 56.30 0309 57 42 34.90 04.70 NGC 7539 2942 0509 02 42 39.70 13.90 IC 0549 0009 20 42 11.00 53.60 PGC 1277283 0409 40 42 32.40 54.60 NGC 2967 06 38 38.60 NGC 296609 31 43 50 06.20 48.90 PGC 130479009 43 12.00 NGC 2085 2964 41 05 34.8009 31 43 55 42.96 43.30 UGC 5187 4412 NGC 2968 41 34 08.90 1864 09 46 02.50 1297 ASK 20795209 46 21.10 1840 01 40 19.40 5921 1949 09 03 46 04 54.10 16.90 UGC 522809 47 00.70 IC 1205 0564 00 30 29.6009 02 48 04 04.70 26.70 UGC 1458 5238 ASK 1538 6164409 32 48 52 38.40 57.00 1409 Mrk 0408 33 25 29.1009 50 04.50 NGC 3003 1758 12 48 26.60 NGC 5988 3020 1775 3721 1529 1409 1443 – RF RF 1 2 1 3 3 A A 1 1 1 3 3 3 1 1 1 NF NZF N NC NZPF NC N NC NF NZ NF NRF U RF U R C C C C C C C C C Table A.1. 0872087308740875 0876 09 28 59.100877 09 29 51.800878 09 28 30 45 10.30 28.600879 11 55 35.80 ASK0880 09 488878 07 31 54 36.20 09.80 ASK0881 427852 IC0883 0540 09 27 34 17 02.70 46.600884 ASK0885 489342 09 28 45.100887 NGC0888 2913 09 35 07.500889 09 35 20.000890 09 05 1228 35 07 26.30 12.200891 09 35 1639 36 54 07.50 49.200892 UGC 5107 29 48 45.400893 UGC 09 5105 29 37 06 31.00 42.900897 UGC 2048 5108 1509 0898 KUG 0933 09 32 37 50 57.99 29.000899 09 38 07.900900 NGC 3048 09 2926 25 38 29 10.20 41.200903 09 09 38 31 36.20 26.00 UGC0905 5129 61 52 12.00 NGC0908 09 2939 43 38 10 59.20 36.40 MCG 0909 2004 1545 UGC0910 5135 06 57 19.50 8135 0911 NGC0913 29480914 4358 0915 0916 4053 0919 09 43 02.20 3326 09200921 05 01 44.40 1718 0922 09 43 22.99 ASK0923 192835 4980 0925 09 58 43 31 57.40 28.800929 09 44 46.20 KUG0930 0939 02 51 04.70 -000932 41 18.30 CGCG0933 035-041 09 46 ASK 29.10 4609340935 30 39 52.70 1963 0937 09 47 45.30 ASK0939 4915060941 09 02 48 37 21.30 37.000942 UGC 5249 09 30 3663 48 45 43.60 33.60 09 49 41.20 ASK 491436 44 04 53.10 09 32 50 13 10.90 15.90 1223 NGC 2998 NGC 3011 28 1466 00 47.70 KUG 0947 1877 1476 4769 1527 Source0871 RA 09 28 55.40 49 14 18.50 Dec UGC 5049 Name 2731

Article number, page 31 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.250.44 4.20.17 30.30.43 45.6 3.70.56 59.1 17.60.26 85.3 15.3 7.70 9.190.42 33.4 10.2 8.850.26 33.1 7.70 26.4 1.33 8.960.31 24.9 0.98 5.7 9.070.42 50.5 -0.11 24.5 8.600.40 14.5 10.17 3.00 0.22 8.6 48.3 0.14 9.6 -0.38 0.25 34.4 7.97 4.9 9.000.15 22.6 16.1 9.160.35 -0.13 -0.12 5.0 7.30.62 43.7 8.54 -0.63 8.40.37 8.12 3.2 8.680.27 7.0 0.43 25.8 14.60.34 -0.68 16.8 0.22 7.420.46 5.4 48.7 8.50 10.90.37 40.1 24.1 0.66 9.13 9.010.23 0.14 17.5 5.4 8.78 47.10.31 -1.17 9.01 7.1 9.190.28 -1.27 8.93 4.2 8.40.11 10.5 0.17 6.50.23 0.42 8.03 5.7 7.90.48 8.29 10.8 5.70.42 0.80 8.80 7.1 0.56 6.10.44 8.43 19.5 10.7 -1.03 0.42 14.1 14.0 7.65 8.43 0.19 50.3 9.28 7.50.42 30.2 8.68 7.65 32.9 9.44 3.19 0.21 15.1 11.5 -0.20 9.230.48 57.0 -0.81 2.90.34 23.2 9.41 0.46 4.9 8.810.14 13.1 9.09 3.2 9.41 0.28 1.04 7.6 9.50.34 24.4 -0.92 12.8 7.550.32 32.6 9.51 9.98 9.70.29 19.9 -0.21 36.80.38 73.8 -0.86 -1.09 7.77 5.0 8.390.49 55.1 4.6 9.130.31 -0.12 8.39 7.9 8.77 6.40.24 0.47 3.3 8.40.61 18.9 8.77 8.17 7.90.35 9.36 7.4 3.10.40 9.63 2.13 49.4 9.4 -1.06 0.52 51.9 13.4 -1.09 7.670.22 78.4 54.5 8.03 109.3 -0.49 0.27 8.63 37.1 151.0 9.14 1.16 9.28 5.6 8.63 64.1 9.54 9.14 0.67 8.48 9.7 9.54 8.48 9.73 0.22 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 612 59 22138 75 77 254 1983 15.89 209 158 0.51 1 237 1305 297 6.63 2841 8.56 155 130 10.14 2 314 2045 3.82 152 262 13.56 2242 99 1.38 284 9.36 147 1376 9.02 189 3.60 15619 6.39 193 1942 1761 3.01 212 1994 277 167 11.11 3 218 93 5.53 191 1014 3.79 13.10 1116 118 132 1.82 6 1.46 40 1511 2222 1.86 63 3703 253 351 0.34 1 391 2524 4.10 379 13.55 1506 272 2548 8.44 171 1304 3.11 301 2605 6.59 143 2243 5.89 2901 67 0.41 260 1001 2.84 2068 5.11 95 1306 90 2343 0.76 89 3.17 239 15.55 1146 433 1192 10.29 260 1043 451 1.05 1 2.06 51 119 141 6.00 1 178 0.59 1 66 159 2122 202 425 1.27 5.03 236 16.81 48 485 26.89 47.47 98 6.45 / HI 2317 73 15032 30 0.74 392 88 464 0.40 2.02 26 47127 548 192 1.50 297 1.35 16 186 252 1.55 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 11 0.654 0.77 -14.433 0.84 -17.423 0.84 -14.843 — 7.86 1.28 -18.213 0.55 7.87 -18.975 -9.33 9.07 1.44 — -17.06 -10.152 0.70 6.07 -10.19 -20.393 3.00 0.83 3.03 8.46 1.48 -16.249 10.55 -8.50 0.98 3.02 -18.342 -10.60 1414 -10.69 0.70 8.10 1416 1468 -19.294 3.51 0.46 9.12 2.23 1478 -17.244 -10.06 2.61 1.45 9.79 -16.022 1554 -9.65 0.30 8.11 2.32 -16.86 1472 2 -9.99 4787 0.54 7.90 -13.376 2.25 -9.10 1.51 9.36 -17.234 1191 2.68 -9.47 0.69 6.76 -19.382 -10.42 3.73 1494 1.39 8.36 -17.337 1.96 10.30 1818 -9.22 0.48 2.00 -19.022 1411 -9.14 -11.48 0.28 -17.83 1930 2 10.06 1.72 — 0.51 -16.82 1243 2 2.74 3.13 -10.50 0.45 9.03 -14.27 1181 1 8.51 1.30 -15.74 -10.00 — 3709 2 1.72 1467 7.22 0.52 -10.37 -18.742 7.73 2.53 0.21 2.71 -16.212 -9.48 1472 3.57 9.83 0.90 -15.094 -9.37 1.13 2914 1376 -12.03 -16.31 3.744 — 1.59 1167 -16.90 2.275 — 1.44 6.09 0.68 -18.54 1103 3 8.87 1.01 — -18.01 1665 2 10.25 2912 -9.38 0.43 -10.88 — -19.624 -10.39 2.48 8.77 1.63 -15.783 1.48 3.26 1.44 0.60 -18.372 2.32 — -9.97 1.44 7.77 1735 5373 -14.952 10.00 1.44 1549 1666 -19.852 2.47 2050 -9.39 0.52 7.76 -21.48 -9.80 —2 10.37 0.59 -15.872 1.56 11.07 2047 -9.96 -12.03 0.68 2.64 2.79 -13.696 -12.71 7.89 0.83 -17.313 1.89 3.05 1432 0.62 2073 4159 -16.472 2.28 — -9.54 1.29 8.65 -15.313 1330 4832 1.55 -20.349 1.58 — -9.81 6200 0.80 6.05 -20.32 —3 10.42 0.33 -16.05 2.432 10.72 1265 -8.61 -10.86 0.74 2.63 -13.48 —8 -12.40 8.16 0.94 -17.22 2.89 2.59 1337 6.87 3.26 0.70 1270 -18.89 2.51 -9.73 -16.892 1717 — 4782 -9.71 1093 3.08 3823 — 8.61 0.64 3.13 — -10.40 -19.52 1281 — 1326 5.25 2.80 9.51 2.66 -9.56 1332 1217 1301 1.89 8494 / 2214 2.28 1.00 -18.93 -13.48 — — — — 2.53 2.41 1236 1000 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± km 3256337 1453 + 275 1427 420 1666 468 4826 + + + . (J2000.0) [log] [log] [log] [log] continued 09 50 27.4009 50 36.30 12 45 55.7009 12 50 48 58.00 32.60 NGC 3024 ASK 42870409 33 52 33 54.40 19.30 NGC 3021 42 50 52.90 UGC 529509 57 29.40 1344 1420 27 45 24.30 PGC 4571034 1603 4806 09 59 29.9909 59 43.50 4110 46 00 01.40 06.20 1110 39 00 38.60 05.80 KUG 1180 0956 4510 31 00 09.60 14.60 CGCG 064-021 43 11 34.30 PGC 2891610 09 00 37 27.10 02.40 ASK 20868110 00 31.60 ASK 294909 0310 22 00 27.70 31.98 03 12 19.00 UGC 537610 04 02 24 35.50 25.40 UGC 5377 UGC 2816 5378 19 10 36.8010 04 05.20 UGC 5403 1694 1679 10 31 05 11 17.60 07.60 5297 NGC 310610 01 08 38 06.70 28.50 2dFGRS 2056 N421Z115 51 50 52.30 2151 UGC 4153 10 5460 12 52.8010 12 59.90 2093 2210 43 13 19.20 31.30 3910 46 13 16.90 31.10 1267 CGCG 123-024 0310 22 13 30.00 58.90 ASK 6192 314091 2210 43 14 51.70 14.30 NGC 3165 07 01 26.40 NGC 316210 03 14 27 58.00 59.40 UGC 5522 NGC 1081 3169 07 48 02.00 CGCG 036-069 1281 1339 1310 1370 1222 1319 8485 09 50 16.96 27 18 17.50 KUG 0947 – F 1 1 3 3 1 1 1 1 1 3 2 3 1 NC F N NF N N NPF NRF A N NF N NRZPF NP C C C C C C C C C C C Table A.1. 0944 0945 09460947 09480950 0951 09 50 55.4009530954 09 28 51 33 28.10 04.0009550956 NGC 3026 09 32 54 56 09.20 35.000957 09 54 49.600958 2MASX 09 J09512804 58 55 20 18.10 27.500959 09 09 55 16 24.50 15.900960 UGC 09 5306 04 55 16 37.70 12.000961 NGC 09 3049 33 56 15 20.10 45.900962 NGC 3055 04 28 36.200963 UGC 09 27 5326 57 13 32.80 39.200964 ASK 09 95056 57 35.600965 IC 09 2520 1477 33 58 37 05.80 11.000966 09 45 58 13 21.10 47.600967 IC 09 2524 37 58 17 47.10 19.000968 UGC 09 5345 32 58 22 53.40 11.60 UGC0969 09 5349 11 1176 59 23 18.70 19.30 NGC0970 3067 47 1457 44 12.60 UGC0971 47 5358 1801 36 58.40 UGC0972 5354 1416 1943 ASK 1823950973 0974 0978 1244 10 00 18.900980 0981 1459 3696 54 32 18.900982 1377 UGC 1451 0984 5369 10 01 47.90 2916 0985 1167 0989 1099 10 36 03 29 02.00 55.300992 10 03 28.80 UGC0993 5394 38 22 37.600994 10 46 04 37 08.70 42.000996 ASK 3136850997 KUG 1000 10 06 07 30 11.50 37.701000 Mrk1001 1549 0714 10 33 09 01 17.40 38.501002 10 10 27.90 NGC1003 10 3118 05 10 24 39.90 14.601005 27 57 21.90 FGC 1430 1006 20 120A 04 12.60 IC1007 2550 1339 UGC1008 5489 10 1252 14 51.50 1336 03 38 52.50 1721 ASK 95840 4779 3795 1080 Source0943 RA Dec Name

Article number, page 32 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.360.22 4.30.22 3.40.29 4.8 6.50.33 6.2 3.30.48 21.5 8.21 6.50.41 10.8 7.41 7.20.19 34.8 8.21 7.81 6.70.36 7.99 7.41 13.3 4.0 8.600.45 14.9 0.67 15.4 7.99 0.42 8.71 8.60 7.3 3.80.70 21.0 8.51 13.8 0.21 0.43 7.32 -1.34 8.53 6.0 8.1 29.10.55 10.30.13 0.10 14.5 8.53 11.1 8.21 8.960.85 21.6 17.9 -1.53 0.32 32.6 8.57 8.96 3.0 9.500.23 23.3 7.1 9.81 8.57 0.39 16.0 0.79 7.96 7.00.34 -0.36 12.8 7.70.89 24.8 0.01 8.88 9.50.65 8.40 12.7 3.3 8.800.25 -1.27 16.5 -0.13 3.50.57 9.58 8.80 4.6 3.20.64 9.19 44.7 -0.89 6.50.37 24.4 8.97 7.1 2.63 70.50.53 8.29 7.50.56 60.8 -1.17 7.95 9.18 7.00.26 21.0 10.29 8.29 12.20.37 -1.27 10.0 0.43 15.6 10.29 37.80.23 9.49 18.30.21 17.3 8.47 10.7 9.46 3.40 0.18 36.4 8.18 3.8 8.47 0.44 25.8 0.02 8.88 5.10.69 0.80 8.20 4.0 3.40.25 -0.04 13.4 4.50.29 8.20 7.43 8.6 6.90.50 28.8 7.57 4.10.74 0.28 10.39 13.5 9.54 7.50.26 -0.50 34.5 -0.63 5.80.43 -1.01 8.12 12.3 4.40.47 59.7 7.87 6.90.32 0.54 8.53 5.4 9.560.14 8.2 15.8 0.52 13.2 -0.45 0.23 -0.09 10.1 9.29 7.20.34 27.3 8.52 4.20.23 -0.61 8.42 2.9 -0.33 8.630.26 9.8 11.0 -1.56 0.31 4.0 -0.72 6.1 7.82 4.10.25 15.6 7.57 6.40.59 -0.09 9.07 9.5 8.42 8.4 11.3 0.59 10.1 -0.95 14.3 0.05 9.10 29.1 8.19 -0.75 8.08 -0.27 9.12 8.08 -1.12 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 55 373 734 504 94 90 1645 0.40 187 144 0.82 3 1885 48 209 6.13 3 62 3.89 244 3.93 62 213 99 270 0.41 248 3.92 2 2.28 7.43 7 572 1354 86 88 169 322 1.60 117 2.41 346 3.21 1 3.18 5 1593 485 193 1761 570 23.60 8 194 248 23.93 1 102 2.84 274 2255 162 13.29 6 248 2.36 854 8.43 49 99 5125 709 0.42 556 1551 0.45 118 12.92 4 169 239 165 260 1.06 2713 3.39 274 27.06 3 1774 1.40 7 64 2135 83 1327 5.26 83 75 96 147 1467 0.81 1142 0.56 0.88 177 81 1.89 395 1.34 132 415 1.84 10.84 / HI 18 9218 148 61 1.23 138 1.36 2217 44011 184 530 21079 308 4.60 325 234 4.79 9.53 3961511 2.98 17 59 19313 186 160 220 99 228 2.27 1.75 14029 2.47 1.00 123 26435 3.73 11131 364 36812 2.11 456 87 1.83 16016 1.63 11 152 325 229 366 3.00 2.91 10 87 133 1.66 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 24 0.301 -0.14 -13.462 0.42 -13.172 0.16 -14.302 — 0.55 -15.55 —3 7.14 0.53 -16.532 1.46 — -17.064 — -9.27 0.41 — -18.393 — 0.32 3.24 8.50 -14.364 2.46 3.28 1.33 9.85 -15.57 —3 1650 -9.20 7.22 0.83 -17.21 -10.42 —3 1273 1149 1.70 2.66 -17.91 3.784 — -9.28 9.74 3.09 0.68 3.00 -19.272 1244 1.07 -11.50 -17.39 2.542 1659 — 0.50 1301 1163 — -19.914 — 2.98 1.34 8.71 -15.963 1035 10.17 3.92 0.84 — -19.594 -9.80 -10.08 7.95 0.82 1225 — -16.437 10.15 2.90 1.35 1339 -17.932 2.68 3.32 -9.55 -11.87 3.28 8.53 0.47 -20.222 1.28 1591 3711 -10.23 -16.90 3768 4 1.50 4.61 10.47 — 1296 1.00 -19.432 -10.66 1.13 2.67 6.56 2243 -17.274 10.14 1078 0.77 -17.65 —3 2.28 -9.17 -10.97 1.98 1465 -17.495 — 0.49 9.23 2.28 -20.244 2.94 6.49 4965 8.75 1.09 -17.74 -10.642 0.98 3762 2029 -10.19 -15.73 3315 —4 — 6.09 0.35 2.32 -18.61 0.90 4.40 4.66 -14.882 — -8.55 1362 9.44 -17.67 —3 1287 7.38 0.35 1156 -10.51 2.882 8.92 0.59 2.94 -10.54 — -14.023 3.69 1.37 -10.14 -15.742 4756 2.24 3.56 7.14 1.67 4131 -20.352 2.56 8.07 0.52 2131 -20.882 10.55 1229 -9.42 0.64 1150 -15.123 11.01 -9.85 -12.14 0.58 1370 -14.045 2.23 -11.84 1.19 7.58 -18.334 2.31 2.25 1.08 7.35 -18.505 1145 3.23 -9.49 0.81 8.98 -19.564 6239 1324 -9.83 1.72 9.65 -17.607 2.14 -9.51 6256 0.90 9.90 -17.857 -10.66 2.44 0.57 8.85 -18.582 1289 -10.18 4.19 0.21 9.98 4.85 -15.401 1199 -9.98 1.26 9.35 1.73 -13.963 -10.86 1436 0.47 7.91 -19.312 1671 -10.21 3.05 0.85 6.97 2.64 -17.135 5350 -10.15 10.02 0.71 2.39 -19.93 1525 4 -9.30 1388 -11.42 0.05 8.37 1.70 -16.73 9.85 1.28 -13.98 1298 2.56 3.06 -9.28 8.46 1314 -19.72 -9.84 2.31 10.24 — 1163 -9.70 5222 2.17 -10.50 2.90 1703 — 4412 3.11 1395 2.37 1586 1163 / 19 0.90 -13.17 — — 1.28 1251 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± km 2001380 1158 135004 1282 + + 365 1169 379B 1700 + + . (J2000.0) [log] [log] [log] [log] continued 10 15 26.50 64 38 08.90 ASK 63743 1659 10 15 40.6010 52 15 32 55.00 02.9010 16 21.70 ASK 194538 02 41 07.70 37 46 48.60 UGC 5539 UGC10 5540 17 11.9010 04 17 19 47.90 48.2010 18 06.70 UGC 5551 2110 52 18 24.00 10.30 21 1151 10 49 18 58.80 19.70 NGC 3187 07 08 34.70 NGC 3190 07 02 57.50 ASK 1288 23032410 19 42.90 IC 1162 060210 20 03.60 22 27 08.5010 38 20 36 13.90 55.90 UGC 5574 1356 UGC 557710 06 20 48 56.80 09.40 1591 PGC 3999200 25 22 00.40 1208 10 3779 22 19.80 UGC 558810 21 23 34 21.60 06.90 3779 NGC 322110 20 25 01 46.40 38.20 1464 2MASX 2058 J10232162 10 05 26 39 30.99 06.70 3744 10 29 43.40 CGCG 037-033 20 16 59.5010 36 31 16 10.40 17.80 PGC 1307 457791510 31 29.98 KUG 1026 26 03 18.10 24 52 10.00 IC 4123 2583 NGC 327010 1154 33 53.70 24 01 1205 19.50 CGCG 124-037 6127 6247 10 35 48.9010 36 5352 16.20 08 28 59.80 37 19 28.80 PGC 4017582 NGC 3294 1127 1567 – F F RF 1 3 3 3 F A 3 1 1 1 1 3 1 1 1 3 1 NF NF NC NR NC NF NF NC A N N N R C C C C C C C C C C Table A.1. Source1009 RA Dec Name 1010 10111012 1013 10151016 10 15 47.9010181019 37 44 58.401020 10 16 28.20 ASK1022 340266 10 16 34.101024 10 45 17 19 02.30 17.701025 21 07 22.90 UGCA1026 10 208 03 17 38 38.60 45.60 NGC1027 3177 ASK1028 96277 21 41 17.601029 NGC1031 31851032 1271 10 19 01.501033 10 19 33.001035 21 17 01.201036 58 12 20.60 1655 LSBC1037 F567-01 10 20 11.10 NGC1039 1290 3182 1038 1041 10 27 20 49 43.30 01.301042 1238 NGC1044 3204 10 65 21 10 17.30 19.401045 10 21 47.60 UGC1047 5576 19 39 06.301049 10 56 23 55 1079 08.70 49.50 NGC1050 3213 NGC1052 3206 10 08 25 58 09.90 47.201053 2099 ASK1054 279019 10 58 25 08 53.10 00.011055 NGC1056 4959 3225 14 21 47.301057 10 30 49.70 UGC1058 3288 56461059 23 57 54.201060 1340 10 31 40.801062 PGC 1158 1697033 10 31 56.701063 10 4756 13 32 50 31.90 05.701064 10 22 32 05 34.80 49.401065 2MASXi J1031407 54 24 03.701066 PGC 2133 10 4563662 65 34 02 29.80 27.901068 UGC 10 5720 34 42.801070 NGC 1374 10 3259 35 34 15 47.30 24.301071 10 11 34 11 51.10 50.401072 1325 UGC 10 21 5738 34 38 56.10 53.701073 NGC 10 3279 28 35 39 09.40 50.801074 NGC 10 3287 11 35 29 22.70 32.50 PGC 10 1842340 25 35 02 39.30 17.10 ASK 1194 10 379436 37 35 40 42.00 17.90 CGCG 28 124-039 33 56.90 KUG 1032 26 1437 07 33.00 UGC 5749 1679 CGCG 124-041 1524 1389 1323 1273 1173 5244 1395 4411

Article number, page 33 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.220.37 3.50.32 3.70.30 15.0 3.00.44 10.0 4.00.39 32.1 65.8 7.22 12.90.28 11.2 148.5 9.42 8.620.39 7.22 8.40 4.1 24.7 -1.73 0.41 9.25 10.1 0.14 0.18 0.93 9.96 5.0 5.9 9.25 16.50.47 4.00.48 -0.45 9.15 8.63 5.2 7.70.30 60.1 5.3 -1.73 0.33 -0.36 16.7 9.50 143.7 4.90.25 9.14 5.1 -1.62 0.26 29.5 9.54 10.1 9.94 -2.09 0.19 37.7 -0.40 8.47 7.90.40 -1.53 14.4 4.10.28 69.1 24.6 0.60 8.13 8.140.43 90.3 8.93 3.70.74 38.0 20.2 0.89 8.14 182.70.34 -0.64 77.9 7.46 8.54 46.70.51 9.18 154.3 3.4 -0.05 0.44 17.4 0.06 9.75 0.22 0.17 9.54 17.8 6.50.39 35.0 9.75 6.3 0.25 0.29 29.3 9.42 9.61 4.70.32 6.1 8.750.37 7.6 -1.22 -0.26 5.1 6.80.25 37.9 13.8 0.77 7.490.29 19.3 9.27 10.08 5.8 63.60.38 84.5 7.49 27.10.07 -0.19 -1.12 62.7 8.14 174.7 9.180.47 130.3 8.51 4.3 -1.60 -0.02 0.57 9.53 6.40.35 9.49 12.5 8.51 3.0 0.65 0.30 12.3 7.7 0.28 36.10.29 81.2 6.530.30 9.31 77.5 14.4 140.1 9.14 6.53 74.3 -0.76 129.4 8.60 9.10 9.14 124.8 9.05 -0.41 9.10 9.06 2.26 2.29 0.380.37 11.50.31 35.30.27 25.9 2.90.29 54.0 8.5 8.720.19 5.8 8.85 4.10.13 11.0 13.7 8.72 0.69 8.85 7.71 6.1 7.80.25 14.9 8.02 3.70.23 0.04 7.88 9.6 7.84 7.8 1.10 0.54 3.4 7.2 -0.23 13.1 1.05 7.67 4.8 10.13 2.9 8.13 0.08 0.05 6.1 8.89 1.48 8.64 8.89 -1.41 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 582 38 4164 1821 50 4388 69 203 172 0.38 0.99 325 1013 6.32 224 390 2.11 37.41 150 5.93 1741 3.87 6 30686 84 346 3131 42.61 1585 65 343 1612 4.20 113 1091 1.64 1832 84 128 1.81 232 11.16 1 228 124 0.43 255 2562 259 8.11 32.03 1 280 12.50 2936 70.91 9 98 317 73 11.32 203 1225 1002 233 7.57 1092 0.70 1 77 1.63 1292 63 130 1334 1.11 106 100 11.85 2 2104 32 210 3.53 26.41 284 23.26 3441 45 2971 381 108 0.11 1 3.70 12.77 99 149 100 23.15 145 146 20.03 20.22 31 235 2036 261 2304 97 6.10 12.26 3 1359 484 80 2.03 2897 80 82 96 314 1.46 59 109 0.61 3.27 77 1.85 0.40 / HI 14 1292113 171 29410 140 0.95 367 714 178 1.90 753 0.56 1.56 18 373 41614 1.43 207 271 2.38 10 126 182 2.75 3411 77 131 145 176 0.60 1.27 10 166 200 1.98 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 12 0.313 1.62 -14.881 0.63 -21.162 0.37 -17.102 11.14 — 0.76 -15.262 -12.61 8.48 1.38 -19.182 7.47 1.35 — -21.533 1.96 -9.58 0.69 -22.623 10.40 — -9.19 3.37 1.42 -16.88 2.423 10.88 7428 -11.70 1.51 -21.61 3.252 -12.15 8.99 1.68 — -21.83 1172 951 2.182 11.12 1.49 -21.88 1570 2.332 11.23 -12.58 3.19 0.37 -18.584 — 11.48 5623 -12.50 0.68 5547 -17.685 2.35 -0.06 -12.84 9.94 3.16 -13.84 987 1 1.46 7.88 1.19 -15.32 5867 -12.581 1.92 0.65 7.23 7160 -10.44 -18.422 1521 10784 0.68 2.81 -14.60 — -9.70 0.92 2.57 9.57 -17.055 7.51 1299 -17.50 -10.422 1.95 8.47 0.97 — 1215 4 -9.63 8.96 1.41 2.11 -18.542 1301 -9.45 2.56 1.12 -10.17 -20.45 1.794 -0.68 9.29 1254 -19.19 3.853 10.63 1261 1.91 -16.36 1.47 -11.603 1180 -10.69 9.87 0.86 -20.154 7.97 939 4.77 1.53 -10.97 -18.852 985 1.85 1.22 -21.60 -9.92 — 0.77 3.12 9.46 1013 -18.87 6173 1 11.20 4.32 -18.822 -9.89 -11.99 9.74 0.45 2719 — 9.20 0.60 -10.77 -18.51 1239 2.774 1.93 1.79 -18.905 -9.90 10272 3.04 8.88 1.104 4870 9.21 1.70 -20.05 3.506 959 -9.14 0.70 1610 -18.384 10.07 -9.47 0.70 -18.22 2.19 1628 -11.27 0.20 -15.96 2.87 — 9.01 -13.49 1624 2.94 1657 — -9.60 6.79 — 3401 2.82 -9.25 3.16 — 1729 2.58 2.64 1499 1077 1064 2 1.04 -18.19 — — 2.55 1334 52 1.161 0.56 -17.245 -0.20 -15.201 -15.09 0.701 -0.97 — 7.67 -15.925 6.92 0.48 -14.432 -9.54 1.12 8.11 -15.21 —4 -8.71 6.79 0.20 -19.822 2.81 -9.81 7.59 0.63 2.64 2.49 -14.07 -8.76 10.08 1.13 1331 -17.20 2.36 -9.40 -10.30 6.66 2.34 1099 1028 -19.26 1129 1.43 4.29 10.05 — -8.78 989 -10.23 2.57 1270 9265 — 4.14 1240 2.90 2123 6378 / 11 0.13 -15.33 —65 0.01 — -14.84 1.05 6.76 809 — 2.68 1079 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± 303 1.41 -19.98 — — 2.92110 0.85 3039 -14.79 — — 2.71 1374 V ± ± km ± ± 31161261716228 1281 9256 + + 531 948 + . (J2000.0) [log] [log] [log] [log] continued 10 36 36.10 52 50 58.80 SBS 1033 10 37 19.30 43 35 15.3010 38 44.90 UGC 577110 39 11.80 5310 30 39 05.10 20.50 -00 2410 34.10 39 47.40 NGC -00 3310 1210 00.80 40 IC 28.40 0632 4710 56 41 NGC 00.80 31.20 3325 0910 10 41 57.10 50.70 UGC 5798 3710 18 42 46.20 07.50 NGC 3332 3810 43 42 00.40 48.40 NGC 3334 1310 44 42 49.10 52.40 7398 UGC 5819 1310 27 43 35.40 05.50 NGC 3338 13 44 27.80 UGC 5832 13 30 37.30 ASK 431284 958 CGCG 065-090 5625 5606 10 46 34.90 1541 10 46 36.90 5833 1310 45 46 03.00 42.50 7206 6310 13 47 10777 27.20 41.50 NGC 3367 2510 55 47 53.50 45.80 NGC 1296 3359 1110 04 47 37.40 47.70 UGC 1231 5881 1158 56 1266 05 28.00 UGC 5897 12 34 14.80 UGC 5888 NGC 337910 49 17.8010 49 49.97 2967 1210 25 49 02.20 55.10 3210 58 50 48.30 18.90 CGCG 1012 066-029 3210 59 50 26.90 39.80 NGC 6171 3395 1310 16 51 18.60 46.50 NGC 2703 3396 65 43 37.90 UGC 1239 594410 32 53 54 23.99 00.10 NGC 339410 920 53 29.60 NGC 3424 1610 46 53 20.70 29.60 16 1172 43 59.60 NGC 3447a 16 47 09.60 PGC 4578229 NGC 3447b 1624 1704 1033 3399 1592 1054 1073 1054 10 54 21.90 27 14 22.10 NGC 3451 1356 10 54 29.50 17 20 38.5010 55 44.50 NGC 3454 17 00 18.0010 57 19.00 CGCG 095-07010 17 58 16 53.40 23.0010 59 09.00 2MASX J10571931 50 10 00.00 61 31 50.40 ASK 183866 NGC 1092 3471 1137 6392 2112 – 1 P P ZF R ZPF 3 1 3 1 1 1 3 1 3 1 1 1 3 3 1 1 3 1 3 1 1 N NRF F NF NUF NZP F NRF NC NP NC NC NC NFA NC F R R C C C C C C C C C C C C C C C C Table A.1. Source1075 RA Dec Name 1077 107910801081 1082 1083 10 38 07.901084 10 38 25.701085 10 22 51.001087 47 42 36.60 CGCG 065-0741088 PGC 23029941089 1090 1091 1092 109310961097 1149 1098 1577 1099 10 43 38.901100 10 45 09.801101 10 14 45 52 22.40 18.601103 10 15 46 26 12.60 59.40 NGC1104 3346 55 57 37.30 PGC1105 3090611 01 48 47.80 NGC1106 3353 NGC1108 3365110911101112 10 47 54.601114 10 48 11.901115 10 00 48 48 12.20 45.10 1222 1249 1116 10 04 48 59 24.80 54.80 CGCG1117 28 010-016 36 06.40 NGC1120 3386 34 42 941 41.00 NGC1121 3380 996 NGC 33811122 1123 1124 1126 10 53 08.10 4855 33 54 37.30 10280 NGC 3442 1587 1627 1728 1127 112811291130 11311133 10 54 29.701135 10 55 39.201137 60 43 26.801139 10 02 56 23 13.90 44.70 ASK1140 10 92234 56 20.10 CGCG 038-051 12 00 40.60 10 31 57 16 38.10 13.10 LSBC D640-13 2MASX J10562004 13 58 44.50 LSBC F640-V02 1021 1321 1001 1243

Article number, page 34 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.370.64 6.30.21 5.70.28 21.8 9.60.33 61.4 10.40.66 22.4 8.67 8.00.56 95.8 9.97 8.9 8.070.45 1.20 13.3 -1.11 7.9 9.200.31 17.0 1.06 4.80.42 8.06 15.9 9.20 5.40.31 9.47 22.7 -0.13 8.10.46 9.36 10.4 -0.43 8.1 42.20.31 12.3 9.54 0.24 22.90.24 8.71 8.75 5.3 -0.85 26.70.17 8.60 4.40.56 2.62 10.6 8.75 12.8 8.830.42 1.61 6.9 7.50.45 16.9 9.65 -0.85 14.30.33 25.5 13.5 -1.30 9.30 7.900.61 32.2 8.20.16 31.4 -1.49 9.33 -0.40 5.2 8.990.23 11.0 -0.33 6.9 8.750.48 -0.17 10.00.44 8.7 17.9 8.13 10.8 2.68 0.85 12.5 9.88 9.70.41 29.3 1.22 7.97 4.8 8.280.54 -1.11 14.5 16.5 -0.12 9.790.39 -0.17 5.30.28 9.1 29.6 8.24 -0.31 8.40.41 10.6 9.72 8.891.57 9.2 0.40 15.6 9.60.88 16.4 -0.74 -0.34 6.7 9.730.25 9.26 14.8 6.2 8.460.28 -0.94 16.7 -0.49 6.20.60 8.69 12.6 0.50 5.70.26 9.82 10.0 -0.45 10.29 9.50.15 -0.69 4.9 8.40.30 -0.71 8.25 22.9 14.70.56 8.18 6.8 8.25 8.8 20.10.56 8.45 20.6 -0.51 0.28 8.07 8.08 5.0 8.45 8.7 32.20.44 13.1 -1.62 0.56 2.01 8.12 8.77 7.1 8.90.58 13.2 5.90.42 -0.35 21.0 2.68 10.6 9.67 7.920.39 15.1 5.20.28 52.5 -0.92 9.56 1.32 6.90.39 9.41 66.7 -0.93 9.62 9.50.20 11.0 111.8 -0.54 3.90.48 -0.91 8.29 7.00.75 8.72 14.4 9.10 6.9 -0.91 -0.68 5.2 9.7 27.5 9.10 9.67 7.84 9.18 9.6 -1.44 -0.48 0.30 9.24 -0.70 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 79 1561 4781 1873 39 516 1325 2.14 1645 4.33 61 157 247 183 231 15.83 2.50 2821 2.69 2622 6.87 1684 5.54 191 190 207 209 10.89 5 241 4.37 1 7.46 952 252 1316 87 269 1.55 7 72 1273 8.47 1094 91 7.72 3 60 319 1.94 126 1358 81 372 0.96 6 159 1507 1.62 8.61 4367 4.39 238 2083 4594 93 6.27 254 164 3.29 419 149 3.63 186 441 2.39 3 3.69 16.85 10818 1341 298 5.21 862 99 46 342 1268 117 1.52 46 373 1.41 1161 10.81 6 3.20 66 158 3324 1871 1.97 2.66 359 219 210 115 19.08 3 2421 2.44 140 144 2.71 195 18.35 159 211 1.17 8.24 / HI 2514 172 91 259 14425 1.98 28 1.30 355 16517 450 252 248 2.34 0.98 33214 4.28 422 47620 3.35 401 468 4.79 1113 50612 203 558 12726 259 7.21 174 145 1.43 1.29 235 1.19 14 295 35225 5.09 45512 523 226 1.72 271 4.33 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 34 0.573 1.57 -14.763 0.50 -21.332 7.47 1.25 -14.345 11.08 0.92 -18.473 -9.44 -11.77 1.09 7.01 -15.543 0.70 -19.522 2.95 3.11 — -9.21 1.09 8.19 -18.547 0.55 9.91 -20.63 -10.193 2.96 2119 6666 9.13 0.52 -17.46 —2 10.38 -9.28 0.69 2.61 -16.302 -9.96 -10.05 6.09 1.32 993 2.38 -13.45 4.232 1.49 -18.75 3.773 3.05 945 — -9.94 6.99 1.55 1433 -21.083 2998 9.68 0.75 6002 -21.34 2.775 2942 10.95 -9.70 1.08 — -10.77 -16.241 10.79 -12.28 1.10 2868 -18.873 2.28 -10.44 0.31 3.31 3.21 8.30 -17.422 1.58 0.27 9.66 -16.952 -10.00 1375 1.67 1.42 9.16 1028 1371 -14.05 6270 8 -10.26 0.75 6.07 1.56 -21.415 -10.40 6498 0.72 6.91 3.32 -15.773 10.99 -9.56 1.41 2.74 -16.712 1037 -9.09 3212 -11.31 0.76 8.09 -20.562 4.36 1.68 8.45 -15.002 1548 10.10 3.42 3.05 -9.88 0.80 -19.873 1224 -9.88 -10.68 1.63 7.84 -18.501 6909 10.46 1.54 1207 1.03 -20.062 2.76 2.71 -9.86 -10.89 0.22 9.23 -19.473 10.67 1420 1.14 -16.582 3.80 4.29 1556 -9.75 3854 1.37 -11.10 9.76 -17.344 1.52 7.96 -20.282 -10.61 4759 2.86 2.78 1.01 9.13 903 -21.192 10.51 -9.15 0.86 2.66 -17.50 -10.233 11.00 -0.60 1588 -11.49 5799 -16.95 2.49 -12.35 -14.90 1.37 3.23 3239 2 8.13 — 8.68 -18.263 4.12 1587 0.70 1660 —4 -9.96 2855 9.69 0.85 7520 — -16.593 1.33 -10.30 -16.28 2.263 — 1.67 8.47 0.51 -20.534 1.85 6.08 1550 1.45 -12.873 10.59 5.63 1598 -9.80 1.11 -20.084 1437 -10.39 1.64 6.60 -19.554 2.90 — 10.50 1065 1.20 -19.944 3.17 -9.23 -12.21 1.22 9.95 -17.23 5.593 1395 10.53 1.26 -17.773 -10.45 3.66 3.81 5481 -10.47 1.47 9.20 -18.743 1057 0.96 9.40 3.24 -21.47 -10.793 3.30 5341 0.85 929 -15.33 -10.42 11.11 — 3245 1.19 3.12 -17.35 2129 -12.34 8.32 2.74 -19.48 8.88 1291 — 1.90 9.94 1998 -10.38 — 2.54 -10.25 7486 3.55 1.68 4.93 1194 1957 1101 2881 / 13 0.50 -15.01 6.08 -10.30 2.32 1284 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± km 1738228 1039 4731541 1422 0937188 1588 + + + 09-18-06609-18-070 1004 2864 + + . (J2000.0) [log] [log] [log] [log] continued 10 59 10.80 61 41 06.50 ASK 155380 2060 10 59 27.4011 46 00 07 01.10 20.50 NGC 3478 14 50 17.40 NGC11 3485 01 58.9811 45 02 13 35.20 40.9011 03 59.80 UGC 6103 1611 44 04 05.20 02.90 27 56 16.10 UGC 611211 28 04 02 36.90 12.50 PGC 6644 457178111 05 32.50 NGC 3512 45 07 30.70 1471 17 38 22.50 UGC 6135 2MASX11 J11053253 08 19.90 5994 53 36 27.80 1424 ASK 1027 235925 1371 6486 1184 11 11 28.3011 06 12 54 17.30 27.0011 12 39.80 UGC 6233 65 13 35.1011 09 13 03 00.20 21.00 UGC 623711 13 20.10 IC 0676 0711 51 13 42.70 40.99 5911 54 13 29.40 43.60 CGCG 039-068 4711 34 13 42.10 44.90 UGC 6249 53 38 48.30 UGC 6255 48 16 21.70 PGC 2446875 1592 NGC 357711 15 06.90 1032 14 1396 47 08.30 1412 NGC11 3596 17 46.50 1035 5464 51 928 28 35.70 UGC 6309 5333 1214 2850 – 1 1 A 1 3 3 1 3 1 1 3 3 1 3 2 1 NF NP NA N NF A NF NRF C C C C C C C C C C C C Table A.1. Source1141 RA Dec Name 1142 11431144 114511481150 11 00 00.201151 1152 11 54 00 25 23.80 31.601153 11 01 23.60 MCG 1156 11 16 01 41 50.95 31.701157 57 40 39.60 UGC1158 11 6083 16 02 36 07.40 25.00 NGC1159 3488 UGC1161 6104 54 27 18.301162 MCG 1165 11 04 34.5011671168 16 03 42.401169 11 06 04.601170 UGC 6137 11 07 03.401172 11 43 08 940 19 02.90 51.901173 2996 12 03 36.101174 2945 UGC 11 6149 53 08 37 33.90 00.201175 UGC 11 6169 08 39.501176 UGC 11 6182 04 09 49 23.30 54.801177 11 47 09 31 25.30 53.701178 NGC 11 3535 10 09 50 36.50 02.701179 -00 2MASX 05 11 J11083946 51.70 09 51.701181 CGCG 11 6288 067-014 50 09 55 55.90 36.20 IC1182 0673 11 62 10 17 44.80 30.601183 UGC 11 6202 10 10 43 45.20 15.001184 UGC 11 6199 04 3226 10 50 54.50 47.201185 NGC 11 12 3547 1548 10 00 56.50 58.101186 UGC 11 6216 09 1234 10 37 56.90 18.601188 NGC 11 3559 61 11 20 06.40 49.201189 2MASX 53 J11105448 6926 23 1555 15.90 NGC1190 11 3543 43 12 37 03.90 58.80 NGC1192 3549 IC1193 0674 28 29 10.90 3843 1194 11 12 52.00 893 UGC 62411195 4760 1196 1584 10 11 59.301197 5800 UGC1198 3233 624811991200 1673 11 13 56.501202 2847 11 14 10.901203 11 12 14 18 27.40 03.801204 7503 11 48 14 19 37.20 06.601205 1551 IC 17 0677 15 35.90 NGC 11 3583 30 15 18 43.80 50.90 NGC 11 3592 16 1302 26.30 UGC 11 6271 13 17 46 40.20 56.10 04 20 11.40 IC 2666 38 03 09.20 CGCG 039-094 UGC 6307 3241 2105 1299 2003 1094 7472 1938

