M´asterUniversitario en Astrof´ısica Universidad Complutense de Madrid Trabajo de Fin de M´aster

Search for new bright nearby M dwarfs with Virtual Observatory tools

Alumno: Rub´en Fedriani Lopez´ I

Directores: Enrique Solano II (CAB), Jos´eAntonio Caballero III (CAB)

Tutores: David Montes IV (UCM), Rosario Lorente V (ESAC)

Septiembre 2015

[email protected] [email protected] [email protected] [email protected] [email protected]

Resumen:

Contexto: Existen numerosas estrellas enanas M en el vecindario solar sin identificar. Estos objetos son muy impor- tantes para los siguientes surveys de velocidad radial en la b´usqueda de exoplanetas de baja masa en el infrarrojo cercano. La identificaci´onde estos exoplanetas es m´assencilla en enanas M, en comparaci´oncon otras estrellas, tales como G o K, debido a su favorable contraste en el cociente de radios planeta/estrella. Objetivos: En este Trabajo Fin de M´aster,buscamos estas nuevas estrellas enanas M. Preparamos una lista a partir de una muestra suficientemente testeada de candidatos a estrellas M. Adem´as,estimamos temperaturas efectivas, gravedades superficiales, distancias y tipos espectrales. M´etodos: Cruzando los cat´alogosde CMC15 y 2MASS elaboramos una tabla de objetos. Aplicamos numerosos filtros de movimiento propio, colores y magnitudes con herramientas de Observatorio Virtual con el objetivo de catalogar nuevas estrellas enanas M. Inspeccionamos visualmente cada estrella usando el programa Aladin sky atlas y estimamos par´ametrosastrof´ısicoscon VOSA. Usamos los lenguajes de programaci´onPython y R para estimar distancias y tipos espectrales usando datos fotom´etricosde trabajos previos. Por otro lado, tuvimos la oportunidad de ir al Centro Astron´omicoHispano Alem´an,gracias al M´asteren Astrof´ısica con la asignatura de T´ecnicasExperimentales en Astrof´ısica.All´ı,observamos espectroscopicamente con CAFOS en el telescopio de 2.2m seis de nuestros objetos. Resultados: Hemos elaborado un cat´alogode 1929 estrellas, de las cuales 849 son completamente nuevas y est´an presentes por primera vez en este trabajo, y hemos estimado sus temperaturas efectivas, gravedades superficiales, distancias y tipos espectrales. Casi 100 de nuestras estrellas pueden estar a menos de 25 pc, y otras cinco tienen tipos espectrales M6.0 V o m´astard´ıo. Adem´as,derivamos tipos espectrales de las seis estrellas observadas con CAFOS, que est´anentre M4.5−5.0 V, identificando bandas moleculares t´ıpicasy caracter´ısticasespectrales de enanas M. Los resultados obtenidos en la identificaci´onvisual se corresponden con los resultados estimados en nuestro estudio fotom´etrico,validando nuestro trabajo. Conclusiones: Este nuevo cat´alogode 849 candidatas a estrellas enanas M ayudar´aa estudios relacionados con la b´usquedade exoplanetas, estudios de estrellas fr´ıasen el vecindario solar y para surveys espectrosc´opicosen la identificaci´onde estrellas cercanas. Palabras clave: Herramientas de Observatorio Virtual — estrellas: actividad — estrellas: tipo tard´ıo— estrellas: baja masa — estrellas: enanas — estrellas: par´ametros fundamentales — Galaxia: vecindad — t´ecnicas:espectrocop´ıa

Abstract:

Context: There are several unidentified M-dwarf stars in the Solar neighbourhood. These objects are very important for next radial-velocity surveys of low-mass exoplanets in the near infrared. Their identification is easier than other kind of stars, such us G or K, because of their favourable planet/star contrast ratio radius. Aims: In this MSc thesis, we search for such new M-dwarf stars. We prepare a list from a well tested sample of M-dwarf candidates. In addition, we estimate effective temperatures, surface gravities, distances and spectral types. Methods: By cross-matching CMC15 and 2MASS catalogues, we prepared a list of M-dwarf candidates. We applied several proper-motion, colours and magnitude filters with Virtual Observatory tools in order to catalogue new M- dwarf stars. We visually inspected each target using the Aladin sky atlas and estimated astrophysical parameters with VOSA. We developed both Python and R scripts to estimate distances and spectral types using photometric data. On the other hand, we had the chance to go to the Centro Astron´omicoHispano Alem´an,within the Astrophysics Master degree framework of the subject T´ecnicasExperimentales en Astrof´ısica. There, we observed spectroscopically with CAFOS at the 2.2 m telescope five of our previously unknown objects plus a known object. Results: We computed a catalogue of 1929 stars, of which 849 are presented for the first time in this MSc thesis, and estimated their effective temperatures, surface gravities, distances and spectral types. Almost 100 of our stars could be at least than 25 pc, and another five have spectral types M6.0 V or later. Besides, we derived M4.5−5.0 V spectral types for the six stars observed with CAFOS, after identifying typical molecular bands and spectral features of M dwarfs. These results go in the same direction of our photometric study. Conclusions: This new catalogue of 849 new M-dwarf candidates serves for studies related with exoplanets hunting, for studies of cool dwarfs in the solar neighbourhood and for spectroscopic surveys aiming at the identification of nearby mid-late type M dwarfs. Keywords: Virtual Observatory tools — stars: activity — stars: late-type — stars: low-mass — stars: dwarfs — stars: fundamental parameters — Galaxy: neighbourhood — techniques: spectroscopy Index

1 Introduction 1 1.1 A brief introduction to M dwarfs ...... 1 1.2 Search for M dwarfs using astrometric and photometric catalogues ...... 3 1.3 Why M dwarfs? ...... 5 1.4 Objectives ...... 6

2 Analysis 7 2.1 Visual inspection ...... 9 2.2 Diagrams ...... 10 2.2.1 Colour-colour diagrams ...... 10 2.2.2 Colour-magnitude diagram ...... 11 2.2.3 Colour-reduced proper motion diagram ...... 11 2.2.4 Coordinates ...... 13 2.2.5 Histograms ...... 13 2.3 Spectral type estimation through photometric data ...... 15

2.4 Distance estimation through spectral type and MJ relationship ...... 16 2.5 Effective temperature and surface gravity estimation using VOSA ...... 17

3 Results and discussion 18 3.1 Spectral types and distances ...... 18

3.2 Teff and log g ...... 19 3.3 Top 20 stars ...... 19 3.3.1 Reddest ...... 20 3.3.2 Fastest ...... 21 3.3.3 Nearest ...... 22 3.3.4 Brightest ...... 23 3.4 Completeness and limiting for the CARMENES input catalogue ...... 23 3.5 Spectroscopy ...... 24

4 Conclusions and future research 25

Appendix A: Tables 28

Appendix B: Application for Observing Time 69 1 Introduction

1.1 A brief introduction to M dwarfs

M dwarfs are the most common stars in the Solar neighbourhood, around 66%. Besides, the nearest star to the Sun, Proxima Centauri, is a red dwarf (M5.5 V). Red dwarfs are by far the most common type of star in the Milky Way, but they are not visible to the naked eye because of their low luminosity. The Research Consortium on Nearby Stars( RECONS1) studies the nature of the Sun’s nearest stellar neighbours and according with its, the most common spectral type in the solar neighbourhood is M. The RECONS 25 Parsec Database (Henry et al. 2006) together with the RECONS Movie2 (Adric Riedel and the RECONS Team) allow us to know the statistic concerning the spectral types in the Sun’s 25 pc neighbourhood, which is:

Table 1: Statistics of the Spectral Type of Sun’s 25 pc neighbourhood.

SpT O B A F G K M

Number 0 1 29 141 244 550 1093

Spectral classification is based on morphology where we notice regularities in the appearance and disappearance of particular spectral features. The traditional method of defining a spectral classification system is to take observations of a set of stars, ideally with known absolute magnitude and luminosity class (Reid & Hawley 2005). Identifying spectral features, strong enough to recognise in an easy way, provide us a correct classification. Particularly, M dwarfs are main-sequence stars whose spectra display bands of TiO (L´epine& Gaidos 2011), so the TiO bands which dominate spectra of M stars are a really good feature to be studied as a primary indicator of spectral type. The first Morgan & Keenan (MK) system was limited in M dwarfs classification because initially it was defined for stars with earlier type than M2 due to most photographic observations around 1940s were dominated to the blue region where the spectral features were saturated with low temperatures (intermediate and late type M). With the advent of larger telescopes and modern spectrographs and detectors, it became necessary to extend the classification to later types than M2, i.e., cooler stars. There were problems between different systems, such us Yerkes and Mount Wilson, because to the same stars they were classified as a different type. One of the problem in classifying M dwarfs using spectra located in the blue part of the electromagnetic spectrum is that those wavelengths lie far from the peak of the energy distribution. For this reason Boeshaar (1976) and Kirkpatrick et al. (1991), among others, extended the MK system by adding spectral features to redder wavelengths, designated KHM system which looked for features in the range 6300-9000 A.˚ There were several different systems to classify the luminosity class based on TiO or VO bands but the more widely used is the KHM system. Nowadays the best classification is given in Alonso-Floriano et al. (2015) and in a near future will be adopted a standardization for M. Figure 1 shows optical spectra of late-type K and M dwarfs covering the range 3800-9500 A.˚ In addition, it shows the principal spectral features. TiO is present, but weak, at K7, and grows in strength until type M6, where more bandheads saturate. Bands due to several metal hydrides, such us MgH, FeH and CaH, also become detectable among K7 stars and grow in prominence with later spectral type. Moreover, VO becomes evident at 7330-7530 A˚ and FeH bandheads also appear in the latest spectral types at 7786, 8692 and 9020 A.˚ It is also remarkable the strongest atomic lines, such us, Ca I at 4227 A,˚ the Na I doublets at 5890/5896 A˚ and 8183/8195 A,˚ the K I doublet at 7665/7699 A˚ and finally the Ca II triplet at 8498, 8542 and 8662 A˚ (Reid & Hawley 2005). Considering M dwarfs as main sequence stars with a clear spectral feature in TiO bands absorption, we can make the following summary:

• Their spectra are characterized by molecular absorption bands, mostly of TiO and VO. Besides, there are metal

hydrides, such us MgH, FeH and CaH at optical wavelengths, together with H2O and CO in the red part of the electromagnetic spectrum.

• They have absolute visual magnitudes between MV = 7.5 and MV = 20 mag.

−4 • Their luminosities range from 0.2 L to less than 5 × 10 L .

1http://www.recons.org/ 2https://www.youtube.com/watch?v=up_MqNBv0FE#t=171

1 • Their masses lie between 0.6 M and 0.1 M approximately and their radius lie between 0.6 R and 0.1 R

approximately. In fact, there is a roughly linear relationship between radius and masses, with a 0.4 M (0.1

M ) M dwarf having a radius of 0.4 R (0.15 R ) (L´epine& Gaidos 2011).

• Their effective temperatures lie between ∼ 3800 K (M0) and ∼ 2300 K (M9).

• They often have active chromosphere and coronae.

There are several reference providing different bounds for the previous physic parameters. Anyway all of them are close to each other.

Figure 1: Left panel: blue optical spectra of a late K dwarfs and M dwarfs, highlighting the main features. Right panel: red optical spectra of a late K dwarfs and M dwarfs. Molecular bands and atomic features have been highlighted (from Reid & Hawley 2005).

In short, M dwarfs are cool, low-mass and low-radius stars. They are fully convective later than M4.0 V and mostly convective for spectral types earlier than M4.0 V. Since the peak of the energy distribution is around 0.7-1.4 µm, it is easier study this kind of targets in red range of the electromagnetic spectrum than in the blue-visible one (this is one reason why we have chosen red magnitude to make our study, as explained in depth later). Whether we look for M dwarfs on the Hertzsprung-Russell diagram, they lie on the bottom-right or lowest part of the diagram (whether we put the diagram in the standard way, see Figure 5). Owing to M dwarfs burning their fuel very slowly, no M dwarfs of advanced evolutionary stages exist, because of the relative short age of the Universe. Table 2, from Reid & Hawley (2005), we summarize the fundamental properties of M dwarfs (note that we have used more recent references for our study, but this reference is a fundamental one):

2 Table 2: Fundamental properties of M dwarfs.

Spectral type Temperaturea Radiusb Massc Luminosityd Log gravitye −2 −2 −1 [K] [R/R ][M/M ] [10 L/L ] [g cm s ] M0 3800 0.62 0.60 7.2 4.65 M1 3600 0.49 0.49 3.5 4.75 M2 3400 0.44 0.44 2.3 4.8 M3 3250 0.39 0.36 1.5 4.8 M4 3100 0.36 0.20 0.55 4.9 M5 2800 0.20 0.14 0.22 5.0 M6 2600 0.15 0.10 0.09 5.1 M7 2500 0.12 ∼0.09 0.05 5.2 M8 2400 0.11 ∼0.08 0.03 5.2 M9 2300 0.08 ∼0.075 0.015 5.4

aTemperatures compiled from several photometric and spectroscopic calibrations. bRadius calculated from L = 4πR2σT 4. cMass estimates from 8-parsec sample for each spectral type. d 26 L calculated from Mbol using Mbol = 4.62 mag, L = 3.9 × 10 W. elog g calculated from g = GM/R2.

1.2 Search for M dwarfs using astrometric and photometric catalogues

Since the final of 20th century and the beginning of the 21th century, the way to understand photometric a astrometric surveys has changed. With the advent of new telescopes and CCD cameras with their high and fast development, large-scale photometric surveys have could done. Two Micron All Sky Survey (2MASS), Sloan Digital Sky Survey (SDSS) or Carlsberg Meridian Catalogue (CMC), among others, provide us accurate, homogeneous data for huge fractions of sky. Data from these catalogues provide us the necessary information to identify candidate stars, in our case M dwarfs, by colour index. The point is that 2MASS is not well suited to identify nearby M dwarfs, whether it is working alone, because J − K colour provides highly uncertain distances estimates for spectral types K5 to M7 (Reid & Hawley 2005). But whether we combine optical/infrared colours from 2MASS and SDSS such us R − J would prove extremely effective in selecting nearby M dwarfs. However in the past fully cross-referenced optical/infrared data sets were not available. Nowadays, we can cross-match several catalogues using Virtual Observatory tools. The easy access to catalogues has provided us do deeper and more complete studies. In our particular case, we have used the last series of the Carlsberg Meridian Catalogue, CMC15 (Mui˜nos & Evans 2014) together with the Two Micron All Sky Catalogue- Point Sources Catalogue, 2MASS-PSC (Skrutskie et al. 2006). As we said optical/infrared colours can provide us very good indicator studying M dwarfs, that is why we were studying the r0 − J colour (among others). CMC15 is an astrometric and photometric catalogue in the red magnitude range from 9 to 17 magnitude, r0 magnitude from CMC15 has a band between 0.6 and 0.75 µm. This catalogue is based on the observations of the Carlsberg Meridian Telescope (CMT, a Grubb refractor telescope) with an objective of 178 mm diameter and focal length 2.66 m, which is located in Roque de los Muchachos in La Palma, using a CCD camera (Kodak 2k x 2k with 9 µm pixels) with a Sloan r0 filter operating in a drift scan mode. The observations were made between 1999 and 2011 with the CMT where the sky coverage is −40◦ < δ < +50◦, see Figure 2. 2MASS is another astrometric and photometric catalogue covering 99.998% of the celestial sphere in the J(1.25 µm), H(1.65 µm) and Ks(2.16 µm) near-infrared photometric bands, see Figure 3. Observations were carried out from two dedicated 1.3 m telescopes located at Mount Hopkins, Arizona (North Hemisphere), and Cerro Tololo, Chile (South Hemisphere). Each 2MASS camera contains three NICMOSS3 256 x 256 HgCdTe arrays to work in the three different bands. Besides, the use of a proper motion catalogue is a convenient way to identify nearby M-dwarf stars (nearby stars in general), because proper motions selected samples discriminate against distant background sources including M giants that would otherwise significantly contaminate a sample of cool stars selected by colour alone (L´epine& Gaidos 2011). For this we also have used in our study the PPMXL catalogue of Positions and Proper Motions on the ICRS (Roeser et al. 2010) and because neither CMC15 nor 2MASS-PSC contain no proper motions.