Article number, page 35 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.290.40 4.90.36 44.70.54 7.1 7.40.19 82.3 5.10.21 13.0 11.0 9.63 9.740.32 4.6 7.80.61 15.8 -1.66 8.96 -0.24 28.00.30 12.1 9.10 7.87 6.80.32 2.88 34.4 59.50.58 23.6 -0.20 1.60 7.69 7.4 9.410.42 95.6 10.1 8.860.30 27.4 7.69 15.0 0.20 9.300.34 16.4 -0.01 12.7 60.90.39 8.98 16.6 1.10 9.040.31 14.2 76.3 -1.26 9.230.41 32.0 -0.30 127.9 8.21 8.50.28 0.21 5.9 9.170.52 10.1 9.28 8.21 12.10.43 10.4 9.17 6.10.22 14.1 9.28 8.62 37.90.27 9.83 10.1 11.4 8.160.45 0.32 54.1 -0.98 5.80.44 16.6 9.22 0.97 4.5 9.220.47 5.4 8.40 8.9 0.01 0.33 -0.67 25.2 6.50.28 -0.12 11.9 7.89 6.9 51.50.27 8.88 6.7 20.70.12 0.69 8.12 9.46 6.00.37 -0.51 9.50 3.4 9.50.64 -0.08 0.90 12.4 8.40.44 0.62 8.22 4.7 3.50.23 9.61 13.3 8.30.41 0.77 7.69 -1.33 3.5 8.50.91 8.51 20.7 9.90.32 -0.07 9.83 3.8 4.6 0.24 0.23 9.26 16.5 6.90.26 -0.45 88.8 8.30 -0.29 7.10.35 9.80 58.8 10.9 143.80.35 10.30 0.24 16.8 -0.30 0.39 99.8 8.35 9.21 48.6 -0.76 0.35 31.3 113.9 6.7 9.12 0.99 0.40 9.21 4.4 8.870.57 22.9 9.13 13.5 1.28 0.33 12.4 0.79 -0.52 7.80.20 30.3 9.45 16.9 25.80.34 21.3 8.01 -0.16 9.670.15 29.4 9.16 3.9 28.60.32 -0.17 0.71 7.0 9.060.24 -0.18 8.25 5.2 8.20.55 24.3 0.61 8.9 -0.30 9.61 9.8 9.9 48.2 7.87 -1.03 16.8 9.73 9.56 0.37 -1.22 8.56 0.30 -0.41 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 14 2878 1313 314 137 152 20.87 1 53 1682 2.43 1 59 2.53 79 1559 100 1.57 2 80 178 3091 137 248 6.23 2 8.78 355 206 16.18 2 2691 2.94 49 236 1833 5.95 15.59 1119 75 212 1715 136 393 2.27 6.54 189 29.42 1 81 4304 2.35 1157 88 2.75 1205 2.18 1086 93 151 1371 13.86 1235 75 2.08 152 233 1.38 1133 1.83 98 2564 160 15.00 475 1.70 9 3.82 66 4926 95 2.18 77 263 1514 0.26 298 2.55 17431 5.61 204 12711 4.18 98 144 1191 166 1474 2.11 151 2547 17.93 182 267 14.77 1 272 1274 6.81 286 25.06 3 59 148 2092 3.39 1019 1.65 78 2498 53 137 339 6.93 8.86 1 60 5.38 93 3646 225 2.80 1.79 99 107 247 0.66 149 7.28 5.14 / HI 20 433 50327 1.35 82 168 0.65 14 226 286 3.48 13 106 16519 1.42 42524 48826 99 3.42 525 157 597 0.57 4.16 24 420 510 1.97 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 34 1.582 1.17 -21.743 0.69 -19.372 11.29 0.65 -16.032 -0.14 -12.53 9.98 -19.009 -14.39 0.59 6.082 -12.22 1.42 0.52 9.30 -15.39 -10.171 6.27 0.66 2.47 -18.42 8102 4 -0.55 -9.74 3.20 -17.865 -8.42 — 1.69 -17.14 9.21 2329 5 4.54 8.88 0.95 2.26 2782 -18.882 8.20 -9.95 0.33 -18.25 —2 10.23 3210 -9.76 -0.01 -18.58 3.87 985 -10.07 -14.29 9.34 0.69 1.72 — 4.953 9.02 -10.23 -16.023 1.84 2926 1252 0.59 2.80 —4 1314 -9.89 1.51 3.81 -16.232 — 2595 0.19 -8.45 1594 -20.743 2.95 0.82 8.29 1947 -14.232 10.81 3.75 1.16 -18.163 — 1506 -9.86 -10.61 0.74 7.18 -19.638 0.45 9.21 1209 2.50 -16.95 -10.082 2.46 2.18 0.89 9.90 -14.252 -9.97 0.31 8.52 2.83 2177 -17.72 -10.482 1917 7136 0.90 7.20 -14.641 3.35 -9.79 0.53 9.39 4.50 1172 -18.753 -9.65 7.22 0.44 3177 -18.432 1.90 9.54 1.75 1583 -15.17 2.641 — -9.11 8.88 0.65 -20.404 1574 -9.77 7.45 0.61 -15.06 3.97 4.752 1079 10.94 -9.43 1.61 -16.73 3.163 -9.35 -11.14 7.76 1.11 -19.10 2.855 2943 1262 0.74 8.27 -19.60 2.39 1995 1.31 10.28 -9.71 1.24 -16.574 4142 -9.48 -10.83 9.55 1548 -19.96 1.502 6235 8.05 0.42 -10.03 3.272 10.10 3.20 0.67 -14.567 1970 -9.58 -12.09 2.75 0.21 -17.14 6374 4 1616 7.37 0.53 -15.09 2.034 3.14 1.27 2609 -15.933 — -9.59 1.09 7.84 2696 -18.185 5597 0.43 8.08 -18.713 2.84 0.94 9.65 -14.56 —1 — -9.92 0.87 9.61 -19.774 -11.44 1487 0.29 7.29 2.08 -18.59 -10.284 2.25 2.80 0.67 9.83 2.29 -17.702 -9.46 9.35 1.28 2.53 1369 -17.18 -11.533 1360 1503 0.32 8.45 1058 -20.773 3.11 -9.83 8.56 1.39 4.89 4155 -15.231 10.64 -9.26 0.80 -21.49 3.93 1128 -9.66 -10.59 1.03 7.50 3723 -18.46 3.00 10.95 -17.06 2.23 1843 1.94 -9.23 -10.60 9.25 2111 8.97 -10.12 1.60 1156 1.58 6838 -9.41 1.66 7487 1520 4.87 3205 1204 / 34 1.30 -18.27 — — 3.62 1154 54 1.57 -21.07 11.06 — 4.12 9975 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± km 307 1610 + 09-19-052 2946 + . (J2000.0) [log] [log] [log] [log] continued 11 17 50.60 26 37 32.80 NGC 3609 8099 11 18 21.30 45 44 53.50 NGC11 3614 19 33.20 03 00 53.3011 20 14.70 CGCG 039-12011 02 20 31 31.30 25.20 UGC 634511 57 20 46 37.30 53.0011 20 39.90 NGC 2327 3625 6411 01 20 08.20 59.30 31 13 19.10 ASK 105593 53 1237 11 25.70 UGC 6355 NGC 363111 22 17.90 1620 59 04 28.2011 22 25.30 NGC 1937 3642 53 1199 41 16.4011 22 39.99 MCG 2188 11 22 50.70 1154 1311 19 23 49.90 02.10 12 20 41.50 IC 277611 34 23 29 07.00 51.70 IC 278111 23 10.70 UGC 6397 30 28 44.10 1571 34 29 23.00 KUG 1120 11 24 05.90 CGCG 185-05311 24 10.60 45 48 39.8011 27 24 00 25.80 51.10 UGC 641011 24 25.00 UGC 6415 03 19 46.10 4131 11 03 24 13 26.10 16.40 1547 NGC 6227 3664 NGC 3664A 11 6364 20 31.90 NGC 366611 25 31.80 5596 11 38 26 03 01.00 38.00 9967 UGC 643311 01 26 59 17.80 02.80 1382 1328 UGC 6440 46 58 26.70 NGC 1062 3677 2110 6822 7461 – F 1 3 1 A R 3 3 3 3 1 1 1 1 3 1 1 3 3 1 NP F NC NRZPF A NZP NC R R R C C C C C C C C C C C C C Table A.1. Source1206 RA Dec Name 1208 1209121112121213 1214 11 18 28.101215 11 18 36.301216 11 45 19 18 28.10 46.401217 63 16 50.301218 PGC 11 09 2262856 19 35 45.90 44.201219 Mrk 11 0165 20 12.40 ASK1220 271488 59 16 49.901221 11 67 20 14 26.20 29.60 UGC1222 6335 NGC1225 3622 11 03 20 35 31.80 08.201226 NGC1228 3633 26 57 48.101229 2791 NGC1231 3629 11 21 32.201232 11 3212 21 32.90 985 1233 11 39 21 17 51.30 58.501234 11 02 22 48 02.60 37.501235 UGC 2918 6372 03 24 17.401236 NGC 1301 11 3644 42 22 49 18.60 09.301237 NGC 11 3640A 22 23.20 UGC1238 2596 6383 13 03 54.101240 11 13 22 04 35.70 40.10 IC1241 1513 11 2763 22 39.00 IC1242 2767 58 58 40.501243 37 45 54.30 PGC1245 2584984 NGC1246 3652 1923 11 23 06.961248 7143 1192 1251 39 57 24.201252 3183 11 23 19.10 ASK1253 505696 11 23 20.50 -001254 55 21.40 -03 1571 1255 07 50.80 UGC 1259 6402 1079 1256 11 24 ASK 13.20 102691257 1989 1259 26 14 43.501261 11 24 25.801263 FGC 12401265 1946 11 27 24 27 40.30 23.101268 11 24 44.501269 UGC 11 6421 14 25 56 19.00 47.401270 11 15 25 16 26.80 31.40 2616 1271 UGC 6424 63 2698 43 45.201272 ASK 11 433202 57 25 43 53.50 16.401273 UGC 6429 NGC 3669 11 09 26 59 08.30 14.90 1485 IC 0692 11 04 26 03 34.00 44.50 11 26 44.30 PGC 1489 1262899 11 26 24.20 59 09 19.50 IC 4156 2822 1118 IC 0691 3724 1837 1522 1158 3207 1201

Article number, page 36 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.670.14 8.30.19 20.50.59 29.1 12.00.70 25.8 6.30.48 42.4 11.8 8.34 7.980.65 12.6 11.6 8.33 33.8 8.34 0.51 0.36 6.9 24.90.53 9.74 0.37 9.30 6.00.88 15.7 -0.29 9.04 5.60.44 -0.96 11.2 10.8 10.110.56 -1.00 12.9 5.00.31 26.0 -0.35 9.82 38.70.27 9.92 18.6 -0.92 9.61 7.60.20 94.2 -0.93 5.80.33 27.5 3.24 7.96 3.3 9.170.08 8.4 8.69 8.00.26 1.03 9.17 5.1 5.40.28 14.6 0.05 8.37 3.80.16 37.0 8.93 6.10.22 -0.03 8.69 4.1 4.80.42 65.5 37.9 2.50 7.15 0.08 0.16 10.06 8.16 6.9 6.10.22 60.0 0.38 8.0 -0.25 0.43 -0.54 15.6 9.14 5.4 9.130.49 13.4 10.20.48 -1.81 8.68 32.9 0.44 8.1 23.50.55 8.05 11.7 0.51 56.30.82 7.82 9.28 5.2 0.39 0.59 22.7 9.26 7.00.22 -0.22 0.04 10.06 10.9 4.90.28 12.6 9.26 11.5 -0.63 0.74 9.16 3.4 8.70.33 16.5 9.59 15.3 -0.20 0.30 8.68 -0.80 7.1 7.89 3.70.35 29.6 6.00.13 -0.08 26.2 10.5 0.73 8.64 9.000.33 11.0 4.60.82 50.1 9.05 2.50 9.00 4.20.26 8.94 -1.16 3.6 9.13 4.60.22 18.6 6.60.25 1.52 0.57 7.33 4.30.28 4.0 27.9 8.34 6.50.63 -0.03 4.5 9.98 8.400.42 2.3 13.0 0.93 8.90.27 -1.29 41.0 0.68 7.25 6.90.61 28.2 21.5 103.5 8.040.37 -0.01 33.1 8.16 8.880.39 33.4 9.50 1.46 7.00.48 49.9 -1.17 18.4 0.21 8.460.35 0.23 10.8 9.18 9.9 33.3 17.1 2.24 -0.61 9.50 18.4 8.61 33.7 -1.17 9.13 0.17 8.97 9.13 0.41 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 421 928 48 1188 80 2812 77 356 4.64 6 99 317 406 1.85 421 407 4.81 8 4.35 424 14.24 2 437 481 7.64 2576 6.63 5142 274 2003 4.49 14.43 85 359 1035 25.45 1115 118 1335 4.85 1 1.31 50 1674 99 1041 2.85 69 290 1139 137 154 0.28 3 304 0.75 10.60 2254 1782 0.65 61 267 1261 8.14 2374 3.90 82 1424 98 260 367 0.91 4 1.08 196 134 6.35 400 2984 15.33 211 6.96 3203 29 3.77 4 6.01 1548 71 1571 188 1347 1.49 177 141 12.80 3 1695 80 2.13 156 1123 1.94 394 10.90 1027 1239 66 408 0.34 1127 1.37 1073 69 2.21 133 1001 3.67 213 1102 0.30 121 2601 245 1.15 85 1.15 292 282 10.72 2 26.51 1223 309 1541 4.93 18.93 155 183 176 175 7.80 196 5.43 7.30 / HI 12 42414 477 3.52 73 12031 1.69 91 163 0.54 16 18535 241 102 2.92 186 0.50 11 66 121 1.97 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 22 0.552 0.20 -16.445 0.53 -16.394 0.98 -16.003 — 1.73 7.63 -20.055 1.47 7.97 -18.504 10.03 -8.98 1.61 -18.89 —3 10.27 -9.61 1.43 -19.55 -9.962 10.03 1.72 -10.83 1.56 6.67 -20.471 2.10 10.46 -11.62 3.65 1.15 -20.592 3.70 10.73 1042 -10.79 0.16 -19.687 2.52 10.86 987 -10.21 1.85 962 5116 -14.052 3.42 1710 -12.28 0.73 6.37 -18.221 2.58 1718 0.53 6.93 -16.932 2.58 6313 -8.51 0.49 -17.18 6224 3 — -9.17 0.80 8.64 -17.082 5.73 6235 8.40 0.40 -16.84 -10.223 4.30 0.74 6.43 -13.31 —2 2428 -9.41 8.61 1.22 3.16 1058 -17.474 -9.01 1.41 6.77 3.17 -21.85 2.671 -9.91 8.70 0.58 1446 -21.231 1.71 10.31 -9.29 0.89 1092 -17.872 2.79 10.95 1933 -9.78 0.29 5674 -18.335 1.09 -12.22 0.69 8.69 — -15.743 2.61 1898 1.01 8.17 -14.965 1.02 1015 -9.56 2.60 0.09 7.66 -18.662 1989 7.78 1.13 -15.532 1.81 — 6648 -9.29 9.50 0.91 4746 -21.122 -9.82 1.45 -10.46 -18.598 2.77 1.88 10.69 1866 — 0.78 -19.741 1.97 -11.59 0.45 2.91 9.36 -17.802 1595 10.39 1599 0.40 -14.10 -10.00 —2 1123 2.62 -12.18 0.74 8.76 2494 -16.402 1.32 7.15 4.09 4.56 -17.759 4.98 -9.70 5865 0.42 6.14 -19.822 -9.37 0.42 2819 1561 -15.52 4.09 10.21 — -9.30 3651 0.72 -17.063 2.75 -11.59 7.42 -14.20 1850 3 2.20 1.47 8.563 — 2.66 1026 -8.90 0.31 7.36 4254 -21.784 -9.85 1.06 5.78 -16.002 2.50 11.27 -9.52 3322 0.68 -13.524 3.03 1.13 -12.39 7.72 -13.765 1269 1.37 3056 0.82 7.26 -17.991 4.51 1608 -9.12 0.98 6.58 -17.243 1137 -9.74 0.16 9.33 -18.074 2.69 -9.97 9471 1.23 8.67 -16.183 2.03 -9.93 9.27 1.26 -19.211 2.58 1195 -9.74 0.83 6.22 -10.55 -20.923 2.77 1104 9.79 0.39 -16.24 4.32 10.67 1409 -8.89 0.65 2.63 -10.72 -17.07 1609 -11.01 8.44 -17.44 2.65 1215 3.75 1568 -10.53 3.65 — 8.56 1100 3.14 1288 -10.68 5754 — 2.70 1037 3.91 1621 2279 / 10 0.49 -14.71 7.41 -9.40 3.26 1825 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± km 1449313 1117 + 358368 1882 405148 1971 1607 1123 576 1561 + + + + + . (J2000.0) [log] [log] [log] [log] continued 11 26 50.50 64 08 16.80 UGC 6448 984 11 28 31.0011 29 03.00 0911 06 29 15.90 06.50 0911 06 29 43.00 11.50 IC 2857 08 59 18.90 IC 069811 57 30 08 02.60 18.60 IC 0699 NGC 3683A 09 16 59.2011 31 03.70 NGC 370511 54 31 24 08.90 29.30 ASK 23685411 13 31 34 32.10 13.40 6316 -02 ASK 18 43334811 33.00 31 44.60 6238 11 2395 31 UGC 57.80 6510 6190 34 20 00.20 -02 55 27.40 UGC 1171 6512 CGCG 012-00311 32 02.1011 5685 32 13.40 57 22 51.7011 00 1019 32 49 28.10 09.40 SBS 1129 NGC 3719 62 30 26.20 4742 UGC 1564 11 6520 33 20.20 1871 63 16 45.70 UGC 653411 33 59.20 5857 49 03 43.40 3622 IC 070811 1264 36 36.9011 00 36 49 58.00 00.70 UGC 657811 55 37 09 51.00 43.40 NGC 3759A 56 08 31.00 9480 UGC 6596 1097 5752 2253 – F 1 1 1 3 1 3 3 1 3 3 1 1 N F NRF A A F NC NF N N C C C C C C C C C Table A.1. Source1274 RA Dec Name 12751276127712781279 11 27 10.901280 11 27 12.201282 11 08 27 43 19.20 51.70 -001283 59 11 40.70 27 31.80 IC1284 11 2828 59 28 37 24.00 35.90 UGC 64571285 56 52 37.40 UGC1286 09 6452 24 27.40 NGC1287 3683 NGC1288 36921289 11 29 59.4012901291 11 63 30 13 17.30 24.101292 11 30 27.70 SHOC3301293 58 08 02.001294 1034 966 11 36 31 44 07.41 14.30 CGCG1296 5114 291-076 Mrk 1709 1297 0424 11 35 31 35 09.54 23.00 1704 1298 KUG1299 1128 11 36 31 36 41.10 02.501300 KUG1301 1128 03 29 16.801302 11 31 59.08 NGC1303 1059 3716 11 1447 32 01.901304 11 40 32 14 02.40 00.901305 14 36 38.801306 KUG 1129 36 1947 41 52.701307 KUG 1129 11 32 20.30 UGC1308 65171309 11 53 32 54 39.50 16.001310 11 32 44.001311 UGC 11 6518 35 33 19 06.10 42.201312 6626 02 28 24.801313 UGC 11 01 6526 33 29 40.52 28.901314 PGC 11 1228108 33 41.601316 2dFGRS 11 N444Z258 61 33 53 45.30 16.801317 11 49 33 35 50.10 57.201319 -03 NGC 2497 26 11 3725 13.20 33 51.501322 ASK 14 219382 49 28.20 CGCG1323 012-022 11 34 34 45 19.50 04.101324 2MASX 11 J11335011 2819 34 56.501325 ASK 4272 11 535108 13 35 19 18.40 19.101326 1027 11 16 1848 35 14 49.90 52.501327 IC 11 2934 04 36 57 26.50 17.201328 PGC 11 35 4548254 36 20 33.40 06.901330 PGC 1275866 58 11 28.901332 UGC 11 6570 36 1636 3311 36 24 3056 48.00 37.20 UGC 6575 NGC 3755 11 54 37 17 37.00 36.80 1854 NGC 3756 11 16 38 33 02.10 22.30 UGC 1139 6594 35 12 12.90 1415 1199 UGC 6603 1611 1210 1578 1285 1039 1623

Article number, page 37 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.190.22 6.20.36 5.50.27 10.30.41 5.1 5.90.87 6.2 19.9 27.3 7.320.80 10.6 7.24 8.47 8.20.27 46.2 0.01 8.10.24 27.6 10.7 0.40 0.39 8.13 8.840.42 23.9 5.0 9.590.33 22.2 53.6 0.55 8.84 0.49 -0.74 9.62 129.7 7.6 8.78 8.50.38 26.2 9.62 0.51 -1.19 9.20 20.6 11.2 7.67 68.30.18 -0.74 7.80.19 40.0 8.47 0.11 9.33 4.70.41 30.8 17.8 9.12 8.47 0.41 13.5 9.33 0.17 9.6 42.0 9.58 1.18 6.00.51 25.8 4.8 8.74 -0.72 8.370.42 10.1 8.47 9.00.35 -1.46 1.35 7.7 6.0 17.40.60 -0.40 9.56 4.80.56 12.6 7.34 8.61 3.90.19 -1.37 8.6 7.90.49 8.17 0.10 0.77 9.9 6.80.31 12.7 12.8 8.36 0.50 0.21 14.3 9.66 6.1 22.20.32 -0.03 9.12 3.00.40 -1.52 7.96 -1.17 8.78 8.6 5.50.56 7.8 1.17 3.00.31 0.07 16.2 7.84 7.90.27 19.8 8.48 8.60.27 9.01 7.84 17.7 3.50.36 9.97 1.69 13.8 5.1 1.24 0.46 8.60 31.9 -0.34 4.60.20 8.57 9.1 7.40.19 0.37 68.2 8.54 -0.77 3.10.39 15.9 8.02 3.9 8.770.92 -2.10 12.0 3.30.66 -0.25 9.13 -1.22 7.9 4.10.25 23.8 7.34 4.5 0.04 0.48 18.0 7.68 6.5 9.420.39 11.2 0.12 6.70.36 9.45 -0.26 7.68 12.4 7.10.46 28.3 17.5 8.27 -0.74 0.40 9.51 43.6 10.22 11.60.60 28.5 0.07 -1.39 5.3 -0.85 81.00.48 8.41 18.8 9.490.23 9.52 7.2 8.6 1.25 0.36 38.3 28.4 0.27 10.0 0.88 14.9 7.75 9.35 31.1 19.9 8.86 0.53 1.49 8.22 -0.26 8.82 8.22 -0.82 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 44 30 1571 499 191 1077 0.49 3007 4.24 132 4879 366 297 11.01 1 529 111 14.16 353 255 12.04 2 1434 3.56 285 2908 1.17 33.57 1299 328 3531 185 20.52 3292 396 68 8.38 358 1807 5.72 3 1.10 87 1983 73 116 4.68 6.52 1434 97 1434 164 5167 0.57 5.18 4054 3.26 5297 62 429 127 2.68 111 43 4.57 168 1.31 2 6.09 748 177 0.85 1038 1901 154 97 6.17 3386 2.31 1284 3643 58 1.15 15.31 6 76 182 71 284 89 2115 0.40 321 0.48 5.68 412 10.18 21 458 192 2252 8.71 2176 246 4271 6.45 23.25 2146 456 41 245 14.42 208 4.35 64 249 3.72 4.29 / HI 2614 28 124 93 0.41 150 1.15 10 80 135 1.84 10 495 53618 2.37 106 168 1.44 1413 14017 86 170 386 16411 0.39 477 2.48 215 4.77 26 242 105 0.76 26816 3.03 16 172 32412 223 396 92 2.53 28 1.90 151 46 2.29 147 1.27 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 24 -0.312 0.60 -15.436 0.20 -15.902 6.84 0.72 -15.112 1.44 8.08 -16.612 -8.33 1.58 7.58 -19.605 -9.70 1.44 2.09 -19.612 10.33 — -9.24 0.77 -18.772 2.82 -12.05 1.29 -14.412 930 2.40 — 0.10 9.97 -19.23 —2 4.90 1196 7.56 1.30 1557 -16.15 -10.812 9.95 0.31 3.81 -19.02 —2 -9.75 2392 1.54 1.31 -10.58 -16.692 — 1.55 3.77 1145 -19.944 2.17 — -0.39 2.69 7.94 1873 -19.072 10.30 0.90 -14.58 2689 —2 10.20 -9.16 1.78 -11.09 902 -16.62 — 991 7.02 0.41 -10.52 3.03 -20.534 3.05 2.82 8.87 2.92 -14.462 -9.56 10.93 1.05 1817 0.64 -11.143 1816 -11.22 3710 0.58 7.24 -15.26 2.24 1463 2 3203 1.57 3.13 -16.953 1.93 -9.29 7.67 1.36 -21.453 1021 0.51 8.38 -10.33 -19.69 5645 1.84 11.18 974 1.32 -14.503 10.29 -9.37 -12.67 3.58 -17.16 -10.72 6.80 0.30 899 2.943 2.84 8.71 -10.85 -16.576 966 2.94 1.46 1808 2 -9.82 5956 1.92 6.79 0.76 -19.533 2455 1.30 -16.62 4.044 10.31 -9.52 1.57 1206 -17.504 -12.04 0.81 8.23 -19.983 1.79 1424 9.33 1.70 -16.092 10.64 2.00 -9.84 0.54 3997 -18.081 -9.84 -12.61 0.45 8.28 -18.67 6401 4.35 0.81 9.99 -14.113 2.72 1.87 -9.85 9.09 -17.761 -10.82 1154 1.35 7.22 3055 3 2.59 1811 -9.88 0.64 2.03 -19.982 — -9.65 1.45 -16.293 3.06 10.19 1378 1.37 -21.152 2.58 895 -10.59 0.15 8.21 3048 -21.782 — 10.90 0.74 -14.903 11.07 5.54 1070 -9.51 -12.37 0.85 2.21 -18.59 -10.51 0.58 7.17 -18.324 4.78 1.39 2393 9.23 -14.54 1447 2 2.47 -9.07 8.64 1.01 1256 -10.19 5959 3 7.22 0.91 -17.65 3.39 -9.95 6287 1.08 2.69 -17.09 -9.38 9.12 1530 -18.74 3.17 3164 -10.52 3.60 — 9.64 1726 3.30 -10.50 958 — 2.48 1851 3.10 1785 961 2 0.52 -14.19 7.31 -9.50 2.90 947 / 16 0.54 -15.28 7.84 -9.9930 4.58 0.5124 -15.90 1282 0.44 -13.06 — 7.77 — -9.95 3.87 2.71 1294 2924 54 0.79 -19.43 9.68 —58 2.92 0.97 3103 -14.85 7.86 -10.73 3.02 1796 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± ± ± km 5953112 1281 + 327 1803 + . (J2000.0) [log] [log] [log] [log] continued 11 39 43.96 31 54 38.60 NGC11 3786 41 07.5011 41 16.90 3211 25 41 37.20 29.80 3611 32 41 42.70 39.30 KUG 1138 32 20 59.50 NGC 3813 24 48 01.80 Mrk 0746 NGC 3815 2562 11 43 32.7011 43 34.70 31 27 28.40 1337 08 56 32.80 UGC 6684 1804 IC11 0724 3700 44 52.1011 45 06.70 5711 52 45 24.60 22.10 0911 30 45 09.10 30.00 CGCG 292-024 09 09 43.60 PGC 4001338 09 43 44.00 ASK 273153 CGCG11 068-056 45 58.70 1815 11 46 07.80 58 32 06.70 5971 47 29 41.10 1294 PGC 36687 NGC11 3877 47 06.30 4030 2978 13 6409 42 24.50 UGC11 6758 48 03.40 30 21 33.50 1386 NGC 389111 49 08.50 906 11 49 23.60 2711 05 49 08.80 41.50 26 44 29.60 3118 PGC 4562228 48 25 33.60 UGC 6791 NGC 3906 6289 1654 1834 956 – F ZP 1 1 3 A 1 3 1 3 1 3 3 3 1 1 NC NF NF NZ N NC NF R C C C C C C C C C C Table A.1. 13351337133813401341 11 38 35.701342 11 38 51.501343 11 57 39 52 01.10 26.901345 11 43 39 09 21.30 56.301346 Mrk 11 1450 01 39 20 22.30 11.601347 UGC6611 58 16 07.301348 ASK 11 56 73694 40 16 18.50 14.30 NGC1349 11 3795A 40 56.70 NGC1350 11 3780 09 40 00 58.80 35.501351 14 04 27.10 IC1352 0719 11 28 16.10 ASK1354 433748 NGC1357 38101359 11 41 39.701360 950 1190 11 42 19.00 1587 1361 11 15 42 1138 57 26.30 56.501362 11 14 42 59 44.86 46.301363 UGC 2391 11 6653 51 43 35 26.99 52.701365 UGC 11 6669 52 43 46 27.00 46.401366 UGC 11 11 6667 43 23 31.10 54.30 896 1368 NGC 1833 3824 60 40 34.901371 PGC 1393002 55 28 990 44.00 UGC1372 6691 11 44 04.90 UGC1373 6685 11 44 10.601374 11 60 44 07 14.80 11.20 -031375 40 07.60 NGC1376 55 3835 3224 02 05.90 ASK 108161377 1029 NGC1378 3846A 979 1380 5632 11 905 45 35.601381 11 45 1283 36.901383 11 55 45 53 45.60 12.801385 31 979 17 58.401387 NGC 10 3850 49 28.501389 IC 2957 11 46 12.401391 NGC 2443 3869 11 1206 46 34.101393 11 10 1426 47 35 00.70 43.901394 55 49 17.001395 -00 CGCG 17 11 068-062 39.10 47 34.401396 PGC 11 2515483 47 45.30 UM1397 452 11 55 48 58 00.20 02.001398 59 53 12.001399 NGC 1159 11 04 3888 48 29 10.60 17.301401 2MASX 11 J11474525 48 12.80 -01 UGC1402 1785 3001 11 59 6771 48 20.80 50.401403 11 13 48 12 3068 55.50 33.70 2dFGRS -02 N240Z166 01 56.00 IC 1079 0735 47 34 57.60 UGC 6780 ASK 348043 11 50 04.40 1468 2394 26 28 1540 45.20 NGC 5949 3899 1716 3149 962 1792 Source1334 RA 11 38 17.30 00 36 48.10 Dec ASK 373928 Name 947

Article number, page 38 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.160.36 4.30.30 40.10.16 7.8 7.2 47.60.40 30.70.48 43.4 15.2 7.57 8.590.14 41.6 12.60.43 -1.04 80.9 -0.28 8.65 4.7 8.180.25 20.1 4.6 8.90 0.58 0.62 8.18 6.2 8.38 4.40.50 11.3 0.30 6.50.36 -0.99 18.6 7.28 8.60.24 25.3 23.0 8.700.41 -0.13 33.9 26.3 7.77 9.790.30 44.8 13.1 8.70 8.710.19 35.0 -0.36 0.33 4.1 8.91 18.00.30 8.71 7.8 8.390.46 10.4 8.91 8.26 4.50.25 1.27 4.5 8.60.28 13.3 0.20 7.62 5.50.39 7.59 3.8 8.03 5.50.90 17.2 0.27 8.20.57 0.54 1.28 8.14 6.9 5.20.44 29.9 24.1 7.680.22 0.34 10.7 8.83 5.1 9.290.54 47.3 -0.90 18.00.68 -0.23 9.48 21.9 8.83 9.89 9.20.36 32.0 -1.05 6.30.31 46.0 -0.60 8.26 4.7 9.300.99 10.51 10.8 7.60.59 0.28 0.98 4.2 -0.66 6.30.70 9.76 21.7 9.60.66 17.8 7.76 -0.08 7.60.43 33.1 14.9 7.930.36 36.4 10.34 0.11 9.7 8.980.19 28.8 1.02 -0.88 4.9 8.960.38 17.1 8.98 8.7 8.660.16 -0.73 15.0 7.70.31 8.38 17.2 0.96 9.3 25.20.51 61.5 8.97 0.60 19.40.86 38.5 7.94 147.2 8.58 -1.23 0.35 19.1 7.93 10.070.40 78.6 7.94 2.44 5.40.48 39.9 -0.05 -0.37 10.03 4.80.47 30.9 11.5 8.770.17 0.20 28.2 6.50.17 75.6 9.57 1.46 4.10.98 64.4 -1.31 7.97 4.6 8.940.35 16.0 10.03 5.10.33 18.1 7.97 8.94 6.70.24 32.1 0.06 11.7 8.33 32.3 19.4 7.74 9.04 19.5 -0.23 9.54 26.8 0.15 0.26 8.64 0.31 8.51 0.77 8.51 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 132 44 17515 47 67 194 1536 9.02 2.82 80 88 1753 38 19.82 123 3.12 91 84 59 5.09 2796 142 0.31 1 99 3564 52 164 1.28 9.23 65 10.20 1504 702 93 6.21 113 35 4.58 69 3.73 573 85 0.84 2242 2.38 259 13021 7.14 164 1146 498 15.77 8 147 2737 526 121 4.16 302 16.32 2 56 1462 4.68 1015 1.34 96 2155 135 1366 1.48 248 142 11.00 3 192 220 15.52 2 177 10.40 1 40 243 1062 4.26 3 1.74 44 62 132 162 140 0.94 5.60 63 2636 218 23.55 1.65 1 20.98 1092 2389 131 256 2791 60 1.55 297 21.93 2 174 18.47 2 86 1822 191 113 0.48 207 19.57 54 135 6.95 3.83 87 3.24 / HI 24 110 182 0.59 12 153 191 1.62 30 6012 1452117 81 0.56 40 112 12125 120 157 1.34 35215 0.77 0.82 470 129 5.48 183 2.20 15 162 210 4.57 1923 201 186 452 274 14.92 28 2.23 50 138 0.44 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 52 1.002 0.58 -17.273 -0.04 -15.854 8.87 -15.22 0.863 8.07 1.13 -11.14 -17.151 0.27 -17.92 — -9.89 4.73 0.01 8.61 -14.523 9.36 -17.33 -10.42 2.322 7.41 1.27 — -10.191 948 0.50 3.28 -19.691 1822 — -9.58 1.81 4.69 0.67 -14.905 10.15 -0.44 -17.962 1.89 918 -10.61 1004 0.61 -15.98 —2 984 — 0.38 -15.53 1126 3.59 -0.43 — 7.12 3.34 -15.452 -13.59 8.06 —1 -8.22 3708 2524 7.35 0.49 -11.57 —1 7.04 0.67 4.19 2.69 -16.324 -9.13 0.06 4.11 3.17 -17.403 -9.45 1.06 7.79 1018 -16.59 1053 5 2.70 8.58 1.59 2.76 1005 1649 -19.722 -9.38 1.25 1243 -19.792 — -9.40 0.51 9.52 -20.422 4.49 10.54 973 0.39 -16.21 -10.784 2.45 10.49 -12.67 1.54 1453 -17.152 — -10.70 0.85 7.97 2.64 1132 -21.832 4.49 0.58 8.32 2.45 -19.923 11.17 4.81 -1.07 -9.43 2385 -15.10 3337 2 4127 -12.23 -13.75 9.83 1.494 3.48 — -4.42 3186 7.65 -22.513 2.59 6.92 -9.88 1.11 -15.63 1299 4 2.00 11.21 -9.61 0.83 -10.61 -18.982 4.29 6387 -10.53 0.52 -15.752 3.20 — 3172 3.42 1.31 9.70 -15.351 5028 7.61 0.10 7.70 -19.52 -10.322 1098 7.78 0.34 951 — -14.69 9941 3 10.19 -9.27 0.52 4.82 -16.842 -9.94 -12.14 5.48 1.64 -16.00 5.122 — 6.14 0.57 1108 -19.70 3.474 2.49 1341 7.98 0.26 -19.81 10.45 -8.57 1.45 956 — -15.123 1075 3319 -9.57 -10.47 9.83 -22.40 3.573 2.65 7.32 1.38 2.124 2.07 10.88 -9.40 1.20 -17.322 1191 -11.95 0.73 1392 -19.973 3.72 1039 — 3221 0.49 -16.792 2.33 — 0.60 9.96 -15.238 4.38 3271 0.75 8.55 -17.45 5903 -10.11 0.77 7.59 1027 -18.91 -10.02 — 8.78 2.95 -16.07 -9.34 9.23 1.98 3.12 7.87 3451 1.53 — -9.94 3028 -10.20 910 1608 7.68 2.63 3.06 1077 3216 1544 2 0.84 -16.64 8.61 -9.89 1.31 1145 / 11 1.03 -14.51 7.44 -9.54 2.6810 0.18 974 -13.61 6.76 -9.41 3.56 971 39 0.92 -14.01 — —35 0.48 3.77 -16.74 1120 — — 2.72 1445 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± ± km 5615114 949 + 258A 1823 400 1053 141 1447 + + + . (J2000.0) [log] [log] [log] [log] continued 11 50 39.8011 50 55.99 2511 31 51 34.90 45.80 14 35 41.40 KUG 1148 38 00 53.70 CGCG 097-16311 51 58.10 NGC 393011 61 52 55 02.04 54.0011 52 04.80 ASK 156312 1611 48 52 34.80 32.00 52 06 27.00 NGC -03 3933 40 17.30 UGC 6840 UGCA 992 24911 54 01.6011 54 04.40 16 43 921 24.00 30 06 34.60 PGC 16611611 2523 54 13.10 PGC 430130911 50 54 53 33.70 34.50 3705 ASK 1018 219863 58 22 1647 01.30 NGC11 3958 55 28.70 11 58 06.10 983 980 11 55 54.90 NGC 396811 56 10.30 4011 55 56 18.50 13.52 60 4109 31 21.10 ASK 497175 58 11 57.20 NGC 3978 UGC 3316 691211 57 12.4011 57 24.60 -02 41 11.30 6360 11 57 57 55 ASK 36.90 33.90 1176311 57 44.10 UGC 6931 32 1108 11 16 57 39.40 47.60 32 17 38.60 NGC 9945 399411 53 58 14 34.30 04.10 NGC 1303 399511 58 37.90 UGC 6940 53 20 43.70 47 15 41.30 ASK 186426 NGC11 4010 1394 59 09.40 1201 52 42 27.3011 59 33.80 UGC 3081 6983 3323 13 53 13.90 1110 1193 KUG 1156 918 1081 – F ZP 1 1 1 1 3 3 1 1 1 1 N NF N NRF NC A A NF NRPF NF F NC F NRF NZ R U R C C C C C C Table A.1. 14061407 1408 1412 1413 11 50 38.9014141415 55 21 13.901416 NGC1417 3913 11 51 47.601418 11 51 53.701420 48 40 59.201422 11 53 52 05 01.90 58.20 NGC1423 3928 ASK1425 186073 13 52 43.201426 CGCG1427 068-079 11 52 37.201428 11 52 39.101429 -02 11 28 53 09.90 948 14.101430 50 02 16.00 UGC -03 68501431 24 32.20 UGC1432 6849 11 54 PGC 07.60 1257871434 11 1124 54 972 12.301436 -03 40 957 56.401437 11 00 54 08 25.00 11.80 CGCG 012-1131438 1439 -02 IC 19 0745 11 10.40 54 58.701440 11 55 04.90 UGC 68791441 11 58 55 29 24.91 37.00 1040 1443 01 43 11.30 NGC1444 1242 1006 11 3963 10 55 12 35.13 05.60 CGCG1445 11 012-116 55 37.10 PGC1447 1455 4001590 25 53 22.001448 56 15 11.101451 IC 0746 2MASX1452 J11553712 11 56 28.101454 1135 11 56 41.70 2392 1455 11 55 56 07 55.40 30.801457 11 48 1299 57 20 08.49 17.80 NGC1459 3186 3982 57 30 47.40 3164 NGC1460 30 3985 23 32.20 UGC1463 6926 11 57 25.70 UGC1464 69271465 39 45 39.10 5027 1466 KUG1468 1154 11 58 23.801469 -021470 16 38.501471 1113 11 58 UGC 45.67 69581472 11 58 961 56.191474 1081 11 27 59 27 00.70 08.70 3299 31 25 10.80 NGC 11 04 4017 59 40 10.20 10.70 ASK 11 527351 59 10.30 ASK 172529 37 47 36.20 -02 35 27.20 NGC 4025 UGC 6978 5897 3448 3021 1607 3223 1544 Source1404 RA 11 50 12.30 42 04 28.10 Dec UGC 6805 Name 1158

Article number, page 39 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.400.35 3.20.50 5.50.36 38.7 3.90.37 10.4 8.10.21 99.1 18.7 7.620.15 15.4 31.3 8.02 9.500.26 33.5 0.30 8.4 8.450.75 48.2 13.3 0.17 9.50 8.920.20 21.8 0.93 8.79 8.30.78 19.2 -0.25 13.70.25 41.7 25.9 1.34 7.48 8.080.45 17.0 7.1 9.070.42 53.6 -0.72 16.2 1.39 8.210.17 0.82 9.6 9.26 9.80.20 41.9 8.21 5.70.29 -0.78 15.8 8.20 7.8 9.350.12 6.5 8.30.50 -0.86 9.38 -1.09 12.8 6.30.15 11.2 11.2 7.63 -1.15 0.34 8.03 3.8 8.20.32 16.7 8.63 0.60 -0.49 3.70.63 26.0 7.26 8.59 5.3 0.83 0.20 4.4 7.30.69 38.0 -0.06 7.26 8.29 6.20.24 56.0 9.48 8.88 7.30.21 0.13 151.1 8.9 6.80.25 -1.55 8.88 8.44 3.30.39 9.25 10.0 7.66 8.30.24 54.0 1.74 2.70.49 9.25 7.74 0.48 121.4 6.6 6.70.40 7.31 7.00.15 0.80 61.0 9.38 7.65 6.50.11 0.17 124.9 5.1 9.20.18 9.38 7.65 7.67 3.10.34 9.42 8.07 4.1 6.90.47 55.2 0.86 -0.25 2.7 -1.27 0.61 8.06 100.0 5.8 5.10.52 16.6 6.770.55 0.41 9.06 20.6 13.1 7.38 48.90.27 0.19 13.2 0.94 54.90.34 9.44 0.03 10.04 9.70.36 31.8 10.08 89.7 -1.02 -0.15 0.33 13.2 156.7 -0.41 8.60 6.00.31 62.00.24 8.07 9.09 8.60 6.9 9.80.50 96.4 3.8 8.07 0.35 9.09 20.0 14.5 9.70 8.710.22 13.7 5.60.29 31.7 -1.32 8.35 14.2 8.71 0.19 24.9 26.5 9.25 8.77 0.13 16.3 4.2 9.06 41.6 -1.81 0.92 8.02 -0.15 8.75 3.4 0.90 8.75 7.89 0.67 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 41 74 33521 91 367 1952 30.95 1 1.68 87 2219 34 1163 89 7.67 1922 49 5.77 1054 69 328 221 0.66 2 2.94 15.66 1003 91 258 3015 1.86 300 25.25 1144 331 86 322 1.44 120 11.82 1073 4.23 1467 0.80 111 1.48 1121 136 130 106 4.93 1 0.47 1225 3204 7.35 4 36 3671 31 63.15 3 70 70 2116 421 1.10 42 96 238 2416 0.31 206 29.06 0.94 6 58 273 92 228 0.87 1 2.78 33 30.96 115 130 47 0.60 6 155 0.16 5 20.40 3441 2961 436 74 342 16.83 1181 10.56 6 87 182 37 191 28.07 2.16 2 1152 220 1182 11.71 1831 2.74 1514 45 209 97 9.15 38 5.30 71 124 1.87 51 6.93 0.36 / HI 35 6215 139 109 0.68 214 2.60 1014 113 62 16019 121 1.77 54315 0.45 12 593 158 28 1.59 204 2.67 79 0.52 1311 7115 493 109 278 541 0.48 459 3.86 15.28 14 48113 543 171 2.26 206 0.83 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 52 0.494 0.73 -14.041 1.49 -15.682 7.32 0.42 -21.712 0.49 7.85 -10.20 -15.731 0.62 -17.762 -0.61 — 3.65 7.52 -18.282 — 0.92 -13.11 9.181 1131 -9.20 0.56 7.45 -17.14 —4 3.99 6.09 -9.93 0.74 -16.802 2.67 8.80 1.25 2.83 -16.423 -8.15 2.72 1135 — 0.89 8.24 1501 -10.20 -19.153 1.72 2.24 1459 -17.592 2.13 10.04 1504 — -9.38 1.19 2.68 -19.682 -10.57 0.24 9.06 -20.811 4.49 1489 10.43 974 0.65 -14.661 — 10.53 926 -0.01 5.25 -9.71 -11.76 -17.104 1191 -10.93 -15.20 0.78 7.03 2.172 2.54 2.69 1218 0.78 8.52 -15.583 2.54 7.80 -9.02 0.63 -17.64 1340 2 1507 -9.66 1975 1.75 -16.092 -9.89 1.73 — 3434 8.64 0.56 -20.712 1.74 8.16 1.54 2.45 -10.17 -16.122 11.03 1055 0.49 -17.50 —9 1227 -9.67 -12.19 2227 1.71 4.62 -14.69 -0.23 — 6.70 1.17 -18.09 1.38 1.52 -13.72 7.18 1273 911 6247 3 — 2935 — — 6.94 -9.404 0.20 -10.92 3.123 4.79 2.42 1.44 -13.602 — 3.03 1.39 1461 1349 -17.20 1470 2 0.44 6.81 3.88 -18.274 1017 9.34 0.64 -15.422 -9.71 0.51 9.67 -11.17 -12.392 764 7.65 0.38 -14.27 -12.13 3.382 3.23 6.58 1.39 -17.082 -9.42 7.34 2.86 1.37 -19.974 1059 -9.56 8.12 1.40 -19.44 1.51 937 10.46 -9.97 1.56 1324 -20.28 1.752 10.19 -9.29 -12.17 -19.02 1.833 1994 10.48 -10.30 1.07 2.968 2.19 -11.68 861 1.55 1022 -17.722 3.08 — 1.03 3844 -21.15 1075 3 2.72 0.81 3881 -14.271 11.02 — 1.56 — -15.914 3831 -11.94 0.36 -21.125 — 1.04 3.20 8.22 -16.52 —5 1.71 11.06 0.02 -17.491 -9.92 -11.17 0.60 7.85 2.73 -14.32 6766 — 888 0.35 9.21 -15.98 2.26 1.82 -9.11 7.12 3.31 -14.45 -10.67 958 -10.24 6708 4.40 1294 — 7.22 2.60 950 2.84 1152 -9.34 2113 — 1076 2.83 2.80 2103 1293 / 1142 0.5413 0.09 -13.76 0.66 -13.47 7.14 -18.36 — -9.53 — 3.47 — — 1166 2.78 2.73 995 1309 60 0.49 -15.06 — — 3.13 1059 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± ± km 4933501 1124 4344395 1063 + + 292 920 + . (J2000.0) [log] [log] [log] [log] continued 11 59 43.30 53 36 38.90 PGC 2445913 1132 11 59 57.7012 00 23.10 49 33 49.80 -01 05 51.70 2MASX J11595776 12 01 10.40 NGC 4030 -01 17 41.5012 01 44.30 UGC 700012 01 44.20 62 19 47.00 05 49 17.00 UGC 700912 02 42.20 CGCG 041-023 01 58 36.50 1481 NGC 4045 1495 12 04 1340 20.00 1126 12 04 20.30 01 34 03.30 -01 31 49.00 UGC 705712 05 31.00 UGC 7053 1961 50 31 43.80 NGC12 4088 07 36.30 02 41 43.2012 08 11.10 NGC 4116 6242 12 02 08 52 24.20 41.80 1473 NGC 412312 03 08 00 42.30 47.9012 08 47.30 ASK 075814 3612 48 09 899 09.90 01.40 2912 18 09 17.20 10.00 UGC 7125 2912 15 09 00.30 31.20 NGC 4131 2912 10 09 1343 36.80 49.10 NGC 4132 4312 40 10 52.40 09.20 NGC 4134 43 14 04.80 NGC 413812 39 10 53 21.06 41.20 1286 UGC 7146 NGC 414512 39 10 12 880 49.60 52.10 ASK 505224 39 28 22.10 1069 3709 NGC12 4156 11 27.50 3998 3822 02 55 34.60 999 1077 UGC 7185 958 901 6780 1328 12 04 04.50 28 58 58.20 KUG 1201 – 1 RF 1 F F 1 1 3 3 1 1 3 1 3 1 N NRF F NF N NFA NP NC A NF NZ NRF N R RF C C C C C C C C C Table A.1. Source1475 RA Dec Name 1479 1481 148214831484 14851486 12 00 47.401488 12 01 10.50 -031489 25 12.301492 12 14 01 06 22.30 13.50 PGC 1572451493 12 01 23.70 NGC1494 4019 02 11 08.301495 13 24 03.601497 SHOC357 12 02 12.201499 NGC 4037 12 02 37.101500 62 08 13.901501 12 64 02 22 50.70 35.301503 NGC 12 4041 03 22.901504 UGC 1492 12 7020A 48 03 38 40.10 10.301505 12 43 04 44 04.30 39.101506 NGC 1536 4047 02 38 28.301508 2MASX 12 J12032304 04 04 48 11.90 47.101509 UGC 12 7035 04 974 12.50 ASK1511 173171 62 30 928 19.301512 00 48 09.301515 IC 0758 12 04 33.401517 PGC 1175879 1204 12 05 1500 19.901519 64 26 15.501520 -00 28 12 48.70 05 36.001521 NGC 3429 12 4081 06 38.70 PGC 11422951526 12 41 06 17 41.70 21.901527 1228 66 2241 18 34.101528 ASK 12 39 498950 07 00 41.30 33.301529 PGC 12 4567536 07 46.11 2934 ASK1530 533228 39 22 45.901531 1276 12 43 08 07 20.00 34.80 PGC1533 4102605 NGC1535 4117 12 02 08 30 24.50 19.90 1371 1537 1506 ASK1538 75810 41 24 04.801539 1035 1180 ASK1541 3492581543 966 1545 1067 1546 1547 12 10 07.991552 947 1553 12 35 10 52 1995 35.70 39.401554 1555 NGC 1039 4148 12 11 10 45 54.50 38.90 12 11 19.90 IC 12 3028 39 11 45 21.80 26.50 01 29 32.20 NGC 12 38 4145A 12 32 10.90 23.50 UGC 7184 PGC 2807146 02 52 55.70 ASK 76169 6742 1285 1147 1071 2117 2095

Article number, page 40 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.230.28 6.20.40 5.80.43 55.8 9.00.73 105.7 6.0 7.90.39 8.47 4.70.55 9.20 19.9 11.2 7.650.78 54.4 0.44 7.60.46 0.61 39.2 9.34 0.89 109.8 9.80.60 10.7 -0.93 9.43 9.340.11 9.19 17.5 6.50.48 24.5 -1.13 -0.38 4.50.32 0.29 9.81 32.4 11.4 9.180.17 -0.78 3.5 5.60.30 72.8 9.11 9.18 4.50.37 12.5 7.52 -1.20 9.050.20 5.3 6.4 6.90.20 21.4 1.34 9.05 7.78 9.10.32 29.5 8.94 8.92 9.10.31 -0.94 10.7 8.60.35 36.1 2.42 0.40 7.94 7.60.61 20.6 11.4 7.56 8.420.21 -2.04 8.2 8.81 8.30.60 14.5 0.66 1.05 4.90.21 -0.33 16.2 8.59 8.44 7.40.09 7.3 5.20.24 9.59 0.29 0.49 26.1 6.70.24 13.3 -0.41 8.97 9.10.56 8.70 9.7 7.70.13 8.65 8.97 10.1 -1.61 6.30.21 13.3 7.28 -1.41 4.40.13 8.55 15.3 3.00.41 7.89 0.85 5.1 5.1 1.87 0.32 9.38 23.0 -0.15 4.10.27 52.3 7.98 -1.20 5.5 57.70.32 7.32 108.2 4.40.18 1.48 7.81 8.95 3.4 -0.38 0.12 25.0 9.13 6.60.34 0.61 8.95 8.8 -1.27 6.1 34.40.35 8.14 4.20.49 10.6 7.81 8.27 4.20.35 -0.73 8.3 7.10.32 7.71 61.8 7.81 1.28 5.80.25 16.9 7.73 122.2 4.7 7.71 0.36 8.11 4.20.27 -1.35 8.60 12.4 9.50 6.80.29 -2.07 -1.18 4.1 4.2 18.1 9.50 0.40 8.26 5.30.45 7.36 8.66 8.2 5.5 -0.46 0.74 19.8 8.40.24 -0.60 0.97 10.4 21.6 8.17 38.2 16.2 8.31 10.19 22.9 1.05 9.32 25.7 -0.57 0.54 9.95 -1.60 8.96 -0.71 -0.53 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 891 768 42 158 1115 2221 80 177 1.12 3361 256 26.24 243 1.03 3 355 2383 2.96 267 3733 3.58 257 2575 9.42 399 338 37.65 1 282 69 8.78 354 379 7.10 4 4.41 88 4065 126 21.94 3 0.36 3441 162 44 3673 52 3.69 5 2.09 648 55 756 0.91 46 292 3.94 745 44 85 3374 1.46 161 2.44 4 6.09 66 40 1875 0.59 525 1.73 62 3379 827 0.36 98 3622 1.29 99 1141 49 5.44 340 117 0.41 362 74 378 0.51 1 389 14.42 0.37 5 21.46 637 422 91 2591 75 310 3.35 279 2536 0.63 3235 1.28 2766 59 5.25 212 26.41 1254 77 2551 142 498 0.59 4 3.92 3802 0.91 524 438 407 99 5.69 469 10.76 10.90 124 3.53 / HI 5233 60 45 184 151 0.64 11 0.44 112 19893 3.22 116 58410 4.57 43 108 1.32 2320 88 331 16015 378 0.86 162 1.19 20418 1.40 113 17218 1.13 120 185 1.30 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 34 0.092 0.62 -13.735 1.23 -17.554 6.76 1.86 -19.823 8.59 1.01 -19.754 10.27 -8.80 1.00 -19.194 10.56 -9.73 -11.16 1.26 -17.213 3.31 -10.03 1.32 9.72 -20.742 3.28 2.92 1.34 8.90 -19.21 -11.643 10.59 4.21 0.45 951 -19.843 1120 3934 -12.40 2.30 2.55 -13.812 10.31 — — 3949 0.73 -18.432 4.28 -11.03 0.57 6.18 2207 -16.752 3.69 0.46 -17.422 — 3.48 — 3894 1.52 8.72 -17.424 — 0.25 6.52 926 2.99 -18.343 -10.89 2465 0.51 8.52 -14.323 — 1.30 -8.85 0.80 9.98 2.56 -13.793 2112 -9.34 0.96 6.90 2.57 -18.983 -12.83 1.54 -0.02 1373 1399 7.37 -15.562 2.54 -9.22 1.17 -17.51 9.14 2.06 6424 -10.66 1030 2 -0.14 8.30 -19.494 2.63 7.95 2182 -17.26 1.48 2.502 10.00 932 — 1.15 -19.52 -8.44 — -10.68 0.17 914 1182 -19.75 —2 2.45 10.32 4.11 -13.352 3.92 3.63 10.06 -11.87 0.65 2022 2 -10.33 1.56 6.44 — -16.293 1524 2345 2.69 3656 0.42 -20.071 1.69 -8.62 2.78 0.82 8.04 -15.28 1731 3 10.58 0.27 -14.425 1.21 -9.61 2316 -10.24 5698 6.50 1.60 -14.812 7.71 2.07 -10.02 -17.93 2.52 3.20 1053 7.20 1.07 -10.15 -17.825 1.36 1101 -16.85 10.40 — -8.96 -0.06 3039 2.084 -11.12 -14.41 8.87 2191 1.602 1.37 —4 924 1.73 6.99 -9.90 1.68 -17.372 1888 1.59 2.25 -18.752 -9.57 2.30 1143 9.08 1.59 -17.783 10.18 0.85 2.03 1822 1137 -10.81 -19.416 -10.57 0.04 9.78 -17.013 1.30 2.56 -13.04 -13.28 1069 9 2.29 — 8.72 0.22 -17.972 6.39 2.93 0.77 906 -15.183 -9.98 1444 9.25 1.55 — -14.982 -8.85 7.13 1.56 1252 -10.31 -20.57 2.602 2.25 7.77 1.46 -20.74 3.07 10.76 -8.62 2.46 0.65 1833 -10.02 -20.53 10.92 -10.90 1570 -19.61 2.44 10.66 -11.60 895 2.34 1547 1.92 -11.92 9.49 1841 2.39 1808 -10.05 3.74 7545 2007 2.28 4133 2320 1 0.28 -16.87 8.03 -9.10 2.34 2341 / 15 -1.30 -14.78 6.68 -9.56 2.9014 2384 1.6310 -17.74 -0.08 -14.91 — — — — 1.79 1.51 1042 1294 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± km 310 1098 + . (J2000.0) [log] [log] [log] [log] continued 12 12 20.6012 12 26.90 2912 12 12 36.90 31.90 29 08 57.10 NGC 4173 29 09 58.70 NGC 4174 NGC12 4175 13 45.10 13 25 26.5012 15 47.80 NGC 4189 47 05 00.20 NGC 1129 4217 4025 12 4109 17 04.20 10 00 20.00 UGC 7307 2103 12 19 12.5012 19 22.20 -02 47 1174 44.90 06 05 UM 55.20 49012 20 33.90 NGC 4260 02 58 03.80 VCC 1189 42312 21 07.0012 21 32.80 0012 27 21 40.80 42.50 14 36 22.20 ASK 570 14 35 5703 53.90 NGC 1776 4298 NGC 4302 2387 12 22 38.5012 11 22 48 54.60 03.30 NGC 4313 15 49 16.4012 23 1894 15.10 NGC 1124 432112 23 23.40 1098 1112 21 23 49.50 30.00 0112 48 23 54.20 41.58 NGC 4330 02 00 29.10 ASK 7645312 02 23 57 58.80 40.50 FGC 1424 UGC 7464 48 46 46.10 1431 NGC 4357 1474 1481 1887 1814 7533 4120 12 22 03.9012 09 22 02 08.20 05.60 NGC 4307 15 47 56.40 VCC 530 962 1301 – 1 1 F F 1 1 1 1 1 1 3 3 3 1 NC N NRF N N NU A NC NC NFA NFA NRPF NRF NC R R C C C C C Table A.1. 15591562 1564 1565 1566 12 12 17.1015681569 39 15 29.601571 ASK1573 507259 12 12 32.301577 12 13 16.901578 12 12 13 07 22.20 25.701579 43 41 54.901580 IC 12 0769 28 13 30 53.60 39.501582 NGC 12 4183 15 18.901585 NGC 4185 13 10 22.201587 12 02 15 55 56.30 37.301590 NGC 12 4193 15 58.50 952 1592 PGC 12 4103522 14 16 25 00.40 58.901599 12 02 16 02 11.71 22.001600 IC 12 3077 04 16 39 38.70 03.501601 ASK 76013 47 52 59.701602 -01 VCC 27 12 172 06.60 17 07.901606 NGC 12 4220 2210 19 05.10 ASK 918 131321613 12 3887 03 19 40 09.90 56.201618 12 04 19 39 12.20 42.401619 NGC 1365 03 4234 2463 51 23.501620 VCC 320 49 21 16.701621 UGC 7354 12 19 52.601622 UGC 7358 12 20 25.801624 6410 1413 27 37 15.601625 12 33 20 14 35.50 31.70 2196 1626 NGC 12 4275 20 916 47.50 917 ASK1627 12 506495 30 20 47 54.60 48.701628 12 58 21 05 06.10 33.00 KUG1631 2014 1218 03 24 09.60 NGC1632 4290 11 35 43.10 2347 ASK1633 1538 76564 VCC1636 3647 453 12 21 57.801637 1638 12 02 22 20 06.10 42.301641 2304 1046 VCC1642 513 12 39 22 44 26.30 52.301643 ASK1645 507390 12 29 22 12 42.20 32.501646 3018 2192 NGC1648 4310 12 09 22 19 56.60 56.901649 12 23 07.99 937 NGC1650 4316 02 44 49.001651 53 01 20.20 VCC1652 597 ASK 187265 1830 1060 12 23 53.90 -03 26 12 34.50 24 01.50 918 NGC 4348 12 12 17.10 1251 NGC 4351 1834 894 2004 2302 Source1557 RA 12 12 14.70 00 04 20.20 Dec Mrk 1313 Name 2347

Article number, page 41 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.710.33 5.80.43 14.50.52 12.4 5.10.31 24.7 4.30.39 9.72 11.4 8.33 8.00.22 12.0 -0.65 10.11 5.00.21 2.27 16.1 4.10.44 21.3 -1.14 7.86 3.50.37 8.98 8.43 9.3 4.90.49 -1.68 17.7 8.98 5.10.24 16.9 8.43 17.4 8.110.17 33.6 7.96 5.40.88 38.0 -1.94 9.63 5.2 9.350.38 -2.00 10.5 10.06 -0.51 6.50.29 -0.75 6.8 -0.58 8.10.25 19.4 38.4 7.770.13 11.0 8.28 2.9 9.590.31 93.2 -0.62 4.20.33 -1.14 8.20 -0.41 2.9 9.61 4.30.34 8.4 2.7 0.19 0.26 -0.55 76.9 7.51 3.20.26 12.6 156.1 7.08 7.00.21 -2.24 7.60 8.00.34 8.88 9.25 0.61 10.3 7.00.36 18.6 7.60 11.8 -1.30 0.28 0.14 8.07 6.4 8.90.36 34.7 8.26 10.3 -0.20 0.38 14.5 8.05 8.96 5.3 2.18 0.34 15.5 52.00.37 -0.10 8.88 29.6 0.22 10.8 128.8 8.400.77 30.0 -1.43 0.12 47.5 -0.32 9.75 9.20 9.0 50.90.37 -1.18 8.81 3.9 -0.86 0.25 10.6 15.9 9.160.17 30.4 0.48 3.0 20.90.34 -0.12 8.50 3.70.50 39.0 14.3 7.15 8.78 8.50 0.28 40.6 8.36 3.90.42 22.9 -0.83 7.15 13.50.30 66.9 11.3 8.36 7.28 8.410.26 20.1 8.6 9.020.40 20.3 -0.97 7.28 7.4 9.040.42 16.5 12.0 9.02 8.540.13 20.0 14.1 0.90 0.50 32.7 8.23 -0.90 3.70.15 38.8 8.03 27.5 -0.77 8.710.38 4.5 8.72 4.8 0.92 0.38 68.7 -1.01 34.00.44 -1.03 38.1 7.02 9.80 5.10.89 63.3 8.6 69.8 -0.16 13.5 9.80 7.44 8.76 19.0 9.14 36.3 -1.87 2.71 9.29 0.13 9.79 -1.03 -0.59 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 55 919 265 1455 354 281 4.23 1225 4063 1.63 164 1701 3.08 3314 4.68 184 3085 350 372 0.68 3253 73 4.96 4286 7.88 258 11.67 1 95 172 282 3085 0.90 202 10.74 7 3392 41 2.53 229 16.70 1 2992 57 244 168 316 101 0.19 9 0.63 1923 2.68 114 32.55 31 1323 1.63 8 74 1821 96 216 0.81 1 6.64 284 1231 248 1106 314 2.47 1457 2.43 133 161 30.37 2 1721 9.67 35 199 11.36 1844 7.15 45 55 2051 0.19 2 4.83 88 76 4202 102 131 4.85 3 445 2216 124 4.17 185 21.31 1 2412 84 3.29 203 284 5.34 429 1152 2.21 299 460 2.04 3161 8.30 10.16 1 362 1477 191 20.85 4 180 360 210 357 14.00 401 16.35 394 5.22 20.16 / HI 13 34511 400 459 5.45 50121 3.25 99 160 0.57 15 117 17021 0.73 204 244 0.64 10 6510 121 221 1.50 267 3.14 10 104 131 0.39 2211 39 144 94 177 0.27 0.46 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 32 1.543 0.87 -19.432 1.49 -19.005 10.38 1.52 -22.074 -12.71 6.06 1.25 -17.763 11.25 0.78 -20.985 3.87 -8.18 -11.74 9.54 1.41 -17.763 1.36 4491 -12.21 -20.483 2.96 2.14 — 1.45 -18.783 10.05 — 1.26 3.36 -19.16 9046 2 1020 -11.34 1.54 9.96 -19.62 —2 10.14 0.82 — -20.464 -11.27 10.10 956 1.92 -11.43 0.73 1.68 -16.374 10.65 -12.15 1.11 3.30 1.68 -19.13 2176 4 2.57 -10.81 1.34 8.39 2525 -19.703 2.21 0.88 9.42 1098 -17.35 1678 2 10.00 2.61 -9.75 4220 1.29 -16.86 -10.01 -0.42 2437 -10.71 8.01 -18.484 2.64 10.16 4540 -14.57 1.373 5.68 -10.20 1.36 9.753 — 6.47 1162 2329 0.73 -19.46 -11.113 1.69 2735 0.80 -19.37 2.91 -8.222 10.18 0.30 1.71 -16.272 2247 -10.48 9.11 0.60 1.85 -16.174 1146 1026 8.27 0.61 -16.792 2.04 -9.70 6.08 1.34 -10.35 -17.29 1137 3 0.81 8.15 -19.15 2.673 2421 -8.51 2.61 8.74 1.36 -17.963 10.31 1.48 -21.634 2.59 1062 — -9.72 -12.40 8.72 1.01 1224 -18.623 10.93 0.90 1594 -16.23 2.68 2.75 2.40 10.06 -9.92 -11.14 0.57 -19.193 -10.41 8.33 -16.75 2248 2.69 1705 1696 2.50 9.27 1.444 2.32 -9.88 -10.10 -18.413 1448 — 6925 1.07 3.216 1042 3.07 9.61 0.58 -15.629 1.39 — -10.96 -19.996 1179 0.61 1619 -19.454 — 5.88 2.82 9.37 1.36 -16.384 1.21 -17.564 — -9.57 0.53 8.14 1617 -16.34 —5 963 1.37 9.44 -13.987 3.23 -9.80 1.49 9.01 1.64 -18.40 -11.05 —4 0.69 7.11 -18.80 -10.506 2.68 1127 1001 9.72 1.61 2.94 2.58 -13.511 -9.53 1.48 9.76 2.24 -10.90 -19.424 2642 7.18 0.23 1155 1007 -17.072 2.62 0.78 2.50 1269 -15.863 — — -9.88 1.47 9.31 -17.37 1052 1.37 6.06 1130 -19.41 -10.75 2.10 1.49 9.01 -20.05 — 10.32 -8.62 1.25 -10.14 10.38 1038 893 -10.71 2.82 3.02 1114 -11.12 2.81 2.39 2493 4.85 929 1321 2783 2510 / 30 0.77 -16.46 — — 2.13 1144 27 0.4115 -14.59 0.44 -15.79 — — — 1.71 — 3.06 1244 990 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± km . (J2000.0) [log] [log] [log] [log] continued 12 24 11.30 58 21 38.30 NGC 4362 4505 12 24 36.4012 25 00.50 39 22 55.1012 28 25 33 46.70 30.90 NGC 4369 NGC 437512 12 26 39 54.61 42.7012 28 43.30 -00 NGC 52 4388 39.40 14 59 NGC 58.20 435512 31 22.90 IC 3392 29 08 11.30 NGC 1012 4495 9039 12 36 32.70 2585 11 15 28.7012 39 04.70 2123 NGC 4567 14 43 52.00 1668 12 39 50.30 IC 361212 40 02.90 4569 0112 40 40 21.40 08.70 -01 03 02.80 UGC -00 7824 2112 04.80 41 ASK 12.20 1643 6dF J1240088-00210412 11 41 53 44.50 11.90 2271 12 43 56.60 NGC 4607 35 03 45.90 13 07 36.00 NGC 461912 45 1313 32.00 1707 NGC 465412 46 49.30 1312 19 47 57.30 45.60 1221 0312 00 48 22.60 00.10 1593 IC 3742 1312 45 47 46.10 59.80 CGCG 043-022 04 26 03.30 NGC 468912 04 48 41 23.40 41.50 CGCG 2244 043-029 CGCG 043-03012 08 49 29 50.20 03.60 6923 NGC 1048 4698 02 51 04.50 1190 UGC12 7982 53 28.50 1025 12 02 958 54 10 40.61 01.10 1604 1023 NGC 477212 28 54 56 51.10 19.20 NGC 4793 02 39 14.70 1039 NGC 4809 1153 1028 2491 976 – PF 1 3 1 3 1 3 1 3 2 1 BC NF N NZ F F NF NF N N NC NRF F R R R RF C C C C C C C C Table A.1. Source1655 RA Dec Name 1657 1659 16621665 16661667 1672 12 25 22.2016771678 12 10 25 01 50.70 00.501679 NGC1681 4380 10 27 32.601685 12 30 20.701687 NGC 4390 12 30 26.801689 03 44 24.501691 12 04 32 14 33.50 47.601694 UGC 12 7644 33 56.701695 NGC 12 4480 09 34 10 34.14 25.101698 12 15 35 21 36.60 17.301699 UGCA 63 284 31 30.201700 IC 12 0800 03 37 02 948 48.40 04.201704 NGC 12 4545 38 06.90 NGC1706 1089 4544 05 22 06.601707 12 10 39 09 12.40 56.00 NGC1709 12 4580 39 18.70 VCC1710 1744 4210 06 00 44.20 -001711 31 2429 55.00 NGC1714 4577 NGC 4592 1144 1718 12 41 11.6017201721 2330 2743 12 01 41 24 22.90 37.001722 1120 -03 UGC1725 03 7841 28.101728 1035 12 44 CGCG 28.80 014-104 1137 1729 12 45 31.991730 00 28 05.00 -00 2431 1731 32 08.60 1065 UGC1732 7911 NGC 466817351737 1740 12 48 13.70 1461 1692 17471748 -03 19 12 58.20 49 25.701749 NGC 46911750 12 04 50 23 38.90 33.101752 12 52 59.101753 PGC 1176 12 1267592 01 53 27 21.20 1624 52.201754 14 24 01.901755 UGC 12 7991 01 53 16 40.20 08.701756 LSBC D646-051757 NGC 4771 12 04 54 04 44.20 32.20 ASK 175666 12 13 55 14 12.60 14.10 1126 12 55 15.50 UGC 2643 12 8032 00 55 06 21.90 59.90 02 53 47.80 UGC 8041 58 20 1050 38.70 NGC 1268 4799 NGC 4814 1125 902 1116 1319 2779 2490

Article number, page 42 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.200.24 7.50.51 13.10.48 4.3 8.5 17.20.29 4.20.14 42.0 7.58 8.14 9.90.33 4.6 7.90.20 61.4 7.58 8.14 9.58 4.10.25 23.0 8.09 8.510.26 4.8 -0.76 3.70.35 6.6 43.3 -2.20 61.9 0.84 7.290.37 22.9 111.5 7.73 8.99 4.10.13 25.6 0.37 0.35 48.3 8.82 1.62 0.93 8.00 3.90.11 35.3 9.9 8.830.31 2.53 -0.67 3.9 8.89 3.70.26 67.7 16.1 8.83 0.31 14.7 2.87 6.95 114.9 5.70.23 8.47 13.10.68 19.4 18.4 0.25 9.27 7.13 1.27 0.43 20.4 7.7 8.360.42 23.8 9.27 7.13 5.2 8.420.38 15.9 13.7 0.55 8.080.22 0.71 7.1 7.20.63 24.9 9.24 0.38 6.00.39 10.7 10.32 13.5 7.98 -0.37 0.32 4.0 -0.85 7.80.57 21.1 9.58 12.4 0.36 0.37 7.55 -0.08 9.37 6.9 7.90.32 21.9 10.50.29 0.36 0.45 13.4 9.45 4.3 9.420.37 17.9 17.50.37 -1.45 9.88 9.42 5.2 9.79 6.50.57 33.6 19.9 -1.18 0.66 -0.92 8.05 6.1 9.52 5.90.34 36.8 92.60.33 -0.05 0.32 14.5 234.3 7.90 4.3 8.620.47 11.0 10.270.13 -0.59 9.55 0.91 7.40.26 4.6 19.8 -1.10 3.90.24 9.55 14.2 8.41 7.5 8.370.69 18.1 3.30.38 -0.51 9.64 10.0 0.83 4.70.30 23.4 21.2 6.93 -0.38 0.47 7.94 5.0 8.17 3.70.31 44.1 11.4 6.93 0.43 0.30 15.3 10.3 1.08 9.41 8.650.44 22.5 17.90.14 27.5 -0.40 9.58 10.11 0.57 7.50.36 35.0 8.0 -0.74 8.59 9.58 0.24 22.9 11.8 9.26 19.6 0.24 8.5 40.7 8.95 0.92 7.85 13.2 8.74 0.24 1.75 8.09 0.50 0.14 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 239 47 73 5831 60 1003 610 0.98 68 2.31 1 3.27 50 100 1311 62 9.38 1 1592 0.38 86 190 5.17 143 1374 220 14.85 180 100 10.27 11 7.62 129 11722 3.25 68 140 1118 20.90 90 85 132 2383 1163 2.94 3.81 282 131 3.19 3095 5.62 1695 329 2103 6.29 4746 3.36 252 1305 490 440 7.97 160 1552 2.05 4719 4.22 191 1866 4.92 1364 4.05 211 1141 168 658 6.13 196 4353 1.28 6783 6.81 462 1197 5.51 313 96.82 4 1482 59 333 70 3.78 2 55 4.28 786 92 1663 0.23 82 328 1.47 2 200 455 3.03 2 352 1328 9.99 486 1414 2.01 159 1711 6.84 172 73 5.02 212 140 6.26 3.04 98 157 1.59 8.96 / HI 17 44142 49012 70 2.33 188 40 0.87 15 7020 0.50 43 45 84 0.23 9822 0.28 8711 167 39 1.46 8613 0.76 108 146 1.18 21 123 185 0.83 22 190 264 1.45 11 71 137 1.49 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 24 -0.093 -14.52 1.641 2.28 -22.265 0.78 -17.89 — 10.34 0.55 -14.444 10.30 -13.302 -12.01 0.22 — 7.67 —3 0.69 6.92 -16.352 2.33 2.59 -9.74 1.06 2.24 -17.391 -9.42 1.01 8.06 -18.072 1063 3.07 1113 0.53 8.68 4935 -19.073 1.88 -9.26 0.03 6.29 -16.78 -9.55 0.19 849 -13.981 1.72 — 1033 -8.71 6.03 -14.693 3.17 6.70 0.36 -10.193 2.38 1988 7.19 0.56 2047 — -17.252 -9.03 0.48 2.99 -15.865 -9.33 0.44 2.56 961 -15.621 1.53 — 1.08 7.82 1461 -15.203 3.34 0.55 7.71 1172 -18.72 -10.003 904 1.51 7.70 -15.092 — 1361 -9.93 0.75 9.61 3.04 -21.823 -10.45 0.41 7.62 2.79 -19.76 -10.183 2.94 11.18 0.60 2.35 1278 -14.66 -9.58 -12.39 1.67 9.65 4.39 -18.24 1360 2 1200 7.19 -22.203 3.58 3.57 881 -9.76 8.91 1.49 2543 2 10.91 -9.50 1.42 1187 -21.464 2.31 -9.69 8329 -12.10 0.54 -20.878 2.58 11.06 0.87 -15.393 4.30 10.70 1.95 4837 -12.38 0.88 -19.375 965 -10.31 1.20 7.73 -12.785 2465 2.85 5373 1.65 9.57 -17.732 2.97 -9.57 1.82 6.99 -21.76 -10.541 5652 0.76 9.22 -19.165 2.89 11.37 -9.85 5613 0.24 2.20 -17.76 -9.97 -11.79 1.46 1402 -15.814 3.07 — 8.92 3365 -18.743 2.87 2.40 0.53 7.543 -10.40 10.03 1131 0.19 -14.962 — 1132 -8.92 8363 -10.60 0.94 2.68 -15.073 0.46 7.51 3.29 -19.443 2.89 2.80 2529 1.49 7.09 -16.602 -9.49 1.39 9.80 -21.192 -9.39 1134 871 4622 8.08 0.62 -21.04 -10.023 2.89 0.44 -16.467 2.88 10.85 — -9.47 0.60 4.65 -17.152 1112 -11.59 0.33 8.35 -17.513 2.92 1011 6030 0.53 8.33 — -15.41 -10.32 2.32 8.71 0.76 -16.85 -10.55 1.75 6.10 964 2.64 -15.34 -9.90 6237 8.24 2.49 7.94 6245 1261 3.26 — -9.44 2450 -9.97 1.57 3.09 2476 2.22 1129 964 1301 / 23 0.79 -16.34 6.11 —69 2.60 0.57 1135 -14.37 — — 1.22 985 25 -1.64 -13.93 — — 1.53 881 64 0.39 -14.47 — — 2.78 893 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± 100 0.13 -16.27 — — 2.78 3600 V ± ± ± ± km ± 3456110 929 + 09-21-092 1356 07-27-055 1124 + + . (J2000.0) [log] [log] [log] [log] continued 12 57 59.5012 58 01.20 -03 3712 16.90 59 13.30 01 34 NGC 33.00 4843 34 56 10.60 NGC 4845 2MASX J12591328 13 01 03.70 -01 57 12.2013 03 44.20 UGC 5134 812713 04 31.20 1108 02 02 23.10 -03 3413 20.60 05 18.80 PGC 135818 UGCA 322 36 06 10.40 IC 417113 06 45.20 1467 35 06 02.0013 08 50.10 UGC 819913 970 09 06.50 -00 49 02.30 1373 05 14 2MASX 35.10 J13085009-0049018 ASK 176668 1201 13 5379 11 15.80 36 59 11.4013 13 27.10 PGC 4891 4574306 36 36 07.00 3605 NGC 503313 16 35.84 1041 03 03 51.7013 17 58.70 CGCG 044-04813 18 45.10 04 24 12.20 1081 41 56 58.70 IC 087113 20 32.10 UGC 836513 05 20 24 44.60 29.10 UGC 8382 43 6032 03 37.50 PGC 3084928 6218 1247 973 1311 12 55 26.90 32 59 04.90 PGC 166149 932 – 1 1 1 1 1 2 3 3 1 NC NC NZ NRUF A NZP NRF F NUF NZ RF R C C C C C C Table A.1. 17591764 1765 1769 1772 12 55 38.901775 -001776 15 53.601777 UGC 80481778 12 59 52.401780 13 00 17.501781 13 03 00 37 24.99 58.501783 -03 13 03 00 58.90 34.901784 ASK 13 176173 13 00 40 39.20 13.10 PGC1785 4473 13 64 00 26 58.10 49.601786 UGC 8114 02 30 02.60 -001787 UGCA 01 13 317 30.10 02 40.80 NGC1790 13 4900 02 55.70 NGC 1111 49041791 01 04 26.801792 55 41 40.101793 UM 538 13 04 31.801794 MCG 1040 1795 -02 59 13 16.90 05 1134 24.601796 13 05 24.90 PGC1800 1078534 2009 13 32 05 54 41.50 00.301802 2089 13 56 06 19 04.40 21.901804 UGC 36 8181 01 961 02.80 1190 1806 NGC 13 4964 55 06 39 56.10 21.901808 IC 13 4178 08 37.601810 NGC 4977 14 48 26.601811 54 04 903 27.701812 CGCG 101-001 13 09 33.10 1278 1813 UGC 8231 13 09 47.501814 13 01 10 40 45.70 23.001815 13 28 10 54 56.50 25.001816 NGC 4999 58 09 897 24.801817 NGC 2535 13 5000 11 11 28 31.20 38.501819 ASK 13 215211 12 06.301820 UGC 1190 8306 8255 36 16 55.601821 969 13 46 14 11 06.50 46.101822 NGC 13 5014 14 10.801823 NGC 2461 13 5021 48 14 09 53.40 22.501824 13 39 15 08 21.50 55.401826 UGC 13 8316 27 16 00 00.60 29.201827 UGC 13 38 8315 5633 16 03 10.60 08.001828 UGC 8325 40 5592 58 1411 09.801829 PGC 13 2116640 25 16 40 52.30 23.201830 MCG 13 3365 17 16.60 PGC1831 4362343 12 32 53.601833 06 1135 02 17.30 NGC1834 5058 8441 13 18 46.70 NGC 5060 13 20 18.60 2525 27 43 56.10 1147 13 50 20 43 38.70 13.30 912 UGC 4628 8363 UGC 8386 09 47 10.00 988 UGC 8385 968 6241 2436 2486 1102 Source1758 RA Dec Name

Article number, page 43 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.490.51 10.40.51 5.10.32 21.3 6.80.38 10.1 5.4 9.150.42 60.0 13.80.40 9.68 9.15 127.9 9.2 9.20.39 8.92 -1.30 9.60.55 14.9 9.12 16.0 8.980.21 0.69 18.9 7.10.32 31.7 -0.62 0.22 9.41 5.00.46 9.29 14.7 -0.04 3.4 9.330.57 -0.93 10.23 8.2 7.00.51 0.22 6.0 3.30.43 -0.85 21.5 19.0 9.250.43 26.0 11.9 8.62 10.100.15 44.2 12.1 3.02 10.020.37 48.0 -1.22 -0.98 22.9 8.980.41 23.0 -1.19 5.6 8.850.55 30.2 -1.11 8.0 8.640.23 11.4 8.85 8.10 8.50.40 17.6 12.4 0.65 26.20.19 15.4 8.10 8.16 20.10.79 8.35 9.39 4.00.40 34.5 0.51 18.5 8.10 0.72 0.13 25.5 0.10 9.280.82 4.3 28.6 8.10 4.40.40 41.7 -0.81 12.6 10.53 8.230.50 51.0 8.91 -0.76 4.0 22.70.68 -1.16 27.4 115.20.29 2.89 7.09 9.24 5.8 10.300.49 61.0 5.40.49 -0.06 -0.57 -0.37 10.21 7.1 9.80.35 7.4 -0.53 9.80.39 16.5 12.7 8.870.48 15.3 9.50 8.10.24 33.3 9.59 0.38 4.70.47 -1.50 9.25 18.5 11.7 9.69 0.45 0.30 -1.58 7.2 9.00.25 31.0 -1.01 8.37 22.90.45 40.1 13.0 9.44 8.490.71 0.83 27.2 6.60.27 63.7 -1.03 9.08 0.50 5.1 8.640.36 11.9 6.2 8.79 0.51 0.45 10.7 0.40 3.40.31 8.91 10.3 8.79 5.40.44 8.77 -0.88 4.6 7.20.24 8.10 50.7 13.0 -0.78 0.22 14.9 9.22 129.3 0.65 6.50.34 9.47 9.50.32 25.9 -1.46 10.2 9.35 8.52 0.61 17.9 5.5 8.27 16.4 9.35 1.17 9.24 0.69 9.22 9.8 0.12 -0.43 9.18 -0.95 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 4 191 22412 6.35 1882 1652 221 3297 180 228 28.98 346 275 4.23 253 4.89 3135 7.70 2 5.17 4991 2232 523 1521 262 1486 4.49 177 13.54 4 54 171 106 12.43 41 92 5.98 81 130 242 117 2.36 4 1.87 53 2752 2.90 1 8.85 87 71 585 135 1002 2.55 6168 155 0.51 258 14.87 1 367 10.11 5 278 658 671 11.63 1849 689 22.46 206 187 19.71 32 4.11 232 2868 1221 3.70 323 2197 137 1361 7.33 245 1851 2.77 1563 44 2.71 221 1227 4.55 2503 3.62 68 141 2668 266 110 4.33 9.52 293 397 3.41 1261 4.74 4162 1.68 2722 1.68 1198 299 1816 141 35.46 78 199 341 3.71 140 2.53 365 2.77 1.99 / HI 1111 38610 149 425 154 200 3.25 191 3.97 1.73 3251 13917 38 251 474 160 0.75 576 0.34 5.36 10 144 25015 6.81 37 8317 0.23 44817 513 294 1.76 380 4.32 1810 374 93 443 124 3.54 1.16 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 12 0.531 1.70 -18.524 0.39 -20.505 0.95 -16.694 10.99 — 0.52 -19.083 -11.52 0.78 8.23 -18.013 1.31 9.60 -18.973 — 2.69 -9.15 0.73 8.90 -19.655 -10.26 1.34 9.44 3.57 -18.63 5555 5 -10.84 3.91 10.22 0.31 2.49 -22.01 -10.082 -10.73 1.16 9.11 2.74 -17.71 2076 2136 3 11.09 3382 1.46 3.37 -19.17 -10.434 2.35 -10.73 6.23 1.63 -21.54 972 1.80 9.84 2.66 3541 -21.392 3.44 11.08 -9.22 2886 -17.93 -11.149 11.21 -12.38 0.55 2388 1 1.48 10.09 8295 -11.11 0.33 2.75 -16.072 2.11 -10.29 0.37 6996 -15.343 2.74 4978 0.32 7.99 -15.46 6980 1 3.40 0.86 -15.782 — -9.56 6940 7.65 0.29 -18.583 1219 7.63 1.27 -14.29 3.543 -9.34 9.29 0.93 — -19.491 -9.14 1.60 -18.542 3.54 1231 10.10 — -9.95 0.37 1.76 -21.552 4.03 -11.15 0.39 9.39 -16.772 3.58 1270 11.29 1.34 1049 -14.37 — -10.222 1264 2.71 -12.78 1.36 6.03 -18.912 2400 7.15 1.52 2.90 2.08 -22.27 2414 3 3.50 -9.49 9.81 0.51 -22.143 10.67 -9.45 1.59 1016 2636 -10.82 -17.453 3.46 10.74 6837 -10.56 0.58 -22.39 1.561 -11.10 5.29 8.49 1.57 -18.813 1.67 11.00 1295 1.55 1042 -20.022 2.07 -9.45 -12.24 9.13 0.40 1762 -21.865 10.83 4284 1.40 -15.36 5.115 1.39 10.70 -9.62 4148 -11.72 0.72 -20.04 -12.39 0.73 7.54 6100 -15.54 3.493 1946 2.72 10.47 -17.035 2.14 -9.25 -11.82 0.34 7.99 2925 4 4659 1.16 8.57 -16.136 3.57 3.33 3719 -9.89 1.39 -19.10 -10.072 0.50 -17.727 2.08 1327 — 4597 1.36 9.80 3.39 -14.371 9.55 1.39 -20.65 -11.783 1188 7.44 0.15 2628 -10.52 -20.07 —2 10.67 1.57 3.00 -15.743 -9.60 -12.28 0.50 4.48 8.85 2.24 -19.083 0.72 7.35 2229 -15.242 2.58 1.92 -9.40 1.03 1613 1162 -19.10 — -8.65 1.37 7.58 -18.58 2.31 1240 4507 9.13 -19.23 3.05 -9.48 9.66 4153 — 10.13 -9.96 2450 2.17 -9.98 -11.68 2.76 1.72 3.13 1.81 1019 1150 3790 3531 3972 / 60 0.73 -17.85 — — 3.48 1086 13 0.62 -16.41 8.24 -10.95 3.96 1446 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± km 5741501 2050 4246450 1276 + + 08-25-002 1263 + . (J2000.0) [log] [log] [log] [log] continued 13 20 52.30 57 38 29.70 NGC 5109 2103 13 21 23.9813 57 21 41 56.40 40.30 2MASX J13212499 38 44 04.90 NGC 511213 23 41.6013 24 00.70 31 38 46.70 09 42 36.70 CGCG 161-04113 26 21.40 NGC 512513 02 27 05 01.20 58.40 978 NGC 5147 10 03 21.3013 28 10.10 UGC 845013 28 12.20 4613 4976 40 28 19.60 25.30 0213 16 28 42.50 49.80 NGC 5169 46 35 29.90 PGC 6966 135827 46 15 44.50 NGC 5173 CGCG 246-005 1103 13 30 06.1413 30 11.50 -01 1067 43 14.10 -01 3913 47.20 31 NGC 45.90 5183 NGC 5184 -02 2417 4213 1006 47.00 32 10.4013 2620 33 IC 05.30 0892 2420 6213 46 33 03.90 14.74 -01 02 08.80 NGC 521813 45 33 50 NGC 31.80 13.80 5211 UGC 8538 38 36 19.5013 35 45.50 4300 UGC 8542 3981 08 58 08.60 UGC13 8575 36 07.30 6282 13 36 16.64 2853 51 14 08.90 3701 13 38 37 20 31.99 23.70 NGC 1329 5250 NGC 5243 08 53 32.20 1189 NGC 5248 1162 4501 4337 1048 – 1 1 3 1 1 2 1 1 1 1 3 3 NF NF N NF F N NP F NRF R C C C C C C C C C C C C Table A.1. Source1835 RA Dec Name 18361837 18381839 1840 13 21 23.0918411842 13 00 21 20 36.00 32.6018431844 NGC 5104 13 42 22 16 32.50 57.701845 13 22 55.601848 UGC 13 8400 54 22 49 56.50 05.501850 13 26 23 58 10.50 50.601851 CGCG 13 271-034 28 23 18 40.30 59.101852 NGC 43 5116 05 10.501853 NGC 5117 04 30 55.40 NGC1854 5123 13 24 35.20 ASK1855 177443 13 25 13.901856 5561 06 31 44.801857 13 43 26 16 36.60 02.10 UGC1858 3389 8427 3539 NGC1859 5145 13 42 27 45 02.60 51.401861 13 27 24.60 UGC1862 2884 8449 42 46 49.201863 2389 45 26 18.90 2MASX1864 8291 J13270262 7006 MCG 18651866 13 29 25.901867 13 29 38.701869 6924 13 11 29 00 55.70 28.401870 1226 13 45 30 23 03.60 16.401871 NGC 01 5162 32 38.20 UGC1872 1230 8489 62 30 41.60 PGC1873 135828 13 30 59.60 NGC1874 52051875 13 62 31 01 56.02 27.601876 UGC1878 8514 31 01 58.401880 UGC1881 8517 13 33 20.201883 6811 1884 1293 13 51 1047 35 29 16.18 25.101885 13 35 42.721886 1759 NGC 5225 44 45 41.101887 13 45 35 55 55.20 46.401889 UGC 13 8577 36 01.20 UGC1891 1982 13 8588 35 36 35 02.20 17.701892 49 57 39.001894 NGC 4665 08 5240 11 11.101898 IC 0902 13 36 22.851900 FGC 1642 13 39 38 42 30.60 16.50 4585 13 38 45.43 PGC 13 101496 08 39 26 35.95 32.30 -00 2639 25 13 00.60 40 15.21 1443 UGC 8629 43 03 10.00 CGCG 017-048 38 52 09.50 Mrk 2226 0267 CGCG 218-035 1616 1230 2457 3799 1020 3957 3533

Article number, page 44 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.520.56 5.30.30 22.30.29 3.8 9.20.20 41.0 5.10.41 8.94 3.8 9.45 5.70.14 4.8 6.70.56 -0.70 -0.04 9.28 3.5 5.40.41 8.80 3.5 8.50.42 -1.68 11.7 9.02 3.10.53 0.42 8.61 9.8 7.80.26 21.1 -0.65 7.45 4.70.67 0.04 16.3 9.76 4.9 8.640.54 0.27 9.0 5.90.56 9.00 44.7 3.34 0.59 6.20.12 35.5 23.5 8.63 102.4 0.91 0.13 8.08 5.50.39 78.8 -1.01 9.50 9.99 4.20.39 -0.52 -1.32 7.0 9.48 5.90.28 0.78 17.5 6.00.12 -0.42 36.4 7.29 9.70.41 37.8 7.56 4.20.48 69.7 0.60 8.85 6.7 8.880.26 0.17 6.5 8.90 3.90.80 0.13 13.2 0.53 3.50.24 -0.69 10.2 7.26 5.50.44 8.97 4.3 3.40.14 8.66 32.2 0.81 12.8 -0.67 0.33 9.14 5.8 8.66 0.33 5.8 62.0 9.31 6.30.18 -2.13 8.92 4.6 -1.38 9.76 7.30.43 11.2 3.80.27 -1.51 -0.40 13.3 8.21 7.80.42 8.30 33.9 4.8 24.40.48 2.09 15.1 8.36 0.60 0.38 53.5 9.08 9.65 5.20.34 32.0 0.44 7.0 9.880.40 -0.30 56.5 2.87 9.31 8.40.36 15.8 12.0 9.88 0.38 95.0 -0.13 8.71 5.50.54 30.3 8.85 6.7 9.270.48 31.9 8.71 9.91 9.9 0.05 0.29 -0.35 25.2 12.7 61.50.37 -0.74 9.31 6.40.61 51.3 8.74 9.73 6.20.31 9.31 3.7 9.61 0.39 8.90.59 -0.66 10.8 4.50.23 -0.06 8.61 3.7 4.50.48 9.65 12.6 7.8 -0.51 0.81 12.9 8.89 -1.02 8.2 18.60.33 23.5 9.59 -1.42 23.7 9.48 8.41 6.8 -1.62 43.3 8.94 -1.09 -1.47 15.3 9.85 0.74 -0.86 9.85 0.36 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 19 2308 540 254 158 565 14.23 5 187 1.12 7 47 1.18 3 148 60 149 205 0.25 3 1711 4.79 4611 4.20 4006 484 307 429 10.06 7 37 333 34.69 6 123 27.48 1 61 1555 158 2074 0.34 2303 47 2.17 226 2494 7.93 155 12.19 8 64 267 3374 171 406 0.27 1 3.44 349 3238 3.02 439 3086 0.58 338 69 6.47 324 254 0.92 17.60 1037 2801 0.55 1315 2.32 89 202 183 1181 5.60 2382 8.31 2104 7.73 2904 236 1861 317 158 20.02 1 202 2984 7.71 180 298 2.30 3219 2.95 92 321 20.81 192 15.55 1102 217 1.54 2 1251 1.72 1515 150 390 175 248 2.61 415 6.92 274 22.41 3.21 / HI 39 163 3061812 2.27 105 168 154 207 0.60 15 2.04 15 198 31 249 1.83 8213 0.64 70 107 0.42 2016 143 136 207 18021 1.40 12 0.50 336 165 412 222 2.37 2.54 24 1551521 262 298 290 2.08 345 346 1.54 2.96 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± 107 279 542 2.11 ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 36 1.393 1.00 -17.813 1.58 -18.703 0.81 9.64 -20.841 1.10 9.48 -16.238 -10.39 10.96 0.64 -18.71 -11.943 -11.67 0.35 8.39 3.21 -17.147 1.65 9.68 3.79 -14.08 -10.049 1.39 2859 8.56 0.32 -20.93 -10.024 7.18 0.46 2.29 2017 -15.871 -9.74 5935 1.37 6.42 1.77 -16.624 -9.34 0.52 8.04 3348 -18.072 3.06 -6.41 6046 2.44 8.09 -17.39 -10.804 1.96 9.63 0.95 2033 -19.222 2.64 -9.39 8.61 1.20 3.09 -10.53 -17.941 10.83 1521 7601 0.56 -18.942 3.48 -9.49 -13.19 0.48 3.63 9.21 1380 -13.122 0.72 9.90 -14.695 -10.06 3.05 3.29 2234 2190 0.74 6.69 -17.372 -11.71 1.12 7.39 2.80 1968 -16.484 -9.24 2567 0.01 8.72 3.30 -17.582 -9.43 1.22 8.35 -13.93 2403 3 1.59 -9.87 0.66 9.59 -18.61 1503 -10.072 1.40 6.45 1.54 -16.46 -11.482 3.33 1087 9.65 1.65 2.79 1334 -21.824 -8.48 1.46 2.02 -10.38 -20.252 11.27 2617 — 1.27 1407 -19.723 1.67 10.69 -12.64 0.02 2.73 1170 -19.652 10.42 1.54 -10.58 -15.08 —1 10.16 1174 1.52 -12.53 0.59 2374 -17.214 4.14 -12.26 0.48 6.12 3.94 -15.682 1.43 7039 7.70 1.09 -18.154 2.67 -8.74 2549 7.92 1.37 1765 -11.62 -19.753 4327 6.22 0.86 -22.133 1.49 -9.49 2618 2.15 9.94 1.37 -18.976 -9.45 0.65 -11.11 -19.262 2.46 2469 — 1.02 9.44 1334 -17.404 1.44 1.49 3.29 1840 -19.881 -10.13 — 0.50 8.80 7084 -20.40 — 0.54 9.62 2.95 4060 -17.21 -10.45 10.64 2.70 -16.87 -13.18 —3 -12.73 2.73 2328 2 — 8.34 0.87 2.41 2.54 4362 2 2.45 2418 1.41 -18.182 -9.54 2127 1.45 1381 — -20.522 4652 9.12 1.38 -19.61 3.055 10.67 1.47 2.79 -10.49 -23.563 10.31 -12.21 1.49 -20.26 1960 11.21 -12.32 3.00 0.65 4309 -18.122 10.57 2.52 -10.95 -16.25 4.50 -10.93 9.89 0.59 2344 6661 1.87 8.20 -12.03 -19.62 3.47 3065 7253 -10.14 2.07 9.49 4610 3.93 -9.57 1436 1608 2.18 6765 / 2813 1.38 1.64 -19.91 -21.03 10.39 9.66 — — 3.2455 2.90 1.66 2322 -19.95 2321 10.70 — 4.33 2552 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± km 3852244 6000 3927163 1812 + + . (J2000.0) [log] [log] [log] [log] continued 13 40 29.82 42 59 33.60 UGC 8656 2868 13 40 55.44 38 52 24.0013 41 39.30 2MASX J13405544 13 41 42.40 55 40 05.10 38 29 56.60 NGC 5278 UGC13 8667 45 19.2013 46 18.66 41 42 45.20 43 51 04.80 NGC 5290 NGC 529613 47 45.48 7610 38 15 33.20 1375 NGC13 5303B 49 18.1013 49 38.80 5813 39 49 49.60 44.30 2549 04 14 17.80 UGC 8743 2247 39 59 05.10 UGC 8740 NGC 531313 51 1404 43.2013 51 47.20 -02 1413 11.10 52 04.20 5013 58 52 2dFGRS 41.90 09.80 N202Z127 -02 12 23.80 IC 1752 0951 43 14 NGC 34.40 5327 7028 NGC 2539 533613 53 14.30 7083 13 03 53 53 21.60 52.3013 53 26.40 ASK 179168 40 21 50.1013 40 54 17 04.64 28.70 NGC 5350 4354 NGC 4054 535313 13 54 35 14.20 37.80 2334 -01 CGCG 26 073-09513 11.30 54 58.4013 55 NGC 35.90 5345 0513 20 55 01.40 39.90 4326 5913 37 55 13.90 44.72 NGC 5356 40 27 42.30 UGC 8859 08 11 2323 21.40 NGC 5371 2363 CGCG 046-005 6647 7253 1372 1610 6779 2549 – F F ZP 1 1 3 1 3 R 3 1 3 3 1 1 3 3 3 3 3 1 3 3 3 NC NF NC N NC NC NC NRZP C C C C C C C C C C C C C C C Table A.1. Source1901 RA Dec Name 1902190319041905 1906 13 40 39.901907 13 40 39.961908 13 54 40 19 43.30 58.301909 38 47 38.601910 UGC 13 39 8658 41 33 17.20 10.501911 NGC 13 5267 41 23.501913 ASK 322268 33 46 21.401914 33 51 29.60 UGC1916 8662 13 41 49.50 PGC1917 2040056 13 42 16.101920 13 47 45 53 18.10 19.801921 60 46 36.801922 UGC 55 8676 17 26.901923 UGC 2009 8684 13 46 24.671927 NGC 5916 5294 13 3337 47 15.991928 13 46 47 06 22.10 25.301931 13 13 47 10 33.70 37.801932 1529 NGC 2025 5301 38 18 10.001933 ASK 13 442182 40 48 21 16.00 03.80 ASK1934 13 512353 48 22.70 UGC1935 13 8721 03 49 57 04.50 03.101936 2240 08 12 41.701937 NGC 2204 5300 39 29 51.501938 PGC 1966 13417841942 UGC 8736 13 49 50.601943 13 50 20.401944 1504 13 33 1102 50 37 31.20 18.301945 13 41 1339 50 21 35.90 58.30 -01 NGC1948 37 13 5312 58.30 51 31.08 NGC1950 2616 42 5320 32 29.50 ASK 1988701952 39 27 17.00 1160 UGC1955 1172 8756 2MASX1956 J13513107 1957 2367 13 52 23.701958 13 52 34.901960 13 39 52 41 54.50 35.601962 13 38 52 42 56.50 18.70 -011964 NGC 4287 06 5337 52.60 UGC 2475 1966 2609 13 8793 02 53 48 16.20 51.30 NGC 53341967 NGC1968 1323 5335 40 47 45.901969 13 53 34.20 UGC1970 88071972 13 37 54 31 09.36 20.001974 IC1975 4341 13 60 54 40 29.20 40.90 2125 NGC 2437 5370 54 19 50.30 1374 NGC 4632 5368 1964 2344 3035 4596