3 Figure 2: Sky coverage of Carlsberg Meridian Catalogue 15 presented in equatorial coordinates. Intensity is propor- tional to source density.

CMC15 and 2MASS-PSC together with PPMXL catalogues have been the core of our study. In addition, we used other catalogues, such us, the ninth Data Release of the Sloan Digital Sky Survey, SDSS/DR9 (Ahn et al. 2012), the fourth US Naval Observatory CCD Astrograph Catalog, UCAC4 (Zacharias et al. 2013) and the All sky Wide-field Infrared Survey Explorer Data Release, AllWISE (Cutri et al. 2013) to complement our study. With SDSS/DR9 and AllWISE we complemented the CMC15 and 2MASS information and with UCAC4 we complemented the PPMXL information. All of them have been part of our study searching for new bright nearby M dwarfs where were managed by VO tools.

Figure 3: Sky coverage of Two Micron All Sky Survey presented in Galactic coordinates. The image is a colour composite of source density in the J (blue), H (green) and Ks (red) bands.

4 1.3 Why M dwarfs?

Figure 4: An artist’s conception of GJ1214b, a watery super-Earth orbiting the red dwarf GJ1214 which spectral type is M4.5 V.

Are we the only Planetary System in the whole Galaxy or Universe? The answer is clear, no. By nature humans are very arrogant thinking we were in the centre of the Universe, or in the centre of the Solar System. Other classic question would be: Are we alone in the Universe? The answer now is not so clear, in my opinion no, but there are no evidences to sustain it. The first step to find live is to find places can hold live. As first approach, by mean every star has at least a exoplanet orbiting it, so whether in our Galaxy there are around 1,000,000,000 stars (some estimations say even 1 trillion stars), it would be around 1,000,000,000 exoplanets just in our galaxy. Let us hunt! In the last years several researches worldwide are looking for exoplanets around stars. In addition, NASA’s Kepler mission in space and different instruments, such us CARMENES, are dedicated observing potential stars with exoplanets. For example, the main goal for CARMENES is looking for low mass exoplanets orbiting mid to late M dwarfs (Quirrenbach et al. 2014, Alonso-Floriano et al. 2015). There is a special interest in those exoplanets orbiting in the habitable zone (HZ), which is the region around the star where a planet can have liquid water on surface. M dwarfs are ideal targets for these missions because of their lower luminosity respect earlier spectral types. This fact allows us easier planets detections, due to the HZ lies closer to the star. There are two principal methods to detect exoplanets, Doppler radial velocity and transit method. M dwarfs are prime targets for exoplanets surveys because of their low mass and bright apparent magnitude. Kepler has identified exoplanets candidates in stars with typical colours of M dwarfs (Dressing & Charbonneau 2013, Kopparapu 2013). M dwarfs could also be used to characterize an exoplanet’s atmosphere because of the contrast between star and planet (Kaltenegger & Traub 2009). Moreover, in the last years there were no all sky catalogues of well characterised M dwarfs. We had to wait to the catalogues of bright, nearby late type K and early type M dwarfs of L´epine & Gaidos (2011), with 8889 stars, and Gaidos et al. (2014), with 2970 stars, to have a good sample on these kind of targets. In this line we want to contribute with our 1929 mid late type M dwarfs sample, which those 849 stars are presented for the first time in this MSc thesis. Finally, being good targets for finding exoplanets, M dwarfs have very high main sequence lifetimes, in fact they have lifetimes longer that the age of the Universe, for this reason M dwarfs can be used as a trace of the stellar evolution in the Milky Way and the evolution of its disk (West et al. 2011).

5 1.4 Objectives

The main scientific goal for this study is the search for new M-dwarfs in order to provide a clean table to the community. Remember that on the Hertzsprung-Russell diagram M dwarfs lie on the bottom-right, where the coolest stars lie. Some of these stars could be study for other groups searching exoplanets. In addition, with the work developed we are writing a paper, which will be published in next months.

Figure 5: Hertzsprung-Russell diagram showing the relative sizes of some stars. M dwarfs lie on the bottom-right part of the Figure. Image credit: From: http://uofgts.com/Astro/allthestars.html, from Astronomy Magazine.

After the brief presentation we star to work with M dwarfs. In section 2 we explain the whole process to obtain our sample and how we have got different estimations. In section 3 we extract all results from our study, plotting several graphics and writing tables with the most important targets of our sample. Finally, in section 4 we highlight the principal results and we mark the future research on this study.

6 2 Analysis

We started our analysis by cross-matching the Carlsberg Meridian Catalogue 15 (CMC15) with 134,653,515 rows and the Two Micron All Sky Survey Catalogue with 470,992,970 rows, using 5.0 arcsec of match radius. We made this 0 cross-match because we are interested in the r magnitude from CMC15 and J, H and Ks magnitudes from 2MASS. The cross-matching result was a table with 134,585,218 rows (that table was zeroth filter). The first filter we applied was J < 11.5 mag, in order to consider bright targets and quite near to the Sun with 6,661,577 rows. We extended the study of Aberasturi et al. (2014) who imposed J < 10.5 mag. Since we only want the best quality photometry of our targets, we applied a second filter considering only the best quality flags of observation, i.e., Qfl = ‘AAA’. In order to keep the reddest objects, we applied a third filter, r0 − J > 3.9 mag, with 1,234,728 rows. Finally, we applied another colour filter to ensure that we are not working with giants stars, 0.8 mag < J − Ks < 1.0 mag. After applying all these filters, we saved a table with 5023 rows. We summarise the filters in the following table:

Table 3: Filters applied to the CMC15 and 2MASS cross-match.

Filter Rows % Size

0th ··· 134,585,218 100 66.1 GB 1st J < 11.5 mag 6,661,577 4.77 4.4 GB 2nd Qfl=‘AAA’ 6,296,310 4.67 4.1 GB 3rd r0 − J > 3.9 mag 1,234,728 0.91 810.2 MB th 4 0.8 mag < J − Ks < 1.0 mag 5023 0.003 3.3 MB

We are interested in those stars with registered proper motion, so we cross-matched the 5023 rows with PPMXL catalogue with 3.0 arcsec of match radius and we obtained 3364 rows. PPMXL and 2MASS epochs of coordinates are the same, and similar to those of CMC15, so we did not expect losing any high-proper motion star outside the relatively small cross-match radius of 3.0 arcsec. As we knew many objects of our sample were in the Galactic plane, we applied an additional density filter. Dense fields at low Galactic latitude have a lower completeness due to faint stars often being lost to nonlinearity in the crowed areas of photographic plates (L´epine & Gaidos 2011). We made 77 visual inspections to obtain the density along the Galactic plane in the neighbourhood of our targets. We visualised with Aladin a region with a radius of 5.0 arcmin centred on an object of our sample and we counted the number of objects in the region (see Table 4). After the inspection, we determined the bounds of the sample in terms of Galactic latitude (l) and longitude (b). We rejected all objects that fell in the areas between 320 and 60 degrees in b and −10 and +10 degrees in l, plus between 60 and 75 degrees in b and -5 and +5 degrees in l. We took all objects between 75 and 320 degrees in b (see Figure 7). The result of this cleaning was a table with 2183 rows.

Table 4: Density of the Galactic plane in term of l and b.

l/b [deg] −15 −10 −5 0 +5 +10 +15

0 275 1088 2391 3451 2055 1326 540 15 523 1014 1579 3306 1546 666 568 30 368 669 1162 2770 877 706 349 45 384 696 1394 2246 1013 317 427 60 323 497 1119 1937 1426 705 283 75 299 397 944 1059 1316 483 196 90 277 247 827 808 808 ······ 150 194 227 367 518 ········· 180 141 254 318 392 285 283 129 240 237 510 614 735 355 349 ··· 345 ······ 1875 2413 1542 748 438

7 We plotted the data from Table 4 to see the density effect near the Galactic Centre. Figure 6 shows the stars number with respect to Galactic longitude and latitude, respectively. There is a high concentration of objects near the Galactic Centre reaching ∼3500 objects in just 5.0 arcmin. Furthermore, near the Galactic plane, i.e. ±10 degrees in l, there are also high density regions. For this reason we rejected these objects because it was difficult resolve sources on it.

Figure 6: Left panel: stars density in terms of Galactic longitude. Right panel: stars density in terms of Galactic latitude.

We show in Figure 7 our sample distributed in Galactic coordinates after the cleaning. The subsets that we have mentioned are shown in different colours, and the clean sample is also shown on the right panel.

Figure 7: Left panel: different rejected subsets in terms of high density. Labels show the region considered. Right panel: clean sample after removing objects included in high density regions. Galactic coordinates are used in both panels. Egg-like voids are areas close to the north and south equatorial poles not covered by CMC15.

All technical details on how we applied filters with TOPCAT and STILTS and the visual inspection with Aladin can be found in M dwarfs and Virtual Observatory. An ESAC traineeship at the Centro de Astrobiolog´ıa(INTA-CSIC) (Fedriani Traineship 2015). Since we are interested in unknown objects, we cross-matched our clean sample of 2138 stars with Simbad with a 5.0 arcsec match radius. We obtained two different tables, one of them with objects found in Simbad and another one with objects not found in Simbad, with 1200 and 1039 rows, respectively. Since these tables have repetitions, we inspected with Aladin one by one all objects of these tables to ensure that our final sample had no repetitions, false sources, fakes by stellar multiplicity, multiple PPMXL sources or bad Simbad correlations. We made a Simbad script loading the following catalogues together with an image of DDS from ESO (Garching/Deutschland- DSS.ESO, POSS

8 II): Simbad, 2MASS-PSC, CMC15, PPMXL, ALLWISE, UCAC4 and SDSS-DR9. Besides, we cross-matched with All-sky catalog of bright M dwarfs (L´epine& Gaidos 2011) and Trumpeting M dwarfs with CONCH-SHELL (Gaidos et al. 2014), because these objects are not in Simbad yet and we focus on unknown objects. After the inspection, we rejected 156 rows because 79 of them had stellar multiplicity, 77 multiple PPMXL sources and 34 were already known objects, we obtained a final sample of 849 objects. In Table A1 from Appendix, the reader find the unknown targets not included in Simbad, with 849 M-dwarf candidates and in Table A2 the known targets included in Simbad and L´epine& Gaidos (2011), with 1080 known stars which several of those are catalogued as M stars.

2.1 Visual inspection

Since we are going to provide to the community a well tested table with candidates to medium-late type M dwarfs, we made a hard visual inspection. Stringent quality control procedures, including visual confirmation of all objects, guarantee no false detection in our table. We analysed row by row our tables using Aladin. With this inspection we have ensured our objects’ information has no mistakes, we have ensured that they have the correct proper motion, the correct r0 and J magnitude and they were resolved sources. Normally the process was simple because the targets were well resolved, however, sometimes we have had to determine how the star moves in order to discern which is the correct proper motion. Sometimes we could not resolved sources clearly because in this region there were several objects near our target, i.e., it is a high density region. Normally in these regions the correlation was incorrect because it takes the brightest magnitude source instead of the correct one. Besides, since there are many objects in these high density regions there are bad correlations with PPMXL. In the practical and technical report you can find a detailed explanation how we made this visual inspection with Aladin.

Figure 8: Left panel: a typical well resolved region. In these regions we can study perfectly our targets. Right panel: a typical high density region is shown. We rejected this object, called CMC15 183014.3-333553, with the flag ‘stellar multiplicity’. It is difficult to resolved catalogues sources concerning proper motions and different magnitudes in these high density regions.

We spent several days making the visual inspection, it was a hard process, but necessary to ensure the quality of our table. We used all catalogues that we have mentioned in Section 1. As we said these catalogues complement each other and as they have different date we could checked the correct identification for our targets. For instance, in Figure 9 we can see clearly how the star move just following the points from different catalogues.

9 Figure 9: Typical good correlation between catalogues. Following different points from different catalogues you can see the proper motion of this target (CMC15 003221.4+292746) with a proper motion of µ = 79.6 mas/a

Since catalogues used in our study have different observation date we can infer the proper motion and checked whether our target is moving in the correct way corresponding with catalogue data.

2.2 Diagrams

After the visual inspection we drew some diagrams concerning both samples unknown objects (849) and known objects (1080). Diagrams below contain both samples where the blue points are the unknown objects and the red points are the known objects.

2.2.1 Colour-colour diagrams

We found in the literature several colour-colour diagrams concerning M dwarfs, we drew these diagrams for our samples and we confirmed that our M-dwarf candidates go in the direction of these studies. Red points represent the known objects catalogued in Simbad or L´epine& Gaidos (2011), these objects are important too because we can compare both samples, they follow the same tendency (Aberasturi et al. 2014). r0 − J colour index is another indicator for Teff, so reddest objects, located on the left region of the left panel, also indicate that they are the coolest objects in our sample. We know that giant stars have different colours from M dwarfs, in the infrared colour-colour diagram we can see clearly where dwarfs have bluer J − H colours than giants, this means that the three blue point on the upper-right corner could be giants stars. As we expected most objects are in central region of the plot (L´epine& Gaidos 2011), proving that most of our objects are dwarfs.

10 0 Figure 10: Left panel: r − J vs J − Ks colour-colour diagram. Blue points represent the unknown objects of our study and they are the most interesting targets for us.. Right panel: H − Ks vs J − H colour-colour diagram for the unknown candidate objects together with the known objects.

2.2.2 Colour-magnitude diagram

A colour-magnitude diagram is a variant of the Hertzsprung-Russell diagram. In this kind of diagram we can infer several information about spectral types and the colour of our targets. Once again r0 − J colour index indicates that the reddest objects are the coolest one. The unknown sample lies on the bottom of the panel due to brighter objects have already been studied; then, the brightest objects in r0 magnitude lie on the top-right. The apparently asymptotic line crossing the panel is due to the magnitude cut in J magnitude, remember that we made the 1st which is J < 11.5 mag; hence r0 = (r0 − J) + J and r0 cannot be larger than (r0 − J) + 11.5 mag.

Figure 11: r0 − J vs r0 colour-magnitude diagram. Our sample (blue points) are in general fainter than the objects already known (red points) in r0 magnitude from CMC15. The most interesting objects lie on the bottom right of the panel due to they are the reddest objects, i. e., mid-late type M dwarfs.

2.2.3 Colour-reduced proper motion diagram

Proper motion is an effective measure of identifying stars in the neighbourhood of the Sun. Since we are searching for new bright nearby M dwarfs, we need targets with proper motions registered (PPMXL cross-matched done). The reduced proper motion diagram provides us a great tool to divide objects of kinematically-distinct stellar populations. 0 We used r apparent magnitude to calculate the reduced proper motion Hr, which is defined by:

11 0 Hr = r + 5 log µ + 5 (2.1) where µ is the proper motion defined by:

p 2 2 µ = (µα cos δ) + (µδ) (2.2)

Figure 12: r0 − J vs Hr reduced proper motion diagram. The distribution in both samples unknown and known objects are similar, however the unknown objects have Hr values lower than known objects, because the speediest targets have already been studied.

In addition, the reduced proper motion Hr is a good indicator to distinguish giants and dwarfs stars, normally background sources, including M giants, have a lower proper motion registered comparatively with nearby M dwarfs. In the unknown sample there are high proper motion objects with no previous studies.

12 2.2.4 Coordinates

It is also interesting study the stellar distribution on the sky. For that reason we plot the panels below, on the left panel we can see the distribution of our objects throughout right ascension (α) and declination (δ) in J2000, on the right panel same as the left panel but using Galactic coordinates. It is clear that we rejected stars near both Galactic Centre and Galactic plane. We used TOPCAT to transform the equatorial coordinates to galactic coordinates.

Figure 13: Left panel: distribution of all objects which pass the colour filters and the visual inspection in equatorial coordinates, right ascension (α) and declination (δ) in J2000. Right panel: same as left panel given in Galactic longitude and latitude using the standard IAU 1958 Galactic Longitude.

In Figure 13 objects have distributed uniformly along the sky, however, our unknown objects sample lie near the galactic plane (remember we cleaned the galactic plane neighbourhood to avoid high density regions) and stellar cluster, such us Hyades (α = 4h27m, δ = 15◦520). There is no problem because we made the visual inspection and we ensured that there are resolved sources. Since our catalogue is formed from CMC15 (among others) we could observed our sample (specially the unknown objects) mostly from north hemisphere, ensuring the whole covering from Roque de los Muchachos in La Palma (Spain).

2.2.5 Histograms

We present four diagrams with some typical values which were studied. We see on the r0 histogram that the unknown sample is fainter than the known sample where the mean is around r0 ∼ 15.2 mag, and its distribution is close to a Gaussian, being its minimum at ∼ 13.3 mag; in spite of the other distribution also peaks around ∼ 15.2 mag , it reaches brighter magnitudes, around r0 ∼ 10.0 mag. Nonetheless, the faintest magnitude are close in both distributions, 17.2 mag approximately. In the J histogram we have another situation. They are still in the same direction but, unknown objects are clearly fainter than known objects, there are more objects with faint magnitude than brighter. On the one hand the mean of the blue distribution is 11.1 mag with minimum of 9.0 and maximum of 11.5 mag. On the other hand the mean of the red distribution is 10.6 mag with its minimum and maximum of 5.6 and 11.5 mag, respectively. In the case of the µ histogram the difference between samples is clear, all high proper motion objects have already been studied as expected, new M-dwarf candidates have slower proper motions, but they are still interesting for us. In the last panel, r0 − J histogram, we can see really close distributions, which means we are considering new objects in our study that have consistent properties with previous works. In Table 5 is summarised the statistic of these variables:

13 Table 5: Statistics for unknown objects.

Variable mean sd min max

r0 [mag] 15.252 0.483 13.062 17.203 J [mag] 11.086 0.372 9.023 11.498 µ [mas/a] 93.0 91.1 0.6 838.0 r0 − J [mag] 4.166 0.278 3.901 5.874

Figure 14: Top left panel: r0 histogram showing the distribution of our sample. Top right panel: J histogram proving that the unknown objects are fainter than the known ones. Bottom left panel: µ histogram, in general we are considering slower objects. Bottom right panel: r0 − J histogram, displaying a similar distribution between both samples.

In conclusion, in this section we show that we are studying the objects never studied for other groups, faint objects, not high proper motion, sometimes in high density region, such us near to Galactic plane or stellar cluster. Nevertheless both samples are in the same direction.

14 2.3 Spectral type estimation through photometric data

Deep wide multi-band photometric compilations of different catalogues are an useful tool for the estimation and assignment of spectral types. Owing to M dwarfs are better understanding in the red region of the electromagnetic 0 spectrum, we have r magnitude from CMC15, J and Ks magnitudes from 2MASS which are red magnitudes, with 0 0 that we calculated the colour index r − J and r − Ks which are representative colour index for M dwarfs. There are several previous works which found a relationship between a colour index and expected spectral types (L´epine& Gaidos 2011, West et al. 2011, Holgado 2014, Aberasturi et al. 2014), or temperatures (Kaltenegger & Traub 2009). We decided use photometric data to estimate spectral type because the estimation through temperature introduce high uncertainty. With both colour index we can estimate the spectral type just using photometric data, we use estimation from Holgado (2014), which is being used by the CARMENES3 consortium4. We expected intermediate-late type M dwarfs (≥ M4.0 V) because of the colour filters applied, so using data from Table 10 of Holgado (2014) (Tabla 10: Valores medios de los ´ındices de color) we estimated spectral types from colour index r0 −J where we found a quadratic relation between those, hence in order to be more accurate we made a weighted quadratic fit with the available data.

Table 6: Colour index vs Spectral Type.

0 0 SpT r − J r − Ks [mag] [mag]

M0.0 V 2.49±0.25 3.32± 0.26 M0.5 V 2.48±0.09 3.32± 0.11 M1.0 V 2.63±0.12 3.47± 0.13 M1.5 V 2.79±0.11 3.62± 0.12 M2.0 V 2.93±0.09 3.77± 0.10 M2.5 V 3.05±0.14 3.90± 0.13 M3.0 V 3.25±0.10 4.10± 0.11 M3.5 V 3.49±0.12 4.33± 0.12 M4.0 V 3.71±0.13 4.56± 0.16 M4.5 V 4.04±0.18 4.90± 0.20 M5.0 V 4.47±0.21 5.38± 0.24 M5.5 V 4.90±0.28 5.82± 0.27

We can see the result of this fit in Figure 15 which was made in R. This fit define the bounds to determine, given a colour index, which spectral type correspond.

Figure 15: Weighted quadratic fit made in R. Black solid points represent points given in Table 6 and vertical lines represent the error. Red line is the quadratic fit and red solid squares represent the colour index considered for each spectral type defining ours boundaries.

3Calar Alto high-Resolution search for M dwarfs with Exoearths with Near-infrared and optical Echelle´ Spectrographs. 4https://carmenes.caha.es/

15 Note that whether a star has a colour index r0 −J greater than 4.90 we derived their spectral type thanks to the fit, we extended the definition and we can reach the spectral type M6.0 V. There is an intrinsic error of ±0.5 concerning the spectral type, that is the minimum uncertainty in spectral type. There are 20 stars with a colour index r0 − J greater than 4.98. These targets are very interesting because are the reddest one in our sample. We will explain in depth in Section 3. In Fedriani Traineship (2015) you can find a discussion about which is the best colour index estimation between West et al. (2011) and Holgado (2014) and why we finally took the Holgado estimation. Besides, you can find the code developed in Python and R concerning these tasks. In this way we redefine the boundaries to estimate spectral types given r0 − J colour index, see Table 7.

Table 7: Colour index vs Spectral Type new boundaries.

r0 − J [mag] SpT r0 − J [mag] SpT

[2.51, 2.54) M0.0 V [3.50, 3.78) M3.5 V [2.54, 2.61) M0.5 V [3.78, 4.11) M4.0 V [2.61, 2.71) M1.0 V [4.11, 4.47) M4.5 V [2.71, 2.86) M1.5 V [4.47, 4.86) M5.0 V [2.86, 3.03) M2.0 V [4.86, 5.29) M5.5 V [3.03, 3.25) M2.5 V [5.29, ∼ 5.7) M6.0 V [3.25, 3.50) M3. V & 5.7 > M6.0 V

2.4 Distance estimation through spectral type and MJ relationship After obtaining spectral types through photometric data in the previous section, now we can obtain absolute magnitude

MJ . There are different relationships between spectral type and absolute magnitude (Hawley et al. 2002, Pecaut et al. 2012, Pecaut & Mamajek 2013). We adopted one of the last relationships because the M standards have changed significantly since the 1950s-1970s, and the 1990s used by Kirkpatrick, Henry, and collaborators. Older compilations of colours in relation with other astrophysics parameters from 1980s and early 1990s are likely to be out of date, so this fact helps us to use recent compilation with modern M standards.

We used a relationship between spectral type and absolute magnitude MJ given in “A Modern Mean Stellar Color and Effective Temperature Sequence for O9V-Y0V” by Eric Mamajek5 (University of Rochester). Part of this table is into Pecaut et al. (2012) and Pecaut & Mamajek (2013), but not all, we only used the relation mentioned, see Table 8.

Table 8: Spectral Type vs MJ .

SpT M0.0 V M1.0 V M2.0 V M3.0 V M4.0 V M5.0 V M6.0 V

MJ [mag] 6.14 6.54 6.89 7.40 8.39 9.25 10.28

Using the relation given in Table 8 we made a quadratic fit in order to infer the MJ value of each subspectral type. We created a R script for this task, we made the quadratic fit and then we obtained the points in our curve to define our boundaries to assign absolute magnitudes, see Figure 16 and Table 9.

5You can find the whole table in: http://www.pas.rochester.edu/~emamajek/EEM_dwarf_UBVIJHK_colors_Teff.txt

16 Figure 16: Quadratic fit made in R. Black filled points represent points given in Table 8. Blue line is the quadratic fit and blue solid squares represent the MJ value considered for each spectral type defining ours boundaries.

Table 9: Spectral Type vs MJ .

SpT M0.0 V M0.5 V M1.0 V M1.5 V M2.0 V M2.5 V M3.0 V M3.5 V M4.0 V M4.5 V M5.0 V M5.5 V M6.0 V

MJ [mag] 6.17 6.29 6.46 6.67 6.91 7.20 7.52 7.88 8.29 8.74 9.22 9.74 10.31

0 So given a spectral type we can infer its MJ , that is, given a r − J colour index we can infer a spectral type and hence a MJ . As before, we define new values obtained in the fit, see Table 9. Once we have estimated absolute magnitudes MJ for each object in our sample we can obtain distances. For this, we used the well-known formula:

m − M = 5 log d − 5 (2.3) being m = J and M = MJ . Since we are working with stars in the Solar neighbourhood (. 45 pc), we considered a null extinction, AJ ≈ 0 mag in our distances estimations. In Section 3 we present the distances distribution which is consistent with our study.

2.5 Effective temperature and surface gravity estimation using VOSA

Astrophysical parameters, such us temperatures and surface gravities, are fundamental to understand the properties of a star. The Virtual Observatory tool VOSA (Virtual Observatory SED Analyzer6) developed by the Spanish Virtual Observatory (SVO), which has been described in Fedriani Traineship (2015), allow us to estimate these parameters. We have to upload a plain text with the names and coordinates of the objects, after that VOSA collects all VO photometry available for our objects. With this photometry VOSA creates synthetic SED’s, besides using chi-squared and Bayesian fits VOSA can estimate effective temperature and surface gravity for each object. To do that, VOSA compares for each object its SED with those derived from theoretical spectra obtained from VO services. There are several models available7 to make the fit, but we used the BT-Settl-CIFIST theoretical model which is integrate in the last version of VOSA. We can choose the parameter ranges for temperatures (Teff), surface gravities (log g) and metallicity (meta) for both fit chi-squared and Bayesian. We made the fit with the following values: Teff ∈ [2000, 4000] K, log g ∈ [3.5, 5.5] and meta=0, being typical values for M dwarfs (notice that we have put conservatives bounds, in order to work with all parameters space). The difference between chi-squared and Bayesian model is that the Bayesian model also gives a probability of this particular parameters (Teff and log g). We expect temperatures around ∼ 3100 K, with a maximum value ∼ 3200 K and a minimum value ∼ 2500 K. Regarding the surface gravities, we expect surface gravities around log g ∼ 5.0, with a maximum value log g ∼ 4.8 and minimum value log g ∼ 5.2. In Section 3 we show the histograms of these parameters.

6http://svo2.cab.inta-csic.es/theory/vosa50/index.php 7We collect the available models in Appendix of Fedriani Traineship (2015).

17 3 Results and discussion

We present a catalogue of 1929 stars. Of them 1080 stars are already catalogued in Simbad or L´epine& Gaidos (2011) (see Table A2), and 849 stars are completely new (see Table A1), they are presented for the first time in this MSc thesis. As explained in detail below, we derived spectral types and distances through photometric data and we estimated Teff and log g using VOSA. Besides, we observed spectroscopically six stars of our catalogue confirming our study. In the following subsections we present the results concerning only the unknown sample.

3.1 Spectral types and distances

In Figure 17 we present the spectral type histogram for our 849 M-dwarf candidates. We have obtained the expected results, i.e., mid-late type M stars (≥ M4.0 V). According to our estimates we got 475 stars with M4.0 V spectral type, 270 with M4.5 V, 73 with M5.0 V, 26 with M5.5 V, 4 with M6.0 V and one later than M6.0 V. We expected this distribution of spectral types where earlier types dominated over later types, it is normal because late type M dwarfs are fainter than earlier types and it is more difficult to find. We obtained 104 stars with a spectral type M5.0−6.0 V which are very interesting targets.

Figure 17: Spectral type histogram.

The results obtained in the distance estimation verify our initial constrain, we wanted to study the solar neigh- bourhood, that is, d ∼ 30 pc. In Figure 18 we present the distances histogram where the mean of the distribution is d¯= 32.6 pc. The minimum value of the sample is 9.5 pc and the maximum is 43.7 pc. The results obtained have been the expected values, being these near stars very important for other groups aiming the catalogue of the nearest stars in the Solar neighbourhood.

Figure 18: Distances histogram.

18 3.2 Teff and log g

Using the VO tool VOSA we obtained Teff and log g through the VO photometry collected for each object. In Figure

19 we present Teff and log g histograms. On the one hand, the temperatures distribution explain mainly our unknown sample, but there are some outlier values on the tails because we do not expect objects with high temperature (> 3200 K) and with very low temperature (< 2500 K). Due to we have spectral types between M4.0−6.0 V we expect temperatures between 3100−4200 K that they are the most common in our histogram, besides the mode is ∼ 3100 K which corresponds with the mode in the spectral type M4.0 V (if we take the median, which is a robustness measure of position avoiding outlier values, we obtain 3100 K as well, and M4.0 V), showing that mainly the histogram is correct. On the other hand, the surface gravities distribution is a bit far from our expected values because we expected log g between 4.9−5.1 and we obtained values between 3.5−5.5 (see right panel of Figure 19). The reason of this difference could be the grid size of the theoretical model, because it is a step of 0.5 in log g, which very high considering that we want a precision of 0.1. Actually it is not a problem in the tool just in the grid of the theoretical model BT- Settl-CIFIST. Notice that the most common bins are 4.5 and 5.0 in log g, which correspond with our spectral type estimation (see Table 2), hence when we have a smaller grid size in the theoretical model we could be more accurate and obtain better results in log g.