Article number, page 45 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.510.22 7.60.44 4.10.73 13.7 5.90.44 11.5 10.00 3.00.14 11.1 4.00.41 18.5 -1.06 7.30 3.80.27 9.13 11.5 9.37 7.20.19 7.30 -1.24 7.8 5.40.84 27.3 -0.96 12.0 8.500.35 10.0 7.52 4.4 9.780.47 16.4 -0.55 8.50.57 -0.34 8.15 10.7 0.16 8.19 9.50.30 17.8 16.3 0.81 0.36 9.37 0.73 16.3 9.30.40 51.4 9.03 5.9 9.37 0.53 8.78 10.00 11.0 6.4 0.47 0.60 21.7 -0.89 0.06 8.30.77 8.51 11.2 7.10.25 64.2 9.42 7.1 2.48 0.17 9.26 13.7 12.1 9.890.30 -0.21 12.2 -1.22 3.40.49 25.3 9.82 -1.02 3.80.40 9.40 -1.25 5.7 8.82 2.90.36 -1.20 4.3 7.50.49 1.50 7.63 3.9 9.10.24 24.3 8.96 9.10.27 -0.34 8.64 6.3 7.30.44 -1.27 56.4 9.24 3.30.19 -1.53 9.47 6.1 9.53 9.20.36 -1.18 4.5 5.10.42 -1.59 -0.98 10.7 8.34 3.50.44 10.8 9.08 6.00.37 -0.23 9.66 6.4 5.30.19 18.2 -0.35 7.79 -0.84 4.00.44 13.1 8.25 5.1 8.890.21 21.5 0.29 6.60.22 -0.80 -0.82 8.26 7.6 5.90.42 41.8 14.0 8.39 -1.19 0.16 11.7 7.63 4.9 9.010.15 20.3 0.32 4.50.47 8.23 0.92 0.29 6.5 8.82 8.00.35 -0.21 8.9 5.80.64 55.2 8.82 9.05 7.80.32 17.7 105.2 7.76 8.10.43 -0.27 89.0 7.860.59 8.92 9.39 7.76 12.5 212.6 5.10.79 0.09 6.6 0.08 0.32 9.39 9.34 9.69 6.7 6.60.34 16.2 5.0 0.28 0.30 0.62 12.8 8.55 10.05 7.0 4.6 7.7 -0.86 9.03 0.19 12.7 9.11 9.03 8.6 9.35 -1.08 9.59 1.66 -0.73 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 642 33 299 2887 51 317 310 1125 0.34 3.13 3 8.58 131 908 65 0.46 1162 1549 95 1.57 1464 201 506 1.71 1615 3.32 47 6182 4.79 386 17.45 3 73 4985 411 3771 1.72 532 3145 2.85 395 153 21.51 3426 55 4.70 171 5.91 365 3.95 671 391 0.29 9 4028 2.82 93 429 2346 17.40 131 2546 86 1.24 3 0.88 183 1055 2456 229 0.67 1222 2627 60 4.47 136 1703 3.60 5 84 1.53 82 202 98 219 10.98 1214 0.63 1342 239 1.34 1 72 2.51 2067 2.11 2011 91 223 2097 259 253 0.69 5.22 251 107 21.24 4 270 4.82 133 278 42.88 1.65 297 6.35 / HI 10 448 50516 4.46 21031 256 6433 1.86 316 379 3.37 47710 5.28 237 279 1.82 13 2751315 311 282 500 1.39 323 54211 2.24 1.71 20538 254 124 2.80 215 0.96 23 43 113 0.36 10 4991521 545 22411 6.16 52 277 291 157 1.47 328 1.67 1.62 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 32 -0.482 -13.81 1.394 1.45 -19.90 1.34 -19.79 —6 10.37 -16.607 10.33 -12.35 0.734 -12.08 0.52 9.05 — -19.532 2.68 0.42 -14.61 -10.401 4.52 3.27 1.16 9.62 -15.089 2984 7.34 0.50 2.96 -18.943 -9.93 2381 1102 7.46 0.74 -10.95 -17.573 1870 1.75 -17.424 2.52 — -9.19 2.75 8.56 0.23 -20.443 8.72 0.94 6106 -11.68 2.135 10.89 -9.31 1.80 1364 -10.89 — -19.052 -11.74 2.10 6.03 -19.686 2.70 1371 1.58 4.02 4.18 9.63 -18.995 10.49 2.49 -9.70 1.76 -21.37 -10.192 10.91 2602 -0.25 3045 -11.75 1624 -20.222 3.75 11.06 3459 -10.73 0.58 -13.97 2.332 10.60 2.13 -12.61 1.33 -15.962 2.48 1971 7.32 5510 1.55 -19.59 -9.862 3.28 3659 1.46 7.98 -19.212 -9.42 10.22 2742 1.47 4.50 -19.752 10.18 -9.53 5391 -11.70 1.74 2.08 -21.204 10.42 -11.89 0.73 2958 -19.473 2.25 1.85 11.06 -12.24 0.84 -17.084 1865 2.68 10.51 -12.67 1.20 -18.93 3656 4 2.40 1763 -12.67 0.33 8.57 -20.723 1.70 1799 1.18 9.43 -14.82 4030 6 10.50 2.54 -9.71 1.00 -16.98 5947 6 -9.74 -10.44 7.51 1.54 -19.462 2.31 2019 0.67 9.05 -17.155 1.87 2.99 -0.00 -9.48 9.71 -16.071 -10.41 1909 0.76 -14.35 9.45 5806 4 2.01 5291 -9.90 0.61 8.08 2.67 -17.413 -11.05 6.71 0.09 -18.45 2.99 1384 -9.89 1991 1.22 8.71 2.91 -15.698 -8.49 8.44 -17.65 -10.113 3.45 1888 0.67 2.28 1021 1 — -9.95 0.82 9.32 3.34 -15.072 1836 0.57 -17.65 -10.15 1182 4 2.07 0.88 7.77 1383 -18.21 —2 8.84 0.92 2.92 -17.863 1630 -9.79 0.54 2.06 -10.29 -19.093 — 1.61 9.06 3315 -16.893 1.72 1.28 3.41 9.07 -20.67 2324 -10.045 1.35 8.36 -18.90 -10.55 —3 10.91 1484 0.71 4.38 1822 -19.84 -9.54 -11.26 1.26 2.10 2.36 -18.65 10.19 — 3066 -20.11 4.00 2.77 -10.09 7.70 1538 1556 10.32 6132 -11.66 — 2.10 2119 -9.94 2.98 4.94 4267 1.79 5295 1865 7073 2 1.56 -21.17 11.06 -12.92 2.49 6865 / 15 3.12 -12.40 7.87 -10.34 1.33 1218 51 0.63 -16.11 — — 1.57 1818 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± km 5013235 1766 50004341143112 1909 5309 5500414 2010 + + + + 257 2602 365394 3323 1486 + + + 08-26-010 2117 + . (J2000.0) [log] [log] [log] [log] continued 13 56 09.3013 56 51.00 05 32 33.30 37 47 50.00 PGC 4019959 NGC13 5378 57 19.16 11 58 33.6013 58 16.50 CGCG 074-01613 58 23.80 59 48 48.0013 25 58 32 37.90 59.50 1095 NGC 540213 59 11.60 KUG 1356 37 25 28.10 2985 52 21 41.30 NGC 539513 59 50.80 UGC 8914 6104 38 10 56.2014 00 49.99 NGC 5403 49 30 59.80 3098 ASK14 401152 02 34.2014 02 48.60 3471 1414 33 02 09.10 50.00 1982 09 20 28.90 IC 0970 49 10 21.60 NGC 5423 NGC 2744 544814 05 59.30 1849 14 55 06 00 31.90 42.90 2MASX J14055923 06 01 46.80 NGC 5470 4035 5910 14 09 01.70 2012 14 48 09 00 37.60 47.90 ASK 400926 05 05 46.5014 10 12.90 ASK 99518 -02 3414 32.90 11 37.80 1015 UGC 9057 -01 09 22.3014 12 22.46 NGC 549614 50 2325 12 20 39.90 52.2014 12 58.55 NGC 5520 01 1836 45 17.50 09 55 15.90 CGCG 018-080 CGCG 074-140 1546 1542 1771 5297 7054 – 2 1 3 A 3 3 1 3 1 1 1 1 1 1 N NC F NF NZF NF NF NC F A U R C C C C C C C C C Table A.1. 1978 1980 1982198419851986 1990 13 56 56.001991 13 57 11.481993 13 29 57 09 14.00 51.701994 50 26 08.501995 NGC 13 5375 04 57 18 37.30 26.30 UGC1996 13 8880 57 49.50 PGC1999 1266441 39 28 53.502000 42 13 29.50 ASK2001 322527 13 58 37.90 ASK2002 3097032003 60 47 48.502005 13 59 30.58 UGC2006 8909 13 59 31.412008 2373 38 1214 47 34.702010 1867 14 34 00 46 20.10 24.802013 UGC 14 8913 00 45.702014 NGC 5399 38 1380 54 55.502016 14 59 1368 01 19 14.70 41.80 NGC2017 14 5406 01 49.20 NGC2019 14 5430 50 02 13 11.80 23.102020 37 00 33.802022 2MASX 1609 J14011475 55 48 50.402025 UGC 8945 NGC2032 5443 14 03 00.802033 5517 14 03 12.062034 3637 14 50 03 00 36.74 43.602035 14 11 03 43 57.30 11.502037 2MASX 5387 J14030084 39 03 10.102041 2MASX 3071 14 J14031209 39 06 36 21.60 04.202044 UGC 89802045 ASK 323185 14 50 06 43 38.10 30.302046 3628 14 07 04.402047 NGC 1795 14 5480 54 07 59 25.00 47.602052 14 10 08 42 58.10 45.202053 ASK 302203 55 06 11.00 -022054 ASK 58 14 413724 25.60 09 02.002057 NGC 5486 IC 09782060 14 36 10 19 00.68 24.302062 5798 14 1396 10 03.082063 KUG 1406 39 11 54.102065 14 54 10 13 35.90 05.802066 KUG 1911 1407 UGC2067 9071 14 59 1837 11 21 49.59 28.702068 14 1183 11 53.44 UGC 9080 47 57 58.80 1367 14 38 12 11 31.70 37.80 MCG 1642 UGC 9088 13 18 17.00 NGC 5505 1822 3064 6129 4263 Source1977 RA 13 56 03.40 13 30 21.00 Dec IC 0959 Name 6863

Article number, page 46 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.350.45 10.70.41 5.40.27 21.5 6.80.37 11.5 8.99 3.30.59 17.3 8.10.23 8.81 0.97 5.8 5.00.77 33.0 8.53 4.8 1.77 0.35 14.8 10.7 9.31 9.980.49 8.53 4.2 6.1 49.70.55 -1.83 -0.49 8.30 12.60.36 7.79 9.99 5.3 8.30 4.20.59 19.4 10.10.19 -0.73 1.19 11.3 9.15 8.77 6.80.40 12.8 3.30.23 -1.95 9.22 14.8 1.53 13.5 8.470.64 -0.81 5.1 3.90.56 26.1 9.33 1.48 3.90.27 8.13 3.0 9.09 7.0 3.28 0.24 46.0 6.70.52 0.84 9.09 8.38 4.4 3.8 77.60.48 12.5 8.510.56 0.23 13.9 9.66 8.94 5.2 22.70.26 0.35 12.30.32 34.0 3.01 27.6 0.64 8.02 8.900.24 26.3 5.2 9.060.50 -0.37 40.3 -1.05 10.9 9.650.60 -1.26 5.2 8.95 6.8 17.40.27 14.2 0.01 0.40 0.35 7.92 8.27 4.4 7.7 30.80.20 9.90.40 -0.19 0.66 9.07 8.85 3.8 6.00.28 18.5 20.90.24 2.48 1.71 7.97 4.5 3.50.18 32.4 8.49 3.90.37 -1.93 7.52 -0.56 3.9 8.940.25 3.4 43.4 11.20.20 -0.67 2.67 3.6 8.53 4.70.39 88.5 8.91 4.00.39 -1.65 7.36 -0.43 9.41 9.4 5.30.12 41.3 4.00.43 -0.17 0.15 16.9 8.55 3.50.56 77.7 7.85 9.60.33 -1.66 9.75 5.1 9.24 3.20.47 13.1 7.85 17.0 -1.20 0.35 42.5 0.40 7.30 9.90.21 22.8 9.45 32.40.33 76.1 -0.26 9.65 8.53 8.50.13 9.45 61.4 20.1 9.920.27 -1.01 0.59 13.2 3.7 9.110.60 37.1 9.92 9.0 8.46 11.3 0.65 8.83 3.7 12.2 2.11 22.7 0.67 7.65 8.35 9.35 0.63 -0.06 -0.74 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 45 1535 279 182 1291 299 4.45 155 363 3.28 3 1.97 3846 5832 7.95 572 6204 95 592 24.42 8 117 0.96 66 1852 5.62 93 223 13696 2.54 4.76 163 1161 3268 6.21 141 81 3404 2.54 83 131 1.41 500 1061 10.59 539 0.72 4 80 10.23 107 86 5.91 1179 2.30 14 67 2396 1798 91 263 2261 194 0.40 47 8.11 244 2005 0.61 9 1.71 68 2211 77 20.10 2059 0.46 215 92 2697 68 2432 0.48 3.88 412 18.76 1 89 1151 437 317 0.22 4 141 1731 3.60 342 1017 4.41 201 144 22.68 4 127 12.97 2 68 169 89 1.61 280 7.47 88 117 301 0.28 1.87 8.61 / HI 47 2161124 325 246 41 0.75 291 12014 3.75 0.54 25021 304 11417 3.67 162 106 0.41 16819 0.83 18212 344 11514 5.60 22224 6928 6.99 12124 8129 80 1.05 168 72 354 98 1.75 146 5.71 292 0.74 3.20 27 134 20213 0.71 166 257 3.88 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 36 0.513 1.34 -16.162 0.75 -18.082 8.02 1.51 -16.962 1.28 7.04 -21.511 -9.49 1.04 -20.46 -11.004 11.15 — -17.69 2.772 10.47 — -12.43 1.85 2.822 -10.60 -13.96 1.64 -19.81 —2 2136 1.65 — 1.02 2009 -21.412 2.07 10.72 6.61 1.27 3.56 -14.95 7572 3 11.10 -0.97 -11.04 — -19.27 -8.541 4976 -11.39 7.24 0.45 -11.51 1885 2 3.36 10.03 -3.03 3.72 2.26 -17.551 1.57 -9.44 -1.38 6.99 -11.81 -12.101 2872 1056 1553 0.42 -12.28 6.052 4.91 -8.93 3.40 7.29 5498 0.48 -16.71 -10.551 0.72 4.03 -16.34 3055 —4 -8.91 1471 8.15 0.47 4.26 -18.124 8.17 0.71 1.63 -16.56 1548 3 -9.35 6.65 1.35 — 3069 -16.333 -9.41 2624 8.31 1.50 -18.87 1.912 -8.98 3.37 8.39 0.79 -10.36 -20.37 5.813 9.95 0.76 2438 -19.52 3.34 10.33 -9.97 2031 0.67 2.51 -11.62 -17.351 1631 9.64 -16.113 2.51 8219 0.54 3.02 8.60 1297 — -10.112 0.14 8.11 -17.95 -10.428 1726 1745 2.23 1.16 4.06 -14.132 -9.67 6.59 1.35 2.70 -19.20 3607 7.14 0.86 1540 -20.075 3.10 -9.17 9.91 1770 -15.787 -9.45 1.30 9.04 1284 -11.516 4.16 1.15 8.19 -19.653 -11.73 3.43 0.09 2.38 3673 -17.932 10.18 -9.86 0.65 2.56 1603 -13.13 1608 1.40 -10.81 9.34 -19.713 2.30 1451 7.21 -19.34 -10.652 2.22 9.59 1.492 10.21 1303 0.68 1.67 -10.34 -20.914 -0.26 — -12.06 3403 -17.844 10.96 -14.53 1.65 2.66 3137 4 2.37 1.89 -12.33 1.38 8.84 -21.173 7.55 0.61 1637 -20.55 3227 2 1020 2.62 -9.57 1.35 -16.122 -9.57 10.66 — 0.68 -21.122 2.73 5532 -10.94 7.94 0.66 1.38 -17.112 -0.18 -17.54 —2 2.93 1388 — -9.71 0.23 -16.62 8.46 1376 4 -0.18 6.34 2.91 -14.59 2.98 8.16 5051 -9.73 1.19 -15.91 — -8.07 3874 7.01 -19.70 -9.42 2.66 1253 8.41 2.76 2.01 10.09 -8.97 2.78 1441 -10.32 2746 — 1.52 1921 1363 3.75 2.69 1800 2322 1578 / 13 0.48 -15.06 7.61 -10.4415 2.36 1.18 -18.27 1298 6.2759 -8.61 0.40 2.68 -15.52 1488 — — 2.23 1745 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± km 5328131 1729 3448195 3132 + + . (J2000.0) [log] [log] [log] [log] continued 14 13 36.92 47 24 21.00 ASK 288105 2144 14 13 50.6714 14 22.20 57 46 36.90 -03 01 56.50 NGC 552614 14 49.40 2dFGRS N206Z08214 25 15 19 34.10 05.0014 15 39.20 NGC 5523 36 13 35.6014 14 17 16 02.50 57.40 NGC 552914 17 1885 04.20 NGC 5525 36 34 17.70 -01 30 20.10 NGC 1889 554414 19 17.50 ASK 200015 46 19 13.3014 19 40.90 PGC 1136 5116214 19 45.40 60 00 01.70 2870 14 09 20 21 04.40 52.00 ASK 5529 16040314 20 19.50 UGC 9169 0314 59 20 33.80 26.50 1565 3043 03 55 57.70 NGC 5560 35 11 19.60 NGC 5566 NGC 5579 2018 14 20 54.7014 20 55.90 39 8111 14 54 21 51.10 05.10 03 14 16.80 PGC 1272 215770814 03 21 16 14.70 15.50 NGC 5574 NGC 1733 5576 03 26 23.90 1592 NGC 3596 557714 22 30.7014 23 01.50 -01 1675 13 45.80 40 22 ASK 38.70 200122 1582 14 24 08.40 NGC 1479 5603 34 51 41.60 1372 14 24 42.70 NGC 561414 25 21.00 -03 12 34.10 39 32 NGC 22.40 5604 1723 UGC14 9242 27 10.70 5568 05 08 08.30 UGC 9252 3907 2869 1469 1558 – 3 F R RF RF 3 3 1 1 1 1 1 3 1 3 1 B F NP NRF F NC NZ NF NF N U RF R C C C C C C C C C C C Table A.1. Source2070 RA Dec Name 2072 2073 207420752076 20772078 14 14 51.402079 14 14 52.002081 03 07 51.202082 14 14 14 07 54.10 33.10 IC2083 0989 -02 UGC2085 08 9117 22.902089 14 16 ASK 57.30 1994462091 2092 03 50 10.002093 14 17 16.96 PGC2095 140287 14 19 11.502096 58 42 33.80 -022097 15 14 15.60 19 20.20 UGC2098 14 9151 19 25.60 PGC 1097302 7577 4973 2100 01 09 54.60 1547 2101 39 51 27.40 CGCG2102 019-003 14 19 57.68 Mrk2103 06762105 53 1485 28 11.802106 2MASX2107 J14195772 14 20 32.102108 14 20 2683 40.302110 3080 14 03 20 58 44.50 59.602111 14 40 2443 20 18 44.82 55.10 NGC2112 5569 08 37 35.80 CGCG2113 219-069 51 08 15.50 ASK2114 456677 1618 UGC2116 9192 14 21 09.2021172119 14 39 21 29 25.10 49.302120 14 21 55.702122 UGC 14 9194 35 22 16 12.20 14.202123 14 34 1294 22 48 23.80 19.202124 -01 NGC 1784 53 14 5588 28.70 22 28.70 1305 -002126 2MASX 23 J14215576 15.60 ASK 2003762127 37 07 19.90 NGC 55842128 3663 14 23 27.10 NGC2130 5596 14 23 43.702132 01 43 34.602133 14 05 24 52 22.90 36.602134 UGC 1297 14 9215 24 24.302135 ASK 463118 24 36 50.802136 3406 08 16 34.102137 NGC 1020 5610 14 26 36.00 UGC 9225 14 26 59.80 1655 14 51 27 35 04.80 10.60 3179 08 41 01.00 -01 NGC 43 14 5624 46.70 27 28.40 UGC 9249 ASK 200456 1397 46 1385 08 47.50 NGC 5633 5063 1248 1933 1803 1371 2321

Article number, page 47 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.490.30 16.20.30 16.40.24 37.3 36.60.33 32.0 5.6 9.580.64 80.0 7.4 8.640.13 0.18 7.0 9.070.48 8.2 12.0 0.70 3.80.26 41.4 12.6 0.10 8.330.30 8.43 70.4 4.40.67 84.3 9.68 10.2 0.97 111.50.60 1.06 15.9 7.73 -1.27 9.450.36 17.9 9.62 8.90.30 27.9 31.0 0.31 0.95 8.680.25 9.62 11.6 21.2 9.32 65.90.37 -0.24 13.00.20 22.9 9.55 16.1 3.24 9.110.86 22.4 -0.92 8.50 3.00.32 32.1 -0.15 10.2 9.240.42 1.45 7.9 8.84 3.30.36 26.4 -0.45 6.10.41 13.4 8.84 8.58 8.5 9.400.26 57.6 10.20.80 8.33 17.3 0.26 24.3 9.40 107.00.31 8.52 16.2 -0.03 0.31 31.2 9.49 9.37 30.0 1.21 0.31 40.4 11.7 -1.63 8.740.43 0.21 59.3 67.4 9.650.23 20.2 12.1 0.52 108.4 9.430.20 -1.01 30.3 8.96 18.40.37 9.38 51.1 9.43 47.60.30 -0.91 24.9 117.4 8.92 -0.67 0.33 8.94 9.00.20 57.0 9.36 23.3 2.30 0.62 8.94 11.7 8.4 9.280.47 0.50 26.9 11.10.42 8.33 11.0 0.78 7.6 9.070.23 19.1 6.7 2.16 0.52 8.23 -0.33 10.04 16.1 5.30.26 14.9 13.2 -0.70 0.16 0.54 9.41 17.5 6.50.42 33.2 9.32 16.0 -0.34 0.33 31.0 8.88 -1.02 5.8 9.410.36 41.4 7.3 8.900.45 -1.82 -0.97 13.2 3.0 9.540.52 12.5 2.81 7.90.26 9.09 -0.40 5.8 4.50.54 8.48 17.7 6.0 -0.60 0.12 13.8 11.3 9.60 -0.78 0.37 9.53 5.2 8.11.49 33.7 -0.53 8.93 -0.70 7.7 8.18 -0.49 9.54 5.6 4.0 13.4 -0.15 0.38 12.0 7.55 8.42 9.50 0.14 0.90 0.30 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 23 2391 1505 266 1936 183 11.27 6 97 213 147 5.65 522 14.89 1161 1801 551 1.16 1762 2.33 1032 5.21 205 209 141 24.75 2071 226 16.27 234 183 3.39 11.58 4 2116 14.48 1823 113 234 391 126 6.80 4171 0.41 14.33 2 1812 1481 217 4543 175 25.78 2351 482 1862 4.88 257 20.55 1071 213 114 11.33 1 1332 3.81 92 137 19.70 2305 192 1081 4.71 2537 56 240 6.73 14.44 3 43 12.17 3 62 88 337 67 314 107 1.84 3632 4.69 332 1.09 3 7.66 4111 4.91 1314 431 3406 173 240 11.04 6 357 1664 4.66 257 166 14.38 8 197 3525 3.48 179 2553 2.48 3796 93 1.06 289 275 5.09 115 37 3.64 305 1.23 11.30 58 0.24 / HI 12 124 15615 0.32 3511110 444 103 7.41 86 191 18212 3.30 12 2.59 13692 179 200 518 232 1056 2.33 2.50 4.05 1423 256 227 321 310 3.25 0.86 1419 89 248 163 322 2.41 10.31 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 24 0.483 0.88 -16.374 0.23 -18.002 0.93 7.93 -15.01 1.49 8.97 -16.622 -9.55 7.36 -21.122 -10.83 0.48 7.374 10.95 2.39 -9.15 1.09 2.22 -17.99 -10.742 -12.59 0.94 -19.792 2.37 1268 8.51 0.78 2.64 -17.40 1287 2 2.98 1.50 -18.964 — 1958 -9.81 0.70 8.92 1544 -20.172 4343 0.44 6.08 -18.78 -10.00 3.663 10.47 1.17 -13.73 —5 -8.11 -10.72 9.27 2.17 1.27 -18.392 1541 7.04 0.54 2.37 -18.012 4.77 3.08 -9.93 9.69 1.60 1712 -16.572 -9.40 0.79 2317 3154 -19.86 2.692 1934 — -9.81 8.32 1.00 -16.30 2.352 1.98 -17.772 2.05 1363 — -9.68 8.37 0.94 1381 -20.28 — 0.49 7.31 3710 -17.78 1.905 11.12 -9.87 2.60 -16.90 —4 -11.11 9.16 0.514 2.46 4401 — 8.22 1.14 4.54 1455 -10.42 -18.424 1.20 0.55 1385 -19.13 3.02 -9.20 0.58 2.97 1914 3982 -18.982 — 9.87 1664 -17.07 2.132 10.04 0.67 1373 -10.389 6.62 0.19 — -17.922 1525 2.28 0.47 — -10.95 -17.283 2.06 8.86 0.72 -15.233 2.91 3.97 0.60 8.50 2219 -10.16 -19.055 1.38 6.18 2224 -16.07 -10.043 1.17 1.34 9.40 1582 1907 -21.022 1.43 8.07 2.55 -18.61 -10.922 10.74 — 1.47 1822 -19.81 -10.822 -11.03 1.65 9.75 4.36 1800 -20.634 3.48 10.35 0.73 2.08 -19.33 -10.593 10.70 3.58 -10.05 1.47 2279 -20.244 10.39 1559 -12.15 0.92 2.83 1799 -18.593 2.53 5469 -11.25 0.82 6.09 -19.435 1.45 1.02 9.94 3305 -17.816 3672 2.71 -8.28 1.30 9.69 -20.252 4243 -11.06 1.36 9.26 -19.593 10.12 2.17 -9.81 2211 0.53 3.12 -17.566 10.23 -9.89 -10.07 1.21 -15.551 2.81 1871 -11.10 0.29 9.42 -18.59 2234 2 2.55 2.96 7.79 0.12 -14.60 -10.56 2.53 2721 9.69 0.68 -15.48 -9.46 1589 8768 7.41 3.33 -10.93 -18.76 3704 7.52 2.60 -9.53 3.34 9.20 2190 -8.99 -10.10 1.65 1593 2526 3.15 9.01 1734 1503 2522 2 0.69 -19.38 9.40 -9.83 3.23 2650 / 20 0.49 -14.11 7.42 -10.09 1.10 1858 47 1.71 -19.78 10.6653 0.46 — -15.30 3.95 — 2113 — 2.44 1633 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± km 101 1400 544 8785 + + . (J2000.0) [log] [log] [log] [log] continued 14 28 10.90 13 33 05.70 UGC 927314 29 46.3014 49 30 37 23.00 16.40 NGC 5660 59 27 44.8014 30 48.70 NGC 5667 1296 14 31 25.90 0714 09 31 25.90 27.40 30 47 13.10 PGC 441994314 03 32 00 05.60 38.80 CGCG 163-072 IC 102414 57 32 55 29.10 17.10 NGC 2282 567814 00 32 17 43.90 34.40 UGC 2021 934814 09 32 53 46.80 30.1014 32 53.50 1367 NGC 5669 49 3643 27 28.4014 11 33 35 24.30 42.20 NGC 5676 UGC 935614 04 35 27 22.80 01.70 1509 14 35 33.30 NGC 1902 5668 0514 16 35 35.50 39.90 1214 54 35 29.60 50.10 UGC 1613 9385 13 10 11.70 UGC 9389 02 36 19.70 UGC 1375 939414 36 57.10 ASK 83319 2106 41 49 41.20 2221 NGC14 5696 37 30.80 1582 14 37 52.50 51 33 1526 42.60 -00 23 55.20 NGC 1835 5707 NGC 5691 1772 1569 14 5455 39 52.1614 42 40 44 03.50 32.4014 40 09.21 NGC 5730 2184 34 05 59.50 1927 42 46 46.30 ASK 393433 NGC 5731 2525 1497 2513 – 1 1 3 1 A 1 1 1 3 3 3 3 1 NRF F F F NR NZP NP NZF NC NA F NC N R C C C C C C C C Table A.1. 2141 21422143214421472148 14 28 18.402149 14 28 31.302150 14 13 28 46 37.80 48.802151 14 32 29 52 16.60 34.502153 IC 14 1014 00 29 33 33.40 11.002154 ASK 14 469132 28 29 49 34.60 18.702157 CGCG 04 019-041 10 13.10 -002158 NGC 01 14 5641 05.60 30 01.80 ASK2159 100695 UGC 92992160 14 03 30 46 25.50 22.202161 14 30 39.30 IC2163 1022 35 19 15.702165 07 16 30.30 NGC2166 5656 1966 1542 NGC2167 5645 1288 14 31 49.702168 1825 2169 4317 14 27 32 53 20.80 30.302170 1551 PGC2171 4553986 14 09 32 56 39.80 00.602172 KUG2173 1429 14 36 32 18 45.10 08.00 1722 2174 NGC 3144 2175 5675 02 54 54.00 1364 2176 14 33 09.20 CGCG2177 047-0852178 14 10 34 30 37.00 38.90 4415 2181 NGC2183 5666 59 20 16.102184 UGC2185 93912186 14 36 11.202187 3972 14 1527 36 40.902188 48 35 06.102189 14 11 37 34 13.60 36.702190 NGC 14 5693 37 14.702191 LSBC 14 D723-05 43 37 41 22.10 45.402192 2220 38 27 15.302193 UGC 36 9422 34 04.202194 NGC 1904 5698 14 38 11.502195 NGC 5695 14 38 16.302196 14 46 38 38 18.10 17.702197 14 40 38 27 38.30 24.202198 NGC 14 5714 03 38 24 1804 50.00 37.102199 NGC 14 2284 54 5704 38 16 59.20 38.702200 NGC 14 5692 30 39 26 15.40 33.00 SBS 1437 51 07 14.40 NGC 14 03 5703 3305 39 16 58.30 21.50 UGC 9448 3629 PGC 1248765 4242 02 44 52.40 ASK 83546 2237 2710 1607 3723 1584 2202 1760 Source2138 RA 14 27 36.60 41 15 27.90 Dec NGC 5630 Name 2673

Article number, page 48 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.270.42 6.60.18 21.80.70 10.9 4.50.29 46.2 20.40.37 8.43 10.0 9.11 4.90.31 53.7 7.5 2.10 0.36 18.1 0.53 8.48 9.53 2.80.39 14.6 6.2 8.610.38 -0.14 -1.19 24.0 2.60.41 9.23 11.2 10.4 2.24 45.50.47 28.1 8.08 -0.80 23.00.48 8.40 19.8 9.88 60.81.24 -0.25 -0.38 8.77 5.0 50.70.50 -0.49 12.8 9.310.26 20.3 0.11 9.21 6.0 27.90.25 35.4 0.77 46.90.17 28.8 9.21 8.95 9.41 54.50.27 8.97 6.1 -1.06 0.29 40.8 -0.70 8.89 7.80.35 8.97 4.4 8.740.56 8.6 19.7 8.89 11.90.26 1.76 7.78 5.4 4.51.12 36.4 8.44 5.50.36 0.66 7.88 -1.84 8.94 8.2 9.50.31 28.4 6.80.26 -0.94 14.9 1.11 20.7 8.800.36 42.6 7.81 4.9 10.751.34 -0.01 22.5 16.0 9.170.78 -0.57 1.19 7.5 8.41 6.6 32.41.02 -0.30 10.20.31 16.6 0.59 8.21 8.72 5.70.35 11.1 33.70.28 9.50 0.54 0.22 4.9 9.05 8.6 66.40.18 78.6 -0.27 0.18 0.46 9.82 154.9 9.36 4.1 7.10.36 5.90.36 -1.05 -0.48 11.6 9.47 8.37 4.20.66 4.5 6.10.35 18.0 0.31 0.63 7.99 5.30.28 17.8 8.25 8.80 5.70.26 1.94 10.1 5.70.45 36.6 -0.09 8.25 8.22 6.80.52 9.37 3.0 8.86 7.50.27 16.2 0.03 12.1 -0.41 0.56 -1.30 8.21 7.8 4.60.59 33.6 8.17 3.20.37 -0.10 10.2 9.00 9.53 4.2 8.17 0.44 24.3 5.40.67 -1.14 -0.39 9.59 3.9 8.2 39.6 9.78 9.4 9.59 8.91 9.45 3.9 -0.95 21.8 -0.75 -0.81 8.49 9.75 -0.84 -0.76 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 19 19023 93 210 3846 12.06 146 1224 421 218 167 0.51 23.55 1391 253 3.22 149 2381 3.31 0.50 263 310 11.14 2 326 15.83 32812 3515 67 21.84 4 56 115 75 370 1064 6.95 96 395 4.89 1228 0.85 2.01 1771 484 6.85 184 823 85 199 0.88 3 170 1323 9.57 4244 207 3.61 2801 442 5045 6.90 307 184 14.23 1 521 109 5.37 209 1387 5.72 126 12.46 3 1714 1.52 53 120 24.96 4 1002 84 147 257 113 324 0.58 3.82 274 1.27 3523 4.28 7 8.11 287 49 3251 10.83 5 89 2003 115 1.39 226 388 130 9.02 411 1.04 9.42 / HI 10 112 158 1.61 3112 75 127 2081013 222 1.46 173 21913 4.26 317 266 11.55 94 1.73 27814 8.98 28 81 139 12410 242 0.70 62920 2.64 687 15.19 67 134 0.78 14 61 9914 0.39 1716 50 61 192 105 14316 225 0.93 22 1.33 351 1.27 183 388 246 1.94 2.75 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 12 1.061 0.41 -21.473 0.60 -17.832 2.09 6.33 -17.604 8.58 0.77 -21.392 -7.27 8.62 1.01 -17.786 10.72 -9.63 0.42 -19.883 2.31 -9.54 -11.02 0.83 6.37 -16.621 3.13 10.03 1.39 1873 -17.27 1.784 3.71 -10.44 0.64 8.33 -20.053 1488 — 8.78 1.50 -18.164 10.37 3501 2.54 1725 -9.64 0.55 -18.31 2.442 -9.85 -11.23 8.66 1.07 -16.62 2.732 3266 8.53 1.55 -19.77 2.67 2.61 1627 -9.70 0.70 -19.094 10.01 2248 — 1899 -16.34 2.72 10.12 — 3739 -10.66 -10.95 0.212 -11.36 1695 2.45 -14.292 3.22 2.86 — 1.512 7.16 0.01 6.97 3290 1701 -21.012 1632 1.52 — -14.152 10.28 1566 -8.94 0.56 -18.143 -11.05 0.01 3.26 6.78 -17.682 2.64 9.89 1.80 -13.712 1.46 1463 -8.79 8.81 1.14 -11.60 -21.344 1521 6.62 0.01 -18.271 2.84 11.33 -9.58 1676 0.31 2.82 -16.493 -8.91 -12.49 0.66 9.47 1512 -14.20 3.915 1.77 7.82 1639 -16.88 -11.692 3.04 4.73 7.67 0.77 2225 -18.155 -8.71 8.49 1.47 2.74 -17.06 8804 4 1233 -9.89 1.52 9.76 -20.994 2.88 -9.90 0.63 8.59 1790 -20.40 -12.597 2.39 10.87 -0.16 -15.32 -10.30 2.712 1201 -12.25 9.84 0.55 6.89 -17.41 2085 3 7.75 0.68 4.80 -10.92 -15.961 1253 4.87 9.15 0.03 2139 -18.175 -9.44 0.65 2.29 6.04 -10.06 2082 -18.262 4895 1.09 -16.292 3.40 — -8.69 2.27 1.53 8.89 1956 -19.255 0.53 8.19 -19.193 1.95 1797 -9.94 0.87 1560 9.78 -17.524 — 10.15 -9.69 1.29 2269 -17.581 -11.18 3.20 -10.80 1.44 8.31 2.17 -19.583 3.67 1.01 4.35 -18.653 10.15 2.04 — 1859 -9.49 1.46 -19.82 2514 2 1642 -10.29 9.92 1.30 3369 -20.613 2.89 1358 1.57 -10.73 -18.28 —2 3.27 10.72 — 0.73 1896 -20.60 -12.08 3.14 9.66 1.31 2.32 -18.65 4058 10.26 -10.31 — -20.40 3.13 1520 9.33 2554 10.51 4.07 3.15 — 7983 -9.86 -11.16 2504 2.66 7600 4.14 3.61 2550 2474 3523 / 11 -0.8814 -16.24 -0.61 -13.60 — 7.12 — -10.73 2.57 1.91 1523 1207 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± km 6052290 2292 4854050 2232 + + 031495 1647 7592 + + . (J2000.0) [log] [log] [log] [log] continued 14 40 10.70 -00 17 38.40 NGC 5713 1963 14 40 56.4014 40 58.30 -00 1914 05.50 41 32.00 02 11 NGC 11.50 5719 44 30 45.90 NGC 5725 UGC14 9476 42 45.9014 42 58.00 -00 2114 03.90 43 02.80 04 53 NGC 22.50 573314 04 44 45 24.40 56.30 IC 104814 44 30.90 UGC 9485 0114 40 45 47.10 1725 28.70 0114 31 45 21.90 32.50 NGC 1628 5740 3114 25 45 55.60 33.60 CGCG 3269 020-010 31 24 55.70 UGC 9504 31 54 56.10 UGC 9506 ASK 470206 1702 14 47 44.5014 48 26.70 1644 1700 36 30 16.8014 34 1481 50 59 56.60 53.00 ASK 1566 324646 UGC 9537 35 34 1514 19.5014 51 17.80 1208 UGC 1490 956014 51 35.90 58 58 40.60 58 57 13.80 NGC 577714 52 43.50 UGC 957014 53 42.50 11 1225 40 19.9014 03 54 34 38.60 56.90 ASK 8819 417578 NGC 5774 42 01 22.50 1186 14 58 59.70 CGCG 221-010 53 55 23.70 2142 NGC 2205 582115 1803 01 40.3015 02 25.40 1566 49 22 2495 15.0015 48 07 52 07.70 39.60 KUG 1500 NGC 583515 01 09 32 13.20 39.20 NGC 3344 5850 52 31 42.30 NGC 5875 7985 2544 3506 – F 3 3 3 1 1 3 1 1 3 1 3 1 3 3 1 1 1 NF NUF NC A N A NZF NF N R R C C C C C C C C C C C C C C Table A.1. Source2201 RA Dec Name 220222042206 2207 2208 14 40 26.102211 14 40 42.002212 33 59 20.802213 40 39 38.90 NGC2214 5727 PGC2215 3088035 14 42 16.502216 14 42 29.602218 14 60 42 52 33.20 23.302219 01 30 01.40 2MASX2220 28 J14421771 43 35.20 CGCG2222 019-084 NGC 57352223 14 43 49.202224 3512 1499 2226 53 24 02.302227 NGC2228 575122312233 1907 14 46 11.102234 14 46 20.202235 -00 14 13 46 22.60 21.10 3724 2239 14 04 47 43 21.00 58.70 NGC 57502241 34 22 14.002242 ASK 101615 48 54 04.60 UGC2243 9519 14 48 42.60 2MASX 3289 2244 J14472098 2245 14 12 51 27 06.70 25.902246 14 51 14.40 NGC2247 5762 02 31 26.902248 35 32 32.10 ASK2251 83982 14 51 38.90 1659 UGC2252 9562 14 1515 52 07.902254 40 35 57.00 -022256 1640 31 47.00 NGC2258 5772 14 54 NGC 36.20 576822602261 14 48 56 40 01.60 06.802264 1780 14 58 46.102266 -01 ASK 23 244132 17.20 2070 2269 15 02 00 58 00.40 08.50 UGC2270 9601 1276 15 00 01.302271 KUG 15 1456 01 00 53 26.40 28.702273 -01 05 15 28.10 00 46.102278 NGC 4870 15 5806 01 01 37 32.40 28.00 CGCG 1934 020-0402279 49 59 37.10 NGC2281 5811 48 19 11.00 NGC 5828 15 2256 05 26.30 UGC 9665 15 46 08 33 33.50 54.20 1869 UGC 9703 52 17 46.10 1887 NGC 1346 5875A 1526 4059 2557 2508 2481

Article number, page 49 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.450.75 8.30.40 8.70.80 11.0 5.40.52 12.8 18.02.74 8.63 22.7 9.5 31.40.20 9.40 -0.55 4.0 59.90.64 13.4 -1.08 8.78 9.680.50 10.58 8.0 8.00.13 15.3 -1.49 1.96 -0.36 5.80.34 17.5 9.87 8.30 4.40.47 10.9 8.30.36 9.96 13.0 9.87 1.07 3.30.46 8.82 13.1 -0.64 5.9 24.80.45 7.58 -1.51 5.80.47 8.94 9.39 3.8 8.00.65 0.50 10.8 6.9 0.17 0.61 20.4 9.64 8.00.36 — 8.98 15.4 5.30.55 58.0 0.51 -1.21 8.84 4.80.17 9.11 12.5 5.1 9.890.25 -1.77 3.5 0.55 0.32 5.9 -0.30 20.7 9.86 11.10.34 13.1 8.72 -1.19 0.24 4.4 32.5 9.70 9.90.38 18.0 2.35 8.5 7.70 -0.83 8.950.23 19.2 8.5 8.690.62 10.2 0.26 0.62 4.80.52 8.85 15.7 0.68 3.20.34 8.39 19.2 -0.58 6.20.60 8.78 13.9 5.0 0.80 41.30.46 8.56 -0.43 6.00.23 23.6 9.96 9.37 8.60.25 2.29 38.5 10.7 8.93 -0.66 0.72 1.60 17.2 3.10.23 53.1 9.50 1.53 4.60.25 9.04 17.5 9.15 3.29 3.90.24 11.4 4.2 9.04 0.29 21.5 0.07 8.05 5.40.34 9.56 13.9 8.63 6.90.38 38.9 0.82 -0.93 6.50.24 25.3 22.2 0.80 7.830.35 71.5 43.9 8.16 9.030.41 47.1 0.61 6.4 9.400.38 65.9 0.78 0.48 7.6 9.000.33 34.0 0.67 9.61 8.40.45 -0.14 15.0 5.40.44 74.4 0.20 8.77 3.50.57 9.52 10.2 8.9 9.250.29 0.24 5.0 9.52 4.40.42 9.35 15.8 12.8 9.25 8.73 4.6 9.3 3.12 22.1 9.78 0.30 -1.12 9.93 9.08 7.3 -1.34 9.08 8.91 8.91 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 65 187 4459 2228 479 4917 2.97 5052 8.50 576 6435 646 15.18 33 662 18.73 3995 14.27 4 57 4302 22 128 1.52 7.16 1665 39 1559 188 2539 0.22 2.65 2412 7.14 276 202 266 3666 3.12 247 2.23 395 128 4.28 23.70 1 15148 93 1.30 5 61 129 116 101 44 187 4.74 9 2.93 2 3.60 77 2353 253 1.23 8 255 1154 281 2191 2.06 152 13.44 2908 2556 4.63 60 3162 3.93 72 431 4.98 853 48 90 452 6.73 0.58 2 91 5.32 761 113 1021 2.58 210 170 0.97 9 76 230 12.99 1 250 11.14 5 99 2417 298 215 9.04 2 266 137 3.78 234 136 17.49 2 1566 2.14 152 1.23 86 262 3.53 116 283 3.64 1.96 / HI 26 145 243 1.91 10 347 38721 3.38 68 15813 1.30 4081931 457 349 51 4.87 418 125 3.71 14 0.32 16 132 50 214 104 3.05 0.65 2911 29 128 114 239 0.57 11 3.55 84 134 1.54 33 84 202 2.33 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 23 1.743 0.15 -19.213 2.11 -17.715 10.48 1.90 -18.628 -12.23 6.82 2.04 -20.965 11.16 0.22 -20.46 3.71 10.94 -8.91 -11.56 1.34 -14.903 -11.21 -20.57 2.752 3.60 2473 — 7.23 0.234 2.27 10.60 0.67 2515 -14.214 2549 -9.10 -11.13 0.78 -18.04 —3 6460 0.69 7.07 -18.632 2.84 3.36 11.57 1.54 8.77 -19.152 -9.18 9.38 1.73 -19.084 1656 -9.49 5153 3296 9.13 0.59 -10.40 -19.562 2.31 10.19 1.38 -17.862 2.94 10.60 -9.78 -11.34 3.68 1.50 -19.224 1905 -10.36 8.56 0.46 -20.992 3.18 3.01 10.19 2628 1.33 2660 -16.497 2.96 11.05 -9.05 -11.01 0.39 8332 -20.352 2531 0.33 -12.13 6.37 -14.883 3.22 10.53 3.53 2539 0.39 -16.891 -10.50 3.15 -10.58 0.69 7.45 -16.463 2488 2619 0.47 8.33 3.20 -19.142 5544 2.94 -9.33 0.91 8.01 -15.563 -10.34 0.06 9.43 -18.13 2890 4 5314 1.69 -9.46 1.46 7.59 2.50 -16.661 -9.81 9.21 1.20 -21.12 1797 1 3.42 -9.40 6.27 0.42 1986 -17.77 2.722 10.62 -9.89 0.79 -17.00 2.985 1871 -7.40 7.77 1.71 -17.99 2.807 2014 7.40 0.87 — -11.58 -18.12 2.433 2046 6.20 0.30 2025 -18.403 -8.69 4.33 3.39 1.83 3418 -14.446 — -8.40 9.08 0.07 -19.159 3.03 0.38 9636 7.23 1911 -11.68 -15.571 4.09 10.49 0.46 -14.11 —1 1955 -9.54 -11.14 0.08 2.69 7.83 -14.503 4077 7.22 0.25 2.81 -17.366 2.90 3.68 -9.40 7.38 1.07 2090 -18.702 -9.64 0.63 8.55 2146 -11.09 -17.553 2.85 2004 3758 0.43 8.72 -18.462 2.50 -9.31 1.12 2.60 9.14 -17.832 1852 -9.02 9.40 0.99 1569 -18.53 -10.312 2.05 8.53 0.30 1758 -18.593 2.82 0.58 2.70 2550 -18.163 — — -9.24 1.36 -17.102 1993 — 1.57 6.22 1366 -21.15 2.58 3.283 8.44 1.09 — -21.71 10.90 -8.50 1.38 2820 — -16.26 3047 11.27 -9.52 -12.55 2.62 -20.08 2.35 -12.30 2.51 3.94 3.86 — 4263 4.41 4659 — 1450 3008 5972 8682 — — 2.93 2.73 2613 2936 5 0.85 -17.61 9.18 -10.39 3.27 1730 / 34 1.56 -20.74 10.33 — 2.75 2011 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± km 4820036 2828 4703541 3032 + + . (J2000.0) [log] [log] [log] [log] continued 15 15 05.2015 15 05.20 6115 12 16 10.00 10.20 4215 12 16 33.90 43.00 VII Zw 10 591 30 23.40 NGC 590015 55 19 24 25.30 46.70 UGC 979415 20 55.40 NGC 5908 45 52 48.90 -02 34 40.50 NGC 5918 NGC 591315 26 06.1015 26 07.90 2508 41 40 14.30 2496 15 41 26 40 41.50 33.80 NGC 6710 592915 29 45.00 NGC 3425 5930 40 33 52.20 42 55 07.20 UGC 5146 9858 2013 NGC 5945 2486 15 2633 41 29.9915 41 59.50 27 2613 15 59 42 11.40 18.80 00 5493 15 42 43 45.40 48.71 Ark 484 0015 28 45 38.50 39.10 UGC 9977 57 13 59.70 UGC 997915 28 55 05 22.40 18.30 UGC 1000215 59 02.99 IC 4582 02 55 15.10 51 18 16.80 ASK 104991 UGC16 10123 02 02.1016 05 45.89 18 49 03.30 9574 1917 41 20 41.10 UGCA 1955 411 4063 UGC16 10200 18 29.9916 18 47.60 2138 2216 1998 09 20 47.30 31.99 07 24 52.50 3749 UGC 10327 34 34 11.40 NGC 610616 25 49.99 ASK 24734916 30 06.10 4016 29 34 19.30 24.60 2536 27 41 1991 57.50 NGC 6150 21 32 17.50 UGC 10419 NGC 6186 4233 1423 4578 8747 2601 2936 – F 3 F 1 3 3 1 1 3 1 1 3 3 3 1 1 NF NC NZP F NZ A N N NUZF NF N R UF C C C C C C C C C C C C Table A.1. 22872292 2293 2295 2296 15 11 40.9022992302 59 48 32.102303 NGC2304 58942306 15 18 32.1023092310 31 09 40.202312 15 21 12.50 ASK2313 395533 15 21 58.502314 15 46 23 07 51.70 52.802315 15 41 24 07 30.50 31.20 ASK2318 58 244982 03 10.50 -01 2463 UGC2320 14 9827 18.90 UGC2321 9837 15 26 ASK 30.30 20264523222323 41 17 22.302324 15 1656 29 56.702328 UGC 9856 15 30 00.902329 15 58 30 26 16.70 35.902332 15 23 1909 30 38 47.30 18.202333 ASK 15 111892 03 31 17 52.90 21.502334 IC 2644 15 1124 23 34 03 49.10 57.902335 ASK 8339 2662 15 45 104131 35 25 36.10 50.502336 UGC 15 9875 28 39 39 02.40 18.90 CGCG2338 15 249-027 00 40 22 54.30 31.00 NGC2339 31 5958 45 35.70 ASK2340 20724 56 2476 51 38.90 NGC2341 5974 SHOC5132346 2889 23472348 15 1797 45 44.502350 5305 1866 2352 1999 20 33 37.402357 15 59 12.50 UGC2358 2010 10020 15 59 55.50 2045 2359 16 44 01 42 48.40 59.302360 2015 06 53 02.60 3420 2361 ASK 06 253830 50 18.40 PGC2362 4573815 16 08 17.30 PGC2363 4568096 16 09 20.742364 16 07 11 32 11.51 18.602365 08 45 47.70 IC2366 1197 48 20 04.00 2087 UGC2369 10225 2MASX2370 J16111153 16 20 47.40 16 1854 25 30.50 1564 47 03 53.90 1755 49 50 24.90 2MASX J16204742 NGC 6154 3045 1360 5964 Source2285 RA 15 10 16.50 01 56 03.30 Dec UGC 9746 Name 1731