Figure 19: Left panel: effective temperatures histogram. Right panel: surface gravities histogram.

3.3 Top 20 stars

In this section we present the most interesting objects that we found in our unknown sample attending different properties, such us colour index, proper motion, distance and magnitude. To make these tables we have considered objects with a proper motion greater than 30 mas/a (µ > 30 mas/a) to ensure that they are potential M-dwarf candidates, because with a low proper motion the objects could be background or giant stars. This filter was also applied for other authors cataloguing M dwarfs (L´epine& Gaidos 2011, Gaidos et al. 2014) considering µ > 40 mas/a, however, they used the USNO-B1 catalogue which is less accurate than the PPMXL catalogue. With a cut in µ of 30 mas/a we are considering 6σ in velocities dispersion in PPMXL catalogue, hence we are considering equivalent proper motion cut as previous authors. With this filter, we keep 676 stars (80% of the final unknown sample), being the remainder also interesting objects, because we can do other type of research with it (see Section 4). From this point each table presented has the first column with a number (No.) which is the identifier of the star to refer them and find easily in the complete table (Table A1), where the reader can find more additional information about the stars presented in the following tables.

19 3.3.1 Reddest

In Table 10 we present the top 20 reddest objects considering the colour index r0 − J. These objects are at the same time, obviously, the latest type of our sample to M-dwarf candidates. Notice that object No. 46, 336, 597, 230, 357 appear in Table 12, where we tabulate the nearest objects. It makes sense because if we identify this late-type object they should be near to us because they are very difficult to find far away due to they are much fainter. The object No. 46 is the reddest object in our sample with a colour index of r0 − J = 5.874 mag and it is at the same time the latest type in our sample. We think that it could be later than M6.0 V because when we made the spectral type estimation, the colour index r0 − J was greater than the maximum value for our quadratic fit which correspond with M6.0 V. For this reason we think that, perhaps, the star could be M6.5 V which would became a really interesting object because there are several groups worldwide searching for such late-type M dwarfs. These reddest objects are perfect to observed and find more information about them.

Table 10: Top 20 reddest.

0 0 No. CMC15 r JKs SpT r − J [mag] [mag] [mag] [mag]

46 022957.4−360639 17.203 11.329 10.340 >M6.0 V 5.874 336 111548.1+274616 16.735 11.284 10.324 M6.0 V 5.451 597 164049.9−261653 16.694 11.282 10.386 M6.0 V 5.412 230 062920.1+172516 16.551 11.162 10.302 M6.0 V 5.389 357 122150.1+463244 16.584 11.259 10.286 M6.0 V 5.325 492 154910.6−352307 16.670 11.383 10.414 M5.5 V 5.287 474 153348.6−291126 16.344 11.105 10.272 M5.5 V 5.239 576 162632.7−262259 16.685 11.452 10.490 M5.5 V 5.233 103 041950.2+292647 16.596 11.369 10.473 M5.5 V 5.227 644 174919.2+475605 16.438 11.214 10.285 M5.5 V 5.224 658 183801.5+341806 16.561 11.419 10.526 M5.5 V 5.142 676 190543.4−271125 16.291 11.152 10.259 M5.5 V 5.139 44 021922.1−392522 16.466 11.381 10.404 M5.5 V 5.085 449 152012.7−355925 16.523 11.472 10.639 M5.5 V 5.051 548 161703.3−214102 15.967 10.971 10.047 M5.5 V 4.996 438 150950.9+150250 16.435 11.450 10.525 M5.5 V 4.985 715 201822.7+000507 16.370 11.387 10.447 M5.5 V 4.983 835 232416.9−152223 16.144 11.190 10.196 M5.5 V 4.954 105 042044.6+180558 16.129 11.194 10.313 M5.5 V 4.935 464 153013.7−140144 16.178 11.243 10.396 M5.5 V 4.935

20 3.3.2 Fastest

In Table 11 we tabulate the fastest objects in our sample. These objects with high proper motion have high probabilities of being M dwarf, because there are no giant stars with these high proper motions. The fastest objects lie on the bottom of the Hr diagram (see Figure 12), because of the definition of the reduced proper motion. Take into account that we have to consider the proper motion with the r0 magnitude, so a higher reduced proper motion does not imply a higher proper motion. All of these objects have a proper motion µ > 380 mas/a, and there are more than 300 objects with a proper motion greater than 100 mas/a, being ideal targets to be considered. Notice that object No. 662, which is the fastest one, is also one of the nearest one (see Table 11), being a good target to observe in next campaigns. Besides, object No. 669 is one of the targets that we observed spectroscopically at CAHA (see Table 15 and Figure 21). Finally, object No. 644 is also one of the brightest stars (see Table 13), being another good target to observe.

Table 11: Top 20 fastest.

No. CMC15 µα cos δ µδ Hr µ [mas/a] [mas/a] [mas/a] [mas/a]

662 184249.7−321247 −673.3 −498.6 18.1 837.8 598 164109.9−225444 +207.6 −793.2 19.8 819.9 426 144713.8−321739 +596.3 −478.5 20.1 764.5 235 063051.5−065809 +350.6 +406.2 18.6 536.6 669 185955.9+432359 +351.4 +396.6 18.4 529.9 470 153140.8+021042 +14.6 −529.2 19.3 529.4 198 053506.4−170633 +480.3 −92.2 17.7 489.1 89 035342.3−252700 −326.3 −348.3 18.0 477.3 20 011113.4+030640 −385.7 −280.0 18.1 476.6 313 101107.6−053328 −352.2 −261.8 18.4 438.8 368 124358.7−161434 −429.2 +82.3 17.3 437.0 207 055128.1−153034 −233.9 +352.8 18.5 423.3 465 153021.8−135846 −163.0 −385.8 18.5 418.8 644 174919.2+475605 −408.7 +86.5 19.5 417.8 308 100009.7+064703 −356.9 +212.7 18.0 415.5 208 055204.0+355027 −19.1 +414.1 18.3 414.5 205 054801.0−250104 −102.8 +384.2 18.4 397.7 267 075313.5−101219 +146.3 −360.5 18.8 389.1 295 090913.2−021611 +90.6 +375.1 18.1 385.9 101 041806.4−240626 −115.3 −368.1 18.3 385.7

21 3.3.3 Nearest

In Table 12 we tabulate the nearest objects according with our estimations. These 20 objects are in our solar neighbourhood at a distance less than 20 pc. One of the most interesting results in our work is these nearest objects because we can contribute with the census of the nearest stars in the solar neighbourhood. In this table we only list the 20 nearest, but there are almost 100 object with a distance d < 25 pc. According to previous research around ∼ 66% of the stars in the Solar neighbourhood are M stars (the 100 nearest stars meet this percentage8). The RECONS group (Henry et al. 2006) is carrying out the census of the nearest stars considering distances less than 25 pc (see Table 1), taking this information we can infer the currently percentage of M, it is just 1093/2058≈0.53. Extrapolating the information of the 100 nearest stars, how many M stars do we need to complete this percentage? With this simple relation we obtain it:

1093 + x = 0.66 (3.1) 2058 + x where x is the M stars needed. Solving for x we can write:

0.66 · 2058 − 1093 x = ≈ 780 stars (3.2) 0.34 We found in our sample 97 M-dwarf candidates with d < 25 pc, which meet with the requirements of the RECONS group searching the nearest stars. When our paper is accepted and our work confirmed, we can provide the ∼12% of these nearest stars unknown. In next years Gaia will resolve this task confirming the distances and parallaxes for several stars. As we said in the previous subsection, objects No. 230, 357, 597, 336 and 46 are also in Table 10 being the reddest objects as well.

Table 12: Top 20 nearest.

No. CMC15 SpT d [pc]

573 162416.4−321213 M4.5 V 12.1 230 062920.1+172516 M6.0 V 14.8 357 122150.1+463244 M6.0 V 15.5 597 164049.9−261653 M6.0 V 15.6 336 111548.1+274616 M6.0 V 15.7 46 022957.4−360639 M6.0 V 16.0 368 124358.7−161434 M4.5 V 16.1 547 161658.8−313638 M4.0 V 16.1 282 084040.8−383238 M4.5 V 16.2 397 135821.6−004626 M5.5 V 16.3 332 105850.4−234620 M5.0 V 16.4 527 160905.2−080946 M5.0 V 16.8 548 161703.3−214102 M5.5 V 17.6 662 184249.7−321247 M4.0 V 17.8 441 151355.4−394114 M5.0 V 17.9 722 202527.1−194803 M4.5 V 18.2 474 153348.6−291126 M5.5 V 18.7 781 211757.1+460130 M4.0 V 18.9 220 061114.6−003537 M5.0 V 19.1

8http://www.recons.org/TOP100.posted.htm

22 3.3.4 Brightest

In Table 13 we tabulate the brightest objects, in r0 magnitude, for our sample. They are mainly early types (M4.0 V) because the colour index r0 − J could not be so high. Notice that object No. 662 is the fastest object in our sample and one of the brightest objects as well. These stars are the easiest one to observe. We encourage the observation of these targets in future campaigns.

Table 13: Top 20 brightest.

0 No. CMC15 r JKs [mag] [mag] [mag]

573 162416.4−321213 13.321 9.150 8.154 547 161658.8−313638 13.394 9.329 8.475 662 184249.7−321247 13.451 9.544 8.679 673 190259.2−202239 13.687 9.738 8.889 781 211757.1+460130 13.698 9.673 8.807 377 131640.5−085825 13.954 10.043 9.199 51 024816.8+053705 14.026 10.072 9.162 232 063001.8−192336 14.052 10.092 9.254 282 084040.8−383238 14.087 9.790 8.868 91 035624.6−311138 14.090 10.072 9.121 368 124358.7−161434 14.113 9.777 8.896 174 051429.4+091807 14.130 10.103 9.241 845 234208.6+010918 14.192 10.194 9.313 92 040044.9+135422 14.209 10.260 9.344 198 053506.4−170633 14.209 10.178 9.295 475 153444.6−280026 14.260 10.332 9.422 284 084615.3+040638 14.268 10.244 9.320 722 202527.1−194803 14.284 10.042 9.149 646 180113.4+094837 14.286 10.294 9.369 300 092311.4−352313 14.306 10.404 9.584

3.4 Completeness and limiting for the CARMENES input catalogue

There is a star subsample in our unknown star sample very interesting for currently surveys. In Table 1 of Alonso- Floriano et al. (2015) they define a strict requirement in order to keep with the most favourable targets to observe. They were selected according to mid-late spectral type and brightness. In Table 14 we write the table of the paper, with the requirements of the CARMENES input catalogue, alongside with the stars in our sample that meet with these requirements. The point to meet this requirement in J-band magnitudes per spectral type is the following: if we have a star with a specific spectral type, for instance M4.0−4.5 V, the J magnitude has to be less or equal than the values written in the columns of completeness and limiting, being the limiting value the maximum allowed value considered for the CARMENES input catalogue. In our sample there are 65 stars meeting the limiting requirement, where 48 are M4.0−4.5 V, 12 M5.0−6.0 V and 5 of them M6.0−6.5 V, and one of them also meeting with the completeness requirement. These objects could be part of the CARMENES input catalogue searching for exoplanets around M dwarfs, but they also have to meet other coordinate requirement, i.e., stars must be observable from Calar Alto with target declination δ > −23 deg. The object which meets the completeness requirement is CMC15 162416.4-321213

(No. 573) which is a M4.0 V star with high proper motion (µ573 = 169.5 mas/a). However, this object does not meet with the coordinate requirement (δ573 = −32.20364 deg), hence it could not be part of the input catalogue. If we take only the objects which pass the limiting requirement with δ > −23 deg, we keep with 40 stars (29 M4.0−4.5 V, 8 M5.0−5.5 V and 3 M6.5−6.5 V), being these 40 stars really interesting targets for the CARMENES input catalogue, in fact the CARMENES panel are planning to include these stars in the catalogue. Nonetheless, the star which meets completeness requirement and the 25 reminder in the case of limiting could be interesting for other surveys, such us

23 HARPS9 which is a survey from the European Southern Observatory (ESO) hunting exoplanets.

Table 14: Stars that pass the CARMENES input catalogue selection criteria.

Spectral type J [mag] Our sample Completeness Limiting Completeness Limiting M0.0-0.5 V 7.3 8.5 0 0 M1.0-1.5 V 7.8 9.0 0 0 M2.0-2.5 V 8.3 9.5 0 0 M3.0-3.5 V 8.8 10.0 0 0 M4.0-4.5 V 9.3 10.5 0 48 M5.0-5.5 V 9.8 11.0 1 12 M6.0-6.5 V 10.3 11.5 0 5 M7.0-7.5 V 10.8 11.5 0 0 M8.0-9.5 V 11.3 11.5 0 0

3.5 Spectroscopy

On 8th and 9th April 2015, we used the Calar Alto Faint Object Spectrograph at the 2.2 m telescope, CAFOS 2.2, in the Centro Astron´omicoHispano-Alem´an(CAHA), Calar Alto (Almer´ıa). CAFOS is a focal reducer which provides the facilities for do direct imaging and spectroscopy with grisms and longslit, moreover we can do polarimetry and imaging through a Fabry-P´erotetalon, with at spectral resolution R ≈ 82000. We used the configuration with both grisms G100 and R100. G100 has a coverage wavelength from 4900 and 7800 A˚ and R100 from 5900 and 9000 A˚ which allow us to determine the spectral type of our targets. We knew that we had a unique opportunity to validate our study, so we proposed to the responsible of the subject T´ecnicas experimentales en Astrof´ısica, Jaime Zamorano, observing our own targets that we had been studied during our traineeship at CAB-ESAC. We made a real application for observing time to CAHA10.Finally, we collected low resolution spectra of 6 M-dwarf candidates, which are shown in Table 15 where we indicate some properties of our targets, besides we put the estimated spectral type made with our photometric study. Exposure times ranged between 350 and 2400 s, depending of the target brightness. Raw data were reduced with standard procedures within the IRAF environment, bias and flat-field correction, cosmic-ray rejection, spectra extraction, wavelength calibration using Cu- Ne-Ar arc lamps taken during the observation, spectra calibration. Every M-dwarf candidates are unknown objects, less the star No. 693 which is already studied by L´epine& Gaidos (2011) (see Table A2).

Table 15: Observed stars with CAFOS.

0 0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ Hr r r − J SpT SpT [deg] [deg] [mas/a] [mas/a] [mas/a] [mag] [mag] (photometric) (spectrum) 273 081202.5+070932 123.010691 7.159164 +77.5 +74.4 14.7 14.546 4.009 m4 ±0.5 M4.5 V 693 141707.3+085136 214.280502 8.860157 −139.4 +17.9 14.0 13.229 4.120 m5±0.5 M4.5 V 467 153116.7+344126 232.81972 34.690684 −101.3 +39.8 14.8 14.640 3.908 m4±0.5 M5.0 V 643 174814.3+133747 267.059614 13.629873 −63.5 −85.3 14.9 14.779 4.445 m4.5±0.5 M5.0 V 669 185955.9+432359 284.982935 43.399788 +351.4 +396.6 18.4 14.749 4.022 m4±0.5 M4.5 V 691 193620.0+354736 294.083602 35.793454 +156.5 +89.5 15.8 14.488 4.061 m4±0.5 M4.5 V

The result of the observation and data reduction was the following spectra of our M-dwarf candidates, see Figure 20 and 21. 9HARPS - High Accuracy Radial velocity Planet Searcher http://www.eso.org/sci/facilities/lasilla/instruments/harps.html 10Find the whole application in Appendix B.

24 Figure 20: CAFOS/CAHA spectra our M-dwarf candidates with G100 grism.

Figure 21: CAFOS/CAHA spectra of our M-dwarf candidates with R100 grism.

On spectra above we identified spectral features, such us molecular bands (TiO, CaH, H2O band, O2 A-band, VO), lines and doublets (Hα,Hβ, KI, NaI). We obtained spectral types through the comparison with spectra collected in Alonso-Floriano et al. (2015). In Table 15 we wrote both spectral types through photometric estimation and visual comparison identifying typical features, as we see there are to close, validating our work. Considering the errors, using photometric data to estimate spectral type or doing spectroscopy are almost the same, for sure the most accurate procedure is to take the spectra and determine their spectral type, but we can reach a really good approximation using our study in order to manage big number of stars.

4 Conclusions and future research

Taking advantages of VO tools, we present a catalogue with 1927 stars, which 1080 are already known stars and 849 are unknown M-dwarf candidates. We cross-matched the photometric CMC15 (r0) and 2MASS (J) catalogues applying several filters to constrain our sample using VO tools. We also showed the potential and importance of the Virtual Observatory, working with VO tools and data archive, for finding new nearby bright mid-late type M dwarfs. Perhaps, some stars catalogued by us can host exoplanets and who knows if their exoplanets can have liquid water hosting life in them, we will know in a near future. We estimated distances and spectral types for the unknown sample through photometric relationships, obtaining expected results. In addition, we derived effective temperatures and surface gravities for each star using VOSA. Our work could increase the census of the nearest objects providing 97 stars with distances less than 25 pc. In a few months, when we have information from Gaia, we will be able to confirm our study. Our catalogue includes many stars which are identified here for the first time as members of the solar neighbourhood. In particular, most of the sources are not listed in the Catalog of the Nearby Stars. Besides, we contribute with 40 stars to the CARMENES

25 input catalogue in order to search exoplanets orbiting these M-dwarf stars, which are low-mass stars being easier to detect extra-solar planets in habitable zones with relatively low masses. We used the Calar Alto Faint Object Spectrograph at the 2.2 m telescope, CAFOS 2.2, in the Centro Astron´omico Hispano-Alem´an(CAHA), Calar Alto (Almer´ıa)for obtaining low-resolution optical spectroscopy of 6 targets, 5 of them had not been spectroscopically analysed before. We did not obtain spectra of the rest of the sample, but we encourage community involvement to complete the spectroscopy survey or Radial Velocity (RV) monitoring programs. The next generation of extremely large ground based telescopes and space telescopes, such us the James Webb Space Telescope, will have an important role observing such stars hosting exoplanets. Future research: We have to validate the objects with a proper motion greater than 40 mas/a, on the other hand objects with less than 40 mas/a are very interesting because with the colour filter applied could be interesting giants objects in the middle of star supercluster, we have to study the spatial distribution in the Hyades cluster. Besides, we found several objects with X-ray emission so we can correlate with the ROSAT catalogue in order to find active stars. We also found several pairs that could be wide companion, so in a future research we will investigate in deep these pairs. This MSc thesis have been the first step for a refereed paper.

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27 Appendix A: Tables

Table A1: New M-dwarf candidates (not in Simbad).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

1 000238.8−214833 0.661843 −21.809337 −106.7 −80.6 14.629 10.514 9.642 M4.5 V 22.6 2 000453.0−103220 1.221038 −10.538929 +62.4 −20.6 14.707 10.530 9.681 M4.5 V 22.8 3 000636.3−090603 1.651329 −9.100843 −164.8 −1.6 16.276 11.467 10.575 M5.0 V 28.1 4 001024.0−262321 2.600022 −26.389441 +74.3 −67.7 15.214 11.266 10.375 M4.0 V 39.3 5 001652.4+085041 4.218501 8.844823 −12.2 +27.1 15.523 11.331 10.457 M4.5 V 33.0 6 001931.9−055440 4.883245 −5.911376 +111.4 −74.1 16.072 11.171 10.324 M5.5 V 19.3 7 002111.3−084140 5.297174 −8.694606 −62.7 −67.8 15.268 11.096 10.219 M4.5 V 29.6 8 003221.4+292746 8.089319 29.462960 −62.7 −49.1 15.359 11.217 10.363 M4.5 V 31.3 9 003237.2+391100 8.155314 39.183407 −9.6 +28.1 15.497 11.366 10.481 M4.5 V 33.5 10 003244.5+274444 8.185711 27.745740 +87.3 −82.7 15.142 11.207 10.384 M4.0 V 38.2 11 004036.0+335408 10.150005 33.902487 +117.1 +31.2 14.937 10.975 10.098 M4.0 V 34.4 12 004217.6−035443 10.573443 −3.912215 −12.0 +230.0 15.464 11.400 10.495 M4.0 V 41.8 13 004434.5+160701 11.144141 16.116962 +52.7 +30.7 15.267 11.280 10.444 M4.0 V 39.5 14 004725.0+480327 11.854270 48.057735 +39.9 −22.3 15.364 11.201 10.342 M4.5 V 31.1 15 004826.6−184720 12.111222 −18.789064 +70.0 −46.5 14.911 10.745 9.862 M4.5 V 25.2 16 005020.4+175109 12.585207 17.852661 +70.2 −38.9 15.321 11.265 10.430 M4.0 V 39.3 17 005410.3+050928 13.542933 5.158032 +39.5 −17.0 15.752 11.084 10.195 M5.0 V 23.6 18 005548.5−151745 13.952250 −15.296101 +46.0 +53.5 15.355 11.452 10.585 M4.0 V 42.8 19 010301.3+065849 15.755602 6.980333 −82.6 −71.7 15.230 11.317 10.468 M4.0 V 40.2 20 011113.4+030640 17.806162 3.111346 −385.7 −280.0 14.675 10.677 9.799 M4.0 V 30.0 21 011131.4−110017 17.880854 −11.004819 −42.0 −251.3 15.719 11.413 10.576 M4.5 V 34.3 22 012127.0+051925 20.362627 5.323838 −7.9 −25.3 15.196 11.131 10.264 M4.0 V 36.9 23 012645.2−360942 21.688385 −36.161740 +153.1 +11.5 15.446 11.463 10.527 M4.0 V 43.0 24 013035.3+200839 22.647405 20.144224 +50.4 −43.2 15.591 11.052 10.190 M5.0 V 23.2 25 013055.3−332904 22.730673 −33.484685 +118.8 +6.0 15.786 11.292 10.422 M5.0 V 25.9 26 013304.4−063128 23.268607 −6.524537 −53.8 +50.5 15.200 11.217 10.407 M4.0 V 38.4 27 013958.2+464259 24.992527 46.716471 −16.8 −64.3 15.197 11.151 10.279 M4.0 V 37.3 28 014101.6+433550 25.257006 43.597312 +48.1 −40.1 15.306 11.151 10.287 M4.5 V 30.4 29 014256.1+342622 25.734099 34.439719 +88.4 −102.9 15.225 11.245 10.384 M4.0 V 38.9 30 014516.7+163658 26.319958 16.616383 −74.2 +30.2 15.632 11.150 10.239 M5.0 V 24.3 31 014947.9−133633 27.449697 −13.609309 +62.4 −100.6 15.152 10.944 10.029 M4.5 V 27.6 32 015139.5+465240 27.914695 46.877963 +46.8 −3.3 14.403 10.165 9.268 M4.5 V 19.3 33 015324.4−342611 28.351723 −34.436439 −31.3 −146.0 15.372 11.276 10.369 M4.0 V 39.5 34 015730.6+391824 29.377507 39.306719 −59.4 −45.1 15.290 11.236 10.402 M4.0 V 38.8 35 015736.3−305828 29.401477 −30.974520 −23.5 −129.9 15.611 11.461 10.603 M4.5 V 35.0 36 015901.0+360955 29.754415 36.165433 +74.0 −58.3 14.839 10.739 9.865 M4.0 V 30.8 37 020150.7−072658 30.461581 −7.449626 +96.7 −53.5 14.950 10.899 10.085 M4.0 V 33.2 38 020837.0+261713 32.154523 26.287176 −102.2 −36.7 15.403 11.489 10.620 M4.0 V 43.5 39 021156.3−014215 32.984700 −1.704377 +94.0 −130.2 15.031 10.986 10.097 M4.0 V 34.5 40 021437.7+243548 33.657094 24.596777 +107.1 −79.7 15.520 11.463 10.652 M4.0 V 43.0 41 021521.1−390918 33.838199 −39.155151 +118.6 +47.5 15.294 11.306 10.401 M4.0 V 40.0 42 021548.3+205755 33.951614 20.965303 +31.2 −27.7 15.548 11.287 10.436 M4.5 V 32.3 43 021750.5+082950 34.460648 8.497300 +54.7 −20.5 14.453 10.476 9.641 M4.0 V 27.3 44 021922.1−392522 34.842403 −39.423039 +106.0 −35.7 16.466 11.381 10.404 M5.5 V 21.2 45 022213.6−054919 35.556795 −5.822085 +19.1 −50.5 14.505 10.452 9.548 M4.0 V 27.0 46 022957.4−360639 37.489289 −36.111097 −35.3 +103.7 17.203 11.329 10.340 M6.0 V 16.0

28 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

47 023927.1−033241 39.863324 −3.544785 +118.5 +89.6 15.675 11.332 10.451 M4.5 V 33.0 48 024052.6+191342 40.219441 19.228509 +55.5 −24.9 15.063 11.048 10.188 M4.0 V 35.5 49 024508.3−070812 41.284605 −7.136810 +38.4 −43.0 14.974 10.786 9.950 M4.5 V 25.7 50 024612.3+351605 41.551656 35.268297 +49.0 −78.8 15.003 11.070 10.205 M4.0 V 35.9 51 024816.8+053705 42.070027 5.618301 +74.1 −53.8 14.026 10.072 9.162 M4.0 V 22.7 52 024857.6−120349 42.240086 −12.063787 −96.2 −34.5 15.177 10.686 9.784 M5.0 V 19.6 53 024920.4+435712 42.335411 43.953396 +35.2 −49.9 16.028 11.480 10.579 M5.0 V 28.3 54 025354.0−162453 43.475193 −16.414934 +20.5 +0.1 14.658 10.700 9.859 M4.0 V 30.3 55 025407.5+334336 43.531429 33.726735 +98.1 −72.3 15.070 10.943 10.142 M4.5 V 27.6 56 030228.1−325702 45.617489 −32.950697 +55.4 −29.9 15.347 11.299 10.387 M4.0 V 39.9 57 030251.6−191150 45.715005 −19.197224 +93.3 −36.9 14.757 10.541 9.684 M4.5 V 22.9 58 030303.1−075345 45.763151 −7.895873 +21.3 −76.6 15.398 11.435 10.583 M4.0 V 42.5 59 030448.9+223639 46.203772 22.610955 −52.3 −145.5 15.508 11.219 10.326 M4.5 V 31.3 60 030501.9−055430 46.257944 −5.908373 −49.8 +3.4 15.523 11.357 10.504 M4.5 V 33.4 61 030602.8−124354 46.511826 −12.731729 −15.6 −16.2 15.427 11.440 10.565 M4.0 V 42.6 62 030840.0+135652 47.166781 13.948049 +10.4 −7.7 15.270 11.300 10.448 M4.0 V 39.9 63 031035.9−104607 47.649974 −10.768827 +51.2 −77.5 15.622 11.440 10.587 M4.5 V 34.7 64 031312.2+094738 48.300890 9.793979 −6.0 −24.3 15.340 11.288 10.414 M4.0 V 39.7 65 031719.9−011349 49.333100 −1.230419 +81.1 +14.3 15.032 11.089 10.233 M4.0 V 36.2 66 031951.9+213828 49.966441 21.641301 +57.3 −60.4 15.346 11.176 10.302 M4.5 V 30.7 67 032000.5+103246 50.002402 10.546206 +48.1 −29.8 15.448 11.383 10.516 M4.0 V 41.5 68 032141.4+140604 50.422775 14.101272 +60.9 −96.3 15.015 11.109 10.260 M4.0 V 36.6 69 032247.1+030953 50.696445 3.164744 +130.3 −8.7 15.513 11.419 10.593 M4.0 V 42.2 70 032409.4+274737 51.039203 27.793747 +28.5 −63.5 15.302 11.208 10.340 M4.0 V 38.3 71 032435.8−322152 51.149440 −32.364700 +39.4 −13.2 15.244 11.294 10.397 M4.0 V 39.8 72 032950.3−381200 52.459672 −38.200144 +91.3 −54.4 14.799 10.879 10.051 M4.0 V 32.9 73 033114.7−211727 52.811584 −21.290875 +87.9 −94.0 14.696 10.782 9.907 M4.0 V 31.4 74 033322.6+284034 53.344547 28.676385 +32.4 −6.0 14.739 10.797 9.896 M4.0 V 31.7 75 033431.6−350103 53.631987 −35.017582 +30.0 −4.8 14.642 10.727 9.866 M4.0 V 30.7 76 034049.5−101630 55.206605 −10.275070 +94.1 −46.7 15.065 10.805 9.979 M4.5 V 25.9 77 034252.0−191401 55.717038 −19.233850 +8.2 −14.4 16.722 11.445 10.539 M5.5 V 21.9 78 034311.6+070216 55.798499 7.037834 −10.8 −116.6 15.454 11.078 10.210 M4.5 V 29.4 79 034422.8+311744 56.095245 31.295791 −40.1 −42.2 15.131 11.229 10.389 M4.0 V 38.6 80 034433.8−200538 56.140969 −20.093972 +63.8 −18.9 15.314 11.318 10.485 M4.0 V 40.2 81 034727.8+320955 56.865842 32.165543 +94.0 −80.3 15.459 11.438 10.541 M4.0 V 42.5 82 034729.3+465756 56.872266 46.965646 +9.5 −10.7 15.567 11.458 10.568 M4.0 V 42.9 83 034827.1−194426 57.113160 −19.740717 +9.0 −55.6 15.340 11.197 10.270 M4.5 V 31.0 84 035027.9+040645 57.616485 4.112583 +138.7 +4.6 15.376 11.456 10.627 M4.0 V 42.9 85 035056.4+364834 57.735103 36.809681 +21.8 −47.0 15.596 11.389 10.509 M4.5 V 33.9 86 035236.5+173726 58.152153 17.623925 +3.0 −14.6 15.262 10.984 10.120 M4.5 V 28.1 87 035305.9−183550 58.274938 −18.597246 +15.5 +10.8 15.413 11.104 10.273 M4.5 V 29.7 88 035306.2−183559 58.275977 −18.599871 +18.8 −5.4 15.606 11.239 10.408 M4.5 V 31.6 89 035342.3−252700 58.426462 −25.450177 −326.3 −348.3 14.600 10.473 9.518 M4.5 V 22.2 90 035612.8+015139 59.053519 1.860893 +7.0 −4.0 15.465 11.444 10.569 M4.0 V 42.7 91 035624.6−311138 59.102760 −31.194166 +39.0 −119.5 14.090 10.072 9.121 M4.0 V 22.7 92 040044.9+135422 60.187375 13.906316 +131.0 −16.2 14.209 10.260 9.344 M4.0 V 24.7 93 040123.5+010649 60.348318 1.113620 +106.7 −23.0 15.064 10.893 10.000 M4.5 V 27.0 94 040424.9−170159 61.104013 −17.033321 −64.0 −198.6 15.348 11.257 10.399 M4.0 V 39.1