Article number, page 50 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.440.67 11.70.26 5.20.21 21.4 13.80.44 12.3 6.8 9.730.32 21.3 6.4 10.330.43 10.5 0.25 8.17 8.31.03 -0.84 11.6 5.10.58 18.0 1.22 7.62 3.00.29 9.84 9.15 6.5 9.10.37 0.65 30.8 -0.05 5.50.42 9.15 10.7 8.92 7.70.22 30.2 9.38 7.50.35 -0.39 9.24 14.4 9.72 3.80.42 0.37 11.8 16.9 10.11 2.50 0.52 -0.19 12.2 3.4 22.60.28 -1.09 9.88 4.30.22 23.0 8.25 -0.60 9.55 6.00.39 7.3 9.63 7.60.39 0.43 9.55 10.1 4.70.27 -0.91 9.79 4.4 7.40.34 9.73 13.1 9.50.23 -1.38 7.96 -1.44 3.8 6.80.26 21.2 9.49 3.40.30 13.4 0.57 9.32 8.35 7.00.29 0.26 6.4 7.7 20.60.27 -0.69 1.78 9.30 3.60.18 15.1 9.19 9.93 3.40.20 0.06 4.5 4.50.40 -0.89 -0.80 9.66 3.4 3.40.20 11.0 -0.24 8.570.28 6.5 9.00 5.40.34 5.0 21.0 0.51 2.6 9.120.20 -1.37 4.6 9.12 9.38 9.40.24 0.31 2.6 3.10.32 -1.88 0.37 9.04 4.9 6.10.29 7.62 5.4 3.50.36 0.54 9.80 3.2 6.80.39 1.45 8.86 3.3 9.50.35 2.95 15.3 9.25 2.80.20 10.3 0.65 9.28 5.4 32.50.61 2.88 9.28 5.0 22.50.18 0.88 8.71 9.95 4.2 -1.88 0.36 9.79 7.2 6.90.52 0.35 0.06 3.8 8.80.28 -0.19 10.0 9.51 5.10.50 10.10 4.1 6.20.27 9.14 2.62 10.5 -0.99 9.80.33 8.80 5.3 10.36 9.14 5.60.19 16.3 5.0 -0.97 0.46 9.41 4.6 6.4 9.49 8.6 0.44 8.62 0.32 6.8 9.72 0.81 8.99 9.72 0.31 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 37 2661 4855 2904 90 5125 57 5.93 303 105 5.50 129 80 321 3.36 4 167 0.95 1 3.31 1288 3.30 3 27 149 295 5252 3.78 52 3411 545 280 4.29 3.44 2933 4.65 2983 308 2065 5.07 7 86 6.23 220 2183 264 1049 1.84 237 145 288 0.95 2032 2.39 174 1.70 229 121 3.44 7 1.51 148 368 3.25 3 3845 202 0.60 165 2288 186 5.26 148 1.16 7 163 1392 0.45 9 156 2345 212 0.52 261 1422 278 7.94 163 1776 4.62 7 0.86 191 3994 2536 1.16 422 163 275 111 3.70 192 1.03 133 4.97 1.03 / HI 1411 148 312 198 335 2.23 25 3.62 2412 90 428 0.27 467 2.55 21 2272135 276 26913 1.07 96 36432 139 185 2.64 146 182 0.62 11 22211 0.71 74 0.55 1511013 94 189 141 133 0.51 10 1.30 178 182 186 1.00 1.74 21138 1.21 39317 507 161 3.23 20613 1.31 11 364 149 410 186 1.82 0.77 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 32 1.505 0.65 -21.603 0.33 -13.862 11.17 1.09 -13.834 -12.03 6.95 0.31 -19.252 6.97 0.84 -18.162 3.27 -9.31 9.89 0.63 -18.323 -9.30 0.74 -10.13 -18.36 2.753 — 8996 1.02 9.31 -16.86 2.517 2.67 9.02 1.43 -19.79 -10.271 960 6.74 1.94 — -21.879 -9.55 961 9.91 0.39 3.31 6614 -10.11 -21.613 11.20 2.66 0.33 -10.66 -15.77 6.133 10.48 2776 -11.93 5.13 1.39 -17.552 -12.02 4.42 7.81 1.49 3734 2974 -21.392 2.24 1.48 3090 -23.291 1.97 10.54 — -9.75 0.26 5027 -22.906 11.18 8808 -12.17 0.55 -14.951 2.58 11.17 5799 -12.22 1.13 -18.61 —4 2.60 -6.28 -12.81 7.40 3718 -19.713 2.65 0.55 -14.32 9.23 2.204 10.00 2.07 -9.52 3792 1.51 -18.95 7116 3 6.58 -9.57 -10.59 1.31 3798 -18.727 2.29 7750 9.24 1.48 -22.593 -9.67 2.80 2.51 10.08 0.63 -20.044 10.73 1418 -9.90 -10.43 1.54 2.23 -16.603 5183 5046 -10.84 9.91 0.52 -19.481 2.46 1.51 1.56 8.06 -10.10 1168 -17.815 2.32 10.37 0.75 -22.56 5482 1 5241 -9.60 -10.33 0.35 1.74 8.81 -18.843 10.99 7398 0.35 -16.975 2.30 1.49 6009 -9.72 0.69 -12.22 9.01 -15.903 0.36 8.50 -18.35 3506 2 1.50 1.49 -9.98 5835 0.96 6.17 -16.80 -11.083 0.30 6.85 -17.97 6206 7006 2 2.90 1.83 8.21 1.57 -17.536 — -8.93 6.37 0.42 -20.885 3093 -9.41 8.40 0.74 4436 -10.70 -17.39 3.11 2.782 11.16 1.03 -20.01 1.732 -9.12 10060 -11.90 2.01 8.36 0.27 1305 -20.67 9.89 1.45 -18.13 2.592 2.58 5799 6063 -9.18 9.98 -21.513 6.89 0.53 4759 -10.36 2.732 11.10 — 8718 1.69 -17.565 -9.45 -10.63 2.30 0.54 2977 -23.81 2.623 8.34 0.80 -19.07 1.702 3.00 11.33 0.56 5268 -18.184 4824 -9.38 -12.38 0.89 8.97 -16.30 9039 8795 9.17 0.71 -18.50 2.75 2.84 -9.43 7.82 -10.62 -16.44 3174 11325 1.87 — -9.28 3.93 8.68 2.51 7216 -9.46 3589 — 1.53 2907 1.79 5111 7772 3 1.00 -18.37 9.48 -11.02 2.80 4350 / 14 1.02 -19.37 — — 1.42 4955 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± km 3430296 6605 0115175 5458 0056318 2976 + + + . (J2000.0) [log] [log] [log] [log] continued 16 36 32.60 39 01 40.3016 42 28.90 NGC 619517 00 14.60 3417 30 00 30.30 45.10 23 06 22.80 2MASX J16422897 17 23 10 02 10.40 38.30 UGC 10650 NGC 627617 61 11 21 59.70 01.9020 35 23.80 UGC 10745 23 22 47.70 -06 1420 37.90 55 21.60 NGC 8989 630820 55 MCG 27.60 -01-52-008 -01 12 24.10 -01 1321 30.80 02 ASK 03.50 224823 2964 UGC 11649 -06 17 48.70 2732 2MASX J21020359-061748821 20 3087 06.00 5795 21 11 7721 23 55 18.40 06.30 8814 CGCG 426-04021 01 30 15 25.88 18.10 3718 21 35 03.60 -00 2MASX 28 J21231841 27.70 3787 21 10 41 57 2MASX 11.20 36.20 J21302589-0028272 ASK 138954 12 43 15.80 5964 ASK 139485 1146 21 45 22.60 12 16 06.3021 52 37.90 ASK 13952021 3490 54 17.99 1221 32 56 09.00 19.80 00 6206 56 31.50 CGCG -01 427-032 1022 03.50 00 44.10 2MASX J21541799 22 03 UGC 15.99 11853 1222 18 05 03.00 42.20 00 34 15.90 ASK -00 140028 3322 40.60 19 57.20 NGC 7189 5776 22 20 ASK 19.80 22128 -07 39 58.10 -08 8724 46 17.00 2MASX J22195727-073958222 21 33.70 2MASXi J2220198-08461722 22 08.80 11328 12 4817 31 22.30 12 04 24.10 7288 ASK 140519 8800 ASK 141077 4945 9020 7771 5125 – F 1 1 1 1 A A A 3 3 1 3 3 3 1 1 1 3 2 2 1 1 1 1 1 1 1 1 N N F NC N A A A A A A A N A C C C C C C C C C C C C Table A.1. 2374 237623772379 2383 2384 16 40 21.402385 16 40 22.202389 28 45 55.902390 28 28 17.50 ASK2391 406178 ASK2392 406174 17 01 12.9023932395 17 60 11 15 40.20 05.002396 Ark2398 514 59 59 44.302399 20 41 56.90 IC2400 1248 -052403 17 56.50 977 2408 21 01 963 ASK 07.70 1200562412 2413 -00 11 21 42.60 03 47.202414 21 14 44.80 NGC 70012415 -00 49 21 49.70 16 32.902417 10 52 21.40 ASK 225125 3743 2419 21 11 20 29 21.10 43.40 CGCG2420 426-026 CGCG 5021 2421 426-030 21 10 26 19 57.80 14.10 3717 2422 -07 CGCG2424 01 426-041 17.502425 21 40 NGC 20.90 7065A2426 7109 2427 21 12 41 21 53.70 17.202428 1410 21 5261 44 39.402429 -06 CGCG 42 21 427-012 5044 31.80 44 44.702431 -06 41 21 22.70 44 51.70 NGC2434 7108 21 01 5244 45 13 16.30 55.20 FGC 2339 -082435 45 36.80 ASK2437 21 11 227703 45 02 31.50 29.10 PGC 9995602438 21 7391 50 35.10 -07 ASK2439 14 139251 27.602441 10 53 5811 10.70 ASK 2573822443 ASK2444 139593 21 58 05.802445 6883 -072446 50 42.60 3090 2447 4441 2MASX J21580576-0750428 1286 2448 22 10 20.60 10094 2449 -092450 11 5265 31.40 6081 22 20 ASK 47.30 134108 4749 22 21 00.00 14 14 04.60 -09 38 30.20 UGC 11992 ASK 135097 3175 3595 2901 Source2372 RA 16 34 55.40 20 34 43.70 Dec UGC 10453 Name 4361

Article number, page 51 of 71 ? HI A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 M M

HI M NM / SNR S s / HI F 0.170.27 5.30.32 21.30.31 4.3 8.00.20 30.7 5.00.29 8.71 8.79 4.8 5.60.20 3.5 7.60.33 0.34 1.36 8.06 5.7 5.10.29 11.2 9.19 6.00.22 8.06 7.85 5.6 8.70.24 21.8 2.69 9.40 3.30.29 1.16 10.0 9.06 5.9 9.680.33 0.27 6.6 4.30.19 9.65 0.48 10.8 0.67 5.10.29 11.0 -0.32 9.23 3.60.33 9.11 4.7 8.10.24 8.86 43.3 9.23 0.52 0.17 5.6 9.28 7.8 8.86 0.49 6.2 70.1 8.86 4.00.37 0.42 11.8 9.16 9.9 9.320.44 -1.24 7.6 2.70.18 -0.31 9.13 26.0 0.80 8.80.24 12.4 6.98 5.70.28 9.13 9.95 15.4 3.60.35 9.47 17.9 0.19 -0.69 8.60.38 9.37 4.9 4.20.22 9.47 28.3 35.1 8.37 9.37 0.24 8.76 4.4 9.00 7.50.36 60.4 0.97 9.90.39 -0.75 -0.13 9.66 4.3 9.66 3.90.31 14.6 4.50.27 -0.17 41.8 1.67 8.400.15 8.1 8.84 3.40.58 6.8 81.6 2.27 8.75 4.90.33 1.60 2.9 9.32 9.570.21 4.5 0.89 4.20.18 8.0 0.65 8.56 3.20.43 5.6 — 7.6 8.62 7.40.43 2.49 5.6 9.82 4.20.23 11.1 0.51 8.95 3.70.28 -1.00 14.2 12.2 8.780.10 8.33 0.40 6.30.31 6.2 21.2 -0.49 9.39 4.2 0.93 0.47 10.2 -0.09 9.8 9.98 8.510.39 17.8 5.20.15 -1.35 8.68 20.6 0.55 7.00.37 43.1 18.4 8.460.19 1.15 9.13 16.5 10.14 13.90.42 21.2 -2.42 -0.09 4.4 -0.27 0.43 32.2 9.25 9.9 9.190.34 9.89 4.8 6.1 0.38 -0.55 17.9 7.8 -0.59 8.81 9.7 9.64 13.3 10.02 0.72 -0.30 8.96 -0.76 0.19 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 62 127 63 1516 0.84 936 58 4.47 3 1758 78 219 199 2862 0.57 2424 1.10 318 1476 4.58 1259 1.85 158 184 147 2111 1.64 2083 1.97 234 157 1.67 1139 0.66 1818 132 365 14.24 4 235 1.72 432 162 2812 7.83 1895 2.82 1031 4.19 2895 128 2623 308 46 4.66 290 1.72 81 14.25 1 62 1076 227 0.48 119 2.02 248 133 15.80 0.76 6 25325 277 93 1244 3.34 1162 147 1838 2.84 3271 1.75 210 1882 354 45 3.89 228 170 13.02 4 3.23 69 202 2183 1.66 7.28 249 151 4.64 171 2.80 / HI 2013 87 14913 148 195 174 0.89 1.38 20711 1.07 146 17410 0.59 19512 228 30 1.11 15 6310 0.21 63 81 123 108 0.75 0.57 1321 136 193 17620 25934 1.69 11518 1.54 32720 184 16014 399 127 0.63 21315 49 1.99 171 1.40 235 121 0.52 13 275 0.86 40 1.72 8015 0.26 13814 187 356 0.66 405 2.70 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 21 0.513 0.03 -17.277 0.46 -16.729 8.38 0.84 -16.802 -0.41 7.42 -15.791 -9.39 0.62 -14.633 — -8.44 0.52 6.50 -19.294 1.54 6.69 0.47 -18.193 3.02 -9.02 1.30 9.14 -18.40 —4 -8.26 3559 8.58 0.58 -19.045 2.44 1686 -9.82 0.59 9.01 2.81 2.43 -17.782 -9.39 1.06 9.98 4829 -17.92 -10.343 2.19 1644 0.60 -17.37 -10.53 1599 2 1.58 — 8.59 1.48 2.33 7000 -18.663 0.85 1.77 -20.473 4624 — -9.73 0.67 8.85 4645 -19.112 — 10.10 -0.16 7110 -17.212 2.07 -11.15 0.37 -16.47 9.47 1.837 — — 1.49 8.53 -13.812 4014 1.33 -9.83 7706 0.84 2.63 -22.66 -10.37 — 2.50 0.35 6.79 -20.175 2.09 10.64 4810 2.68 2777 -18.317 4842 -9.27 1.18 —4 5197 — 0.81 -18.25 — 1753 2 2.33 — 2.26 1.15 -19.267 0.30 9.51 2.58 -20.17 —2 963 0.32 9.13 4030 -16.78 -10.831 — 9.83 0.51 2.43 4840 -16.05 -10.542 0.50 7.98 2.48 3.51 -10.54 -15.445 0.65 6.12 2.68 4662 -15.883 -9.09 4605 0.56 2.19 7.24 -19.752 3399 -9.72 0.61 7.87 2114 -18.333 2.40 -9.08 0.53 9.32 7472 -16.892 3.01 -9.44 1.33 8.93 -17.013 2.54 2567 -9.63 0.67 6.07 -21.189 -10.10 2.96 3283 1.02 8.11 -17.183 10.81 2.67 -8.48 2668 0.26 2.13 -18.014 2625 -9.48 0.76 -10.59 8.55 -15.809 5304 2.57 1.38 9.27 -19.394 2216 1.21 3.20 -9.67 0.29 7.40 -22.243 -10.18 3136 0.51 9.48 -15.041 3716 8289 2.47 11.33 -9.22 1.70 1.79 -14.99 -10.504 0.87 -12.30 7.96 -20.50 3636 2 1.81 4892 1.21 7.54 2.83 -18.395 10.88 2.90 0.74 2290 -20.524 — -9.55 -12.35 0.90 9.21 10701 3888 -18.542 10.42 1.44 -19.772 2.30 2.54 1.27 -9.71 -10.47 0.34 8.88 -20.233 0.88 9.74 -16.76 4846 3 2.30 10.48 2.74 1533 2398 -9.95 1.46 -19.73 -10.23 -10.68 0.82 8.09 -20.82 2.80 2678 4702 9.94 1.91 -17.40 2.84 10.78 -9.18 3386 -9.85 -10.57 8.77 4396 1.52 4712 2.88 2.39 -9.99 4486 8932 2.83 4407 2590 / 20 0.20 -15.36 7.40 -8.99 1.80 2549 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± km 0046511 4903 + 137130 7102 5197 134 2652 131 2582 + + + + 00-57-004 4663 + . (J2000.0) [log] [log] [log] [log] continued 22 27 26.70 12 05 40.30 ASK 140924 3547 22 27 30.7022 27 41.50 -09 3922 53.90 27 54.20 -09 43 36.70 ASK135512 -01 08 57.20 MCG -02-57-007 ASK 2321922 34 36.8022 00 39 10 31.31 24.30 -00 MCG 40 36.1022 40 1643 48.20 ASK 23608 1697 22 40 57.58 -01 09 13.60 -01 15 08.70 4832 ASK 23496 PGC 112319722 49 44.87 7728 15 05 21.00 UGC 12205 4842 4747 22 59 07.2922 13 59 43 32.60 16.60 KUG 2256 13 40 39.00 ASK 142526 3399 23 06 04.70 2627 14 52 01.60 UGC 1235923 14 13.20 13 25 34.90 NGC23 7536 17 07.6023 13 18 25 15.70 22.80 10689 ASK 143813 00 15 40.10 NGC 7589 4695 4470 8932 – 1 P 1 1 A 3 3 1 1 1 2 3 3 N NC N NUA NF N U C C C C C C C C Table A.1. Source2453 RA Dec Name 2454 2455 2456 2457245924602462 2463 22 30 36.792464 22 31 02.302465 -00 22 06 31 36.90 58.962466 -09 30 04.20 PGC -09 690182468 47 22 52.40 36 25.90 PGC 9902482469 ASK 1353972470 22 14 39 01 34.70 26.302471 22 39 49.502472 -09 KUG 22 2233 17.002473 -08 23 22.90 ASK2474 135833 22 41 PGC 10.602475 069438 22 41 33.872476 22 13 41 20 1580 34.60 23.602477 6980 22 00 43 24 59.92 03.002479 -08 KUG 4655 48 22 2238 25.70 44 24.402480 -10 UGC 22 07 12151 47 01.00 04.20 ASK2481 136034 -00 09 43.50 ASK2484 -00 136263 04 22 27.20 51 12.25 NGC2485 7364 4023 22 53 04.47 UGC 121832486 2788 22 12 58 46 10.06 47.102488 22 01 58 08 28.30 40.002489 ASK 142691 14 18 30.502491 -10 NGC 33 22 7402 32.20 59 24.562493 NGC 7437 FGC 1768 2494 2436 -10 29 4031 22 14.90 59 50.422495 23 00 957 13.20 PGC2496 4125627 23 13 01 44 18.70 09.802497 4844 -09 23 56 01 39.40 4675 26.402498 ASK 23 143127 14 02 20 39.60 22.40 2MASX2499 J23001322-0956393 2549 23 00 02 51 40.30 54.002500 -01 UGC 23 13 12308 03 50.40 16.802501 ASK 23 25059 13 4625 04 5285 19 04.10 44.60 PGC2502 3092568 23 13 2098 05 33 56.30 48.302504 CGCG 7469 23 430-054 00 05 46 56.50 50.40 3295 2506 -10 ASK 02 143002 57.002507 2MASX 23 14 J23040415 06 21 14.90 27.60 ASK2508 136890 23 07 2624 20.102509 UGC 23 12354 14 12 39 21.40 27.402513 23 13 14 05 05.40 59.30 2211 2514 PGC 4019347 14 36 33.70 3694 2516 3068 ASK 23 143524 13 14 10 8289 17.20 40.202518 NGC 23 7509 14 33.102519 -09 UGC 50 23 12434 10.30 16 3614 44.70 00 14 09.50 MCG -02-59-007 2279 23 13 17 28 36.40 58.80 UGC 12446 3883 NGC 7570 23 14 18 00 33.60 04.30 1542 NGC 7580 13 2401 26 17.80 KUG 4862 2316 3396 2673 4391 4718 4410

Article number, page 52 of 71 ? HI van Driel et al.: NIBLES – the Nançay HI survey M M

HI M NM / SNR S s / HI F 0.580.25 25.00.19 3.70.14 54.3 3.60.44 4.2 9.690.26 2.8 5.70.52 3.5 -0.94 5.6 8.63 5.10.23 8.68 7.9 9.40.35 -0.19 8.43 3.7 7.60.30 -0.12 12.3 13.3 9.800.34 0.05 9.25 7.0 6.20.15 22.7 -0.50 9.58 5.00.46 0.10 11.2 -1.05 8.81 6.2 9.600.20 11.4 9.00.20 9.32 8.81 0.27 6.60.24 7.9 19.9 8.66 -0.63 4.10.30 12.2 4.8 8.37 9.660.29 1.52 4.8 4.60.33 9.31 -0.52 2.19 9.2 8.80.31 23.2 9.07 8.60.18 0.21 13.6 9.00 5.70.29 35.5 0.52 9.16 3.80.12 9.49 31.8 0.19 9.35 8.60.33 0.65 5.1 0.19 4.60.39 54.4 23.4 9.35 8.550.18 9.06 5.9 9.870.41 6.3 38.6 8.55 3.20.27 -0.71 13.8 11.6 0.50 8.05 9.420.24 3.90.25 3.8 30.0 -0.29 9.37 0.49 3.00.58 5.4 8.40 -1.73 9.100.33 8.7 3.50.30 4.7 0.37 0.13 3.8 9.960.17 8.5 5.6 8.970.28 5.6 -1.07 9.32 9.80.17 6.7 -0.06 10.05 8.40.30 6.0 -0.66 15.7 3.5 9.44 -1.33 0.27 12.1 9.41 5.20.17 -0.08 9.56 5.50.45 5.2 -1.22 9.69 3.70.43 6.9 0.11 8.98 5.1 -0.15 0.20 9.4 7.6 9.040.31 5.8 -0.46 10.0 9.58 4.00.34 17.7 1.15 7.6 9.03 10.160.26 -0.31 19.4 10.20 6.00.16 -0.20 13.1 1.48 6.8 42.20.55 -0.84 9.26 8.0 10.180.18 10.33 11.1 5.70.40 -1.40 -0.70 17.9 6.0 -0.60 9.58 47.7 13.6 9.56 10.1 101.6 -1.21 10.44 -0.28 9.24 -0.15 9.55 0.95 1.05 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 1 5106 534 100 20.26 65 120 132 2543 0.43 1568 282 188 1.22 1064 4.36 2142 148 1103 4.92 2306 1.87 131 211 249 197 0.73 2266 5.83 2151 1.57 132 0.58 92 1721 113 2.30 1731 6.86 5 199 1457 5742 9.70 170 1194 596 190 7.60 135 493 2.97 2166 0.43 507 7.51 6399 1.63 2 655 3894 1706 2.22 425 2517 187 1679 1.18 277 89 1.71 183 245 2.15 1155 0.57 282 423 1.21 9 1.63 5 452 393 196 5.02 443 265 2.69 1 8.43 183 225 23.82 / HI 1011 235 17521 261 203 297 0.44 11 0.41 383 217 2.48 22 246 75 0.87 15223 1.40 28 167 72 24517 16410 1.18 57 1.14 15511 124 183 38 1.19 0.51 7919 0.33 27 13621 65 176 239 168 0.66 296 0.90 1.34 2616 71 25614 140 318 274 0.48 13 2.78 31614 34213 0.76 22911 407 351 310 120 1.79 407 1.71 167 4.84 1.05 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 22 1.502 0.55 -21.741 0.80 -17.935 10.63 0.50 -17.282 1.21 -12.39 8.82 -17.682 0.58 8.80 -21.386 2.73 -9.70 1.46 8.38 -18.776 10.30 -9.86 1.64 -20.753 1.68 -9.45 -10.34 2231 0.75 9.15 -18.681 1.48 10.63 0.95 -18.62 4492 3 1.37 -0.16 2.49 -9.61 -11.53 -20.94 4922 4 — -15.65 0.44 9.325 7256 2.29 3.37 3624 1.07 9.95 -15.994 -10.49 7.14 0.85 -20.373 — 5480 -9.93 4263 0.65 6.17 2.60 -17.932 -8.58 10.18 0.77 1.57 -17.756 2.65 -11.31 0.50 9.10 2.97 -17.70 4075 — 0.77 3913 8.55 -17.763 3.18 4803 -9.99 2597 8.81 -18.295 1.46 -9.67 8.51 0.25 -10.203 1.45 4034 9.30 1.01 -15.362 1.47 2569 -9.28 0.94 1.70 -10.04 -20.34 5183 0.65 -18.422 2.56 6468 — 4197 2.40 9.77 -16.546 1.77 9.36 5164 2 -10.25 0.51 8.35 5300 -21.082 -10.20 — 0.99 1.45 -16.402 11.10 -9.92 1.46 2.23 3.02 -17.473 6850 -11.65 0.59 8.02 -22.895 1.41 0.93 2500 8.97 -19.173 3969 -10.04 11.04 1.75 1.66 -21.082 -10.26 2641 1.02 -10.77 9.03 1.71 -23.227 4031 1.73 9.98 3.01 -18.744 11.38 1.36 -9.51 0.84 -21.19 -10.13 3451 1.10 -11.12 9.52 -18.832 1868 10818 10.64 1.95 2.13 -20.385 2.53 -9.94 0.22 9.452 5429 7015 1.28 9.84 -16.054 — -10.39 10246 2.09 1.00 -20.262 -10.14 1.14 7.88 1.62 1.36 -19.794 6545 1.54 9.89 1.83 -20.613 -9.25 1.53 7.55 -21.283 6755 -10.51 6639 10.36 1.51 -21.803 6853 11.04 3.05 1.29 -10.70 1.80 -21.043 10.66 — -10.29 1.70 -22.943 10.88 2.80 4339 -11.92 0.95 -20.23 6976 8 1.61 10.94 2.24 -10.74 10382 1.11 -20.552 10.79 1.24 -10.44 0.37 6790 -21.24 1.66 8116 -10.39 0.52 9.84 -16.61 7086 2.32 10.59 -18.99 -10.17 10782 1.42 -10.56 8.29 7283 8.49 1.03 6665 3.05 -9.59 6658 10854 1.54 — 5857 2.87 1749 / 23 0.69 -16.5013 — 0.97 -17.30 — 8.93 3.32 2604 — 2.70 2679 11 1.00 -18.52 9.43 -10.26 1.41 5872 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± km 1428506 5879 + 136 5154 + . (J2000.0) [log] [log] [log] [log] continued 23 19 04.80 -08 29 06.30 NGC 7606 2214 23 25 19.10 13 55 14.60 CGCG23 431-062 31 02.10 -00 07 55.00 ASK 2616923 35 3854 40.1023 36 31.30 01 11 53.30 -00 29 43.30 UGC 1269023 36 46.90 PGC 1141927 2589 00 37 24.30 SHOC608 2621 2500 2642 23 56 07.8023 00 56 32 42.00 58.10 NGC 7787 13 46 34.90 UGC 12854 6658 10860 – 2 3 1 N N N N R C C C Table A.1. Source2521 RA Dec Name 25222523252425282531 23 19 09.402532 23 19 43.502533 23 15 19 43 58.00 37.202536 23 15 21 20 51.90 46.202537 -00 LSBC 23 59 F677-02 24 07.90 44.602538 -00 ASK 41 23 144498 40.90 24 49.30 2MASX2540 J23195800-0059077 01 01 48.30 CGCG2541 380-043 23 15 27 16 10.20 32.102542 CGCG 23 380-053 3634 27 14.802544 NGC 23 7653 15 28 01 12.30 02.002545 -09 23 13.102546 -01 UGC 03 23 12601 46.20 32 24.40 NGC 4429 2547 7665 23 32 59.30 SHOC6042548 23 15 34 50 4922 27.80 52.202550 23 7265 00 34 43 35.50 18.802551 -09 NGC 46 23 7691 02.00 34 5480 44.802552 ASK 23 26251 15 35 09 15.20 26.70 PGC 9866912553 13 56 39.402554 UGC 12673 00 4257 02 10.902557 KUG 2332 23 36 34.40 4062 2559 UGC 12685 23 36 37.102560 4804 -09 31 32.002564 2598 23 14 37 09 23.90 26.10 PGC2565 989944 23 38 41.202566 UGC 23 12705 4033 00 39 23 52.00 30.002568 5196 23 6513 15 40 57 20.70 16.602569 -10 UGC 13 23 12709 39.30 41 07.80 4194 2571 NGC 23 7722 01 41 14 13.32 44.70 ASK2572 124322 -01 23 02 41 15.20 23.80 5303 2574 -10 UGC 59 23 12729 30.10 41 52.60 CGCG2575 -09 381-024 53 23 53.10 42 26.03 2MASX2577 J23411334-1059310 -08 23 38 6845 44 53.40 03.00 2MASX2578 J23412383-0953530 23 00 44 15 22.20 21.50 2MASX2580 3976 J23415266-0838537 23 00 45 5425 31 04.86 16.802581 PGC 23 1161165 00 46 7030 05 2678 51.90 46.802582 -00 10284 NGC 16 23 7738 15.10 48 17.502587 LSBC 23 14 F894-05 3442 48 4003 28 23.90 50.40 2MASX2590 10805 J23450487-0016152 -10 44 23 19.60 50 10.402592 -09 1884 2MASX 08 23 J23465184 03.90 50 48.10 ASK2593 124158 -01 23 01 51 00.70 6871 06.20 2MASX2595 J23482382-0908036 23 15 53 39 49.20 04.20 2MASX2598 J23501037-0101000 23 01 55 03 16.10 24.102599 -00 CGCG 23 58 6555 432-034 56 28.00 6980 07.102600 UGC 12810 14 6792 22 31.70 CGCG 6633 -00 381-059 54 23 59.40 6748 56 13.50 CGCG 432-040 IC 1516 -00 32 23 26.50 58 44.00 23 4343 59 37.00 CGCG 382-005 16 05 26.20 10377 14 48 25.00 ASK 146725 NGC 6970 7800 8089 10791 6645 7275 5854 1751

Article number, page 53 of 71 A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 ? HI M M

HI M NM / SNR S s / HI F 0.19 3.0 2.8 9.25 -2.05 0.34 3.5 5.1 8.58 0.78 0.230.18 2.4 2.5 2.0 2.2 8.20 8.48 0.14 -1.52 0.16 2.7 2.2 8.93 2.27 0.23 3.7 4.3 9.04 -1.75 0.15 2.1 2.4 8.38 -0.15 0.15 3.2 4.1 8.46 -0.35 0.12 3.3 3.0 7.65 -0.36 0.250.19 3.2 3.9 1.1 3.2 8.40 8.81 -1.34 -1.48 0.16 3.5 1.3 7.65 1.05 0.22 2.9 3.5 8.71 -0.55 0.16 3.0 3.3 8.65 -2.41 0.17 3.3 1.2 7.18 1.16 0.44 2.9 4.9 9.18 -0.49 0.440.07 2.70.17 3.7 3.5 2.7 2.9 8.78 2.4 7.11 0.27 7.98 -0.08 0.24 0.09 3.0 2.7 7.98 -0.77 0.17 2.4 1.5 8.62 8.62 0.16 3.6 3.6 8.65 0.16 0.17 2.9 3.2 8.05 0.11 0.320.18 4.0 2.0 3.6 3.3 9.19 8.60 -0.76 0.21 0.15 3.0 3.2 8.84 0.32 0.13 3.4 3.7 8.18 0.61 0.290.08 2.2 3.1 2.6 2.6 8.31 8.49 0.41 -1.07 0.24 3.0 3.8 8.22 0.22 0.270.28 2.4 2.4 2.9 2.4 8.28 9.14 0.28 9.14 0.430.67 2.3 3.0 2.9 4.3 9.72 9.83 -1.45 9.83 0.20 2.8 3.4 8.58 -1.04 0.17 2.4 2.4 7.68 -0.33 0.380.14 2.00.18 3.0 2.8 3.2 3.0 8.82 2.9 7.62 -1.13 7.88 7.62 0.28 0.160.26 2.9 3.2 3.7 3.1 8.11 8.55 0.30 0.04 0.42 3.0 3.9 8.29 -1.29 0.370.16 3.3 3.2 4.8 2.7 7.97 7.61 -1.18 0.26 0.16 3.4 3.1 8.38 1.61 0.200.19 2.5 2.5 2.4 3.4 7.33 8.35 0.03 -1.26 0.11 3.1 2.0 6.99 -0.12 0.17 3.5 1.9 7.09 1.02 0.23 3.8 4.5 7.63 -1.07 0.18 3.6 3.7 7.50 -1.66 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 6 138 149 0.29 4 98 107 0.23 6 240 255 0.18 4 94 105 0.13 0 132 132 0.35 6 50 66 0.12 5 23 38 0.11 9 28 48 0.13 9 151 167 0.16 6 52 69 0.32 6 94 106 0.28 7 84 102 0.28 4 34 45 0.13 5 138 149 0.42 77 41 55 58 71 0.23 0.30 8 97 113 0.37 6 248 263 1.02 7 32 48 0.23 9 46 68 0.27 6 23 37 0.11 6 57 71 0.19 / HI 10 38 61 0.28 53 28 156 0.49 35 130 192 0.21 13 103 129 0.21 12 371 404 0.65 12 103 121 0.22 29 73 136 0.31 20 129 187 0.33 16 260 294 0.47 21 354 397 1.36 21 10112 141 57 0.87 81 0.21 19 23 61 0.22 1124 231 128 262 162 0.74 0.35 10 84 99 0.45 28 33 92 0.36 1310 82 62 103 0.45 79 0.38 1217 126 235 148 273 0.73 1.72 10 141 158 0.25 12 258 276 0.66 11 208 233 0.49 44 55 155 0.68 1211 52 135 74 154 0.26 0.40 18 60 106 0.50 24 28 86 0.24 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 6 2.19 -20.07 11.29 -11.27 2.75 11053 2 0.36 -15.97 7.81 -9.28 3.01 3968 2 -0.09 -15.63 8.05 -9.78 2.07 3350 2 1.37 -19.15 10.00 -10.55 1.44 5406 2 0.61 -18.15 6.66 -8.59 1.59 8847 2 1.49 -20.54 10.79 -12.56 1.28 5969 1 0.41 -17.77 8.53 -9.22 1.51 4636 1 0.46 -18.06 8.80 -9.26 1.42 4404 2 0.79 -15.57 8.00 -9.73 1.26 2012 4 1.05 -19.08 9.75 -10.23 1.73 5439 2 1.45 -19.39 10.28 -12.20 1.55 6206 2 -0.57 -15.11 6.60 -8.04 1.71 2633 7 1.16 -17.38 9.25 -12.00 1.39 4733 2 1.58 -21.24 11.06 -12.42 1.57 5062 2 0.16 -14.29 6.02 -8.49 2.24 1645 3 1.11 -18.87 9.66 -10.91 2.41 4805 2 0.61 -17.15 8.51 -9.63 4.04 3812 21 0.24 0.47 -14.16 -15.60 7.19 7.74 -9.59 -9.43 1.24 2.00 1581 3025 2 0.65 -17.57 8.75 -9.75 1.43 3979 3 0.86 -17.87 — — 1.47 7081 6 0.62 -17.18 8.48 -9.56 2.05 5350 2 0.46 -15.36 7.94 -9.70 2.37 3241 5 0.99 -20.04 9.95 -10.29 2.17 6618 3 0.46 -17.13 8.39 -9.58 1.52 4872 4 0.72 -16.95 8.53 -9.70 1.56 7036 1 0.16 -15.49 7.57 -9.05 1.38 3335 1 0.44 -15.82 7.89 -9.46 3.20 3011 2 0.88 -18.97 9.56 -9.98 1.39 6987 2 0.55 -16.17 8.00 -9.49 2.73 3098 2 0.49 -16.25 8.00 -9.38 2.91 2942 2 -1.10 -17.01 — — 3.48 8448 2 1.27 -22.00 11.17 -9.95 3.93 11794 5 1.04 -18.80 9.62 -10.63 1.79 4306 1 0.62 -15.95 8.00 -9.55 1.46 1988 3 1.29 -18.98 9.95 -10.87 2.52 4473 81 0.77 0.33 -14.27 -15.48 — 7.60 -9.28 — 2.37 1.98 2267 1947 4 0.76 -15.05 7.81 -9.81 1.68 2686 2 0.66 -17.03 8.51 -9.63 1.86 3846 3 1.30 -18.19 9.58 -10.25 2.81 1972 2 0.82 -18.25 9.15 -9.89 3.17 1673 8 0.52 -14.23 7.35 -9.55 2.50 1916 9 0.06 -16.17 6.77 -10.90 2.10 4292 6 0.33 -14.59 7.30 -9.33 2.53 1304 2 1.27 -18.12 9.61 -11.36 1.70 3374 2 0.47 -13.91 7.12 -9.46 1.88 1355 7 0.42 -13.64 6.07 -8.75 2.20 1166 1 0.86 -17.43 8.70 -9.94 2.39 1344 2 1.06 -17.92 9.17 -10.56 2.11 1634 / 10 0.70 -19.29 — — 4.48 8768 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± km 1535261 11071 1503597 5428 1303155 6206 3012543 6979 2155292 3849 0938566 3408 + + + + + + 336 11794 351 8774 + + (J2000.0) [log] [log] [log] [log] 00 15 05.40 15 03 59.70 2MASX J00150533 00 46 05.70 -09 30 10.80 IC 0050 6027 01 49 14.05 13 03 19.20 NGC 0677 5075 01 54 32.70 -00 46 12.30 2MASX J01543275-0046121 4835 02 50 52.0003 07 15.65 00 00 12.10 00 43 52.00 ASK 037212 ASK 37834 1587 3011 04 10 51.36 -05 13 20.40 ASK 57849 4868 07 52 12.30 39 24 38.50 ASK 46197 8449 08 04 25.20 35 02 40.40 KUG 0801 08 35 00.5008 42 25.80 39 36 48.10 06 35 38.60 ASK 167684 ASK 259104 1960 2260 09 08 52.55 21 55 29.70 2MASX J09085253 09 20 02.70 28 20 57.40 ASK 488350 1915 09 24 27.90 46 31 44.70 ASK 169404 4310 09 35 05.80 09 38 57.10 2MASX J09350578 09 43 01.60 58 58 24.90 UGC 05179 1348 Basic optical and HI data – marginally detected galaxies 1 1 2 2 2 1 1 1 1 1 1 2 A A A N N N N A A A A C C C C C Source0024 RA 00 10 52.65 15 35 26.60 Dec 2MASX J00105266 Other name 0032 00 13 43.98 00 22 18.20 ASK 28319 3968 0036 00 15 00.08 -11 08 03.90 ASK 125926 3351 0037 0108 00 41 42.50 14 17 56.20 ASK 40372 8810 0116 0126 00 51 49.40 00 33 53.10 UM 283 4629 0129 00 53 19.60 -10 24 11.80 2MASX J00531961-1024115 4403 0175 01 14 52.70 -01 05 43.30 ASK 31675 2026 0200 01 24 53.30 -08 49 09.90 2MASX J01245329-0849093 5441 02210231 01 31 01.08 01 33 52.56 13 03 15.60 13 42 09.40 2MASX J01310103 ASK 43205 2599 0234 01 34 37.50 -01 03 08.10 ASK 33113 4787 0265 0282 01 53 01.30 -09 38 20.80 PGC 988388 1645 0287 0308 02 20 58.80 -09 31 42.80 PGC 3101275 3815 0329 0349 0356 03 11 17.74 -08 04 48.10 2MASX J03111772-0804486 3978 0384 03 21 30.80 00 11 35.70 ASK 38931 7062 0405 03 38 25.70 -06 38 11.00 ASK 56487 5350 0408 03 38 45.71 -05 38 42.20 ASK 56578 3244 0411 03 39 34.90 -06 02 19.90 2MASX J03393488-0602199 6629 0435 0441 07 20 02.10 41 08 11.20 ASK 475444 7026 0443 07 21 07.30 41 07 40.70 ASK 475415 3321 0453 07 25 24.12 42 25 59.10 ASK 475551 3013 04780520 07 36 07.60 07 44 05.50 30 12 54.20 46 42 34.20 2MASX J07360760 ASK 476552 3105 0533 07 49 33.50 39 44 24.10 ASK 46265 2943 0545 0581 08 03 28.90 33 27 44.50 KUG 0800 0582 0606 08 16 57.60 20 30 44.10 CGCG 119-027 4334 0669 08 33 12.70 39 30 49.80 ASK 191177 2026 0676 08 33 55.25 47 08 04.00 CGCG 237-006 4474 0681 0708 0760 08 56 03.00 -00 29 23.10 PGC 1142061 2693 0801 0821 09 12 44.40 34 55 32.00 NGC 2780 1954 0836 09 17 05.30 25 25 44.90 IC 2450 1652 0850 0864 0869 09 27 53.70 60 24 20.20 PGC 2601707 1317 0882 0902 09 40 03.30 44 59 31.70 ASK 264262 1369 0907 09 42 02.60 57 29 22.50 PGC 2566547 1161 0912 0917 09 43 31.10 31 58 37.10 NGC 2970 1630 Table A.2.