29 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

95 040532.1+273313 61.383956 27.553836 +4.7 −22.8 15.887 11.367 10.477 M5.0 V 26.8 96 040546.6+371942 61.444194 37.328524 +96.8 −78.4 15.273 10.915 10.042 M4.5 V 27.2 97 040553.4+053125 61.472594 5.523641 +34.4 −35.6 14.963 10.917 10.065 M4.0 V 33.5 98 040557.0−280946 61.487905 −28.162901 +56.7 −8.4 15.276 11.192 10.323 M4.0 V 38.0 99 041436.4+090455 63.651865 9.082129 +73.0 −3.9 15.438 11.374 10.528 M4.0 V 41.3 100 041509.2+190426 63.788554 19.074131 +2.0 −17.7 14.995 10.989 10.145 M4.0 V 34.6 101 041806.4−240626 64.526708 −24.107311 −115.3 −368.1 15.377 10.919 10.015 M4.5 V 27.3 102 041840.2−250707 64.667614 −25.118779 +152.0 +132.1 14.416 10.366 9.476 M4.0 V 26.0 103 041950.2+292647 64.959570 29.446589 +10.5 −30.0 16.596 11.369 10.473 M5.5 V 21.1 104 042023.3+455228 65.097472 45.874576 +26.0 +26.7 14.765 10.842 9.961 M4.0 V 32.3 105 042044.6+180558 65.186205 18.099695 +20.2 −39.9 16.129 11.194 10.313 M5.5 V 19.5 106 042100.5−355101 65.252305 −35.850515 +216.7 +64.0 15.077 10.932 10.016 M4.5 V 27.5 107 042126.5+295247 65.360491 29.879861 +5.1 −26.1 15.428 10.644 9.728 M5.0 V 19.2 108 042137.8−094457 65.407817 −9.749171 −38.4 −64.2 15.009 11.093 10.176 M4.0 V 36.3 109 042202.5−133205 65.510721 −13.534849 −11.9 −193.5 15.428 11.458 10.624 M4.0 V 42.9 110 042219.9+051112 65.583265 5.186738 +13.4 −34.6 16.103 11.390 10.520 M5.0 V 27.1 111 042320.8+352119 65.836735 35.355451 −72.0 −36.4 15.136 11.123 10.262 M4.0 V 36.8 112 042424.4+361319 66.101780 36.222043 +34.5 −87.7 16.169 11.329 10.463 M5.0 V 26.4 113 042546.2−215359 66.442679 −21.899919 +48.3 −91.7 15.394 11.170 10.325 M4.5 V 30.6 114 042703.9+240643 66.766461 24.112219 +18.6 −25.4 16.144 11.343 10.362 M5.0 V 26.5 115 042736.0−231658 66.900104 −23.282981 +61.0 −27.1 14.649 10.473 9.578 M4.5 V 22.2 116 042736.4+192645 66.902048 19.445908 +35.0 +7.0 15.108 11.045 10.186 M4.0 V 35.5 117 042741.8+270955 66.924469 27.165291 +8.0 −14.7 16.254 11.246 10.356 M5.5 V 19.9 118 042749.6−332701 66.956983 −33.450359 +68.0 −8.7 15.122 11.210 10.378 M4.0 V 38.3 119 042832.0+415723 67.133465 41.956653 −45.0 −38.9 15.530 11.473 10.650 M4.0 V 43.2 120 042832.8+415723 67.136894 41.956632 −102.5 −40.0 15.305 11.388 10.571 M4.0 V 41.6 121 042923.9−293007 67.349622 −29.501957 −77.5 −69.0 15.853 11.289 10.447 M5.0 V 25.9 122 042930.1+063516 67.375728 6.588039 +28.9 −9.9 15.112 11.158 10.306 M4.0 V 37.4 123 043224.6+232138 68.102705 23.360630 +4.6 −23.8 15.072 10.831 9.899 M4.5 V 26.2 124 043230.5+232856 68.127305 23.482344 +7.1 −18.2 14.822 10.509 9.592 M4.5 V 22.6 125 043329.6−005939 68.373588 −0.994302 +39.8 −38.3 15.317 11.275 10.399 M4.0 V 39.5 126 043352.8+180316 68.470183 18.054587 +16.1 −15.4 15.332 10.865 9.932 M4.5 V 26.6 127 043416.9−252646 68.570640 −25.446362 +41.9 −18.9 15.504 11.353 10.477 M4.5 V 33.3 128 043436.6+183625 68.652659 18.607071 +16.3 −18.9 14.980 10.636 9.670 M4.5 V 24.0 129 043555.6+170739 68.981990 17.127694 +14.6 −19.3 15.274 11.078 10.141 M4.5 V 29.4 130 043556.9+235147 68.987242 23.863154 +10.6 −21.3 15.782 10.994 10.078 M5.0 V 22.6 131 043738.7+184208 69.411407 18.702396 −4.1 −13.6 15.362 11.330 10.526 M4.0 V 40.5 132 044044.7+300755 70.186502 30.132179 −101.8 +38.8 15.528 11.463 10.620 M4.0 V 43.0 133 044154.4+091953 70.476797 9.331500 +14.6 −34.9 15.594 11.451 10.579 M4.5 V 34.9 134 044302.4+163156 70.760202 16.532258 +16.4 −20.7 14.781 10.867 9.965 M4.0 V 32.7 135 044405.5+182130 71.023182 18.358341 +14.1 −25.6 15.163 11.074 10.148 M4.0 V 36.0 136 044417.6+203422 71.073340 20.572980 +0.0 −15.7 15.652 11.297 10.461 M4.5 V 32.5 137 044619.2−094702 71.580112 −9.784024 +16.9 −119.5 15.792 11.316 10.324 M5.0 V 26.2 138 044714.9−013046 71.812226 −1.512918 +37.2 +10.1 15.233 11.261 10.454 M4.0 V 39.2 139 044745.2+302922 71.938365 30.489710 +11.8 −43.2 15.534 11.430 10.574 M4.0 V 42.4 140 044754.8+095357 71.978396 9.899239 +12.8 −22.8 15.521 11.299 10.411 M4.5 V 32.5 141 044840.1−353923 72.167118 −35.656458 −66.4 −133.7 14.753 10.521 9.652 M4.5 V 22.7 142 044910.5+134841 72.294059 13.811444 +86.8 −22.9 15.202 11.245 10.348 M4.0 V 38.9

30 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

143 044925.7+440541 72.357240 44.094860 +75.6 −27.3 15.427 11.374 10.453 M4.0 V 41.3 144 044957.9+271236 72.491608 27.210163 +97.5 −77.5 14.971 11.067 10.205 M4.0 V 35.9 145 045056.2+121759 72.734301 12.299849 −14.7 −1.7 15.012 11.105 10.275 M4.0 V 36.5 146 045103.9−272548 72.766440 −27.430060 +30.9 −3.4 15.325 11.411 10.530 M4.0 V 42.0 147 045218.2+152624 73.075904 15.440120 +8.6 −28.0 16.139 11.401 10.502 M5.0 V 27.3 148 045402.1+082633 73.509103 8.442688 +16.8 −45.3 15.304 11.349 10.516 M4.0 V 40.8 149 045410.4−303636 73.543394 −30.610019 −18.4 +126.1 14.644 10.608 9.732 M4.0 V 29.0 150 045455.7−022832 73.732368 −2.475600 +8.1 −19.7 15.587 11.476 10.607 M4.5 V 35.3 151 045519.0−321223 73.829217 −32.206407 +13.1 +52.7 15.162 10.683 9.814 M5.0 V 19.6 152 045546.3+323903 73.943187 32.651002 −7.9 −0.8 15.432 11.395 10.542 M4.0 V 41.7 153 045757.7+142707 74.490832 14.451959 +69.2 −24.0 15.304 11.304 10.459 M4.0 V 40.0 154 045821.0+105952 74.587525 10.997832 +53.4 −58.5 15.313 11.300 10.437 M4.0 V 39.9 155 045913.2+144838 74.805385 14.810616 +8.3 −28.1 15.266 11.184 10.305 M4.0 V 37.8 156 045928.4+141623 74.868382 14.273289 +8.2 −16.8 14.960 10.974 10.062 M4.0 V 34.4 157 050011.9+055119 75.049846 5.855497 +71.4 +8.2 15.193 11.236 10.367 M4.0 V 38.8 158 050215.7+290323 75.565558 29.056532 +2.3 −18.5 15.526 11.401 10.506 M4.5 V 34.1 159 050324.7+164913 75.853312 16.820550 −2.0 −16.3 15.539 11.388 10.514 M4.5 V 33.9 160 050333.3−382135 75.888849 −38.359909 −3.8 +9.0 14.805 10.863 10.014 M4.0 V 32.6 161 050403.8+243534 76.015932 24.592868 +22.8 −51.0 15.171 11.225 10.353 M4.0 V 38.6 162 050440.3+330039 76.167960 33.010856 +310.9 +74.6 16.065 11.382 10.502 M5.0 V 27.0 163 050531.9−191636 76.383287 −19.276729 +33.4 −23.2 15.588 11.478 10.622 M4.5 V 35.3 164 050550.0+131455 76.458435 13.248661 −2.4 −19.9 15.099 11.139 10.301 M4.0 V 37.1 165 050806.3+302623 77.026500 30.439810 +4.0 −26.8 15.802 11.320 10.425 M5.0 V 26.3 166 050810.4+080726 77.043707 8.124004 +21.0 −37.2 15.403 11.439 10.526 M4.0 V 42.6 167 050856.9+141317 77.237286 14.221436 +20.6 −9.4 15.670 11.462 10.612 M4.5 V 35.0 168 051051.0−164335 77.712906 −16.726581 +118.8 +28.8 15.017 11.103 10.204 M4.0 V 36.5 169 051056.5+130719 77.735637 13.122006 +63.7 −28.0 14.788 10.800 9.923 M4.0 V 31.7 170 051144.8+064940 77.936702 6.828022 +121.0 −65.7 15.695 11.199 10.287 M5.0 V 24.8 171 051146.1−170528 77.942342 −17.091292 +38.4 −24.5 14.835 10.867 9.981 M4.0 V 32.7 172 051317.2+273702 78.321875 27.617223 −92.6 −17.5 14.641 10.732 9.909 M4.0 V 30.7 173 051423.6+203153 78.598548 20.531552 +59.9 −35.4 15.272 11.312 10.498 M4.0 V 40.1 174 051429.4+091807 78.622696 9.302035 −66.1 +42.9 14.130 10.103 9.241 M4.0 V 23.0 175 051514.9+195431 78.812218 19.908846 −33.4 −40.2 15.139 11.030 10.219 M4.0 V 35.2 176 051601.2−312445 79.005052 −31.412702 +39.4 +0.9 14.650 10.628 9.791 M4.0 V 29.3 177 051630.2−094950 79.125878 −9.830598 +60.9 +56.3 15.089 11.071 10.171 M4.0 V 35.9 178 051650.6+022713 79.211062 2.453706 +27.1 −29.2 14.907 10.742 9.873 M4.5 V 25.2 179 051835.4−050435 79.647896 −5.076592 +10.0 −71.6 15.282 11.319 10.476 M4.0 V 40.3 180 051844.5+462959 79.685692 46.499807 +34.8 −111.2 13.961 9.957 9.115 M4.0 V 21.5 181 051915.9+065835 79.816505 6.976581 +27.1 −59.5 14.609 10.698 9.871 M4.0 V 30.3 182 051936.9+185951 79.903817 18.997538 −12.7 −30.3 14.971 10.894 10.019 M4.0 V 33.1 183 052126.0−173333 80.358344 −17.559247 +121.1 −84.9 15.537 11.016 10.098 M5.0 V 22.8 184 052353.4+324934 80.972640 32.826381 +23.4 −63.2 15.785 11.385 10.513 M4.5 V 33.8 185 052445.6+251444 81.190002 25.245714 +19.0 −70.3 15.448 11.312 10.447 M4.5 V 32.7 186 052454.2+420927 81.226008 42.157562 +36.7 −104.6 15.169 11.232 10.371 M4.0 V 38.7 187 052509.8−133524 81.290841 −13.590254 +112.9 −99.8 15.606 11.227 10.329 M4.5 V 31.5 188 052515.3+191713 81.313984 19.286968 −10.8 −29.0 15.616 11.279 10.399 M4.5 V 32.2 189 052632.6−121512 81.636241 −12.253408 +22.2 +4.0 14.753 10.783 9.942 M4.0 V 31.5 190 052634.4+001211 81.643409 0.203068 −128.4 −52.7 15.156 11.133 10.292 M4.0 V 37.0

31 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

191 052701.9−132749 81.758148 −13.463670 −63.0 −38.5 16.186 11.370 10.472 M5.0 V 26.9 192 052706.2−103835 81.776087 −10.643291 +97.5 +41.6 15.110 10.994 10.103 M4.5 V 28.3 193 053052.7+321717 82.719756 32.288139 +77.1 −17.3 15.188 11.122 10.235 M4.0 V 36.8 194 053100.2+231218 82.751140 23.205185 +6.8 −41.9 14.572 10.582 9.685 M4.0 V 28.7 195 053151.8−161142 82.966093 −16.195199 +39.8 −13.0 14.756 10.757 9.875 M4.0 V 31.1 196 053205.9−030116 83.024828 −3.021123 +4.7 −50.2 14.908 10.580 9.695 M4.5 V 23.3 197 053341.7−365444 83.424098 −36.912436 +2.0 +125.3 14.935 10.982 10.146 M4.0 V 34.5 198 053506.4−170633 83.776788 −17.109221 +480.3 −92.2 14.209 10.178 9.295 M4.0 V 23.8 199 053636.9+130036 84.153819 13.010232 +4.7 −35.6 15.255 11.319 10.390 M4.0 V 40.3 200 053850.8−294056 84.712048 −29.682244 +23.6 −1.0 15.285 11.106 10.207 M4.5 V 29.7 201 054109.6+275419 85.290054 27.905481 −13.0 −122.0 15.621 11.331 10.400 M4.5 V 33.0 202 054200.9+181703 85.503921 18.284171 +29.0 −24.2 15.410 11.242 10.333 M4.5 V 31.7 203 054219.7+153936 85.582180 15.660268 +7.6 −40.3 14.914 10.905 10.049 M4.0 V 33.3 204 054328.2−130026 85.867595 −13.007449 +137.9 −169.6 15.453 11.235 10.343 M4.5 V 31.6 205 054801.0−250104 87.004514 −25.017827 −102.8 +384.2 15.423 11.291 10.456 M4.5 V 32.4 206 054923.8−104256 87.349170 −10.715805 +13.7 −18.7 14.924 10.911 10.016 M4.0 V 33.4 207 055128.1−153034 87.867305 −15.509500 −233.9 +352.8 15.367 11.426 10.555 M4.0 V 42.3 208 055204.0+355027 88.017047 35.841031 −19.1 +414.1 15.189 11.272 10.372 M4.0 V 39.4 209 055600.4+154600 89.002073 15.766909 −111.5 +16.5 15.961 11.371 10.507 M5.0 V 26.9 210 055613.0+080303 89.054475 8.050959 +6.8 −28.6 15.538 11.482 10.596 M4.0 V 43.4 211 060043.1−004023 90.179915 −0.673199 −215.8 −215.6 15.364 11.223 10.296 M4.5 V 31.4 212 060115.4+112053 90.314406 11.348141 −29.0 −27.1 15.384 11.297 10.457 M4.0 V 39.9 213 060126.5−151513 90.360434 −15.253699 +20.6 −9.3 15.414 11.466 10.616 M4.0 V 43.1 214 060304.1+360627 90.767224 36.107588 +41.9 −119.8 14.842 10.667 9.839 M4.5 V 24.3 215 060312.3−372243 90.801367 −37.378730 +15.0 −96.5 14.635 10.453 9.614 M4.5 V 22.0 216 060536.3+385116 91.401477 38.854679 +5.8 −53.1 15.032 11.104 10.268 M4.0 V 36.5 217 060749.4−262222 91.955890 −26.372966 +95.3 +136.2 14.574 10.652 9.828 M4.0 V 29.6 218 061003.7+350004 92.515678 35.001150 +45.7 −110.5 14.932 10.877 10.002 M4.0 V 32.8 219 061042.9+025947 92.679124 2.996598 −92.8 −22.9 14.325 10.363 9.473 M4.0 V 25.9 220 061114.6−003537 92.811032 −0.593886 +7.4 +94.3 15.157 10.627 9.693 M5.0 V 19.1 221 061158.0−011717 92.991916 −1.288268 +184.7 −152.6 15.183 11.058 10.189 M4.5 V 29.1 222 061436.1+262919 93.650617 26.488816 −48.4 −99.2 16.049 11.300 10.429 M5.0 V 26.0 223 061533.3−101332 93.889040 −10.225595 +34.2 +27.6 15.646 11.425 10.525 M4.5 V 34.5 224 061539.6+344331 93.915084 34.725368 −59.9 −111.1 15.545 11.265 10.430 M4.5 V 32.0 225 061616.3+323501 94.067919 32.583812 +3.7 −68.7 15.180 11.231 10.370 M4.0 V 38.7 226 062206.7−163048 95.527995 −16.513606 −85.7 −162.9 15.015 10.873 10.027 M4.5 V 26.7 227 062440.7+052045 96.169585 5.345861 −29.5 −12.2 14.992 11.043 10.161 M4.0 V 35.5 228 062607.0−073235 96.529550 −7.543321 +0.6 −19.4 15.296 11.371 10.556 M4.0 V 41.2 229 062701.8−310201 96.757657 −31.033713 −29.8 −86.6 15.498 11.307 10.471 M4.5 V 32.6 230 062920.1+172516 97.334010 17.421307 +16.9 −41.6 16.551 11.162 10.302 M6.0 V 14.8 231 062959.0+285903 97.496024 28.984252 −103.1 −69.5 15.384 11.305 10.447 M4.0 V 40.0 232 063001.8−192336 97.507761 −19.393494 −35.9 −19.5 14.052 10.092 9.254 M4.0 V 22.9 233 063038.1−153904 97.658921 −15.651181 +4.9 +96.2 15.311 11.301 10.401 M4.0 V 39.9 234 063050.8+303159 97.712062 30.533099 +39.3 −48.8 15.474 11.378 10.504 M4.0 V 41.4 235 063051.5−065809 97.714647 −6.969169 +350.6 +406.2 14.976 10.897 9.988 M4.0 V 33.2 236 063851.1−373217 99.713223 −37.538315 −34.3 +163.8 14.723 10.666 9.860 M4.0 V 29.8 237 063944.0−255728 99.933335 −25.957961 −21.5 −96.7 14.844 10.902 10.055 M4.0 V 33.2 238 064137.2−372229 100.405283 −37.374871 −89.4 +94.3 15.358 11.421 10.533 M4.0 V 42.2

32 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

239 064142.8+122643 100.428683 12.445480 +12.6 −21.7 14.405 10.227 9.358 M4.5 V 19.8 240 064149.3+014923 100.455513 1.823119 −26.0 +36.6 15.248 11.316 10.451 M4.0 V 40.2 241 064547.8−191831 101.449367 −19.308711 +19.2 +38.9 14.816 10.890 9.999 M4.0 V 33.0 242 064920.4+065519 102.335219 6.922153 −51.3 −32.1 15.396 11.444 10.549 M4.0 V 42.7 243 065120.2+013458 102.834184 1.582806 −140.1 +12.0 15.828 11.439 10.524 M4.5 V 34.7 244 065150.8−303337 102.961840 −30.560439 −5.9 −1.0 15.078 10.799 9.930 M4.5 V 25.8 245 065211.2−384734 103.046689 −38.793027 −93.8 +6.9 15.351 11.275 10.277 M4.0 V 39.5 246 065301.8−092640 103.257856 −9.444687 −14.8 +66.7 16.019 11.415 10.481 M5.0 V 27.4 247 065549.8−084215 103.957619 −8.704259 −4.8 +5.3 15.405 11.406 10.580 M4.0 V 41.9 248 065649.4+132933 104.205983 13.492616 −35.3 −46.8 15.806 11.444 10.568 M4.5 V 34.8 249 070512.0−100752 106.300107 −10.131188 +123.7 +77.5 14.369 10.196 9.275 M4.5 V 19.6 250 071633.3+084848 109.138890 8.813479 −2.0 −25.8 15.043 11.123 10.241 M4.0 V 36.8 251 071733.0+104849 109.387808 10.813882 −39.8 −25.6 15.403 11.477 10.624 M4.0 V 43.3 252 072055.3+442721 110.230582 44.455922 −12.4 +0.7 15.620 11.470 10.581 M4.5 V 35.2 253 072151.1+211454 110.463206 21.248364 +25.9 −77.5 14.523 10.505 9.640 M4.0 V 27.7 254 072239.0+321328 110.662768 32.224459 −16.8 −26.8 15.326 11.264 10.343 M4.0 V 39.3 255 072305.1+462742 110.771562 46.461744 −23.7 −105.1 15.577 11.466 10.530 M4.5 V 35.1 256 072400.7−263610 111.002945 −26.602849 −101.6 +100.0 15.296 11.299 10.400 M4.0 V 39.9 257 072417.3+183847 111.072163 18.646593 −54.9 −47.6 14.563 10.591 9.739 M4.0 V 28.8 258 072420.1+382053 111.083997 38.348266 +33.7 −49.6 14.388 10.408 9.559 M4.0 V 26.5 259 073001.9−283102 112.508195 −28.517404 −150.5 +92.4 14.979 10.634 9.747 M4.5 V 23.9 260 073100.2−291723 112.751001 −29.289856 −81.1 −14.2 15.646 11.350 10.488 M4.5 V 33.3 261 073227.9−254303 113.116285 −25.717775 −153.0 +59.6 15.316 11.012 10.135 M4.5 V 28.5 262 073255.1−200314 113.229914 −20.054103 −191.9 −146.4 15.656 11.188 10.310 M4.5 V 30.9 263 073655.1+364420 114.229620 36.738973 −83.5 −126.1 15.379 11.217 10.344 M4.5 V 31.3 264 074508.3−070128 116.284850 −7.024495 +163.4 +119.5 15.051 11.122 10.303 M4.0 V 36.8 265 074610.7−185903 116.544733 −18.984391 −107.8 +111.7 15.914 11.402 10.482 M5.0 V 27.3 266 074656.4+430415 116.735015 43.071048 −16.3 −46.0 16.221 11.411 10.573 M5.0 V 27.4 267 075313.5−101219 118.306376 −10.205307 +146.3 −360.5 15.870 11.410 10.601 M4.5 V 34.2 268 075405.3+022344 118.522269 2.395830 +26.3 −3.8 14.922 10.966 10.137 M4.0 V 34.2 269 075529.8+255635 118.874373 25.943137 +39.8 −50.7 15.412 11.401 10.555 M4.0 V 41.8 270 075705.0−222643 119.271122 −22.445296 +5.1 −83.5 14.808 10.785 9.880 M4.0 V 31.5 271 075831.9−293412 119.633038 −29.570096 +47.0 +75.6 14.712 10.693 9.740 M4.0 V 30.2 272 080259.4−163929 120.747535 −16.658249 +27.3 +30.0 15.561 11.468 10.542 M4.0 V 43.1 273 081202.5+070932 123.010691 7.159164 +77.5 +74.4 14.546 10.536 9.688 M4.0 V 28.1 274 082000.3−231826 125.001628 −23.307433 −57.5 +17.1 15.321 11.358 10.513 M4.0 V 41.0 275 082346.6−243404 125.944247 −24.567797 +46.6 −21.7 15.032 11.013 10.154 M4.0 V 35.0 276 082508.6−222513 126.285977 −22.420361 −99.7 +18.2 14.628 10.548 9.671 M4.0 V 28.2 277 082558.9−261135 126.495481 −26.193244 −153.5 +100.5 15.458 11.350 10.461 M4.0 V 40.8 278 083214.0+091027 128.058663 9.174312 −98.2 +22.2 15.191 11.138 10.250 M4.0 V 37.0 279 083505.4+423032 128.772606 42.508916 −2.0 +22.4 15.522 11.288 10.433 M4.5 V 32.3 280 083538.4+162856 128.910324 16.482464 +8.9 −10.3 15.203 11.281 10.443 M4.0 V 39.6 281 083740.5+482303 129.418750 48.384399 −8.9 −124.6 15.670 11.460 10.536 M4.5 V 35.0 282 084040.8−383238 130.170005 −38.543923 +91.6 −62.8 14.087 9.790 8.868 M4.5 V 16.2 283 084247.0−245827 130.696087 −24.974435 −74.4 −89.1 14.407 10.348 9.503 M4.0 V 25.7 284 084615.3+040638 131.563831 4.110666 +16.4 −99.9 14.268 10.244 9.320 M4.0 V 24.5 285 084900.6+285951 132.252532 28.997507 −92.4 −71.9 15.473 11.253 10.387 M4.5 V 31.8 286 085443.9−091103 133.683152 −9.184197 +21.8 +3.0 15.382 11.449 10.567 M4.0 V 42.7

33 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

287 085601.3−103449 134.005657 −10.580546 −26.5 −18.2 15.253 11.290 10.441 M4.0 V 39.7 288 085634.5−311758 134.143837 −31.299563 −162.2 +61.1 15.509 11.445 10.583 M4.0 V 42.7 289 085831.2+401553 134.630216 40.264730 −1.6 −105.6 15.158 11.158 10.217 M4.0 V 37.4 290 090034.9−075758 135.145507 −7.966126 +147.3 −43.4 15.145 10.968 10.160 M4.5 V 27.9 291 090101.4−110159 135.256163 −11.033323 −33.8 −181.0 15.232 11.321 10.449 M4.0 V 40.3 292 090351.2+221445 135.963413 22.245921 −41.7 +0.7 15.168 11.097 10.274 M4.0 V 36.4 293 090358.7+402238 135.994935 40.377370 −29.5 −155.4 15.777 11.497 10.582 M4.5 V 35.6 294 090756.7+374324 136.986575 37.723342 +5.2 +59.0 15.290 11.258 10.446 M4.0 V 39.1 295 090913.2−021611 137.305390 −2.269956 +90.6 +375.1 15.229 11.175 10.321 M4.0 V 37.7 296 090934.7−365452 137.394931 −36.914529 −97.1 +63.8 15.449 11.382 10.490 M4.0 V 41.5 297 091321.8−292716 138.341060 −29.454503 −7.5 +4.8 14.116 10.063 9.183 M4.0 V 22.6 298 091624.4−245529 139.101925 −24.924977 −34.3 −9.1 15.372 11.434 10.597 M4.0 V 42.5 299 091957.2−062535 139.988655 −6.426558 −144.6 −67.3 16.007 11.232 10.296 M5.0 V 25.2 300 092311.4−352313 140.797866 −35.387092 −55.4 −23.9 14.306 10.404 9.584 M4.0 V 26.4 301 092312.2−314522 140.801087 −31.756257 −109.8 +191.0 14.895 10.978 10.172 M4.0 V 34.4 302 092327.7−190931 140.865804 −19.158623 −11.3 −158.8 15.448 11.395 10.464 M4.0 V 41.7 303 093934.1−173555 144.892499 −17.598659 −24.7 −47.8 15.340 11.410 10.511 M4.0 V 42.0 304 094319.7−333506 145.832085 −33.585271 −100.6 +2.3 15.745 11.473 10.588 M4.5 V 35.2 305 094518.3−094024 146.326308 −9.673570 −85.1 −64.2 15.140 10.945 10.030 M4.5 V 27.6 306 095747.7−061108 149.448754 −6.185733 +54.8 −9.3 15.311 11.185 10.313 M4.5 V 30.8 307 100003.6+331305 150.015098 33.218183 −48.5 −135.4 15.632 11.493 10.658 M4.5 V 35.5 308 100009.7+064703 150.040819 6.784411 −356.9 +212.7 14.912 10.929 10.089 M4.0 V 33.6 309 100410.2−032934 151.042895 −3.493011 −101.2 +13.1 15.271 11.343 10.516 M4.0 V 40.7 310 100550.7+350813 151.461660 35.137111 +151.0 +149.6 15.143 11.196 10.326 M4.0 V 38.0 311 100626.9+412656 151.612295 41.449128 +28.5 +14.1 15.445 11.050 10.215 M4.5 V 29.0 312 100754.7−201429 151.978132 −20.241622 −25.1 −120.5 16.043 11.167 10.221 M5.5 V 19.2 313 101107.6−053328 152.781913 −5.558051 −352.2 −261.8 15.206 11.203 10.356 M4.0 V 38.2 314 101114.0−272512 152.808427 −27.420164 −20.6 +16.4 15.391 11.477 10.675 M4.0 V 43.3 315 101114.1−272526 152.809126 −27.423990 −15.0 +17.3 15.297 10.956 10.120 M4.5 V 27.8 316 101206.6+181841 153.027653 18.311619 +14.2 −79.9 15.685 11.272 10.388 M4.5 V 32.1 317 101331.8+160620 153.382770 16.105591 −25.5 −10.4 15.500 11.475 10.603 M4.0 V 43.3 318 102038.0−061534 155.158450 −6.259539 +119.9 −108.5 14.885 10.844 9.987 M4.0 V 32.4 319 102128.0+250722 155.366848 25.123014 −13.4 −77.4 15.482 11.275 10.428 M4.5 V 32.2 320 102207.9+023408 155.533091 2.568929 +40.8 −112.0 14.651 10.711 9.871 M4.0 V 30.4 321 102345.3−132547 155.938952 −13.429823 −129.8 +37.4 14.663 10.620 9.763 M4.0 V 29.2 322 102428.8+175015 156.120100 17.837636 −84.9 −11.1 15.581 11.480 10.622 M4.0 V 43.4 323 102809.5−231457 157.039902 −23.249206 +14.2 −148.5 15.560 11.335 10.424 M4.5 V 33.1 324 102824.8−395923 157.103725 −39.989749 −152.3 +13.3 14.886 10.867 10.025 M4.0 V 32.7 325 103850.2−205424 159.709328 −20.906869 −105.4 +45.8 15.332 11.363 10.548 M4.0 V 41.1 326 103954.8+183904 159.978656 18.651304 +41.2 −151.0 15.244 11.267 10.389 M4.0 V 39.3 327 104306.8+152631 160.778514 15.442066 −87.7 −48.9 15.489 11.468 10.652 M4.0 V 43.1 328 104834.6−151204 162.144335 −15.201147 +0.7 +21.2 14.048 9.986 9.139 M4.0 V 21.8 329 104909.7−010812 162.290428 −1.136771 −5.8 −17.9 15.609 11.120 10.224 M5.0 V 24.0 330 105045.0−073629 162.687630 −7.608272 −77.6 −114.0 15.454 11.398 10.439 M4.0 V 41.8 331 105423.0−150708 163.595843 −15.119003 −102.1 −71.0 15.567 11.097 10.256 M5.0 V 23.7 332 105850.4−234620 164.710387 −23.772458 −99.7 −18.4 14.861 10.302 9.430 M5.0 V 16.4 333 110058.3+480334 165.243162 48.059550 −37.9 −85.8 14.645 10.699 9.780 M4.0 V 30.3 334 110721.9−265344 166.841365 −26.895830 +70.1 −30.9 15.474 11.485 10.646 M4.0 V 43.5