Article number, page 54 of 71 van Driel et al.: NIBLES – the Nançay HI survey ? HI M M

HI M NM / SNR S s / HI F 0.130.13 2.7 2.5 2.7 2.6 7.22 7.25 -0.08 0.24 0.18 2.7 1.9 7.10 -0.01 0.41 3.0 3.7 8.36 2.26 0.22 2.9 3.6 8.05 -1.87 0.420.42 3.1 4.1 3.7 2.5 7.76 7.58 7.76 7.58 0.30 2.3 2.3 7.41 0.12 0.37 2.2 3.7 9.76 -1.07 0.070.45 3.3 3.4 2.5 4.7 6.59 9.17 -0.04 2.92 0.270.35 1.7 3.3 2.8 4.0 8.94 8.20 -1.58 -0.51 0.49 3.3 7.1 8.90 1.89 0.09 3.4 2.6 7.11 -0.28 0.170.13 2.8 2.8 4.4 2.7 8.03 7.17 -1.78 7.17 0.13 4.2 4.2 7.71 0.01 0.49 4.7 5.6 9.76 -1.18 0.18 2.9 1.1 6.61 0.05 0.33 3.2 4.3 7.74 1.18 0.16 3.5 3.2 8.34 1.52 0.130.54 3.30.16 3.3 3.5 3.5 4.2 7.52 3.8 7.89 -0.51 7.55 7.89 0.53 0.24 2.6 4.0 7.69 -1.28 0.290.18 2.3 3.9 3.0 4.3 7.69 7.22 -0.71 7.22 0.29 2.5 3.4 7.74 -0.05 0.19 2.4 2.7 7.19 1.16 0.28 3.1 4.0 7.42 0.51 0.26 3.6 5.4 7.43 0.78 0.140.82 3.70.22 2.1 3.9 2.3 2.8 8.83 2.1 8.07 -2.19 7.35 8.07 -1.22 0.44 3.1 4.4 7.93 1.00 0.78 4.1 6.6 8.84 0.47 0.25 2.9 3.2 9.04 2.62 0.16 3.0 1.7 6.75 -0.32 0.57 3.7 4.6 8.76 -1.86 0.531.26 2.6 3.0 3.4 1.7 7.95 8.61 -0.68 8.61 0.130.33 2.4 3.2 2.5 3.8 7.85 7.74 -1.65 7.74 0.13 3.4 2.0 6.85 -0.35 0.35 3.1 4.4 9.54 9.54 0.19 2.3 3.2 8.09 0.43 0.19 2.8 2.4 7.42 0.22 0.220.27 3.0 2.7 3.2 1.9 8.85 7.95 -2.03 0.43 0.28 2.4 2.5 7.75 -0.41 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 6 85 97 0.21 5 45 55 0.21 7 22 38 0.09 5 163 177 0.87 6 34 49 0.12 5 48 59 0.20 7 47 68 0.29 68 88 115 102 0.28 135 0.36 7 156 170 0.59 9 166 182 0.62 667 37 287 91 55 295 0.29 1.48 103 0.29 7 104 119 1.17 87 113 225 128 240 1.09 1.38 5 128 141 0.78 4 49 60 0.15 5 357 370 0.98 8 87 100 0.36 96 64 127 82 139 0.39 0.32 / HI 10 41 59 0.19 18 48 85 0.74 17 126 160 0.45 3232 198 68 264 0.85 158 0.45 11 146 164 0.42 14 355 378 0.86 20 44 91 0.96 22 320 346 0.47 33 412 487 2.06 15 166 196 0.46 23 344 420 1.67 21 29 71 0.08 23 39 89 0.60 12 90 121 0.28 14 216 249 1.36 1026 137 66 153 0.53 136 0.35 24 91 130 0.28 34 34 105 0.41 28 27 96 0.49 15 723 767 3.23 11 222 245 0.48 12 37 63 0.14 20 271 323 1.55 11 74 92 0.18 19 31 69 0.20 22 60 96 0.36 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 2 0.51 -14.56 7.30 -9.37 1.38 1284 2 0.40 -13.50 7.01 -9.47 1.83 1412 2 -0.38 -11.91 7.12 -9.59 2.67 1128 2 0.48 -16.95 6.10 -8.41 4.81 2501 2 1.25 -19.10 9.92 -11.46 1.87 2241 4 1.23 -16.19 — — 2.76 1211 2 0.41 -13.00 7.28 -9.42 2.50 1116 2 1.45 -20.79 10.82 -10.70 2.14 11347 2 0.50 -12.82 6.63 -9.35 1.29 945 3 0.27 -18.40 6.26 -9.74 5.17 5584 2 1.40 -20.15 10.51 -12.18 1.57 6065 4 0.98 -16.42 8.70 -10.78 2.86 1923 4 1.55 -19.91 7.00 -10.51 2.39 2805 5 0.68 -14.02 7.39 -9.71 1.31 1495 5 1.26 -18.89 9.81 -10.38 1.35 2194 1 0.42 -15.30 7.70 -8.96 1.69 1911 2 1.40 -21.14 10.94 -10.37 2.62 8503 2 0.24 -13.37 6.56 -8.80 2.28 1034 2 0.58 -13.68 6.56 -9.16 3.76 1376 5 0.77 -16.20 6.82 -10.48 1.57 3951 4 0.88 -15.33 8.04 -9.94 1.40 1569 5 0.43 -13.82 7.03 -9.38 1.48 1438 6 1.21 -16.53 8.97 -11.11 2.00 1309 2 0.73 -16.34 8.40 -9.78 2.50 1390 3 0.80 -14.75 7.79 -9.98 2.36 1353 2 -0.05 -13.65 6.03 -10.15 1.78 1082 5 0.39 -13.73 6.91 -9.22 2.93 1144 2 0.49 -13.18 6.65 -9.02 2.88 1067 3 1.45 -21.31 11.02 -12.62 2.09 6777 4 1.00 -16.47 8.57 -10.71 2.38 1270 2 0.53 -13.54 6.93 -9.33 4.37 1223 3 0.48 -17.06 6.42 -9.65 1.72 6708 2 0.69 -13.26 7.06 -9.68 2.16 924 2 1.78 -19.73 10.62 -11.33 3.44 2755 2 0.96 -16.58 8.64 -9.42 5.09 1303 3 0.73 -19.33 9.50 -9.84 1.45 2807 2 0.64 -15.29 — — 2.98 1205 8 0.49 -13.83 7.19 -9.70 1.76 992 8 1.28 -20.49 — — 2.00 8328 2 0.53 -15.07 7.65 -9.55 2.02 2639 3 0.21 -14.48 7.21 -9.32 2.45 1658 2 1.57 -20.62 10.88 -12.50 2.60 5989 5 0.57 -14.70 7.52 -9.55 2.51 2369 3 0.76 -15.80 8.16 -9.90 3.07 1794 / 27 0.68 -15.34 — — 3.63 1280 30 1.13 -16.21 — — 1.81 1233 23 0.79 -13.76 — — 3.68 1088 18 0.49 -14.45 — — 1.70 979 35 0.60 -14.98 — — 5.17 1279 13 1.04 -15.56 8.37 -10.85 3.05 2082 16 1.43 -21.58 — — 8.81 2452 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± ± ± ± ± km 6038030 1294 3831120 1858 + + 09-19-160 1233 10-20-057 1795 + + (J2000.0) [log] [log] [log] [log] . 09 48 47.50 27 52 25.40 ASK 491818 1316 09 54 30.00 32 03 42.00 ASK 492645 1424 10 04 25.10 02 33 31.00 ASK 68781 1125 10 06 10.80 11 06 02.10 ASK 295498 2499 10 17 39.70 22 48 24.30 CGCG 123-035 1260 10 27 57.20 60 38 02.80 2MASX J10275708 10 51 32.00 00 15 26.00 UGC 05973 11362 11 01 47.80 58 39 59.80 ASK 211679 5590 11 18 34.60 12 42 39.90 IC 2708 6029 11 42 27.20 54 49 08.40 MCG 11 44 50.50 -01 36 04.70 IC 0728 8512 11 55 03.70 -03 30 12.40 ASK 11749 1414 11 57 35.30 02 10 04.20 PGC 1218144 941 12 12 24.3012 16 52.40 65 10 26.80 14 30 52.40 ASK 106418 IC 3096 1274 1264 12 18 20.60 04 51 13.60 ASK 173337 2072 12 18 57.60 02 59 25.40 ASK 76344 6662 12 29 52.30 13 25 38.80 NGC 4473 2292 12 54 12.60 00 48 09.10 CGCG 015-035 1191 13 04 57.00 39 55 24.90 IC 4165 8227 13 55 53.40 37 11 47.70 UGC 08854 5975 13 57 21.10 26 12 27.20 PGC 1767195 2391 continued – Z 3 1 1 F 3 1 3 1 1 1 3 1 1 1 1 1 A NA A NF NZ F NZ N NC N NRF A A UA C C C C C C C C Source0938 RA Dec Other name 0952 0987 0991 0999 10 12 48.60 43 08 43.90 IC 0598 2245 1021 1051 1094 10 43 51.80 58 38 39.10 ASK 211533 1172 1119 1134 10 56 38.70 17 23 01.20 PGC 4573180 948 1149 1210 12391247 11 23 01.60 11 23 38.80 38 31 11.90 53 50 31.70 2MASX J11230157 NGC 3656 2871 1267 11 25 40.00 04 40 35.50 ASK 170281 1487 1281 11 28 54.10 35 24 50.30 NGC 3694 2257 1355 1358 11 43 16.10 -01 23 40.90 PGC 1119651 1891 1370 1384 11 46 43.30 57 13 57.80 PGC 4015804 1029 1386 11 47 02.90 54 17 16.80 ASK 238471 1365 1390 11 47 37.20 62 00 58.80 ASK 155870 3944 1400 11 49 12.80 -03 39 34.60 PGC 1068442 1572 14211435 1446 11 52 33.40 11 48 56 17 37.50 34.80 ASK 348681 55 37 59.50 UGC 06919 1049 1289 1449 11 56 56.40 60 19 45.90 CGCG 292-051 1391 1456 1477 11 59 50.80 63 25 34.80 ASK 156744 1331 1498 12 03 30.70 55 03 05.70 ASK 239088 1113 1522 12 07 51.60 41 33 47.10 ASK 349285 1148 1524 12 08 09.70 37 27 24.60 ASK 532911 1068 1534 12 09 09.80 31 34 10.20 UGC 07132 6766 1563 1588 1593 12 17 56.90 67 05 47.80 ASK 65355 1204 1594 1597 1603 12 19 15.10 44 48 01.80 ASK 319572 922 1639 12 22 46.80 65 50 37.60 NGC 4332 2764 1656 12 24 17.00 67 26 23.80 UGCA 280 1318 1673 1703 12 39 48.00 12 58 26.20 IC 3631 2828 1751 1768 12 59 06.50 28 48 42.40 ASK 511090 999 1788 1899 13 39 38.32 42 32 44.80 ASK 309421 2644 1925 13 48 00.10 63 31 20.90 ASK 108389 1654 1976 1987 1997 13 58 42.90 61 51 45.50 MCG Table A.2.

Article number, page 55 of 71 A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1 ? HI M M

HI M NM / SNR S s / HI F 0.19 1.9 2.0 7.84 -1.55 0.27 3.1 4.0 7.95 -1.46 0.540.27 2.7 2.6 2.6 2.6 8.09 7.77 0.38 -0.63 0.30 3.0 4.2 8.14 -0.14 0.20 2.8 2.3 7.38 -0.38 0.35 2.9 3.2 8.07 -0.46 0.23 3.8 3.6 8.97 2.88 0.42 3.1 4.0 8.37 2.27 0.21 2.9 2.8 7.64 -0.70 0.19 3.0 2.4 7.65 -1.44 0.36 2.5 3.1 9.45 2.42 0.260.17 2.8 3.1 3.8 2.5 7.96 7.56 7.96 -0.74 0.19 2.8 2.7 7.72 7.72 0.32 2.4 3.8 8.05 -0.48 0.13 2.4 2.1 7.51 — 0.22 2.4 3.2 9.45 -1.99 0.12 2.9 3.0 7.61 -0.38 0.26 2.8 3.0 8.70 -2.18 0.40 3.1 2.0 8.93 -1.22 0.32 2.6 5.0 9.27 -0.36 0.41 4.6 8.3 9.56 -1.15 0.12 3.2 3.5 8.13 0.63 0.25 3.1 2.9 9.21 -1.93 0.22 3.2 2.9 8.97 -0.29 0.19 2.9 3.3 9.45 2.22 0.12 2.9 2.8 8.18 8.18 0.15 2.0 2.1 8.14 0.59 0.18 2.6 3.9 8.51 -0.28 0.21 2.7 3.4 8.71 -0.30 0.18 2.5 3.3 8.91 -1.34 0.240.25 3.0 2.9 4.0 2.1 9.14 8.89 -1.49 -1.04 0.20 3.0 3.6 8.91 0.35 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± s Jy km / 20 W s km / 50 W s km 9 132 149 0.84 7 33 48 0.31 6 239 251 0.71 54 160 126 171 136 0.63 0.27 7 216 230 0.31 8 269 283 0.45 7 52 66 0.21 6 85 98 0.26 8 76 96 0.39 6 171 184 0.39 7 59 74 0.19 6 221 234 0.62 8 179 196 0.45 / HI 43 97 153 0.20 50 128 233 0.51 10 59 76 0.40 24 107 157 0.66 10 90 109 0.26 10 127 147 0.67 17 99 144 0.45 14 224 254 1.02 13 125 153 0.26 20 125 159 0.69 11 48 66 0.15 15 400 428 0.50 19 129 171 0.46 12 613 635 1.05 15 585 635 2.19 14 153 186 0.43 23 70 103 0.17 16 142 171 0.41 14 74 101 0.40 11 178 198 0.37 22 64 110 0.25 ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± mJy km 1 − yr sSFR rms V

? M M g z M - g s mag mag 2 1.01 -18.40 9.39 -9.96 1.69 2680 4 1.17 -18.01 9.42 -10.16 1.89 1900 2 0.50 -15.44 7.71 -9.29 4.75 1744 3 0.81 -16.45 8.40 -9.92 3.35 1730 8 0.70 -16.08 8.28 -10.21 2.56 2067 2 0.86 -14.42 7.76 -10.15 2.01 1375 4 0.59 -17.27 8.52 -9.81 3.09 1885 2 0.79 -17.48 6.09 -8.37 2.12 6400 2 0.50 -15.78 6.10 -10.19 2.86 2179 2 0.70 -16.54 8.33 -9.97 3.21 1700 3 1.23 -17.08 9.09 -10.45 1.63 1881 3 0.49 -18.01 7.04 -9.77 2.52 8841 3 1.08 -16.48 — — 2.18 1725 2 0.96 -15.57 8.29 -10.10 1.61 1653 4 1.32 -19.64 — — 1.33 1859 5 0.84 -16.23 8.53 -10.40 2.71 1830 4 1.57 -22.08 11.43 -12.21 1.48 10992 2 0.54 -16.01 7.98 -9.56 1.64 1983 7 1.19 -19.72 10.16 -12.27 3.38 6074 6 1.67 -17.63 9.63 -11.17 1.39 6055 3 1.48 -20.60 10.71 -11.52 1.79 5862 2 0.47 -15.37 7.50 -9.18 1.34 3251 3 1.70 -21.05 11.15 -12.19 2.06 8660 5 0.80 -18.43 9.26 -9.81 2.47 7067 3 0.72 -18.30 7.24 -10.74 1.56 11879 5 0.73 -16.05 — — 1.48 4028 2 -0.31 -14.52 7.55 -9.87 1.59 4105 4 1.02 -16.67 8.78 -10.17 1.49 3983 2 0.67 -18.36 9.01 -9.62 2.25 5159 2 1.42 -19.51 10.25 -11.93 1.43 6607 2 1.45 -20.33 10.63 -11.84 1.75 6666 2 0.61 -17.14 8.55 -9.64 1.57 5991 / 14 0.58 -14.59 7.51 -9.63 1.70 2103 58 1.48 -20.81 10.88 — 1.39 4514 11 0.96 -19.67 9.93 -10.10 2.57 7804 opt ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± V ± ± ± km 5448024 1737 0049185 1645 + + 148 4099 156 7848 595 2207 + + + 09-23-057 2059 + (J2000.0) [log] [log] [log] [log] . 14 41 48.50 00 41 28.00 UGC 09470 1884 14 43 11.10 44 59 45.80 ASK 289207 6403 14 48 58.99 33 11 34.90 CGCG 193-002 1700 15 09 04.3015 09 32.80 00 49 19.10 03 03 02.40 2MASX J15090433 NGC 5864 1784 15 18 57.00 00 30 56.50 PGC 1168006 2082 15 29 49.80 03 30 39.10 CGCG 049-183 11053 15 32 49.90 36 12 13.50 ASK 331970 1993 15 35 52.10 39 46 08.10 NGC 5966 4514 21 16 27.60 -00 49 35.30 NGC 7047 5783 21 17 34.60 11 00 43.20 ASK 138402 3271 21 31 37.60 11 49 53.90 CGCG 426-062 8643 23 36 08.50 15 44 36.60 PGC 4125646 4016 23 37 37.10 15 08 26.90 KUG 2335 23 43 55.90 00 13 05.10 CGCG 381-031 6627 continued – ZP 3 1 2 1 1 1 1 1 1 2 N F A F A A NC A A A N N C C C Source2009 RA 14 01 24.00 36 48 00.30 Dec Mrk 0465 Other name 2693 2011 14 01 57.67 46 18 42.80 NGC 5439 1895 2031 14 05 24.60 61 34 01.30 PGC 2620337 1725 20392069 14 07 16.90 14 13 21.76 54 48 01.90 54 40 06.30 2MASX J14071669 MCG 2164 14 32 08.70 38 31 22.50 ASK 324027 1377 2210 2217 2232 14 47 38.90 59 21 51.60 SBS 1446 2236 2262 15 00 16.60 02 18 02.50 CGCG 020-042 1818 2263 15 00 18.60 54 53 39.50 ASK 161566 8819 2267 15 01 03.10 00 42 27.50 Mrk 1390 1724 2280 2283 2290 15 12 31.70 00 48 45.40 PGC 1176138 1844 2301 2319 2325 2330 2354 16 02 16.30 49 12 11.40 UGC 10150 6135 2394 20 54 12.20 -05 11 31.60 2MASX J20541219-0511314 6134 2407 2410 2418 2458 22 30 42.40 -09 37 12.70 ASK 135435 7046 2527 23 21 24.70 14 11 52.90 PGC 4125637 11881 2549 2555 2556 23 38 26.00 15 23 10.90 ASK 145449 3984 2562 23 40 42.68 -09 23 36.50 2MASXi J2340427-092336 5160 2570 2573 23 44 30.08 00 19 13.70 NGC 7739 6605 25792583 23 48 45.10 23 51 14.64 15 55 43.50 15 22 23.80 KUG 2346 ASK 146293 5994 Table A.2.

Article number, page 56 of 71 van Driel et al.: NIBLES – the Nançay HI survey

Table A.3. Basic optical and HI data – non-detected galaxies

Source RA Dec Name V g-z M M sSFR rms SNR M MHI opt g ? HI M? (J2000.0) [log] [log] [log] [log] −1 km/s mag mag M yr mJy M 0003 00 00 47.90 14 16 39.10 2MASX J00004789+1416390 10847±4 1.66 -20.01 10.71 -10.49 2.76 1.7 <10.40 <-0.31 0009 00 03 22.20 -10 46 14.20 MCG -02-01-012 8937±2 1.57 -20.87 10.98 -12.37 4.85 1.5 <10.55 <-0.43 0012 00 04 35.21 00 50 54.90 2MASX J00043518+0050549 6392±5 1.38 -17.81 9.57 -10.61 1.46 2.0 <9.49 <-0.09 0014 00 06 19.61 14 19 38.70 2MASX J00061957+1419389 5448±3 1.31 -18.22 9.66 -11.16 2.22 3.9 <9.56 <-0.10 0015 00 06 29.29 14 10 56.40 2MASX J00062933+1410559 5324±6 1.59 -17.84 9.74 -11.30 2.44 1.8 <9.56 <-0.18 0018 00 08 00.98 14 01 18.60 ASK 146993 5429±4 0.76 -17.38 8.74 -9.73 1.95 2.9 <9.41 <0.67 0023A1 00 10 25.50 14 17 23.00 KUG 0007+140 5452±4 0.93 -18.81 9.50 -10.17 1.79 0.9 <9.50 <-0.00 0025 00 11 43.20 14 28 01.10 ASK 146943 5213±2 0.66 -17.47 8.67 -9.48 2.44 1.7 <9.48 <0.81 0026 00 11 44.80 14 32 13.60 ASK 146940 5121±3 0.64 -16.57 8.23 -9.50 2.91 2.0 <9.47 <1.23 0027 00 12 06.10 -00 24 54.70 IC 0003 5447±2 1.43 -20.33 10.61 -12.34 2.09 1.5 <9.71 <-0.90 0028 00 12 11.60 -10 55 41.20 2MASX J00121162-1055413 5359±3 1.43 -19.44 10.30 -12.37 1.64 0.7 <9.52 <-0.78 0033 00 13 45.42 -09 56 03.70 ASK 126038 3822±2 0.66 -16.45 8.24 -9.68 3.12 1.2 <9.23 <0.99 0034N 00 14 17.63 15 51 06.30 ASK 147688 1943±6 0.44 -14.52 — — 1.77 2.1 <8.24 <8.24 0038NA1 00 15 29.70 14 43 37.20 ASK 147494 5432±4 0.39 -16.55 8.21 -9.54 1.75 1.7 <9.29 <1.09 0040 00 17 34.93 -09 32 36.00 IC 0005 6690±2 1.26 -20.96 10.68 -11.93 2.31 2.7 <9.97 <-0.71 0043 00 19 47.30 00 35 26.70 2MASXJ00194732+0035273 5306±3 1.12 -19.05 9.75 -10.43 2.32 1.2 <9.61 <-0.14 0045N 00 20 25.78 00 49 34.80 NGC 0078A 5072±3 1.49 -20.07 — — 1.52 0.9 <9.48 <9.48 0046 00 20 33.84 00 51 23.40 ASK 28804 5193±14 1.15 -16.63 8.86 -11.38 1.59 2.4 <9.24 <0.39 0048 00 21 35.30 01 09 56.20 CGCG 383-002 5465±2 1.39 -19.27 10.15 -11.84 1.56 1.1 <9.49 <-0.66 0054 00 23 47.66 -00 39 39.30 ASK 29153 5422±2 0.50 -16.92 6.36 -8.78 1.27 3.5 <9.18 <2.82 0058 00 25 07.42 00 18 45.70 UM 240 3269±2 0.25 -16.41 7.66 -8.70 1.46 2.4 <8.75 <1.09 0059 00 25 17.30 14 34 40.80 ASK 147884 5224±2 0.44 -16.59 8.11 -9.47 2.64 1.2 <9.44 <1.33 0061 00 25 52.50 -09 39 42.40 2MASXJ00255209-0939420 5201±2 1.52 -19.96 10.54 -12.25 1.23 1.4 <9.41 <-1.13 0067 00 29 33.17 -09 04 50.60 IC 0022 6049±2 1.48 -20.45 10.66 -11.80 1.80 1.1 <9.74 <-0.91 0069 00 29 49.30 -01 14 05.70 2MASX J00294935-0114055 10117±6 1.55 -20.12 10.64 -12.35 3.95 1.8 <10.51 <-0.13 0078 00 31 36.60 -10 53 17.40 2MASXJ00313653-1053178 5075±2 1.41 -19.75 10.37 -12.30 1.44 1.2 <9.44 <-0.93 0084 00 34 40.10 -10 45 59.40 NGC 0155 6189±2 1.39 -21.59 11.04 -12.33 1.61 3.0 <9.80 <-1.24 0087 00 35 59.80 -10 07 18.10 NGC 0163 5917±4 1.47 -21.23 11.01 -12.08 1.77 1.9 <9.78 <-1.23 0092 00 37 59.80 00 42 36.00 ASK 29753 4167±2 0.78 -16.21 8.39 -9.96 1.22 1.4 <8.89 <0.50 0099 00 39 55.97 -08 51 11.60 ASK 127226 4122±1 0.58 -16.30 8.26 -9.53 1.35 2.4 <8.92 <0.66 0100 00 40 26.90 -00 02 43.60 2MASX J00402686-0002431 5847±2 1.04 -18.56 9.46 -9.95 1.42 1.4 <9.44 <-0.02 0106 00 41 36.00 01 04 25.30 2MASX J00413598+0104262 5423±10 1.20 -17.26 9.20 -11.06 1.92 1.3 <9.42 <0.22 0124 00 50 38.40 -08 43 59.30 2MASXi J0050384-084358 4328±2 0.85 -17.40 8.97 -9.90 2.54 1.6 <9.34 <0.37 0131 00 56 20.99 -01 10 35.80 2MASX J00562098-0110359 11724±4 1.61 -20.66 10.89 -12.17 2.54 1.5 <10.49 <-0.40 0146 01 02 59.50 -00 40 42.30 ASK 31352 4822±4 0.72 -16.93 8.58 -9.87 1.21 1.6 <9.07 <0.48 0147 01 03 01.70 -01 06 39.30 CGCG 384-061 5237±3 1.41 -19.36 10.21 -12.35 3.02 1.6 <9.75 <-0.46 0148 01 03 54.00 -00 26 26.60 PGC 3110619 5248±6 1.31 -17.18 9.28 -11.65 1.50 1.2 <9.28 <0.00 0149 01 04 14.60 -00 50 40.30 PGC 3108496 4616±1 0.30 -16.58 7.87 -9.12 2.29 1.2 <9.26 <1.39 0150 01 04 15.20 -01 06 51.50 CGCG 384-064 5391±3 1.33 -19.31 9.96 -10.42 1.27 2.1 <9.39 <-0.57 0151 01 04 16.80 -01 04 29.90 UGC 00661 5306±2 1.48 -20.35 10.69 -12.37 2.72 1.8 <9.80 <-0.89 0152 01 04 16.96 -00 45 53.60 NGC 0359 5362±3 1.47 -20.55 10.72 -12.45 1.87 1.0 <9.66 <-1.06 0153 01 04 25.30 -09 22 59.30 PGC 991736 4653±2 0.65 -16.96 8.51 -9.74 1.74 1.6 <9.19 <0.68 0154 01 04 40.80 -00 48 09.80 NGC 0364 5117±3 1.55 -20.65 10.89 -12.74 1.80 3.0 <9.62 <-1.27 0155 01 04 56.80 -00 54 21.70 ASK 31281 5028±10 1.10 -16.85 9.02 -11.20 1.61 1.5 <9.24 <0.22 0156 01 05 54.10 -00 59 09.60 ASK 31254 5297±2 0.63 -17.32 6.89 -10.31 1.80 1.9 <9.35 <2.46 0158 01 07 09.20 -00 37 18.20 CGCG 384-076 5307±3 1.37 -20.30 10.58 -12.22 1.89 1.4 <9.64 <-0.94 0164 01 09 42.70 -00 57 13.50 ASK 31197 5203±3 0.69 -16.40 8.24 -9.70 1.48 1.5 <9.18 <0.94 0169 01 12 48.60 -00 17 24.60 NGC 0426 5259±3 1.54 -20.68 10.87 -11.36 1.14 2.5 <9.44 <-1.42 0170 01 12 57.40 -00 20 41.90 NGC 0429 5627±2 1.49 -20.49 10.76 -12.15 1.55 0.9 <9.62 <-1.14 0171 01 13 02.80 00 40 38.70 ASK 31963 4500±3 0.46 -16.42 8.59 — 2.39 2.4 <9.25 <0.67 0172 01 13 41.80 -00 06 09.80 UGC 00771 5152±2 1.50 -20.03 — — 1.59 2.8 <9.52 <9.52 0176 01 15 22.20 -00 09 30.30 2MASX J01152220-0009299 5196±4 1.28 -17.43 9.30 -11.27 1.27 1.6 <9.22 <-0.08 0178 01 15 54.30 13 21 12.00 CGCG 436-016 4184±2 1.46 -19.35 10.24 -12.12 1.55 1.2 <9.27 <-0.97 0181 01 18 44.80 -00 54 22.70 CGCG 385-063 5251±3 1.26 -19.38 10.09 -11.67 1.08 2.4 <9.31 <-0.78 0185 01 19 17.00 -00 06 49.40 2MASX J01191700-0006490 5192±3 1.40 -18.93 10.05 -12.07 1.70 1.8 <9.46 <-0.58 0189 01 20 12.10 14 33 40.60 UGC 00865 11332±4 1.68 -21.44 11.36 -12.72 1.51 0.4 <10.30 <-1.06 0195 01 22 46.00 -00 25 35.40 2MASX J01224599-0025343 5182±3 1.08 -18.27 9.61 -10.62 1.24 1.2 <9.27 <-0.34 0199D 01 24 52.50 -01 14 24.40 2MASX J01245257-0114244 5269±4 1.47 -17.56 9.53 -12.23 0.98 1.1 <9.13 <-0.40 0203 01 25 23.70 -01 11 41.20 2MASX J01252369-0111411 5272±3 1.36 -18.96 9.95 -11.47 1.29 1.8 <9.36 <-0.59 0206 01 26 25.90 -08 33 51.20 2MASXJ01262589-0833510 5336±2 1.30 -19.80 10.19 -11.37 1.45 2.9 <9.48 <-0.71 0207 01 26 42.20 -01 05 16.10 ASK 32676 4370±8 1.27 -16.62 9.19 -11.72 1.97 1.6 <9.19 <0.00 0209 01 26 49.70 -00 58 31.00 Mrk 0570 4853±4 1.34 -18.62 8.91 -9.84 1.51 2.8 <9.32 <0.41 0210 01 26 56.40 -10 13 26.00 ASK 129708 7074±6 0.72 -17.88 7.56 -10.80 2.61 2.4 <9.81 <2.25 0211 01 27 02.40 -10 15 54.80 NGC 0567 6992±2 1.63 -20.69 10.96 -12.72 2.56 1.7 <10.05 <-0.91 0214 01 27 25.10 -08 41 21.50 ASK 130312 3974±1 0.53 -15.62 7.91 -9.52 1.88 1.1 <8.98 <1.07 0215 01 27 35.56 -00 59 19.30 2MASX J01273555-0059195 5053±5 1.28 -17.62 9.37 -11.17 1.35 2.3 <9.23 <-0.14 0218 01 28 59.60 -00 33 42.90 UGC 01062 5464±2 1.44 -20.97 10.85 -12.37 1.25 1.0 <9.54 <-1.31 0219 01 29 43.98 -01 14 29.10 UGC 01072 5190±3 1.45 -20.43 10.61 -12.30 1.20 0.5 <9.43 <-1.18 0222 01 31 04.80 13 38 58.80 CGCG 436-067 5889±2 1.61 -19.53 10.49 -12.29 1.76 1.8 <9.64 <-0.85 0223 01 31 26.60 14 06 15.10 SHOC 071 4155±1 0.56 -17.11 8.45 -9.52 1.73 1.6 <9.10 <0.65 0233 01 34 07.97 -01 01 56.20 UGC 01123 4901±2 1.49 -20.15 10.28 — 1.69 11.8 <9.51 <-0.77 0240 01 37 23.40 -09 10 07.10 2MASXJ01372342-0910075 11612±3 1.52 -21.42 11.11 -12.37 1.45 2.3 <10.29 <-0.82

Article number, page 57 of 71 A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1

Table A.3. – continued.

Source RA Dec Name V g-z M M sSFR rms SNR M MHI opt g ? HI M? (J2000.0) [log] [log] [log] [log] −1 km/s mag mag M yr mJy M 0243 01 38 47.40 01 04 18.30 UGC 01169 4964±3 1.91 -19.31 10.58 -13.34 2.28 2.5 <9.60 <-0.98 0244 01 38 54.76 15 01 17.70 CGCG 437-008 8364±3 1.51 -20.93 10.91 -12.20 1.86 1.6 <10.08 <-0.83 0245 01 40 53.60 -10 16 41.60 2MASXJ01405362-1016415 5296±2 1.45 -19.98 10.50 -12.42 1.78 2.6 <9.58 <-0.92 0248 01 42 30.90 -00 49 09.90 CGCG 386-032 5189±3 0.83 -18.90 9.43 -9.78 1.62 2.3 <9.41 <-0.02 0251 01 45 07.90 -08 55 32.70 2MASX J01450782-0855330 11607±3 1.51 -21.09 11.00 -12.35 2.54 0.9 <10.51 <-0.49 0253 01 46 27.70 12 53 34.20 PGC 4124972 5166±13 0.70 -17.35 6.47 -10.23 1.60 2.6 <9.29 <2.82 0259 01 48 53.10 13 25 26.10 2MASXi J0148531+132526 4659±3 1.31 -17.56 9.41 -10.39 1.20 1.4 <9.11 <-0.30 0260 01 49 00.10 13 12 39.90 UGC 01271 5038±2 1.52 -20.61 10.83 -12.54 1.56 2.8 <9.54 <-1.30 0261 01 49 02.50 12 55 39.00 2MASX J01490255+1255394 5208±3 1.34 -18.62 9.83 -11.57 1.69 2.5 <9.44 <-0.39 0264 01 49 11.60 12 51 11.70 UGC 01274 7867±2 1.74 -20.96 11.17 -12.54 1.72 1.6 <10.00 <-1.17 0266 01 49 14.46 13 01 55.10 2MASX J01491447+1301548 4887±3 1.60 -16.63 9.39 -12.61 3.14 1.2 <9.50 <0.11 0268 01 49 33.50 13 14 00.00 2MASX J01493352+1314007 4994±4 1.42 -18.72 9.95 -11.70 1.24 0.6 <9.28 <-0.67 0269 01 49 53.80 12 58 33.70 2MASX J01495381+1258340 4691±6 1.35 -17.39 9.35 -11.44 1.55 0.7 <9.21 <-0.14 0271 01 50 11.50 12 59 18.70 ASK 44697 4639±30 1.14 -15.87 8.59 -10.61 2.00 0.4 <9.18 <0.59 0272 01 50 27.60 -08 31 22.50 IC 0168 5329±2 1.58 -20.20 10.71 -12.51 2.09 2.3 <9.68 <-1.02 0279 01 51 56.80 -09 20 26.20 ASK 131587 3960±4 0.50 -15.66 7.92 -9.61 1.60 2.3 <8.91 <0.99 0280 01 51 57.50 -08 31 03.40 IC 0170 5192±3 1.42 -19.67 10.31 -12.42 2.61 0.7 <9.71 <-0.60 0286N 01 54 08.00 -00 44 33.00 UGC 01367 4710±4 0.55 -17.61 8.63 -9.70 2.63 1.5 <9.43 <0.80 0288 01 54 41.80 00 36 41.70 PGC 1170628 4617±5 0.64 -16.42 8.24 -9.60 2.56 1.2 <9.31 <1.07 0289 01 55 16.30 -08 51 15.30 KUG 0152-090 3950±2 0.77 -16.82 8.60 -9.86 3.96 1.0 <9.41 <0.80 0297A1 02 00 03.80 14 07 12.90 ASK 43581 4860±3 0.39 -16.52 6.14 -8.70 3.12 0.9 <9.44 <3.30 0303 02 15 41.10 -08 30 29.00 ASK 132678 1385±12 -0.27 -14.00 7.25 -9.54 2.36 3.0 <8.03 <0.78 0307 02 20 42.00 -08 08 26.40 2MASX J02204200-0808252 4710±4 1.04 -18.39 9.44 -10.30 2.67 2.3 <9.52 <0.07 0309 02 26 28.30 01 09 37.70 IC 0225 1540±2 0.78 -17.77 8.85 -9.81 1.48 2.8 <8.23 <-0.61 0311 02 31 13.20 01 14 41.30 2MASX J02311322+0114415 6614±6 1.07 -18.61 9.59 -10.38 2.28 1.7 <9.76 <0.17 0313 02 31 33.60 00 45 22.60 ASK 36263 6220±2 0.59 -17.34 8.58 -9.57 3.02 3.6 <9.71 <1.13 0315 02 31 41.30 -09 18 01.60 NGC 0960 4867±2 1.68 -19.97 10.71 -12.46 2.57 2.3 <9.68 <-1.04 0316 02 31 45.99 -09 08 47.60 SHOC 124 1614±1 -0.12 -15.38 6.93 -8.26 2.27 1.4 <8.24 <1.31 0330 02 51 56.10 -00 50 10.60 CGCG 389-037 6866±2 1.43 -20.72 10.78 -12.19 1.44 1.2 <9.78 <-1.00 0333 02 54 22.30 -00 25 20.90 PGC 3110711 6809±2 1.03 -17.45 8.93 -10.32 1.93 1.9 <9.62 <0.69 0340A1 03 01 11.90 00 18 10.50 PGC 1162351 2779±2 0.61 -15.67 7.94 -9.52 1.69 2.3 <8.63 <0.69 0341 03 02 11.40 -01 09 59.30 ASK 37576 4079±3 0.52 -15.97 8.13 -9.72 0.91 2.0 <8.72 <0.59 0342 03 02 35.00 -07 21 45.20 ASK 55199 5986±4 0.54 -16.64 8.29 -9.42 2.25 1.4 <9.49 <1.21 0345A2 03 04 57.96 00 57 14.10 SHOC 150 3636±1 0.55 -16.02 — — 1.15 1.6 <8.72 <8.72 0346 03 05 30.80 -00 24 18.10 CGCG 389-078 8429±2 1.46 -21.38 — — 1.94 1.6 <10.14 <10.14 0350 03 07 32.30 -00 57 52.30 CGCG 389-084 11584±2 1.38 -22.24 11.30 -12.30 1.63 2.0 <10.40 <-0.90 0357 03 12 02.50 -00 04 42.50 CGCG 390-020 11264±3 1.53 -21.72 11.24 -11.95 1.49 1.7 <10.30 <-0.94 0359N 03 13 22.30 -08 13 52.90 ASK 55333 4877±3 0.52 -16.89 — — 2.61 2.0 <9.40 <9.40 0367 03 16 31.80 -00 28 05.30 UGC 02628 6798±4 1.43 -20.33 10.58 -10.98 2.02 1.7 <9.88 <-0.70 0369 03 17 06.70 -06 30 07.80 2MASX J03170667-0630082 4008±5 1.23 -19.08 9.91 -10.49 1.33 1.9 <9.14 <-0.77 0371 03 17 48.50 -07 37 00.70 NGC 1286 4312±2 1.39 -20.06 10.45 -11.95 2.26 0.4 <9.51 <-0.94 0382 03 20 40.80 -07 23 39.90 NGC 1303 5461±2 1.32 -20.61 10.59 -11.83 0.83 2.5 <9.32 <-1.26 0385 03 22 08.70 -00 50 10.50 CGCG 390-073 10928±3 1.32 -21.45 10.93 -11.54 2.32 1.3 <10.44 <-0.49 0390 03 25 25.40 -06 08 37.90 Mrk 0609 10317±4 1.07 -21.77 10.89 -10.01 2.07 1.9 <10.35 <-0.54 0391 03 30 17.17 -00 55 12.60 CGCG 390-096 6412±3 1.52 -20.67 10.88 -12.58 1.38 1.4 <9.70 <-1.18 0393 03 34 17.74 -06 15 53.90 NGC 1361 5254±2 1.43 -20.65 10.73 -12.28 1.11 2.4 <9.43 <-1.30 0397 03 37 10.36 -05 35 05.10 2MASX J03371039-0535055 8347±3 1.44 -21.02 10.90 -12.23 1.65 2.5 <10.03 <-0.88 0399 03 37 33.40 -06 31 13.50 2MASX J03373338-0631140 5359±2 1.53 -20.60 10.85 -12.78 1.56 2.4 <9.59 <-1.26 0402 03 38 04.10 -05 21 09.10 ASK 56542 4019±2 0.77 -16.83 8.56 -9.79 1.68 2.6 <9.04 <0.48 0403 03 38 08.10 -06 08 29.20 2MASX J03380814-0608295 10397±3 1.60 -21.62 11.28 -12.47 3.70 0.4 <10.62 <-0.66 0409 03 39 07.10 -06 27 02.90 2MASX J03390711-0627028 5381±4 1.30 -19.33 10.08 -10.83 2.74 2.3 <9.73 <-0.35 0415 03 41 03.20 00 28 26.40 2MASX J03410327+0028269 6158±2 0.64 -18.98 9.27 -9.69 1.97 1.2 <9.65 <0.38 0416 03 42 09.40 -07 26 16.60 2MASX J03420936-0726169 10049±3 1.57 -20.91 10.97 -12.43 3.13 1.3 <10.46 <-0.50 0417NF 03 42 12.50 -00 21 15.40 UGC 02832 7661±1 0.85 -19.73 7.55 — 2.59 1.3 <10.01 <2.46 0419D 03 43 13.96 -01 01 07.30 CGCG 391-030 11016±3 1.55 -21.26 11.10 -12.30 2.47 2.1 <10.47 <-0.63 0423 03 45 56.40 -05 08 31.70 ASK 56909 3893±2 0.59 -15.78 7.96 -9.52 2.29 1.2 <9.06 <1.10 0427 03 52 12.00 -06 20 56.20 NGC 1468 9876±3 1.56 -21.86 11.37 -12.59 2.29 1.6 <10.40 <-0.97 0428N 03 58 19.35 -04 43 49.60 ASK 57478 5294±2 0.47 -17.83 8.93 -9.72 3.06 0.9 <9.62 <0.69 0429 04 01 33.50 -06 20 12.40 PGC 1034032 5722±2 0.88 -17.08 8.77 -10.01 1.32 1.2 <9.27 <0.50 0433 04 06 44.30 -04 26 50.50 2MASX J04064426-0426510 11300±2 0.81 -19.57 9.69 -9.72 2.85 2.0 <10.39 <0.69 0437 04 12 11.60 -04 52 27.20 ASK 57882 9047±4 0.68 -18.53 9.19 -9.69 3.54 1.8 <10.20 <1.01 0440 07 19 51.50 41 24 58.00 2MASX J07195149+4124585 10470±6 1.45 -18.93 10.05 -11.10 3.64 1.9 <10.40 <0.35 0442 07 21 00.80 41 03 06.50 2MASX J07210079+4103065 6903±2 0.86 -18.25 9.22 -9.86 1.49 1.9 <9.57 <0.36 0444 07 21 23.42 41 41 59.00 ASK 475472 7001±3 0.52 -17.14 8.48 -9.50 2.94 1.2 <9.78 <1.31 0445 07 21 25.50 41 00 27.20 ASK 475463 6897±16 0.40 -16.58 8.39 -10.12 1.59 2.5 <9.46 <1.07 0447 07 22 46.70 41 39 29.60 UGC 03818 7002±3 1.44 -20.42 10.67 -11.40 2.16 2.3 <9.94 <-0.73 0449 07 24 19.60 38 45 38.70 2MASX J07241961+3845387 7244±3 1.38 -18.46 9.80 -11.79 1.73 1.9 <9.72 <-0.08 0450 07 24 33.10 41 57 02.10 2MASX J07243311+4157021 7960±3 1.35 -18.78 9.96 -10.65 1.96 2.0 <9.88 <-0.08 0452 07 25 04.40 40 35 37.60 ASK 475402 10200±2 0.34 -18.80 8.84 -8.98 3.26 0.6 <10.27 <1.43 0456 07 26 24.70 43 02 54.70 ASK 475844 7583±2 0.97 -18.14 9.30 -10.00 2.91 1.5 <9.94 <0.64 0457 07 26 35.40 43 17 46.80 UGC 03844 3130±2 1.44 -19.77 10.42 -12.36 2.01 2.5 <9.16 <-1.26 0459 07 27 19.40 44 25 38.30 2MASX J07271936+4425388 9742±3 1.51 -20.06 10.89 -13.24 2.44 1.9 <10.26 <-0.64

Article number, page 58 of 71 van Driel et al.: NIBLES – the Nançay HI survey

Table A.3. – continued.

Source RA Dec Name V g-z M M sSFR rms SNR M MHI opt g ? HI M? (J2000.0) [log] [log] [log] [log] −1 km/s mag mag M yr mJy M 0460 07 27 28.10 43 27 50.00 ASK 476000 6623±2 0.63 -17.25 8.70 -9.41 2.22 2.0 <9.63 <0.93 0464 07 29 45.10 43 44 45.10 ASK 476339 3183±4 0.87 -15.31 8.10 -10.02 2.52 2.1 <8.90 <0.80 0470 07 33 27.70 41 53 08.70 2MASX J07332776+4153084 5888±3 1.31 -18.64 9.82 -11.29 1.78 0.6 <9.57 <-0.26 0475A1 07 35 24.20 36 38 36.40 ASK 44962 3902±2 0.42 -16.86 8.23 -9.48 3.15 1.6 <9.28 <1.05 0480 07 36 16.80 33 07 21.70 IC 2201 4694±1 1.70 -19.66 10.59 -11.96 1.26 1.2 <9.31 <-1.28 0482 07 36 44.70 42 26 37.30 2MASX J07364472+4226376 6971±2 1.51 -19.40 10.31 -11.54 2.89 2.1 <9.99 <-0.32 0484 07 36 59.50 30 29 53.30 PGC 1906163 4546±2 0.72 -16.86 8.54 -9.76 1.67 1.6 <9.15 <0.61 0489 07 37 49.90 28 39 10.50 2MASX J07374992+2839102 4731±7 1.01 -16.96 8.86 -11.18 1.47 1.2 <9.15 <0.29 0490 07 37 59.20 33 56 27.00 ASK 85066 7108±2 0.84 -17.39 8.87 -9.94 2.46 2.8 <9.75 <0.88 0492U 07 38 26.50 28 57 47.00 CGCG 147-047 4732±4 1.41 -18.47 9.83 -11.06 3.84 1.4 <9.70 <-0.13 0493 07 38 32.50 29 11 07.90 CGCG 147-048 11784±4 1.45 -21.09 10.91 -12.24 3.13 1.5 <10.61 <-0.30 0506 07 40 22.70 23 16 29.90 UGC 03960 2255±2 1.23 -18.66 9.77 -11.59 2.64 2.9 <8.90 <-0.86 0507 07 40 27.50 30 48 20.00 2MASX J07402743+3048201 10503±3 1.56 -20.69 10.87 -12.26 3.24 1.7 <10.50 <-0.37 0510 07 40 42.60 23 37 34.40 CGCG 117-065 7343±3 1.53 -20.33 10.76 -12.54 2.70 1.4 <10.08 <-0.68 0513 07 41 12.50 42 44 57.70 CGCG 206-016 10723±2 1.50 -21.75 11.24 -12.17 3.63 2.6 <10.65 <-0.59 0515 07 41 54.80 38 29 53.80 2MASX J07415484+3829537 3507±1 0.43 -17.04 8.31 -9.46 2.67 1.8 <9.13 <0.82 0524 07 45 01.45 43 55 52.30 2MASX J07450145+4355525 3736±2 0.72 -16.62 8.43 -9.78 2.21 1.0 <9.08 <0.65 0526 07 46 19.80 39 51 26.00 ASK 45258 3895±3 0.87 -16.62 8.57 -9.97 2.59 2.5 <9.19 <0.62 0527 07 46 37.70 44 47 25.80 UGC 04008 9235±3 1.50 -21.69 11.16 -11.04 3.14 1.9 <10.45 <-0.71 0529 07 47 02.00 41 32 10.40 UGC 04018 8574±2 1.52 -21.16 11.09 -12.60 3.81 1.9 <10.43 <-0.67 0538 07 50 25.19 30 13 32.40 CGCG 148-046 7970±3 1.67 -21.05 11.18 -12.61 1.33 1.6 <9.91 <-1.27 0542 07 51 17.60 50 10 45.40 UGC 04051 6253±3 1.63 -21.07 11.09 -12.54 2.29 1.2 <9.93 <-1.16 0544 07 52 07.80 27 29 02.10 IC 2208 8035±3 1.53 -21.11 10.99 -11.91 1.81 2.9 <10.04 <-0.95 0548 07 54 10.20 26 11 00.70 ASK 203882 4661±2 0.31 -17.02 6.57 -9.49 1.89 1.7 <9.23 <2.66 0562A1 07 59 16.20 23 50 58.10 ASK 265000 2231±2 0.69 -14.88 7.73 -9.96 2.34 1.1 <8.52 <0.79 0564 07 59 29.70 27 01 35.10 NGC 2492 6649±3 1.50 -21.67 11.23 -12.48 3.37 1.7 <10.20 <-1.03 0565 07 59 33.50 39 15 06.00 ASK 86186 3992±12 1.01 -15.83 6.99 -10.88 2.26 2.0 <9.09 <2.10 0569 07 59 54.43 47 24 47.20 UGC 04136 6679±3 1.84 -20.54 11.10 -12.48 3.58 1.5 <10.15 <-0.95 0572 08 00 40.80 39 52 13.80 CGCG 207-017 3975±2 1.36 -18.56 9.87 -12.13 1.50 1.8 <9.15 <-0.72 0575A1 08 01 32.20 21 22 47.80 ASK 363277 2104±3 0.56 -15.63 7.86 -9.52 2.20 1.9 <8.50 <0.63 0579 08 02 57.50 16 17 57.50 UGC 04190 4853±2 1.53 -20.44 10.77 -12.62 2.22 2.7 <9.64 <-1.13 0580 08 03 24.10 41 54 53.30 UGC 04188 9661±3 1.55 -21.72 11.31 -12.62 3.36 2.0 <10.52 <-0.79 0584 08 05 47.80 30 13 52.30 CGCG 148-111 2306±3 0.98 -17.11 9.17 — 2.39 2.3 <8.74 <-0.42 0586 08 06 13.40 17 42 23.60 NGC 2522 4706±2 1.72 -20.78 11.05 -12.37 1.90 1.9 <9.58 <-1.46 0587 08 07 20.20 51 07 53.70 NGC 2518 5256±2 1.45 -21.04 10.93 -12.51 1.78 3.2 <9.66 <-1.27 0590 08 08 09.60 39 09 26.70 NGC 2524 3917±2 1.45 -20.70 10.75 -12.33 1.95 2.4 <9.42 <-1.32 0596N 08 12 54.20 55 40 19.40 NGC 2534 3527±2 1.29 -20.24 — — 2.36 2.2 <9.37 <9.37 0602A1 08 15 38.03 21 15 37.20 ASK 483519 3476±2 0.45 -16.28 7.94 -9.31 2.97 1.0 <9.11 <1.16 0607 08 17 11.10 44 46 37.10 ASK 87147 8330±2 0.59 -18.33 7.42 -9.53 3.67 1.8 <10.12 <2.71 0608 08 17 15.90 24 53 56.80 2MASXJ08171594+2453569 1898±8 1.15 -15.42 8.42 -11.01 3.98 2.3 <8.68 <0.26 0609A1 08 17 21.00 24 57 45.60 KUG 0814+251 2074±4 0.61 -15.55 7.91 -9.58 2.41 1.8 <8.52 <0.61 0611 08 17 35.00 20 54 11.00 NGC 2553 4670±2 1.48 -20.38 10.64 -12.35 1.67 2.8 <9.48 <-1.16 0618N 08 18 08.80 23 02 51.30 IC 2269 3980±2 1.75 -18.45 10.18 -11.95 2.01 1.3 <9.28 <-0.90 0622 08 19 24.28 21 00 12.80 2MASX J08192430+2100125 3906±4 1.28 -18.05 9.67 -12.38 2.94 1.2 <9.38 <-0.29 0623 08 19 32.10 21 23 39.40 IC 2293 4090±3 1.23 -19.35 9.98 -10.82 2.25 2.5 <9.40 <-0.58 0624 08 19 36.04 21 14 28.90 2MASX J08193606+2114291 4566±8 1.27 -17.13 9.17 -11.62 3.75 1.2 <9.55 <0.38 0626 08 19 51.90 20 59 05.90 NGC 2560 4883±2 1.54 -20.57 10.78 -12.04 1.86 1.6 <9.58 <-1.20 0627 08 20 09.90 27 05 36.50 UGC 04341 5869±3 1.62 -20.72 10.92 -11.46 1.23 1.6 <9.57 <-1.34 0628 08 20 23.70 21 07 53.20 NGC 2562 5062±2 1.54 -20.97 10.96 -12.11 2.21 2.4 <9.72 <-1.24 0630 08 20 35.70 21 04 04.00 NGC 2563 4509±2 1.54 -21.55 11.10 -12.52 2.84 2.5 <9.77 <-1.33 0631 08 20 45.80 56 29 27.30 CGCG 287-072 8761±3 1.59 -21.46 11.26 -12.77 2.45 1.0 <10.28 <-0.98 0635 08 22 15.80 46 41 30.40 2MASX J08221577+4641309 2179±2 0.82 -15.86 8.26 -9.91 2.13 2.5 <8.55 <0.28 0637 08 22 23.10 22 41 48.60 2MASX J08222312+2241484 2077±4 1.04 -16.64 8.72 -10.42 2.66 1.3 <8.67 <-0.05 0641 08 23 21.70 04 22 20.90 IC 0505 9312±4 1.63 -22.01 11.35 -12.64 3.20 1.4 <10.50 <-0.85 0642D 08 23 24.10 22 16 00.40 ASK 484591 2055±14 1.07 -15.43 8.31 -11.79 1.14 0.7 <8.20 <-0.11 0645DA1 08 23 41.00 20 41 48.50 ASK 522849 2011±11 0.67 -14.19 7.49 -9.75 1.82 1.9 <8.27 <0.78 0650 08 25 17.50 03 56 00.90 CGCG 032-022 4169±2 1.33 -19.51 10.19 -11.99 2.15 1.4 <9.42 <-0.77 0653 08 26 18.00 27 50 24.40 IC 2365 6019±2 1.41 -20.91 10.77 -12.29 1.75 1.1 <9.76 <-1.01 0654 08 26 28.80 26 04 29.10 ASK 364075 1968±18 0.91 -15.16 8.16 -11.04 2.87 2.0 <8.54 <0.38 0656 08 26 33.80 25 29 59.20 KUG 0823+256 2148±2 0.90 -15.47 8.16 -9.91 1.48 2.0 <8.34 <0.19 0657 08 26 39.20 25 35 53.50 2MASX J08263919+2535534 2332±3 1.17 -16.48 8.81 -10.21 1.60 1.8 <8.54 <-0.27 0666 08 31 25.80 40 57 22.40 UGC 04449 7320±6 1.95 -20.77 11.37 -10.87 1.29 1.7 <9.80 <-1.57 0668 08 33 12.50 41 05 41.40 CGCG 208-015 7287±2 1.44 -21.03 10.95 -12.38 2.44 1.4 <10.08 <-0.87 0671 08 33 30.80 41 31 31.60 UGC 04468 7409±2 1.51 -21.13 11.06 -12.50 2.11 1.6 <10.04 <-1.02 0679 08 34 20.20 50 27 08.90 2MASX J08342016+5027088 3433±2 0.93 -16.65 8.63 -10.00 1.42 0.8 <8.82 <0.19 0688 08 36 28.40 18 21 38.90 CGCG 089-052 4006±2 0.93 -18.24 9.28 -10.07 1.15 3.1 <8.99 <-0.28 0689A1 08 36 41.10 05 16 24.00 ASK 259050 3127±2 0.20 -15.72 7.54 -8.93 2.52 1.4 <8.89 <1.36 0690 08 37 26.60 40 02 08.10 UGC 04498 7091±3 1.46 -20.81 10.81 -10.95 2.64 1.2 <10.07 <-0.73 0694 08 38 09.63 19 43 32.40 NGC 2624 4134±2 1.38 -19.49 10.21 -10.62 1.56 2.4 <9.27 <-0.95 0695 08 38 10.55 18 41 30.30 CGCG 089-054 5859±2 1.46 -19.76 10.43 -11.76 1.47 1.8 <9.57 <-0.85 0697 08 39 00.68 40 20 46.00 UGC 04513 7410±2 1.49 -20.90 10.88 -12.32 1.83 1.9 <9.96 <-0.91 0698 08 39 32.10 40 15 36.10 ASK 168053 7144±2 0.71 -18.00 6.75 -10.29 1.76 3.2 <9.65 <2.90

Article number, page 59 of 71 A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1

Table A.3. – continued.

Source RA Dec Name V g-z M M sSFR rms SNR M MHI opt g ? HI M? (J2000.0) [log] [log] [log] [log] −1 km/s mag mag M yr mJy M 0718 08 44 38.00 55 01 08.00 CGCG 263-080 7601±2 1.51 -21.37 11.10 -12.40 3.72 1.3 <10.33 <-0.77 0719A1 08 44 42.70 29 32 43.00 ASK 281794 2116±3 0.40 -14.49 7.26 -9.29 2.12 2.4 <8.39 <1.13 0723 08 45 23.21 55 07 07.40 UGC 04564 7865±4 1.54 -20.47 10.74 -11.46 2.42 2.2 <10.10 <-0.64 0724A1 08 45 25.40 15 19 46.00 PGC 4176159 1614±8 0.02 -13.43 7.30 -10.72 2.79 1.2 <8.20 <0.90 0726 08 45 41.61 41 16 58.30 CGCG 208-044 8956±3 1.66 -21.00 11.13 -12.84 2.80 1.5 <10.33 <-0.81 0730NF 08 46 36.00 19 00 50.00 UGC 04588 4377±2 1.12 -18.54 — — 3.50 1.8 <9.58 <9.58 0732 08 46 45.22 06 57 35.80 UGC 04594 8732±3 1.55 -21.10 11.01 -12.25 3.05 3.1 <10.34 <-0.66 0733 08 46 49.20 28 10 16.70 IC 2393 6297±2 1.51 -21.41 11.09 -12.35 2.54 1.9 <10.00 <-1.09 0735 08 47 21.98 42 23 55.60 ASK 191682 2980±1 0.69 -15.76 8.03 -9.65 2.91 1.2 <8.94 <0.90 0737 08 47 49.72 18 54 42.80 IC 2399 4225±7 0.97 -18.29 9.44 -10.57 2.53 1.0 <9.39 <-0.05 0738 08 47 59.49 19 02 56.40 PGC 1578852 3844±3 0.87 -16.66 8.50 -10.05 1.54 2.1 <8.96 <0.47 0743 08 48 59.64 41 00 11.30 CGCG 208-047 7389±2 1.52 -20.81 10.83 -12.27 1.53 1.5 <9.88 <-0.95 0744 08 49 01.40 29 29 18.20 KUG 0845+296 8239±2 -0.03 -17.60 6.80 -8.72 2.45 1.8 <9.87 <3.07 0746 08 49 06.59 19 00 26.30 PGC 4178363 3783±19 1.08 -15.52 8.35 -11.82 1.03 1.8 <8.69 <0.34 0747 08 49 15.01 19 11 27.30 PGC 4572078 3827±11 1.22 -16.06 8.71 -11.30 3.10 1.8 <9.23 <0.52 0748U 08 49 24.19 19 04 27.50 NGC 2673 3749±2 1.48 -19.64 10.35 -12.86 2.27 1.3 <9.36 <-0.99 0751A1 08 50 25.19 32 37 18.80 ASK 266943 2221±2 0.56 -14.82 7.21 -9.37 1.95 2.8 <8.43 <1.22 0753 08 51 56.67 16 56 41.30 UGC 04639 8549±2 1.54 -21.59 11.18 -12.34 1.49 2.1 <10.05 <-1.12 0754 08 52 04.95 53 37 02.30 NGC 2675 9303±3 1.58 -21.82 11.36 -12.68 5.13 1.5 <10.68 <-0.68 0756 08 54 40.70 20 35 00.90 CGCG 120-050 3785±2 1.35 -19.39 10.15 -11.81 1.77 2.8 <9.24 <-0.91 0763 08 56 57.99 52 03 57.40 NGC 2692 3773±2 1.50 -20.14 10.54 -11.68 5.34 2.1 <9.78 <-0.76 0768 08 57 59.90 -00 24 36.30 ASK 58627 3344±2 0.46 -15.90 6.17 -9.85 2.38 1.8 <8.96 <2.79 0770 08 58 02.30 39 03 48.80 ASK 262896 6982±3 0.87 -17.34 6.67 -10.74 1.85 2.2 <9.61 <2.94 0771 08 58 30.50 02 55 31.70 IC 2426 3887±2 1.32 -19.03 9.96 -11.39 3.04 1.6 <9.47 <-0.49 0775 08 58 51.20 38 48 34.30 UGC 04702 8495±3 1.52 -21.22 11.13 -12.80 2.51 2.5 <10.25 <-0.88 0788 09 01 28.60 03 43 14.10 NGC 2729 3819±2 1.52 -19.78 10.44 -12.15 1.32 1.3 <9.16 <-1.28 0799 09 07 36.60 03 23 34.40 NGC 2765 3774±2 1.43 -21.10 10.76 -11.56 1.90 0.4 <9.40 <-1.35 0802 09 08 54.40 01 25 57.10 CGCG 006-006 4918±4 0.83 -18.52 9.30 -10.02 2.99 2.4 <9.61 <0.31 0809 09 10 11.90 50 24 04.60 NGC 2767 4925±3 1.60 -20.13 10.71 -12.64 3.15 1.5 <9.79 <-0.92 0812 09 10 32.10 50 25 59.70 NGC 2769 4817±2 1.77 -20.67 11.05 -11.49 3.11 1.7 <9.81 <-1.25 0817 09 11 35.65 30 04 39.10 UGC 04833 7787±2 1.45 -20.53 10.70 -12.26 2.72 1.5 <10.15 <-0.55 0823 09 13 39.50 29 59 34.60 NGC 2783 6749±3 1.43 -21.90 11.21 -12.27 1.96 1.0 <9.99 <-1.22 0824 09 14 13.06 43 08 05.90 KUG 0910+433 4232±2 1.19 -19.53 10.09 -10.12 2.95 2.1 <9.56 <-0.53 0825 09 14 16.60 57 02 39.60 ASK 052929 2514±3 0.28 -15.03 6.37 -9.44 2.44 1.6 <8.64 <2.28 0826 09 14 34.30 30 08 27.00 UGC 04869 6852±2 1.70 -21.29 11.17 -12.09 3.06 1.7 <10.15 <-1.01 0828NZA1 09 14 57.30 06 00 18.60 ASK 261057 1370±30 0.64 -14.37 — — 3.33 0.4 <8.22 <8.22 0830 09 16 01.80 17 35 23.30 NGC 2794 8820±2 1.53 -21.75 11.26 -12.05 4.60 1.4 <10.58 <-0.68 0831 09 16 03.90 17 37 42.10 NGC 2795 8581±3 1.54 -22.18 11.42 -12.52 2.88 1.3 <10.39 <-1.03 0833 09 16 37.67 30 54 19.30 UGC 04893 6959±3 1.46 -19.82 10.44 -12.10 2.73 1.8 <10.00 <-0.45 0835 09 16 50.01 20 11 54.60 NGC 2804 8293±3 1.45 -22.06 11.31 -12.39 2.35 1.0 <10.26 <-1.05 0844 09 18 54.50 50 01 14.30 UGC 04927 10285±2 1.48 -21.92 11.28 -12.53 5.20 0.8 <10.78 <-0.50 0846 09 19 24.20 33 37 26.40 NGC 2826 6339±2 1.63 -20.72 10.87 -11.90 3.35 1.7 <10.08 <-0.80 0848N 09 20 00.60 39 53 33.30 ASK 207278 1439±2 0.56 -13.56 7.06 -9.66 2.89 1.6 <8.12 <1.07 0849 09 20 02.20 01 02 17.80 UGC 04956 5104±2 1.47 -21.15 10.97 -12.61 2.39 2.5 <9.77 <-1.20 0857 09 22 10.30 33 50 54.70 UGC 04974 6985±2 1.48 -21.19 11.03 -12.50 3.81 2.1 <10.25 <-0.78 0858 09 22 55.00 03 09 24.90 NGC 2858 3640±2 1.44 -20.12 10.59 -12.50 1.57 1.3 <9.22 <-1.37 0868 09 27 52.80 29 59 08.70 IC 2476 7993±3 1.50 -21.89 11.27 -12.53 2.21 2.1 <10.19 <-1.08 0886 09 35 44.00 31 42 19.60 NGC 2918 6756±3 1.57 -21.82 11.28 -12.19 1.82 1.2 <9.95 <-1.33 0894 09 38 23.40 43 30 32.90 UGC 05133 4413±2 1.46 -19.89 10.48 -12.27 1.73 1.6 <9.41 <-1.08 0895R 09 38 32.90 17 01 52.60 NGC 2943 8406±3 1.59 -22.39 11.51 -12.72 1.26 1.6 <10.03 <-1.48 0896 09 38 34.40 08 53 16.50 2MASX J09383447+0853159 3228±2 1.42 -18.71 9.95 -11.15 1.19 1.9 <8.88 <-1.07 0901D 09 39 34.70 48 25 18.90 UGC 05145 7378±4 1.74 -21.11 11.21 -10.76 1.96 1.3 <10.01 <-1.20 0904A1 09 40 45.80 32 28 20.80 KUG 0937+327 1293±1 0.44 -14.20 7.13 -9.32 1.88 1.3 <7.89 <0.76 0906A2 09 41 16.60 10 38 49.10 IC 0552 5788±3 1.57 -20.70 10.87 -12.11 1.87 3.0 <9.74 <-1.13 0918 09 43 40.40 11 03 39.00 NGC 2984 6161±3 1.52 -20.66 10.82 -12.37 1.39 2.5 <9.66 <-1.15 0924N 09 46 28.50 -00 26 03.50 ASK 51 1810±2 0.71 -16.52 8.34 -9.77 2.06 2.0 <8.41 <0.07 0926 09 46 45.60 09 15 51.70 CGCG 063-065 4030±3 1.39 -18.54 9.85 -11.55 1.78 1.6 <9.23 <-0.62 0927 09 46 48.99 09 44 10.00 CGCG 063-066 2997±3 1.35 -18.95 9.95 -12.11 1.70 1.5 <8.98 <-0.97 0928A1 09 46 53.00 31 47 44.60 KUG 0943+320 1425±3 0.64 -14.40 7.47 -9.70 2.85 2.1 <8.18 <0.71 0931 09 47 16.10 22 05 22.10 NGC 2994 7417±3 1.49 -21.49 11.16 -12.14 2.68 0.5 <10.18 <-0.98 0936 09 48 41.60 59 15 39.50 2MASX J09484156+5915394 2231±2 1.24 -17.50 9.31 -9.58 2.95 2.1 <8.85 <-0.46 0940 09 49 52.10 34 42 50.80 NGC 3012 11617±3 1.48 -22.27 11.46 -12.52 2.54 1.4 <10.61 <-0.86 0949A1 09 52 35.10 08 11 56.60 ASK 277328 2725±3 0.72 -16.92 8.53 -9.75 1.85 2.3 <8.75 <0.23 0975 10 00 45.20 04 44 03.50 UGC 05383 3968±2 1.46 -19.39 10.33 -12.62 2.13 1.5 <9.37 <-0.96 0976NA1 10 01 09.50 08 46 55.50 ASK 277703 1265±2 0.63 -13.67 7.14 -9.61 2.41 1.4 <7.94 <0.80 0977 10 01 31.10 37 12 14.20 IC 2530 6559±3 1.37 -20.79 10.76 -12.33 2.74 1.5 <10.02 <-0.74 0979 10 02 00.95 59 15 08.30 CGCG 289-027 2802±4 1.82 -17.86 9.60 -10.61 4.40 1.2 <9.30 <-0.31 0983 10 03 58.80 22 16 33.80 UGC 05420 6120±2 1.49 -20.94 10.93 -12.64 1.29 2.1 <9.65 <-1.28 0986 10 04 13.40 60 22 14.10 ASK 154248 3039±6 0.15 -15.41 6.60 -10.69 6.14 1.1 <9.26 <2.66 0988 10 04 31.80 60 06 28.60 NGC 3102 3038±2 1.38 -19.27 10.15 -12.03 2.70 2.3 <9.22 <-0.93 0990 10 06 07.40 47 15 45.50 NGC 3111 7437±3 1.47 -21.70 11.19 -12.37 2.64 2.2 <10.19 <-1.00 0995 10 10 14.90 46 17 44.00 ASK 209206 1099±2 0.25 -13.13 6.55 -9.13 3.06 2.5 <7.87 <1.32

Article number, page 60 of 71 van Driel et al.: NIBLES – the Nançay HI survey

Table A.3. – continued.

Source RA Dec Name V g-z M M sSFR rms SNR M MHI opt g ? HI M? (J2000.0) [log] [log] [log] [log] −1 km/s mag mag M yr mJy M 0998NZF 10 12 41.20 03 07 45.60 NGC 3156 1266±30 1.00 -18.62 — — 2.17 0.4 <8.30 <8.30 1004 10 13 50.50 38 45 53.60 NGC 3158 6920±3 1.58 -22.26 11.46 -12.48 2.67 1.9 <10.18 <-1.28 1014 10 16 23.00 60 14 05.70 NGC 3168 9399±3 1.55 -21.69 11.28 -12.64 5.72 1.7 <10.73 <-0.55 1017A1 10 16 59.00 03 42 35.40 ASK 95821 1204±2 0.63 -14.10 — — 1.98 1.5 <7.85 <7.85 1023 10 17 57.20 41 06 51.40 NGC 3179 7150±2 1.47 -21.36 11.02 -12.02 1.88 1.7 <9.98 <-1.04 1030A1 10 19 59.90 24 47 24.60 ASK 596355 1258±2 0.42 -14.06 7.08 -9.48 1.88 2.5 <7.85 <0.77 1034N 10 20 26.40 40 52 41.10 ASK 314345 1161±2 0.31 -13.02 — — 2.89 1.3 <7.89 <7.89 1038 10 21 21.10 24 20 29.00 UGC 05591 11118±3 1.53 -21.52 11.21 -11.99 3.00 1.1 <10.58 <-0.63 1040 10 22 06.00 21 03 54.30 CGCG 124-015 11738±3 1.59 -21.75 11.33 -12.64 4.94 1.2 <10.87 <-0.46 1043 10 23 15.40 20 10 40.50 ASK 606279 1143±5 1.14 -14.11 — — 1.54 1.9 <7.72 <7.72 1046 10 25 43.30 39 38 46.90 NGC 3237 7023±2 1.45 -21.36 11.09 -12.81 2.33 2.9 <10.06 <-1.04 1048 10 25 47.70 26 34 14.60 CGCG 154-013 5023±2 1.44 -20.35 10.62 -12.04 2.04 1.9 <9.62 <-0.99 1061 10 34 15.20 52 52 14.90 UGC 05734 7055±2 1.51 -21.23 11.07 -12.22 2.33 0.8 <10.05 <-1.02 1067 10 35 04.80 46 33 41.20 UGC 05744 3356±3 0.85 -19.41 9.66 -9.88 2.14 2.9 <9.20 <-0.46 1069A1 10 35 11.10 25 27 04.00 PGC 4243890 1298±2 0.24 -13.32 6.62 -8.98 1.80 2.3 <7.80 <1.18 1076A2 10 36 38.40 14 10 15.90 NGC 3300 3017±2 1.42 -20.24 10.53 -12.29 1.67 2.4 <9.09 <-1.45 1078 10 37 37.90 37 27 20.30 NGC 3304 6937±3 1.63 -21.11 11.11 -12.41 2.10 2.6 <9.98 <-1.12 1086 10 41 12.96 06 22 11.60 CGCG 037-114 5767±2 1.45 -19.93 10.46 -12.24 4.06 1.1 <10.01 <-0.45 1095A1 10 44 20.70 14 05 04.00 NGC 3357 9770±2 1.51 -22.32 11.41 -12.52 2.36 3.5 <10.43 <-0.99 1102 10 47 26.60 06 02 53.20 NGC 3376 5816±2 1.45 -20.66 10.76 -12.23 2.15 1.9 <9.80 <-0.97 1107 10 48 11.60 04 55 39.80 NGC 3385 7759±3 1.46 -21.87 11.20 -12.36 1.31 1.6 <9.93 <-1.27 1111 10 49 14.00 15 48 33.00 2MASX J10491407+1548327 5739±2 1.40 -19.99 10.40 -12.09 2.08 1.9 <9.72 <-0.68 1113 10 49 41.20 00 21 47.10 CGCG 010-027 11592±2 1.47 -21.69 11.25 -12.60 2.66 2.5 <10.57 <-0.67 1118 10 50 45.50 28 28 08.70 NGC 3400 1412±2 1.36 -18.09 — — 2.05 2.1 <8.34 <8.34 1125D 10 53 56.30 60 02 42.90 ASK 91914 1266±2 0.31 -13.77 6.85 -9.11 3.63 2.7 <8.12 <1.27 1132A2 10 56 19.90 17 05 05.90 PGC 4257755 960±2 0.44 -12.53 6.57 -9.47 1.43 1.5 <7.39 <0.82 1136 10 57 31.20 40 56 46.10 NGC 3468 7521±3 1.58 -21.63 11.25 -12.68 1.97 1.4 <10.07 <-1.18 1138 10 58 37.60 09 03 01.60 UGC 06062 2623±2 1.46 -19.20 10.18 -12.22 1.75 1.9 <8.91 <-1.28 1146A2 11 00 35.40 12 09 41.60 NGC 3491 6351±3 1.59 -21.12 11.06 -12.65 2.19 1.8 <9.93 <-1.13 1147A1 11 00 47.10 16 52 55.50 PGC 4260762 1136±3 0.51 -13.25 6.93 -9.56 2.22 2.5 <7.78 <0.85 1154 11 02 56.30 50 39 33.20 UGC 06114 6139±3 1.38 -20.36 10.62 -12.45 2.73 0.9 <9.93 <-0.69 1155 11 03 26.30 16 00 58.20 LSBC F640-02 1235±14 0.86 -14.66 7.74 -10.19 2.87 1.8 <8.09 <0.35 1160 11 04 56.80 17 38 30.50 PGC 4263693 907±7 0.90 -13.48 7.39 -10.61 1.64 1.6 <7.49 <0.09 1163A2 11 06 32.10 11 23 07.50 NGC 3524 1357±2 1.32 -18.37 9.71 -11.27 1.75 1.5 <8.26 <-1.44 1164 11 06 51.10 17 30 02.80 PGC 4578261 939±14 0.96 -12.48 — — 1.24 1.0 <7.32 <7.32 1166A1 11 07 09.90 28 22 31.90 PGC 1833985 1003±2 0.42 -13.87 7.09 -9.49 1.84 1.4 <7.64 <0.55 1171 11 08 40.40 57 13 48.70 NGC 3530 1876±2 1.35 -18.23 9.69 -11.63 4.16 1.3 <8.91 <-0.78 1180 11 10 55.90 28 32 37.60 NGC 3558 9606±4 1.55 -21.65 11.25 -12.52 3.80 1.9 <10.57 <-0.68 1187 11 12 31.70 16 17 22.60 LSBC F640-V04 1198±16 0.89 -14.63 — — 1.56 2.0 <7.80 <7.80 1191 11 13 10.40 27 49 05.60 UGC 06250 9367±3 1.59 -21.66 11.30 -12.67 4.15 2.7 <10.59 <-0.71 1201 11 15 16.10 14 41 54.90 ASK 432755 1093±38 0.41 -13.18 — — 2.21 2.6 <7.73 <7.73 1207F 11 18 03.90 10 14 40.00 ASK 271464 962±77 0.79 -12.68 — — 1.46 2.4 <7.42 <7.42 1223NUZF 11 21 06.90 03 28 07.80 PGC 4097805 1501±99 0.20 -11.71 — — 1.54 1.1 <7.75 <7.75 1224A2 11 21 24.90 03 00 50.10 NGC 3643 1742±2 1.19 -17.98 9.53 -11.41 1.86 1.5 <8.47 <-1.05 1227 11 21 47.60 57 20 48.20 PGC 2563515 1081±2 0.35 -13.64 6.89 -9.32 2.81 2.7 <7.86 <0.97 1230 11 22 04.10 03 36 51.60 ASK 73108 1445±30 0.99 -13.60 7.53 -10.32 1.58 1.6 <7.89 <0.36 1244N 11 23 18.80 03 57 18.80 CGCG 039-161 1582±19 0.89 -15.66 8.23 -10.85 1.72 1.7 <8.16 <-0.07 1249 11 24 06.50 38 51 23.00 2MASX J11240641+3851226 1979±4 1.39 -16.57 9.03 -11.78 1.80 1.5 <8.46 <-0.57 1250 11 24 08.50 03 44 04.70 ASK 170270 1729±19 1.08 -14.31 7.83 -11.28 1.28 2.1 <8.01 <0.18 1258NRF 11 24 42.80 38 46 13.20 NGC 3665 1952±8 1.58 -20.79 6.88 -11.21 1.52 1.9 <8.72 <1.83 1260A1 11 25 04.00 28 09 35.60 PGC 4546173 1593±1 -0.01 -14.24 6.76 -8.80 1.26 1.6 <7.89 <1.13 1262 11 25 26.70 65 46 07.20 SHOC 323 1118±1 0.01 -13.48 6.34 -8.51 2.44 1.6 <7.81 <1.47 1264 11 25 30.40 63 26 46.70 NGC 3668 3446±3 1.35 -20.39 10.51 -10.24 4.46 2.5 <9.63 <-0.88 1266 11 25 35.10 -00 46 05.60 UGC 06435 7584±2 1.48 -21.45 11.15 -12.52 1.24 2.5 <9.86 <-1.29 1295 11 31 42.00 28 09 12.90 NGC 3713 6898±2 1.46 -21.49 11.07 -12.06 2.58 1.9 <10.09 <-0.98 1315 11 34 11.70 12 30 44.30 NGC 3731 3195±2 1.38 -19.57 10.31 -12.59 2.22 1.5 <9.21 <-1.10 1318 11 35 18.10 58 53 18.70 MCG +10-17-017 1037±2 0.78 -14.99 7.92 -10.45 2.05 3.5 <7.81 <-0.10 1320 11 35 38.20 31 10 28.60 ASK 498176 970±49 0.43 -13.37 — — 2.86 1.9 <7.76 <7.76 1321 11 35 43.00 01 53 25.10 ASK 73755 1561±2 0.41 -13.98 7.05 -9.26 1.39 2.3 <7.90 <0.86 1329F 11 37 44.40 54 02 44.70 ASK 236929 868±12 0.72 -14.37 — — 1.92 1.4 <7.58 <7.58 1331 11 37 58.70 59 37 00.90 NGC 3770 3331±2 1.52 -19.78 10.41 -10.97 1.92 2.2 <9.20 <-1.21 1333 11 38 08.60 58 45 29.80 NGC 3795B 1251±2 1.34 -17.64 9.49 -11.97 2.83 2.4 <8.34 <-1.14 1336 11 38 36.20 33 52 04.60 CGCG 186-015 10844±3 1.61 -21.72 11.37 -12.78 3.39 2.0 <10.63 <-0.74 1339 11 39 03.30 -00 12 21.60 IC 0716 5413±3 1.68 -19.95 10.68 -11.73 1.39 1.1 <9.50 <-1.19 1344F 11 40 33.00 57 33 35.10 ASK 297088 1020±8 1.09 -12.93 — — 2.27 2.4 <7.69 <7.69 1353 11 42 19.50 57 53 46.00 MCG +10-17-045 1327±4 0.92 -15.16 7.54 -10.71 1.98 3.2 <8.03 <0.49 1356 11 42 32.84 26 29 20.00 NGC 3826 9090±3 1.59 -21.89 11.38 -12.66 1.64 2.5 <10.17 <-1.21 1364 11 44 04.70 09 09 53.90 PGC 1360766 6036±3 0.80 -17.36 6.14 -9.96 1.43 2.7 <9.36 <3.22 1367 11 44 13.99 33 30 52.20 NGC 3847 9517±3 1.49 -22.05 11.35 -12.64 2.17 2.1 <10.35 <-1.00 1369 11 44 24.50 60 53 02.60 2MASX J11442453+6053022 1497±2 0.92 -15.89 8.40 -9.96 2.31 1.6 <8.26 <-0.14 1379 11 46 04.50 56 33 56.10 ASK 296630 1021±6 0.50 -12.86 6.93 -9.77 2.71 1.0 <7.75 <0.82

Article number, page 61 of 71 A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1

Table A.3. – continued.

Source RA Dec Name V g-z M M sSFR rms SNR M MHI opt g ? HI M? (J2000.0) [log] [log] [log] [log] −1 km/s mag mag M yr mJy M 1382 11 46 13.50 54 10 34.30 ASK 237965 996±26 0.85 -13.29 — — 2.77 2.3 <7.78 <7.78 1388A1 11 47 06.90 03 06 23.00 ASK 74477 1016±2 0.44 -13.16 6.71 -9.29 2.69 1.9 <7.76 <1.05 1392 11 47 51.40 53 50 47.90 PGC 2452508 1019±40 0.77 -13.65 — — 1.88 1.7 <7.65 <7.65 1405 11 50 34.00 -00 32 16.20 UM 456A 1834±2 0.23 -15.29 7.49 -9.35 2.26 0.8 <8.35 <0.87 1409 11 50 59.60 47 57 49.40 ASK 348705 942±3 0.46 -13.16 6.77 -9.39 1.71 2.1 <7.49 <0.72 1410 11 51 13.40 50 09 24.80 NGC 3922 930±3 1.24 -17.55 9.25 -11.00 2.01 1.3 <7.93 <-1.32 1411 11 51 28.10 35 26 03.70 UGC 06827 3095±2 1.32 -19.42 10.13 -12.23 1.46 2.1 <8.99 <-1.15 1419A1 11 52 24.06 32 24 13.90 NGC 3935 3066±3 1.37 -19.60 10.22 -10.77 2.81 2.0 <9.27 <-0.94 1424A1 11 53 00.30 16 02 29.40 ASK 436517 905±29 0.63 -12.08 — — 2.89 -0.6 <7.63 <7.63 1433 11 54 41.20 46 36 36.30 ASK 348521 1009±1 -0.21 -13.65 6.14 -8.25 3.10 1.5 <7.83 <1.69 1442 11 56 07.10 64 21 02.60 2MASXi J1156072+642102 1410±2 0.99 -15.78 8.14 -10.10 3.29 1.3 <8.35 <0.21 1450 11 57 01.90 55 25 11.20 PGC 2501414 1208±2 0.94 -14.77 7.91 -10.16 2.80 3.1 <8.07 <0.16 1453A1 11 57 25.10 02 11 15.90 PGC 1218832 1019±2 0.49 -13.16 6.80 -9.49 2.63 2.0 <7.75 <0.95 1458 11 57 42.90 57 33 56.90 UGC 06939 4915±3 1.42 -20.43 10.63 -12.51 2.05 2.4 <9.61 <-1.01 1461 11 58 11.00 58 09 23.20 2MASX J11581094+5809237 954±3 0.76 -14.23 7.59 -10.21 2.49 1.0 <7.76 <0.17 1462 11 58 13.70 55 23 16.50 PGC 213915 969±6 1.16 -14.12 — — 3.04 2.4 <7.87 <7.87 1467 11 58 49.18 55 18 24.80 PGC 2832101 947±27 0.94 -13.55 — — 1.49 2.4 <7.49 <7.49 1473 11 59 21.80 56 46 46.20 PGC 2547530 1072±2 0.98 -14.08 7.62 -10.03 2.03 3.4 <7.77 <0.15 1476 11 59 49.60 30 50 39.90 IC 2986 3108±2 1.40 -18.91 10.00 -11.92 1.28 1.7 <8.89 <-1.11 1478 11 59 56.30 53 29 44.80 2MASX J11595620+5329451 1059±3 0.91 -14.12 7.62 -10.05 1.77 2.0 <7.70 <0.08 1480 12 00 02.40 42 47 23.00 PGC 2206215 987±7 0.97 -13.72 — — 1.65 1.9 <7.59 <7.59 1487 12 01 39.60 55 12 31.00 PGC 2832106 1188±9 0.89 -14.67 — — 2.58 0.9 <8.01 <8.01 1490 12 01 50.10 55 08 42.20 2MASX J12015013+5508422 1042±3 0.85 -15.27 7.98 -10.09 1.74 0.8 <7.77 <-0.22 1491 12 02 04.30 56 36 48.80 ASK 297309 1193±2 0.53 -13.41 7.05 -9.64 2.32 3.0 <7.85 <0.81 1496 12 02 55.50 55 49 05.60 ASK 239047 1034±12 0.93 -14.46 7.78 -10.51 2.11 1.6 <7.79 <0.01 1502 12 04 05.98 01 50 49.10 NGC 4063 4909±2 1.57 -19.82 10.57 -12.54 1.73 2.5 <9.50 <-1.07 1507 12 04 27.10 01 53 45.40 NGC 4073 5911±3 1.63 -22.18 11.41 -12.54 1.53 3.0 <9.80 <-1.61 1510 12 05 26.70 -00 16 56.20 ASK 375714 1341±7 0.70 -13.39 7.24 -9.77 1.47 1.8 <7.77 <0.52 1513 12 05 59.40 02 29 53.60 CGCG 041-039 6098±2 1.72 -20.46 10.96 -11.01 1.84 1.8 <9.76 <-1.20 1514D 12 06 02.50 36 51 49.20 NGC 4097 6275±2 1.40 -21.03 10.88 -12.43 1.65 2.6 <9.78 <-1.10 1516 12 06 38.99 28 10 28.00 NGC 4104 8441±4 1.41 -22.24 11.48 -12.85 2.31 3.0 <10.28 <-1.19 1518N 12 07 12.10 63 53 26.10 MCG +11-15-024 1425±3 0.89 -15.87 8.39 -10.66 3.32 1.2 <8.37 <-0.01 1523R 12 08 09.60 10 22 43.90 NGC 4119 1651±2 1.27 -19.05 10.05 -11.62 1.74 1.5 <8.48 <-1.57 1525N 12 08 10.70 55 44 47.20 PGC 2512985 1115±2 0.66 -14.73 7.61 -9.97 4.94 1.4 <8.23 <0.62 1532 12 08 55.10 41 44 27.10 UGC 07129 925±2 1.19 -16.79 8.97 -10.18 3.68 0.9 <8.12 <-0.84 1536 12 09 22.20 13 59 32.70 IC 3019 1675±14 0.77 -17.51 9.07 -11.89 1.53 1.4 <8.32 <-0.76 1540N 12 10 03.90 68 41 41.00 ASK 65617 2450±2 -1.18 -15.02 6.63 — 3.77 2.2 <8.83 <2.20 1542 12 10 12.50 64 45 37.80 MCG +11-15-032 1349±6 0.87 -16.22 8.44 -10.81 3.36 2.7 <8.36 <-0.08 1544 12 10 32.80 58 18 14.90 NGC 4149 3057±3 1.61 -19.24 10.37 -10.54 2.50 3.0 <9.20 <-1.17 1548 12 10 58.00 63 54 51.70 UGC 07179 2616±3 1.71 -18.90 6.20 -8.20 3.19 2.9 <9.14 <2.94 1549 12 11 02.70 12 06 14.40 IC 0767 1877±2 1.12 -18.21 9.41 -10.70 2.96 1.6 <8.75 <-0.66 1550 12 11 04.10 00 58 20.30 UGC 07177 6118±2 1.45 -20.81 10.78 -11.27 2.23 1.1 <9.87 <-0.91 1551 12 11 07.80 14 16 29.30 IC 3032 1184±6 1.05 -16.24 — — 2.79 0.9 <8.17 <8.17 1556 12 12 11.80 13 14 47.40 NGC 4165 1868±5 1.16 -18.22 9.49 -11.42 2.59 2.0 <8.69 <-0.79 1558 12 12 14.90 56 10 39.10 NGC 4172 9318±3 1.71 -21.89 11.46 -12.70 4.73 1.2 <10.66 <-0.80 1560 12 12 17.30 13 12 18.70 NGC 4168 2273±2 1.44 -20.70 10.63 -11.06 2.44 1.2 <9.04 <-1.59 1561F 12 12 18.90 15 28 59.10 VCC 50 1209±12 0.91 -15.31 — — 2.62 0.9 <8.09 <8.09 1567 12 12 55.20 44 05 27.40 ASK 319304 968±2 0.56 -12.85 6.74 -9.54 3.00 2.0 <7.74 <1.00 1570 12 13 29.30 50 44 29.30 NGC 4187 9220±2 1.63 -22.15 11.53 -12.77 3.05 2.3 <10.48 <-1.05 1574 12 14 44.20 12 10 50.70 NGC 4200 2341±2 1.30 -19.22 9.99 -11.98 1.66 1.3 <8.78 <-1.21 1575 12 15 08.50 14 58 18.70 VCC 137 1152±8 0.97 -14.14 — — 2.83 0.0 <7.99 <7.99 1576 12 15 12.60 14 25 58.30 IC 3065 995±3 1.09 -16.78 — — 1.41 2.4 <7.77 <7.77 1581 12 15 59.90 66 13 50.90 NGC 4221 1314±2 1.31 -18.77 9.83 -12.09 4.61 0.2 <8.69 <-1.15 1583 12 16 02.20 46 43 58.30 MCG +08-22-086 1061±8 0.99 -15.05 8.04 -11.13 2.01 2.8 <7.84 <-0.20 1584 12 16 09.10 12 41 28.60 IC 3081 1103±4 1.12 -15.70 — — 4.91 1.1 <8.32 <8.32 1586 12 16 28.50 33 53 06.20 ASK 506575 1071±28 0.74 -13.24 — — 1.73 3.3 <7.64 <7.64 1589 12 17 01.10 09 24 27.10 IC 3097 1253±7 1.05 -16.29 8.63 -11.00 1.90 0.8 <8.06 <-0.57 1591F 12 17 08.20 27 47 42.90 PGC 1818175 971±11 0.79 -14.88 — — 2.34 1.1 <7.81 <7.81 1595NZF 12 18 31.90 13 11 28.10 VCC 293 956±31 0.97 -13.70 — — 1.46 1.5 <7.49 <7.49 1596F 12 18 40.10 45 54 34.90 ASK 319587 1036±8 0.96 -14.09 — — 3.59 1.3 <7.99 <7.99 1598 12 19 00.50 06 05 40.50 VCC 315 1589±3 1.20 -17.20 9.13 -10.92 3.47 2.0 <8.60 <-0.53 1604 12 19 21.10 04 46 24.50 ASK 173829 2065±3 0.85 -15.38 8.09 -10.04 1.40 1.4 <8.28 <0.18 1605 12 19 22.20 05 22 35.00 NGC 4259 2474±2 1.40 -18.76 9.97 -12.07 2.45 1.8 <8.96 <-1.01 1607 12 19 32.10 49 48 56.70 UGC 07367 4093±2 1.45 -20.68 10.78 -12.25 2.75 1.6 <9.60 <-1.18 1608 12 19 32.60 56 44 11.60 NGC 4271 4756±2 1.56 -20.97 10.93 -12.15 2.06 2.1 <9.64 <-1.29 1609NRF 12 19 48.30 12 47 26.50 NGC 4267 919±16 1.43 -18.83 — — 1.80 3.1 <7.98 <7.98 1610 12 19 45.30 06 00 21.10 IC 3155 2241±3 1.28 -18.61 9.77 -11.47 2.53 0.8 <8.88 <-0.89 1611 12 19 47.20 05 17 01.60 NGC 4268 2006±2 1.44 -19.15 10.14 -12.23 2.12 1.1 <8.75 <-1.39 1612 12 19 47.60 30 20 20.70 NGC 4272 8446±3 1.47 -21.89 11.26 -12.42 1.95 1.4 <10.18 <-1.08 1614 12 20 03.30 14 57 41.40 IC 0781 1355±4 1.07 -17.19 9.26 -11.62 1.49 2.2 <8.10 <-1.16 1615 12 20 03.70 05 20 28.80 NGC 4277 2187±2 1.30 -18.68 9.79 -12.22 1.70 2.9 <8.69 <-1.10 1616 12 20 18.78 09 32 43.30 IC 3167 1876±8 0.87 -17.62 9.17 -11.12 1.72 2.0 <8.47 <-0.71

Article number, page 62 of 71 van Driel et al.: NIBLES – the Nançay HI survey

Table A.3. – continued.

Source RA Dec Name V g-z M M sSFR rms SNR M MHI opt g ? HI M? (J2000.0) [log] [log] [log] [log] −1 km/s mag mag M yr mJy M 1617 12 20 24.30 05 34 22.10 NGC 4282 937±4 1.52 -16.34 9.11 -11.81 1.39 2.5 <7.69 <-1.42 1623 12 21 04.80 11 45 16.50 IC 3192 1446±12 1.07 -15.74 8.41 -10.84 3.26 1.2 <8.37 <-0.04 1629 12 22 03.60 12 44 27.30 NGC 4305 1921±2 1.07 -19.14 9.75 -11.90 2.01 2.2 <8.67 <-1.08 1630 12 22 04.10 12 47 14.90 NGC 4306 1520±4 1.06 -18.10 9.35 -12.01 1.50 2.7 <8.26 <-1.08 1634 12 22 19.50 14 45 38.80 UGC 07436 982±5 1.10 -16.46 8.76 -11.97 1.66 2.1 <7.81 <-0.95 1635NZP 12 22 19.60 15 44 00.80 IC 0783A 1185±21 1.08 -15.72 — — 2.37 1.1 <8.06 <8.06 1640 12 22 50.80 13 35 34.30 VCC 592 1102±8 1.06 -14.80 — — 2.13 0.8 <7.88 <7.88 1644 12 23 09.90 00 25 37.30 PGC 1165632 2420±2 0.34 -14.88 7.32 -9.20 1.36 3.4 <8.34 <1.02 1647NRF 12 23 24.80 46 59 45.30 NGC 4346 943±8 1.41 -18.74 — — 3.41 1.7 <8.27 <8.27 1653 12 24 05.02 11 13 05.00 NGC 4352 2083±2 1.32 -19.42 10.08 -11.97 2.71 2.6 <8.91 <-1.17 1654NF 12 24 05.30 10 04 03.80 PGC 40315 1370±30 0.85 -15.50 — — 2.77 2.2 <8.23 <8.23 1658 12 24 51.60 13 06 40.20 VCC 753 915±37 0.90 -13.97 — — 2.73 1.2 <7.76 <7.76 1660 12 25 03.50 13 14 40.90 VCC 765 956±5 1.12 -14.58 — — 7.64 0.7 <8.30 <8.30 1661 12 25 18.80 64 56 00.50 NGC 4391 1320±2 1.32 -17.98 9.58 -12.18 2.99 1.8 <8.44 <-1.14 1663 12 25 35.90 15 50 52.00 VCC 816 1071±12 0.83 -14.99 — — 1.62 2.5 <7.75 <7.75 1664NZP 12 25 36.40 15 49 47.40 IC 3313 1071±22 0.89 -16.10 — — 1.52 1.6 <7.80 <7.80 1668 12 27 02.50 15 27 41.30 NGC 4421 1551±2 1.24 -19.47 10.04 -12.38 1.83 2.2 <8.48 <-1.56 1669 12 27 13.30 12 44 05.20 NGC 4425 1891±2 1.37 -19.75 10.22 -12.47 3.00 1.4 <8.89 <-1.33 1670 12 27 41.20 12 18 57.20 NGC 4436 1114±3 1.21 -17.44 9.12 -11.71 2.13 0.6 <8.10 <-1.02 1671 12 28 08.60 12 05 35.80 IC 0794 1921±4 1.31 -18.46 9.64 -11.86 2.08 1.8 <8.65 <-0.99 1674 12 30 02.60 09 24 11.80 ASK 275272 899±14 0.93 -13.23 — — 2.42 1.2 <7.63 <7.63 1675 12 30 10.30 10 46 46.10 NGC 4482 1835±3 1.14 -18.81 9.57 -11.93 2.01 0.7 <8.61 <-0.96 1676N 12 30 16.70 09 05 07.10 IC 3430 2115±2 0.99 -17.36 7.64 -10.80 1.81 1.5 <8.57 <0.93 1680 12 32 14.20 10 15 05.20 IC 3468 1300±4 1.16 -17.93 9.15 -11.95 1.49 2.4 <8.11 <-1.04 1682 12 32 39.00 10 05 31.40 VCC 1446 1196±14 1.05 -15.20 — — 1.60 2.5 <7.86 <7.86 1683 12 32 47.70 63 56 21.10 NGC 4512 2516±2 1.61 -19.91 10.60 -12.06 3.47 1.7 <9.23 <-1.37 1684 12 33 13.40 09 23 50.40 IC 3487 1074±4 0.73 -16.11 — — 1.99 1.6 <7.91 <7.91 1686 12 34 32.20 16 01 57.50 VCC 1570 1001±5 1.03 -14.99 — — 1.92 2.1 <7.76 <7.76 1688 12 35 20.20 06 06 54.30 NGC 4543 2374±2 1.33 -18.73 9.87 -11.88 2.67 1.7 <8.96 <-0.91 1690NF 12 35 38.20 12 16 07.30 NGC 4551 1251±17 1.43 -19.06 — — 1.21 2.6 <8.09 <8.09 1692 12 36 54.80 12 31 12.20 IC 3586 1723±5 1.03 -18.00 9.17 -11.11 1.70 1.9 <8.42 <-0.76 1693 12 37 07.00 05 25 17.90 VCC 1701 1168±4 1.17 -15.39 — — 2.34 1.0 <8.02 <8.02 1696 12 38 17.90 13 06 35.60 NGC 4584 1715±4 1.04 -18.35 9.46 -11.07 1.43 2.3 <8.37 <-1.09 1697 12 39 01.10 00 21 55.90 UGC 07813 6899±3 1.52 -21.16 11.04 -12.56 1.48 1.9 <9.83 <-1.21 1701 12 39 37.70 10 58 32.60 VCC 1803 1355±21 1.01 -15.27 8.24 -11.23 1.67 2.0 <7.99 <-0.25 1702 12 39 42.80 13 36 26.80 VCC 1806 1034±8 1.00 -14.19 — — 1.89 2.2 <7.72 <7.72 1705NRF 12 39 57.70 10 10 20.80 NGC 4596 1967±10 1.65 -20.76 — — 3.10 1.5 <9.03 <9.03 1708 12 40 13.40 12 52 29.10 IC 3635 1560±9 1.07 -16.20 8.69 -11.76 1.63 1.6 <8.18 <-0.51 1712 12 41 29.20 -00 43 11.50 ASK 1622 1175±3 0.50 -13.12 7.01 -9.53 2.48 2.1 <7.85 <0.83 1713 12 41 39.40 12 14 50.60 IC 3663 927±11 0.90 -15.34 — — 2.95 1.3 <7.91 <7.91 1715NF 12 41 46.10 11 29 19.10 IC 3665 1227±30 0.81 -16.16 — — 2.20 1.3 <8.09 <8.09 1716 12 41 59.40 12 56 34.20 NGC 4620 1125±3 0.99 -18.06 — — 1.44 2.6 <7.98 <7.98 1717NRPF 12 43 42.30 11 33 29.50 NGC 4649 1117±30 1.61 -20.32 — — 2.65 5.0 <8.43 <8.43 1719F 12 44 17.40 02 40 02.20 ASK 77655 1085±10 1.10 -12.76 — — 1.53 2.5 <7.56 <7.56 1723N 12 45 35.30 01 59 19.20 ASK 77777 1169±30 0.97 -14.14 — — 2.90 1.5 <8.01 <8.01 1724 12 46 07.30 -03 16 08.90 ASK 14107 1051±16 0.94 -13.48 — — 2.44 1.3 <7.79 <7.79 1726 12 47 16.10 11 45 36.70 IC 3775 1093±14 0.86 -14.76 — — 1.91 0.4 <7.82 <7.82 1727 12 47 20.60 12 09 59.10 IC 3779 1165±5 1.07 -16.03 — — 1.30 4.2 <7.81 <7.81 1733 12 48 55.40 14 54 28.30 IC 3806 1401±5 1.20 -17.59 9.31 -11.95 1.73 2.7 <8.22 <-1.09 1736NR 12 49 38.60 15 09 51.10 NGC 4710 1227±9 1.09 -19.56 8.93 -11.35 1.70 1.1 <8.26 <-0.67 1738 12 50 07.10 52 51 00.30 NGC 4732 9903±3 1.50 -21.61 11.25 -12.58 6.51 0.8 <10.82 <-0.43 1739 12 50 07.30 02 14 52.60 ASK 77703 1075±20 0.52 -14.02 — — 3.12 0.8 <7.95 <7.95 1741 12 51 00.20 01 50 45.10 PGC 1207820 953±14 0.88 -14.00 — — 1.20 1.7 <7.44 <7.44 1742 12 51 16.50 53 41 46.60 IC 0830 4847±2 1.43 -20.54 10.67 -12.30 2.42 1.6 <9.68 <-0.99 1743 12 51 41.50 13 05 41.80 CGCG 071-059 1487±6 0.80 -16.02 8.30 -10.23 1.14 2.8 <7.95 <-0.34 1744N 12 51 55.10 12 05 00.70 NGC 4746 1744±5 1.46 -18.51 — — 3.11 1.5 <8.75 <8.75 1745NRF 12 52 20.10 11 18 27.70 NGC 4754 1304±26 1.46 -20.20 — — 1.10 1.9 <8.18 <8.18 1746 12 52 33.70 -01 43 48.60 ASK 14845 1129±4 0.86 -15.25 8.04 -10.37 1.59 2.7 <7.80 <-0.24 1760 12 55 52.00 63 36 39.50 IC 0836 2658±6 1.20 -17.33 7.62 -8.81 1.51 1.6 <8.69 <1.07 1761 12 56 25.30 52 17 45.10 NGC 4834 11248±3 1.68 -21.50 11.32 -12.31 2.45 1.3 <10.50 <-0.82 1762 12 57 24.40 27 29 52.10 NGC 4839 7338±3 1.58 -21.76 11.39 -12.80 3.85 1.7 <10.35 <-1.04 1763 12 57 31.90 28 28 36.90 NGC 4841A 6765±3 1.53 -21.65 11.19 -12.46 1.51 2.1 <9.86 <-1.33 1766 12 58 09.00 14 51 32.10 UGC 08081 853±16 0.83 -14.90 — — 2.27 1.3 <7.69 <7.69 1767 12 58 12.70 26 23 48.70 NGC 4849 5894±2 1.54 -21.01 10.98 -12.40 1.72 1.2 <9.75 <-1.24 1770 12 59 35.70 27 57 33.30 NGC 4874 7167±3 1.54 -22.29 11.49 -12.58 1.66 2.2 <10.00 <-1.49 1771NZ 12 59 45.10 -00 52 16.60 PGC 1132599 1229±30 0.52 -13.53 — — 1.71 1.8 <7.76 <7.76 1773 12 59 57.80 28 14 48.00 NGC 4881 6706±2 1.52 -20.77 10.86 -12.27 2.67 1.8 <10.03 <-0.83 1774 13 00 10.60 12 28 59.90 NGC 4880 1362±3 1.05 -18.67 9.51 -12.24 1.28 1.5 <8.15 <-1.36 1779NUZPFV 13 00 41.60 37 19 36.10 NGC 4914 4656±74 1.32 -21.81 — — 1.89 1.9 <9.64 <9.64 1782 13 01 06.70 39 50 29.20 IC 4064 10648±3 1.56 -22.51 11.53 -12.61 3.09 0.6 <10.63 <-0.90 1789 13 04 58.40 29 07 20.00 NGC 4952 5920±3 1.45 -21.26 11.03 -12.60 1.62 0.5 <9.74 <-1.29 1797 13 07 38.70 -00 56 32.80 IC 0849 5419±4 0.89 -20.41 10.03 -10.13 2.91 1.4 <9.83 <-0.20

Article number, page 63 of 71 A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1

Table A.3. – continued.

Source RA Dec Name V g-z M M sSFR rms SNR M MHI opt g ? HI M? (J2000.0) [log] [log] [log] [log] −1 km/s mag mag M yr mJy M 1798 13 07 59.10 51 55 45.40 NGC 4987 4699±2 1.45 -20.24 10.64 -12.40 2.42 2.3 <9.63 <-1.00 1799 13 08 19.20 45 21 42.10 UGC 08225 8600±3 1.48 -21.84 11.22 -10.96 2.72 1.3 <10.33 <-0.89 1801 13 08 42.10 52 01 00.60 CGCG 271-017 4705±2 1.49 -20.18 10.63 -12.33 1.86 2.6 <9.52 <-1.12 1803 13 09 03.60 -00 45 57.60 CGCG 016-010 5157±3 1.44 -20.02 10.51 -12.40 3.03 1.7 <9.80 <-0.71 1805 13 09 31.90 00 51 25.20 NGC 4996 5439±3 1.50 -20.83 10.88 -12.55 1.24 1.0 <9.52 <-1.36 1807A1 13 09 36.90 31 40 34.00 PGC 1958740 2159±4 -0.05 -15.06 7.56 -9.91 1.96 2.1 <8.42 <0.85 1809 13 10 23.80 -01 00 37.90 2MASX J13102375-0100373 5602±2 1.38 -20.41 — — 1.76 1.0 <9.66 <9.66 1818 13 14 46.00 53 49 13.20 CGCG 271-026 4711±2 1.47 -19.99 10.53 -12.23 2.03 2.5 <9.54 <-0.99 1825 13 17 07.60 57 32 22.10 IC 0875 2760±2 1.24 -19.38 10.01 -11.98 1.88 2.5 <8.99 <-1.02 1832 13 20 31.60 43 51 55.60 ASK 321949 1221±17 0.93 -13.09 7.29 -10.67 1.82 2.6 <7.76 <0.48 1846 13 23 45.00 31 33 56.70 NGC 5127 4851±3 1.49 -21.30 11.01 -12.70 1.63 0.7 <9.58 <-1.43 1847 13 23 56.94 30 59 16.90 NGC 5131 6846±3 1.52 -21.26 11.05 -12.14 1.99 1.9 <9.95 <-1.10 1849A2 13 24 10.00 13 58 35.50 NGC 5129 6885±3 1.45 -22.28 11.34 -12.51 1.94 2.2 <10.03 <-1.31 1860 13 28 33.04 32 04 09.71 NGC 5166B 4838±4 1.37 -19.22 10.09 -11.60 1.71 1.8 <9.43 <-0.67 1868 13 30 47.80 39 54 45.70 ASK 355809 1236±2 0.39 -13.29 6.86 -9.50 2.55 2.1 <7.91 <1.06 1877A1 13 34 06.90 09 15 43.20 PGC 4544337 1112±12 0.51 -13.70 7.30 -10.09 1.33 1.2 <7.58 <0.28 1879A1 13 35 37.20 14 21 39.40 PGC 1456087 993±22 0.78 -13.81 — — 1.20 1.4 <7.45 <7.45 1882 13 35 48.20 02 59 56.10 NGC 5231 6526±3 1.46 -21.24 10.98 -10.67 1.62 2.6 <9.82 <-1.16 1888 13 36 20.08 38 06 53.60 ASK 508595 5157±2 0.70 -16.97 8.53 -9.75 1.97 1.9 <9.34 <0.81 1890 13 37 27.02 38 36 56.40 CGCG 218-028 3976±3 1.11 -18.47 9.53 -11.11 2.44 0.9 <9.34 <-0.19 1893A2 13 38 43.10 31 16 13.90 CGCG 161-101 4699±2 1.53 -19.85 10.52 -12.39 1.33 2.6 <9.35 <-1.17 1895 13 38 59.05 31 21 54.40 CGCG 161-102 4590±2 1.48 -19.57 10.36 -11.97 1.65 1.7 <9.39 <-0.97 1896 13 39 03.15 43 33 58.60 CGCG 218-031 2740±2 1.38 -18.22 9.71 -11.77 2.01 1.5 <8.92 <-0.78 1912 13 44 23.20 05 47 32.60 UGC 08689 6840±2 1.49 -21.36 11.00 -12.08 1.55 2.5 <9.85 <-1.14 1915 13 45 38.90 56 36 59.60 UGC 08704 10479±3 1.48 -21.76 11.20 -12.34 3.82 2.0 <10.65 <-0.55 1918 13 46 41.40 59 49 22.60 2MASX J13464142+5949225 1865±2 1.06 -16.50 8.71 -10.40 2.80 1.6 <8.59 <-0.12 1919 13 46 46.20 60 59 12.00 ASK 159746 1730±7 1.09 -15.36 8.29 -10.33 2.60 1.6 <8.40 <0.11 1924F 13 47 57.40 04 18 50.60 ASK 178124 1048±26 0.90 -12.70 — — 0.99 3.1 <7.33 <7.33 1926 13 48 15.24 37 42 24.90 ASK 512367 2366±2 0.60 -15.13 7.75 -9.89 2.88 1.4 <8.68 <0.94 1929 13 48 34.70 37 06 47.90 CGCG 190-059 10254±2 1.38 -21.73 11.11 -12.23 1.40 0.8 <10.19 <-0.92 1930 13 48 56.30 59 50 08.60 UGC 08741 2019±6 1.34 -18.01 9.44 -10.62 2.26 1.0 <8.69 <-0.75 1939 13 50 41.50 40 16 45.60 CGCG 218-060 2300±3 1.42 -17.89 9.62 -11.96 2.13 2.7 <8.77 <-0.85 1940 13 50 43.70 33 37 57.30 NGC 5321 4627±2 1.41 -19.70 10.35 -12.38 1.56 1.1 <9.39 <-0.96 1941 13 51 25.40 40 12 47.70 Mrk 0462 2468±3 0.91 -17.76 9.01 -10.00 2.53 0.7 <8.88 <-0.13 1946 13 52 05.60 05 45 54.10 PGC 4389504 984±2 0.71 -13.95 7.52 -10.54 1.53 2.3 <7.56 <0.05 1947 13 52 08.35 14 06 58.40 IC 0946 6798±2 1.46 -21.18 10.94 -12.40 1.76 1.9 <9.89 <-1.05 1949 13 52 10.80 05 30 13.80 ASK 178807 1216±20 0.61 -14.27 6.09 -10.45 2.49 1.6 <7.98 <1.89 1951A2 13 52 26.70 14 05 28.60 IC 0948 6892±3 1.54 -21.33 11.14 -12.69 1.41 2.0 <9.82 <-1.31 1953 13 52 37.40 24 44 55.80 UGC 08788 9077±3 1.53 -21.60 11.27 -12.70 2.41 1.3 <10.31 <-0.95 1954 13 52 53.19 37 41 22.20 2MASX J13525317+3741219 5317±2 1.41 -19.42 10.24 -12.24 4.56 1.2 <9.95 <-0.29 1959 13 53 19.80 05 46 17.90 UGC 08799 1046±16 1.10 -15.04 8.26 -11.39 1.79 2.2 <7.78 <-0.48 1961 13 53 23.30 61 40 20.00 UGC 08822 1855±5 1.10 -16.99 9.00 -10.24 2.63 3.2 <8.60 <-0.40 1963 13 53 33.53 37 23 13.10 IC 4340 7468±3 1.52 -21.28 11.11 -12.61 1.55 1.4 <9.93 <-1.18 1965 13 53 38.40 36 08 02.50 NGC 5352 7956±3 1.50 -21.81 11.26 -12.69 2.32 1.3 <10.20 <-1.06 1971 13 55 07.47 13 52 35.00 2MASX J13550750+1352345 11991±4 1.37 -20.38 10.52 -11.57 1.91 2.2 <10.35 <-0.17 1973 13 55 37.60 04 59 00.10 NGC 5360 1180±4 0.99 -16.27 8.32 -9.66 1.54 1.4 <7.91 <-0.41 1979 13 56 26.60 04 23 48.00 UGC 08857 1115±3 1.04 -16.16 6.22 -8.51 2.45 1.4 <8.05 <1.83 1981 13 56 55.57 05 09 06.70 CGCG 046-013 1517±10 1.04 -16.25 8.60 -11.59 2.26 1.5 <8.29 <-0.31 1983 13 56 58.00 45 58 23.60 UGC 08876 2059±2 1.39 -18.54 9.88 -12.21 2.49 1.2 <8.79 <-1.09 1988FA1 13 57 23.60 05 34 25.20 ASK 179268 994±21 0.35 -14.95 — — 2.73 2.6 <7.90 <7.90 1989A2 13 57 29.52 09 57 03.20 CGCG 074-017 6969±3 1.30 -19.82 10.29 -11.92 1.42 1.6 <9.71 <-0.58 1992 13 58 12.80 06 31 05.40 NGC 5384 5094±2 1.56 -20.74 10.88 -11.68 2.33 2.5 <9.73 <-1.15 1998A1 13 58 45.00 24 09 05.00 2MASX J13584501+2409048 970±2 0.76 -13.86 7.34 -9.86 2.01 1.7 <7.65 <0.32 2004 14 00 37.20 -02 51 28.10 NGC 5400 7446±3 1.58 -21.90 11.30 -12.48 1.71 2.8 <10.02 <-1.28 2007 14 00 58.20 55 34 05.10 ASK 301537 1842±11 0.82 -15.78 8.22 -10.05 2.45 2.5 <8.45 <0.23 2012 14 02 08.70 61 24 44.70 ASK 108562 1691±2 0.39 -14.23 7.14 -9.32 3.19 1.2 <8.35 <1.21 2015 14 02 36.10 39 13 13.20 PGC 50011 1326±2 0.26 -14.89 7.13 -8.97 1.54 2.1 <7.88 <0.75 2018N 14 03 00.70 61 45 07.50 UGC 08982 1649±7 0.99 -16.94 8.73 -11.21 3.14 1.5 <8.56 <-0.16 2021D 14 03 31.50 35 01 31.10 NGC 5445 3884±2 1.46 -20.16 10.64 -12.39 2.74 2.8 <9.52 <-1.12 2023 14 03 47.20 35 44 30.00 UGC 08984 3805±2 1.41 -19.83 10.42 -12.17 3.79 0.8 <9.61 <-0.81 2024 14 03 52.43 55 35 32.50 ASK 301585 1969±1 -0.12 -13.97 6.64 -8.56 3.79 1.6 <8.54 <1.90 2026 14 04 15.80 04 06 43.80 UGC 08986 1239±4 1.26 -17.08 9.08 -11.21 2.67 1.8 <8.27 <-0.81 2027 14 04 42.99 55 26 06.70 2MASX J14044299+5526064 1537±3 1.01 -16.39 8.63 -10.38 4.84 1.2 <8.65 <0.01 2028 14 04 45.70 14 22 55.30 NGC 5454 7603±2 1.46 -21.54 11.03 -12.22 2.83 1.1 <10.23 <-0.81 2029 14 04 58.90 11 52 17.80 NGC 5456 7126±3 1.30 -21.66 11.00 -11.81 1.83 1.7 <9.98 <-1.02 2030 14 05 12.40 55 44 30.60 NGC 5475 1647±2 1.40 -18.84 9.98 -12.18 5.10 0.9 <8.93 <-1.04 2036 14 06 48.20 55 01 47.70 NGC 5484 2029±3 1.31 -17.03 9.19 -11.44 3.20 1.8 <8.77 <-0.42 2038 14 07 11.30 55 00 06.00 NGC 5485 1904±2 1.52 -20.32 10.52 -11.85 2.39 0.6 <8.85 <-1.66 2040 14 07 24.30 59 30 09.40 2MASX J14072420+5930095 1820±1 0.61 -15.43 7.83 -9.62 3.68 1.2 <8.58 <0.75 2042 14 07 39.30 54 47 40.60 CGCG 272-032 2315±2 1.29 -18.40 9.68 -11.69 2.84 0.6 <8.94 <-0.74 2043F 14 07 58.40 50 51 48.40 PGC 4016145 1759±5 0.99 -15.21 6.02 -8.44 2.81 1.2 <8.43 <2.41 2048 14 09 42.00 56 32 31.40 ASK 249604 1704±34 1.00 -14.52 7.94 -10.72 3.09 1.4 <8.40 <0.45

Article number, page 64 of 71 van Driel et al.: NIBLES – the Nançay HI survey

Table A.3. – continued.

Source RA Dec Name V g-z M M sSFR rms SNR M MHI opt g ? HI M? (J2000.0) [log] [log] [log] [log] −1 km/s mag mag M yr mJy M 2049 14 09 48.10 55 39 19.80 ASK 250227 1643±4 0.57 -13.85 7.28 -9.56 2.20 2.3 <8.15 <0.87 2050F 14 09 49.90 57 13 29.30 ASK 249640 1742±24 0.31 -15.05 6.04 -9.39 4.21 2.2 <8.57 <2.53 2051 14 09 54.90 56 49 21.30 CGCG 295-037 1790±5 1.25 -17.16 9.18 -10.89 2.64 2.0 <8.59 <-0.59 2055 14 10 15.20 48 32 45.90 NGC 5500 1905±2 1.30 -18.58 9.71 -11.88 2.21 2.9 <8.67 <-1.04 2056D 14 10 29.22 48 41 39.30 ASK 400932 2035±3 0.51 -14.33 7.46 -9.87 2.14 2.6 <8.36 <0.90 2058 14 10 47.70 35 54 48.50 NGC 5499 8425±3 1.63 -21.83 11.29 -12.05 2.98 1.1 <10.36 <-0.92 2059N 14 11 24.00 -03 10 02.60 ASK 199473 1628±1 0.15 -14.13 7.04 -8.96 1.61 1.9 <8.01 <0.97 2061 14 11 38.70 39 38 30.80 UGC 09081 5415±2 1.38 -20.94 10.78 -12.33 1.89 2.5 <9.70 <-1.08 2064 14 11 56.00 27 06 50.00 IC 4384 10463±3 1.55 -21.80 11.30 -12.60 4.47 0.8 <10.72 <-0.57 2071 14 13 39.38 53 24 52.90 ASK 302080 5553±2 0.66 -16.83 6.38 -9.76 2.48 1.2 <9.49 <3.11 2080D 14 16 52.90 10 48 26.70 NGC 5532 7408±3 1.55 -22.63 11.57 -12.45 1.54 1.7 <10.02 <-1.55 2084A1 14 17 07.50 04 50 13.40 ASK 99987 1643±2 0.37 -14.11 7.09 -9.35 2.17 2.2 <8.15 <1.07 2086 14 18 09.20 07 33 52.30 NGC 5546 7376±3 1.53 -22.12 11.46 -12.65 2.00 1.9 <10.10 <-1.36 2087 14 18 16.38 36 53 00.80 2MASX J14181638+3653012 3396±5 1.52 -17.92 9.72 -10.64 1.69 1.0 <9.01 <-0.70 2088 14 18 38.80 07 22 38.40 NGC 5549 7672±3 1.58 -22.02 11.43 -12.56 1.29 2.0 <9.93 <-1.49 2090 14 19 14.25 36 21 33.70 Mrk 0675 3145±3 1.25 -17.89 9.45 -11.22 1.97 1.2 <9.00 <-0.45 2094A1 14 19 29.08 35 34 01.10 ASK 392553 3207±2 0.80 -16.38 8.39 -9.80 2.47 1.6 <8.98 <0.59 2099A1 14 20 11.10 10 15 46.50 NGC 5562 9142±4 1.61 -21.84 11.40 -12.78 1.77 2.3 <10.21 <-1.19 2104 14 20 43.50 04 08 37.10 ASK 100147 1668±10 0.93 -15.00 6.25 -10.07 2.72 1.8 <8.36 <2.11 2109 14 20 59.40 06 12 09.50 NGC 5575 7567±3 1.58 -21.37 11.16 -12.44 1.32 1.8 <9.88 <-1.28 2115 14 22 00.00 02 34 22.30 PGC 1231137 1648±35 0.91 -14.11 7.70 -10.82 1.71 1.1 <8.08 <0.38 2118 14 22 28.30 40 19 11.30 NGC 5598 5429±2 1.46 -20.90 10.87 -12.21 1.69 1.3 <9.66 <-1.22 2121 14 22 41.50 04 29 58.70 PGC 4113298 8289±4 0.84 -17.99 6.40 -10.76 2.42 1.9 <9.93 <3.52 2125 14 23 46.30 34 01 01.20 UGC 09222 3541±3 1.41 -18.87 10.02 -11.04 4.46 0.9 <9.54 <-0.48 2129 14 24 42.10 35 16 01.80 UGC 09235 2995±3 1.25 -18.64 9.76 -11.44 3.23 1.0 <9.23 <-0.53 2131 14 25 08.90 -01 06 48.50 CGCG 019-019 2643±4 1.18 -17.27 9.21 -10.97 1.40 0.7 <8.65 <-0.55 2139 14 28 07.20 25 52 07.50 IC 1017 4371±2 1.49 -20.18 10.61 -12.29 1.56 2.7 <9.38 <-1.23 2140NZA1 14 28 08.70 01 49 25.60 ASK 082514 1728±30 0.30 -14.29 — — 1.43 1.3 <8.03 <8.03 2145 14 28 49.50 26 01 56.10 IC 1020 4282±2 1.46 -19.55 10.36 -12.27 1.72 2.3 <9.35 <-1.01 2146 14 29 14.45 44 41 56.30 CGCG 247-032 2409±2 1.34 -18.17 9.71 -11.94 1.85 2.5 <8.77 <-0.94 2152NZF 14 30 07.20 08 42 16.00 ASK 457251 1427±35 0.53 -13.36 — — 1.37 2.5 <7.77 <7.77 2155 14 30 25.60 11 55 40.70 NGC 5644 7649±3 1.52 -21.99 11.33 -12.56 1.65 1.9 <10.04 <-1.29 2156 14 30 30.20 40 01 04.40 UGC 09336 7714±3 1.69 -20.79 11.01 -11.02 1.50 2.4 <9.91 <-1.10 2162A2 14 31 53.00 03 22 48.30 2MASX J23244466+0101490 1529±2 0.64 -13.52 6.94 -9.37 1.81 2.6 <7.97 <1.03 2179NP 14 35 50.20 36 32 35.60 NGC 5684 4093±2 1.49 -20.37 — — 1.32 1.5 <9.26 <9.26 2180 14 35 55.60 36 43 10.30 CGCG 192-047 4099±3 1.45 -19.30 10.26 -12.48 1.60 2.7 <9.26 <-1.00 2182 14 36 15.40 29 54 30.10 NGC 5685 10381±3 1.45 -21.74 11.22 -12.47 2.43 1.3 <10.44 <-0.78 2203 14 40 37.90 03 22 37.20 IC 1041 7902±3 1.69 -21.01 11.10 -11.38 1.34 1.0 <9.90 <-1.21 2205 14 40 42.80 03 27 55.50 NGC 5718 8196±2 1.63 -22.15 11.45 -12.61 2.03 1.9 <10.19 <-1.26 2209 14 41 32.90 38 51 04.90 UGC 09473 4669±3 1.46 -20.77 10.80 -10.34 2.03 2.7 <9.59 <-1.21 2221N 14 45 15.80 -00 09 34.30 ASK 8160 1664±4 -0.05 -16.40 8.40 -9.90 1.55 0.7 <8.21 <-0.19 2225A1 14 45 36.30 34 10 43.80 ASK 394208 1642±6 0.40 -14.51 7.15 -10.65 3.60 2.1 <8.40 <1.25 2229D 14 46 21.70 32 46 48.80 UGC 09518 8714±3 1.51 -21.68 11.24 -12.41 2.20 1.6 <10.25 <-1.00 2230 14 47 00.10 11 35 31.20 UGC 09521 9343±3 1.56 -21.66 11.22 -12.32 3.67 1.1 <10.53 <-0.69 2237 14 49 34.40 47 22 34.20 NGC 5767 7731±3 1.60 -21.28 11.14 -12.58 2.38 2.4 <10.14 <-0.99 2238 14 50 22.90 02 57 30.70 PGC 1241857 1697±1 0.71 -15.59 7.96 -9.76 1.60 2.8 <8.18 <0.22 2240 14 50 59.90 02 20 16.40 ASK 84013 1527±27 0.78 -13.53 7.47 -10.80 1.62 2.0 <7.94 <0.47 2249 14 54 23.20 38 50 38.30 CGCG 221-008 8685±3 1.66 -20.91 11.03 -12.15 2.10 0.3 <10.16 <-0.87 2250 14 54 32.70 02 57 59.10 NGC 5776 8165±3 1.48 -21.80 11.22 -12.60 1.91 0.5 <10.14 <-1.08 2253 14 56 01.20 02 27 48.70 CGCG 048-072 2090±2 0.91 -17.88 9.13 -10.56 1.66 1.9 <8.56 <-0.57 2255 14 57 11.20 52 20 45.80 UGC 09629 7822±3 1.57 -20.97 11.05 -12.47 5.19 0.9 <10.47 <-0.58 2257 14 58 48.70 02 01 24.60 CGCG 020-039 1804±2 1.27 -17.90 9.50 -11.41 1.34 2.1 <8.35 <-1.14 2265NF 15 00 33.00 02 13 49.10 PGC 3350778 1312±30 0.88 -14.70 — — 2.31 0.8 <8.06 <8.06 2268 15 01 21.10 01 38 13.40 NGC 5814 10531±2 1.26 -21.93 11.10 -10.29 3.32 1.8 <10.59 <-0.51 2272F 15 05 25.70 02 05 58.80 NGC 5838 1252±4 1.55 -19.90 7.52 -11.90 2.35 2.3 <8.45 <0.93 2274 15 05 28.70 01 17 33.20 PGC 1190358 2303±2 0.71 -15.55 7.33 -8.90 1.87 3.4 <8.53 <1.20 2275 15 05 31.80 01 35 15.50 PGC 4609811 919±13 0.92 -13.24 — — 2.74 1.5 <7.71 <7.71 2276NRZP 15 06 29.30 01 36 20.20 NGC 5846 1715±65 1.55 -20.36 — — 2.24 1.5 <8.74 <8.74 2277 15 06 35.00 02 00 17.30 NGC 5841 1256±2 1.34 -17.51 9.13 — 2.78 0.8 <8.33 <-0.81 2282 15 09 31.60 54 30 23.30 NGC 5876 3253±2 1.53 -20.03 10.63 -12.59 3.90 0.8 <9.51 <-1.12 2284 15 09 38.80 42 42 48.20 CGCG 221-032 5534±2 1.33 -19.89 10.28 -11.76 2.09 0.5 <9.68 <-0.60 2286N 15 11 13.30 46 09 03.30 UGC 09761 5494±2 1.41 -21.47 — — 2.09 1.2 <9.80 <9.80 2288 15 11 48.40 46 15 13.80 CGCG 249-011 5454±2 1.38 -19.68 10.31 -10.52 3.51 2.5 <9.88 <-0.43 2289 15 12 24.00 02 04 48.20 ASK 84838 1682±10 1.08 -15.45 8.32 -10.73 2.61 1.8 <8.38 <0.06 2291 15 13 29.20 58 30 33.60 Mrk 0847 2543±3 1.02 -18.46 9.41 -9.98 3.94 1.1 <9.15 <-0.26 2294 15 15 09.40 02 45 06.40 PGC 1236445 1763±3 0.91 -15.83 8.38 -10.34 1.97 1.0 <8.33 <-0.05 2297 15 17 29.40 03 35 08.00 PGC 3124577 1882±2 0.86 -15.21 8.03 -10.06 1.92 2.0 <8.32 <0.29 2298 15 17 49.20 04 09 45.30 UGC 09804 11039±4 2.15 -21.56 11.78 -12.79 5.27 1.4 <10.85 <-0.93 2300 15 18 43.80 41 51 55.60 NGC 5914 5441±2 1.57 -20.40 10.74 -12.06 3.19 0.7 <9.90 <-0.84 2305 15 21 55.30 08 25 25.60 IC 1116 11706±3 1.50 -22.18 11.41 -12.28 3.02 0.8 <10.68 <-0.73 2307 15 22 36.60 -01 44 00.50 ASK 202484 8225±2 0.73 -17.50 6.17 -9.14 2.89 1.9 <9.95 <3.78

Article number, page 65 of 71 A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1

Table A.3. – continued.

Source RA Dec Name V g-z M M sSFR rms SNR M MHI opt g ? HI M? (J2000.0) [log] [log] [log] [log] −1 km/s mag mag M yr mJy M 2308 15 23 35.20 09 20 46.10 CGCG 077-110 10703±3 1.48 -21.62 11.22 -12.38 2.80 1.9 <10.52 <-0.69 2311A1 15 24 50.10 03 04 53.10 SHOC 505 1753±1 0.38 -14.87 7.56 -9.41 2.74 1.5 <8.37 <0.81 2316A1 15 27 44.50 09 41 56.80 ASK 421256 1820±2 0.51 -15.62 7.96 -9.67 2.57 2.2 <8.44 <0.48 2317A1 15 27 53.00 25 38 37.50 PGC 1744110 1470±1 0.38 -13.64 6.91 -9.26 1.72 1.3 <7.92 <1.01 2327A1 15 33 36.75 33 21 33.60 ASK 313250 1999±2 0.36 -14.56 7.40 -9.43 1.61 2.0 <8.23 <0.83 2331NU 15 37 06.68 58 56 51.40 ASK 111975 3003±30 0.85 -15.65 — — 3.50 1.4 <9.03 <9.03 2337 15 42 35.50 23 40 12.10 IC 4576 6741±3 1.47 -21.04 10.89 -12.47 2.89 1.1 <10.09 <-0.81 2342NPF 15 56 14.40 06 05 53.40 ASK 461670 1797±3 1.41 -11.64 — — 2.80 2.4 <8.14 <8.14 2343 15 56 33.70 21 17 20.70 CGCG 137-004 4397±2 1.23 -20.35 10.40 -11.70 2.21 1.8 <9.54 <-0.86 2344 15 57 03.00 48 10 06.10 IC 1153 5894±3 1.58 -21.25 11.11 -12.25 3.13 1.1 <10.03 <-1.09 2345 15 57 08.10 22 24 16.40 NGC 6020 4304±2 1.42 -20.83 10.84 -12.83 2.16 2.8 <9.56 <-1.28 2349A1 16 00 13.80 17 50 53.80 PGC 1543427 2053±1 0.46 -15.64 7.71 -9.42 2.62 2.6 <8.55 <0.84 2351 16 01 51.40 17 57 26.90 NGC 6030 4403±2 1.47 -20.76 10.74 -12.03 2.63 0.8 <9.66 <-1.09 2353 16 02 11.60 07 05 09.90 CGCG 051-021 2654±2 1.45 -18.69 9.98 -10.27 2.81 1.2 <9.08 <-0.90 2355 16 02 19.80 16 20 45.70 UGC 10144 11494±3 1.67 -22.19 11.53 -12.58 3.15 1.2 <10.69 <-0.84 2356 16 02 30.50 21 07 14.50 CGCG 137-019 4507±2 1.48 -20.42 10.65 -12.30 2.71 2.2 <9.66 <-0.99 2367 16 27 41.10 40 55 37.10 NGC 6160 9511±4 1.64 -21.95 9.94 -9.50 4.79 2.7 <10.68 <0.74 2368 16 29 44.90 40 48 41.90 NGC 6173 8795±2 1.52 -22.75 11.58 -12.53 6.91 2.0 <10.84 <-0.75 2371 16 34 39.90 46 57 37.40 2MASXi J1634398+465736 2452±1 0.61 -16.34 8.26 -9.50 2.64 2.1 <8.77 <0.51 2373A1 16 35 20.70 17 45 55.10 Mrk 0886 2740±1 0.63 -17.82 8.94 -9.52 3.00 1.3 <9.04 <0.09 2375N 16 38 35.70 41 49 43.30 ASK 117223 8575±2 0.53 -17.17 7.17 -10.64 3.71 1.6 <10.07 <2.90 2378 16 41 06.60 46 00 14.50 IC 1226 5312±4 1.38 -19.60 10.26 -11.02 2.74 2.7 <9.74 <-0.52 2380 16 44 56.10 64 15 54.00 PGC 3139142 2863±1 0.64 -14.99 7.77 -9.75 3.98 1.4 <8.98 <1.21 2381 16 46 54.60 31 53 07.80 FGC 2068 4419±8 0.56 -17.45 6.74 -10.73 2.78 2.5 <9.39 <2.66 2382 16 58 50.70 40 07 16.30 CGCG 225-021 8657±2 1.53 -21.21 11.06 -12.46 3.13 2.0 <10.36 <-0.70 2386 17 01 29.60 22 43 52.40 ASK 406590 2820±1 0.75 -15.41 8.11 -9.92 3.65 1.3 <8.96 <0.85 2387 17 08 41.60 61 06 30.70 2MASX J17084172+6106264 6003±2 0.57 -18.74 7.23 -10.99 5.35 2.6 <10.04 <2.80 2388 17 09 44.10 62 58 23.00 NGC 6319 8197±2 1.48 -21.47 — — 4.82 0.8 <10.52 <10.52 2397 20 58 12.50 -07 16 53.70 PGC 3104052 5734±3 0.79 -16.49 8.45 -9.97 2.46 2.0 <9.49 <1.04 2401A2 21 04 51.99 00 26 52.70 CGCG 374-042 4129±3 1.36 -18.88 9.95 -12.02 3.84 1.9 <9.61 <-0.34 2402A1 21 13 07.70 01 13 47.20 2MASX J21130776+0113480 4157±2 0.75 -18.01 8.97 -9.78 1.88 2.6 <9.21 <0.24 2404 21 14 50.20 -07 27 43.30 2MASXJ21145025-0727431 8540±3 1.36 -20.95 10.75 -11.01 3.25 2.7 <10.33 <-0.42 2405 21 15 16.20 09 53 47.10 ASK 138334 5239±2 0.49 -17.14 8.38 -9.40 2.56 2.1 <9.47 <1.09 2406A2 21 16 24.80 10 16 24.10 CGCG 426-029 5175±3 1.26 -19.54 10.15 -11.09 2.01 2.0 <9.58 <-0.57 2409 21 17 06.99 -06 43 27.90 2MASXJ21170700-0643281 8749±3 1.36 -21.65 11.06 -10.79 4.44 1.4 <10.54 <-0.52 2411 21 18 06.60 -07 42 56.70 2MASX J21180656-0742566 2516±3 0.56 -16.28 8.17 -9.74 3.79 2.1 <8.94 <0.77 2416A1 21 28 29.10 10 04 52.60 2MASX J21282910+1004527 4929±3 1.02 -17.63 9.10 -10.14 1.64 1.9 <9.28 <0.18 2423A1 21 42 22.80 12 29 53.80 UGC 11794 5848±4 1.42 -20.12 10.50 -11.28 1.70 2.5 <9.66 <-0.84 2430A2 21 50 27.60 12 38 10.30 2MASX J21502753+1238103 6507±3 1.42 -18.75 9.98 -11.69 2.51 1.5 <9.82 <-0.16 2432DA1 21 50 38.40 13 17 17.40 CGCG 427-027 6045±2 1.50 -20.81 10.88 -11.40 1.71 1.8 <9.75 <-1.13 2433A1 21 52 22.50 -01 10 15.70 ASK 21400 4770±2 0.55 -16.57 8.14 -9.48 3.53 2.9 <9.48 <1.34 2436A1 21 54 47.70 00 13 45.70 ASK 21641 2984±2 0.48 -15.76 7.88 -9.47 3.77 2.5 <9.04 <1.16 2440N 22 01 41.60 11 51 24.30 CGCG 428-014 8943±3 2.04 -20.88 11.33 -11.34 2.73 1.7 <10.32 <-1.01 2442NA2 22 04 08.80 -00 55 31.90 ASK 22153 4825±17 0.82 -16.68 8.66 -10.35 3.50 2.5 <9.52 <0.86 2451 22 24 44.10 12 21 40.70 2MASX J22244417+1221410 5127±4 1.35 -18.54 9.80 -10.43 1.39 2.9 <9.33 <-0.47 2452A1 22 26 19.50 12 15 02.00 ASK 140946 3527±9 0.49 -15.59 7.72 -9.51 2.44 2.0 <8.99 <1.26 2461A1 22 33 49.80 00 28 58.30 ASK 23755 4642±2 0.47 -16.75 8.22 -9.39 1.69 2.0 <9.15 <0.93 2467 22 40 17.40 14 29 56.80 2MASX J22401742+1429556 6384±1 0.70 -18.57 9.20 -9.64 1.39 2.6 <9.50 <0.30 2478 22 51 43.15 00 24 54.90 2MASX J22514319+0024547 7807±2 1.60 -20.47 10.83 -12.68 1.64 2.0 <9.93 <-0.90 2482 22 58 53.20 13 21 31.40 KUG 2256+130 7200±3 1.22 -19.54 10.08 -10.10 2.29 3.7 <9.91 <-0.17 2483 22 59 00.20 13 29 51.60 2MASX J22590020+1329513 8609±1 1.24 -19.81 10.21 -10.30 2.30 0.7 <10.09 <-0.12 2487 22 59 36.30 13 22 11.40 2MASX J22593625+1322112 10195±3 1.57 -20.69 10.86 -12.38 2.49 1.1 <10.36 <-0.50 2490 23 01 03.00 -10 04 46.00 PGC 982638 7196±2 0.69 -17.21 6.92 -9.14 2.61 1.5 <9.76 <2.84 2492N 23 01 20.50 -00 55 33.30 ASK 24839 3027±2 0.58 -15.83 7.88 -9.54 2.03 2.3 <8.80 <0.92 2503 23 09 10.90 -08 37 30.70 ASK 137511 7050±3 1.01 -18.26 — — 2.47 2.1 <9.82 <9.82 2505 23 12 22.70 14 30 22.60 2MASX J23122267+1430223 4982±6 1.16 -17.55 9.24 -11.11 1.38 1.2 <9.22 <-0.02 2510 23 14 49.90 -00 14 28.90 CGCG 380-015 7463±3 1.48 -19.80 10.44 -11.99 3.36 1.6 <10.14 <-0.29 2511 23 15 55.90 13 11 46.00 NGC 7563 4297±2 1.52 -20.69 10.83 -12.51 3.05 1.5 <9.70 <-1.13 2512 23 16 03.80 13 47 05.60 ASK 143916 4504±6 0.94 -16.32 8.38 -9.90 1.88 2.0 <9.16 <0.77 2515 23 17 27.20 -10 01 50.60 2MASXJ23172722-1001504 10063±3 1.44 -21.31 10.95 -11.98 4.00 2.3 <10.59 <-0.35 2517 23 18 08.40 -00 23 25.70 CGCG 380-023 8775±3 1.56 -21.56 11.17 -12.42 2.54 1.9 <10.31 <-0.87 2520 23 18 46.40 -10 23 57.30 IC 1479 9495±4 1.61 -21.63 11.26 -12.58 5.86 1.0 <10.75 <-0.51 2525 23 20 28.20 15 04 20.90 2MASX J23202822+1504211 3828±2 1.28 -18.08 9.57 -11.23 1.49 2.5 <9.07 <-0.51 2526 23 20 29.10 -01 00 08.60 CGCG 380-035 9369±3 1.54 -21.20 11.08 -12.63 2.28 2.2 <10.29 <-0.79 2529 23 23 27.00 14 19 33.00 CGCG 431-053 7651±2 1.60 -20.54 10.86 -12.27 1.25 1.7 <9.80 <-1.06 2530 23 24 23.50 15 26 36.30 2MASX J23242356+1526362 7658±3 1.49 -19.70 10.41 -11.86 1.57 2.3 <9.83 <-0.58 2534A1 23 25 30.20 14 06 20.50 ASK 144855 3996±1 0.54 -15.91 7.91 -9.49 1.44 2.0 <8.89 <0.98 2535 23 25 33.60 14 15 15.00 ASK 144275 3783±6 0.88 -15.72 8.39 -10.55 1.70 1.7 <8.92 <0.53 2539 23 30 04.80 -00 33 40.10 PGC 1140348 2452±3 0.68 -14.71 7.77 -10.78 1.54 1.5 <8.41 <0.64 2543 23 33 27.00 14 20 06.80 CGCG 432-002 5735±4 1.30 -20.01 10.37 -10.54 1.83 3.1 <9.66 <-0.70 2558 23 39 08.64 00 27 48.40 CGCG 381-019 5233±2 1.41 -19.48 10.26 -12.07 1.39 2.7 <9.42 <-0.84

Article number, page 66 of 71 van Driel et al.: NIBLES – the Nançay HI survey

Table A.3. – continued.

Source RA Dec Name V g-z M M sSFR rms SNR M MHI opt g ? HI M? (J2000.0) [log] [log] [log] [log] −1 km/s mag mag M yr mJy M 2561 23 40 32.70 -00 33 03.70 2MASXJ23403276-0033029 6928±4 0.74 -19.64 9.57 -10.30 1.66 2.5 <9.73 <0.17 2563 23 40 44.30 -00 53 14.80 ASK 26514 5736±1 0.19 -16.71 7.84 -8.74 1.61 0.6 <9.30 <1.46 2567 23 41 25.90 -00 39 43.90 2MASX J23412592-0039437 10864±2 1.59 -20.07 10.69 -12.64 2.11 2.4 <10.29 <-0.39 2576 23 47 03.78 14 50 30.30 CGCG 432-030 6622±3 1.22 -20.17 10.39 -10.75 2.50 2.0 <9.93 <-0.46 2584 23 52 36.40 14 33 05.20 UGC 12822 7939±2 1.50 -21.37 11.04 -12.03 2.90 1.1 <10.26 <-0.78 2585N 23 52 42.63 -11 00 53.10 ASK 124704 5374±2 0.41 -16.95 8.38 -10.27 0.92 1.5 <9.03 <0.65 2586 23 53 31.00 -00 44 24.50 CGCG 381-058 6925±4 1.69 -19.64 10.57 -11.20 2.30 2.1 <9.91 <-0.67 2588 23 54 10.10 00 22 58.30 NGC 7783 7835±3 1.61 -21.14 11.25 -12.34 2.06 2.2 <10.08 <-1.17 2589 23 55 08.10 00 15 24.60 2MASX J23550807+0015242 6797±5 1.31 -18.49 9.70 -10.89 2.33 1.2 <9.79 <0.09 2591 23 55 51.97 00 33 28.40 UGC 12847 6819±4 1.42 -20.09 10.49 -12.05 1.89 0.8 <9.84 <-0.65 2594 23 56 11.30 -00 01 45.30 2MASX J23561127-0001452 6739±5 1.40 -18.30 9.76 -11.72 1.85 1.1 <9.68 <-0.09 2596 23 56 18.81 -00 18 20.20 IC 1517 7237±3 1.51 -21.16 11.03 -12.38 0.89 1.2 <9.65 <-1.38 2597 23 56 30.70 -00 23 26.80 2MASX J23563069-0023265 7153±3 1.48 -19.30 10.25 -12.17 1.92 2.2 <9.83 <-0.42

Article number, page 67 of 71 A&A proofs: manuscript no. AA201528048_astroph_lores_wrk1

Table A.4. HI surveys flux scale comparison

survey 1 survey 2 mean FHI ratio N

single-feed / single-feed detectors

Arecibo Nançay calibrators 1.13±0.12 12 GBT Nançay calibrators 0.93±0.24 2 Arecibo GBT 0.99±0.18 16

multi-beam / multi-beam detectors

Arecibo ALFALFA α.40 Parkes HIPASS 1.10±0.36 347 Arecibo ALFALFA α.40 Arecibo AGES 1.20±0.06 14

multi-beam / single-feed detectors

Arecibo ALFALFA α.40 Nançay NIBLES 1.45±0.17 82 Arecibo ALFALFA old scale Nançay NIBLES 1.25±0.14 82 Parkes HIPASS Nançay NIBLES 1.34±0.28 51 Arecibo ALFALFA α.40 Arecibo 1.25±0.16 28 Arecibo ALFALFA α.40 GBT 1.14±0.09 8

Notes on surveys: Arecibo: single-feed data from O’Neil (2004) Arecibo AGES: multi-beam data, see Sect. 1 Arecibo ALFALFA α.40: multi-beam data with flux scale from Haynes et al. (2011) Arecibo ALFALFA old scale: multi-beam data from Haynes et al. (2011), corrected to the flux scale used in older ALFALFA catalogs (see Sect. 1) GBT: Green Bank Telescope single-feed data from O’Neil (2004) Nançay NIBLES: single-feed data, from the present paper Parkes HIPASS: multi-beam data from, e.g., Meyer et al. (2004) and Wong et al. (2006)

Article number, page 68 of 71 ? HI M M van Driel et al.: NIBLES – the Nançay HI survey HI

NM / M SNRS HI F 0.250.34 4.60.34 3.20.20 72.5 4.90.17 13.1 146.3 3.3 7.111.15 8.88 3.7 16.9 7.34 0.30 18.3 7.62 0.31 — 3.7 36.7 0.90 6.79 8.73 — — ± ± ± ± ± ± s / 20 W s Jy km / 50 W s km 1 163 187 30.28 9 853 511 104 193 0.65 81 210 1.79 26.25 / HI 13 3811 79 38 0.55 66 0.32 ± ± ± ± ± ± s km / mJy km sS FR rms V 1 ? − M yr g

M r M - g 143 0.382 -13.60 0.88 7.03 0.28 -17.27 -10.16 -13.50 — 3.59 6.72 834 -9.14 — 2.45 2.69 699 719 7 0.27 -12.31 6.8254 0.38 — 1.07 -12.43 3.03 -16.85 — 699 — — 0.00 2.30 8.57 632 652 ± ± ± ± ± ± not used for further analysis opt 1 − V s mag mag / 850 km s km < (J2000.0) DR9 [log] [log] [log] [log] 12 13 48.3012 49 11.40 12 41 25.9013 39 22.34 03 23 15.70 31 14 57.60 IC NGC 3052 4701 ASK 526959 812 755 703 03 06 46.80 00 28 10.30 PGC 1166738 711 15 33 27.90 56 33 34.80 NGC 5963 663 Basic optical and HI data – galaxies with V 1 1 R N N A A 2259 14 59 01.99 44 10 33.40 ASK 402895 639 SOU RA Dec Name 2326 1734 0347 1572 1897 Table A.5.

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Table A.6. Basic optical and HI data – selected galaxies with redshift problems not usable for further analysis

RA Dec Name Vopt Vopt (J2000.0) DR9 other (km/s) (km/s)

DR9 redshift unconstrained:

02 21 14.10 -00 53 12.1 ASK 35835 1245? [DR6: 1309] 02 33 31.90 -00 44 38.0 ASK 36025 1245? [DR6: 1541] 09 47 58.40 39 05 10.1 ASK 284467 1245? [DR6: 1459] 11 22 11.10 04 39 41.6 ASK 170306 1245? [DS6: 1311] 11 29 29.90 03 13 43.3 ASK 73575 1245? [DR6: 1502] 12 12 11.10 12 53 34.9 VCC 0046 1408? [DR6: 1245] 12 20 36.30 12 53 05.1 VCC 0426 1245? [DR6: 1140] 12 27 37.50 14 27 20.1 VCC 1028 1245? [DR6: 1306] 12 30 44.60 13 47 57.9 VCC 1307 1245? [DR6: 1259] 12 45 15.40 07 36 56.4 VCC 2017 1245? [DR6: 1299] 13 51 42.90 05 26 47.4 ASK 178783 1245? [DR6: 1238]

DR9 redshift too uncertain:

08 36 21.90 04 46 24.3 PGC 4086014 1836? [DR6: 664] 12 52 08.90 03 07 14.6 ASK 78238 1084 [DR6: 957] 12 04 59.60 14 24 20.4 PGC 4102270 1101 [DR6: 1219] 10 47 20.10 12 23 14.9 PGC 4094769 1631472 [DR6: 1173] 14 15 46.47 48 54 24.8 ASK 401526 1984 [DR6: 1496] 07 58 01.43 23 48 24.2 PGC 4017004 63175? [DR6: 2251] 07 41 44.49 23 24 57.9 PGC 4009364 50889? [DR6: 2160] 08 05 32.74 20 46 14.2 — 83 [DR6: 1304] 10 46 37.64 09 56 52.5 PGC 1372368 23170 [DR6: 1017] 15 01 15.90 01 46 24.5 PGC 1205406 1342 [DR6: 1507] 01 54 49.50 -08 37 00.0 PGC 1001373 379 [DR6: 3964] 08 17 05.70 15 18 43.2 PGC 4558563 48 [DR6: 2569] 10 37 01.05 21 53 54.2 PGC 4563644 1193 [DR6: 1314]

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Table A.7. HI line flux calibrator galaxies

Name Arecibo GBT NRT FHI FHI FHI (Jy km/s) (Jy km/s) (Jy km/s)

UGC 1246 8.6±0.1 7.1±0.4 UGC 2432 5.9±0.1 5.1±0.3 UGC 2809 9.9±0.1 9.8±0.3 UGC 3755 8.2±0.1 7.8±0.3 UGC 3946 12.0±0.1 10.9±0.7 UGC 4117 4.1±0.1 3.2±0.1 UGC 4660 6.0±0.1 5.4±0.1 UGC 5160 2.9±0.2 2.9±0.3 UGC 5215 6.8±0.5 7.5±0.8 UGC 5218 6.7±0.1 7.7±0.8 UGC 6886 4.6±0.2 4.8±0.5 UGC 7976 6.4±0.1 5.9±0.3 UGC 8091 7.0±0.1 8.8±0.9 UGC 8249 7.5±0.1 9.0±0.9 UGC 8503 3.7±0.1 3.0±0.1 UGC 9007 1.4±0.1 1.5±0.2 UGC 11578 8.7±0.1 9.2±0.9 UGC 11926 5.2±0.1 4.2±0.3 UGC 11992 5.3±0.1 6.2±0.6 UGC 12695 4.2±0.1 3.6±0.2

Notes: Arecibo (at 8.5 km s−1 resolution) and GBT values are from O’Neil (2004)

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