34 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

335 111015.5−241143 167.564990 −24.195330 −183.0 +3.3 14.814 10.868 9.973 M4.0 V 32.7 336 111548.1+274616 168.950525 27.771116 +95.0 −31.2 16.735 11.284 10.324 M6.0 V 15.7 337 111551.4−345011 168.964278 −34.836469 −53.7 +17.5 15.090 11.160 10.273 M4.0 V 37.4 338 111618.6−254923 169.077540 −25.823063 −105.8 −240.1 14.674 10.650 9.693 M4.0 V 29.6 339 112055.8+164030 170.232621 16.675170 +39.3 +11.4 15.253 11.187 10.307 M4.0 V 37.9 340 112905.6+360701 172.273440 36.117067 +16.9 −94.7 14.938 10.932 10.059 M4.0 V 33.7 341 113049.8+153357 172.707728 15.565974 −64.9 −112.7 15.646 11.094 10.184 M5.0 V 23.7 342 113208.4−131922 173.035220 −13.322793 −130.1 +37.6 15.170 10.913 10.040 M4.5 V 27.2 343 113343.4+464747 173.430903 46.796482 −100.1 −79.6 15.496 11.459 10.597 M4.0 V 42.9 344 113622.0−235628 174.091695 −23.941359 −130.4 +42.7 15.387 11.327 10.431 M4.0 V 40.4 345 113928.8−065214 174.870010 −6.870793 −47.5 −1.8 15.296 11.360 10.549 M4.0 V 41.0 346 114113.5−160151 175.306569 −16.030892 −77.6 +124.9 15.862 11.442 10.569 M4.5 V 34.7 347 114914.6+300145 177.310872 30.029391 +60.5 +34.1 15.533 11.358 10.446 M4.5 V 33.4 348 115102.3−361146 177.759837 −36.196160 −147.9 −45.9 15.528 11.206 10.320 M4.5 V 31.1 349 115637.3+264602 179.155469 26.767284 −140.5 +7.8 15.080 11.130 10.289 M4.0 V 36.9 350 115858.1−274054 179.742445 −27.681881 −93.1 −51.2 15.615 11.487 10.668 M4.5 V 35.5 351 120056.8−375918 180.236732 −37.988578 +110.0 −69.2 15.480 11.121 10.239 M4.5 V 30.0 352 120237.9−332840 180.658107 −33.477899 −75.6 −12.9 14.921 10.686 9.847 M4.5 V 24.5 353 120254.1+414810 180.725451 41.802814 +2.5 −39.0 15.381 11.340 10.474 M4.0 V 40.7 354 120532.3+425502 181.384689 42.917311 +15.4 +21.9 15.283 11.120 10.268 M4.5 V 29.9 355 121004.4+124409 182.518501 12.736087 −34.4 −30.3 14.374 10.311 9.449 M4.0 V 25.3 356 121408.0+471603 183.533728 47.267658 −138.2 −74.3 15.095 11.172 10.315 M4.0 V 37.6 357 122150.1+463244 185.459052 46.545719 +90.7 −9.7 16.584 11.259 10.286 M6.0 V 15.5 358 122409.6+035604 186.040350 3.934561 −19.2 −135.7 15.714 11.378 10.453 M4.5 V 33.7 359 122607.0−002205 186.529188 −0.368190 −157.8 +14.7 15.459 11.395 10.537 M4.0 V 41.7 360 123015.8−312404 187.566081 −31.401337 −112.0 −12.8 16.260 11.382 10.391 M5.5 V 21.2 361 123116.2−152950 187.817644 −15.497318 +28.0 −108.5 15.063 10.987 10.096 M4.0 V 34.6 362 123244.3−153055 188.184935 −15.515476 −180.2 −176.4 16.154 11.384 10.462 M5.0 V 27.1 363 123726.2−352717 189.359203 −35.454808 +59.2 −28.6 15.923 11.262 10.381 M5.0 V 25.6 364 123745.5+384232 189.439706 38.708992 +25.4 −21.9 15.325 11.340 10.494 M4.0 V 40.7 365 123901.6+130955 189.756750 13.165286 −66.1 −22.6 15.413 11.465 10.663 M4.0 V 43.1 366 124046.1−302629 190.192160 −30.441611 +145.9 −95.4 14.699 10.500 9.618 M4.5 V 22.5 367 124112.3−273210 190.301463 −27.536111 −109.4 −93.7 14.841 10.907 10.054 M4.0 V 33.3 368 124358.7−161434 190.994634 −16.242935 −429.2 +82.3 14.113 9.777 8.896 M4.5 V 16.1 369 125348.6−084216 193.452573 −8.704644 −266.2 −170.2 15.215 10.737 9.855 M5.0 V 20.1 370 125657.8+381608 194.240957 38.268998 −3.5 −5.6 14.533 9.769 8.785 M5.0 V 12.9 371 125812.6+462952 194.552663 46.498007 −95.6 +103.2 15.465 11.450 10.616 M4.0 V 42.8 372 130428.0−084530 196.116872 −8.758414 −119.2 −25.4 15.755 11.483 10.568 M4.5 V 35.4 373 130618.1−342857 196.575651 −34.482531 −21.6 −10.3 15.112 10.503 9.632 M5.0 V 18.0 374 130619.9+133009 196.583125 13.502628 −19.5 −115.6 14.969 10.757 9.891 M4.5 V 25.3 375 130728.9+332508 196.870766 33.418932 +66.4 +25.1 15.954 11.432 10.606 M5.0 V 27.7 376 130733.7+111303 196.890585 11.217571 +58.3 −2.8 15.216 11.162 10.279 M4.0 V 37.5 377 131640.5−085825 199.168795 −8.973883 −112.8 −142.8 13.954 10.043 9.199 M4.0 V 22.4 378 131708.2−335443 199.284377 −33.912146 −99.1 +5.3 15.686 11.423 10.554 M4.5 V 34.4 379 131841.5−314307 199.673108 −31.718829 +15.6 −57.0 15.205 11.175 10.336 M4.0 V 37.7 380 132132.7−253615 200.386255 −25.604329 −68.1 −7.8 15.097 11.167 10.309 M4.0 V 37.5 381 132554.4−023214 201.477046 −2.537406 −160.6 +1.6 15.644 11.270 10.417 M4.5 V 32.1 382 132748.2−294107 201.951087 −29.685502 +83.4 −96.1 14.955 10.987 10.154 M4.0 V 34.6

35 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

383 132939.8+055052 202.416177 5.847997 +99.9 −101.0 15.291 11.284 10.450 M4.0 V 39.6 384 133226.9−385147 203.112302 −38.863307 −125.8 −23.5 15.342 11.276 10.368 M4.0 V 39.5 385 133255.6−291620 203.232082 −29.272268 −232.8 −31.8 14.953 10.569 9.676 M4.5 V 23.2 386 133356.0−075822 203.483684 −7.972936 +70.8 −30.5 15.880 11.456 10.554 M4.5 V 34.9 387 133531.2−015930 203.880003 −1.991726 −22.7 +41.7 15.643 11.442 10.605 M4.5 V 34.7 388 133559.6+402146 203.998738 40.362795 +34.0 +27.5 15.837 11.210 10.298 M5.0 V 25.0 389 133823.0−172423 204.596166 −17.406506 −14.0 −58.9 15.269 11.349 10.520 M4.0 V 40.8 390 134058.6−303109 205.244496 −30.519359 +99.2 −71.2 15.459 11.456 10.609 M4.0 V 42.9 391 134513.1−311328 206.304960 −31.224631 −163.2 −17.4 15.790 11.473 10.596 M4.5 V 35.2 392 135104.6+492409 207.769271 49.402599 −22.9 −24.0 15.009 11.096 10.203 M4.0 V 36.3 393 135207.2+462605 208.030360 46.434726 +114.2 −36.9 15.225 11.152 10.279 M4.0 V 37.3 394 135518.3−175345 208.826404 −17.895864 −76.0 −11.5 15.801 11.353 10.506 M4.5 V 33.3 395 135657.6+273100 209.240353 27.516934 −33.1 −150.9 15.807 11.238 10.303 M5.0 V 25.3 396 135753.7+230846 209.473999 23.146156 −86.4 −29.3 15.851 11.425 10.596 M4.5 V 34.5 397 135821.6−004626 209.590039 −0.774022 −82.2 −74.0 15.694 10.808 9.941 M5.5 V 16.3 398 135850.2−331520 209.709499 −33.255801 −34.8 −27.0 15.285 11.265 10.407 M4.0 V 39.3 399 140101.7+174317 210.257202 17.721420 +46.4 +48.2 15.262 11.110 10.302 M4.5 V 29.8 400 140246.4+130327 210.693620 13.057614 −17.8 −9.2 15.317 11.414 10.576 M4.0 V 42.1 401 140637.5−090454 211.656354 −9.081935 +0.6 −134.2 15.102 11.050 10.233 M4.0 V 35.6 402 141147.8−365227 212.949400 −36.874289 −21.9 −29.6 15.522 11.483 10.615 M4.0 V 43.4 403 141230.2+305935 213.125997 30.993139 −106.5 +21.5 15.425 11.438 10.595 M4.0 V 42.5 404 141443.0+261639 213.679542 26.277712 +51.8 −3.4 15.380 11.447 10.633 M4.0 V 42.7 405 142222.8+082422 215.595261 8.406223 +39.3 −119.7 15.340 11.086 10.170 M4.5 V 29.5 406 142225.0+135642 215.604568 13.945210 −62.6 −54.8 15.666 11.268 10.340 M4.5 V 32.1 407 142742.1−003851 216.925761 −0.647571 −27.5 −37.1 15.320 11.358 10.510 M4.0 V 41.0 408 142812.6+160429 217.052745 16.074889 −38.8 +33.1 15.065 11.013 10.143 M4.0 V 35.0 409 143011.6−073139 217.548396 −7.527766 −195.6 +165.9 15.107 11.184 10.370 M4.0 V 37.8 410 143110.2−212858 217.792665 −21.482798 +121.3 −26.6 16.015 11.423 10.532 M5.0 V 27.5 411 143202.4−103321 218.010270 −10.556039 −158.6 −15.2 15.608 11.489 10.604 M4.5 V 35.5 412 143204.8−332626 218.020320 −33.440672 +166.3 −86.7 14.515 10.371 9.534 M4.5 V 21.2 413 143743.1+261656 219.429894 26.282294 −21.3 −143.0 15.494 11.406 10.474 M4.0 V 41.9 414 143856.8−092801 219.736785 −9.467033 −106.9 −42.9 15.250 11.026 10.162 M4.5 V 28.7 415 143915.2−352711 219.813537 −35.453274 −35.7 −32.4 15.402 11.388 10.583 M4.0 V 41.6 416 144109.1−272717 220.288245 −27.454868 +13.4 −7.8 15.205 11.275 10.442 M4.0 V 39.5 417 144126.0+244150 220.358650 24.697308 +60.1 −20.8 15.386 11.466 10.654 M4.0 V 43.1 418 144414.7−365755 221.061488 −36.965306 −8.5 +9.1 14.926 10.937 10.056 M4.0 V 33.8 419 144456.2+235103 221.234227 23.851013 +67.6 −71.9 15.140 11.021 10.183 M4.5 V 28.6 420 144507.1−352634 221.279730 −35.442787 −130.8 −13.3 15.673 11.419 10.493 M4.5 V 34.4 421 144509.3−331338 221.288767 −33.227433 −20.4 −27.2 15.620 11.449 10.609 M4.5 V 34.8 422 144557.5+145812 221.489640 14.970105 −38.3 −37.2 15.595 11.383 10.542 M4.5 V 33.8 423 144624.4+150201 221.601930 15.033698 −51.0 +42.6 15.267 11.364 10.490 M4.0 V 41.1 424 144625.5−373027 221.606480 −37.507681 −39.8 +41.8 15.251 11.281 10.373 M4.0 V 39.6 425 144644.2−365905 221.684325 −36.984740 −11.9 −21.4 15.387 11.430 10.520 M4.0 V 42.4 426 144713.8−321739 221.807526 −32.294236 +596.3 −478.5 15.649 11.487 10.587 M4.5 V 35.5 427 144738.1+035309 221.908914 3.886045 +12.0 −53.2 16.025 11.480 10.611 M5.0 V 28.3 428 144739.2+011634 221.913689 1.276251 −135.2 +7.9 15.168 11.113 10.255 M4.0 V 36.6 429 145232.8−094547 223.136845 −9.763270 −249.5 −199.0 15.617 11.325 10.508 M4.5 V 32.9 430 145313.2+155254 223.305352 15.881778 +4.0 −95.2 15.161 11.240 10.395 M4.0 V 38.8

36 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

431 145536.1−033223 223.900668 −3.539994 −334.0 +68.7 15.196 11.067 10.214 M4.5 V 29.2 432 145937.7−230645 224.907192 −23.112741 −66.6 −75.8 15.669 11.495 10.609 M4.5 V 35.6 433 150113.5−093326 225.306343 −9.557320 −90.1 −89.8 15.515 11.195 10.340 M4.5 V 31.0 434 150455.8−261329 226.232620 −26.224777 −29.1 −32.7 15.545 11.485 10.620 M4.0 V 43.5 435 150516.9−381412 226.320446 −38.236748 −52.7 −11.4 14.838 10.866 9.968 M4.0 V 32.7 436 150731.9−125059 226.882966 −12.849841 −108.8 −5.1 15.851 11.475 10.592 M4.5 V 35.3 437 150744.3−022541 226.934892 −2.428311 +47.8 −40.0 14.600 10.697 9.891 M4.0 V 30.2 438 150950.9+150250 227.462126 15.047394 −35.4 −97.8 16.435 11.450 10.525 M5.5 V 21.9 439 151239.6−163101 228.165320 −16.517036 −108.8 −15.1 14.803 10.793 9.880 M4.0 V 31.6 440 151250.7−390119 228.211486 −39.021954 −83.6 −112.9 14.550 10.351 9.422 M4.5 V 21.0 441 151355.4−394114 228.481247 −39.687272 −75.9 −100.8 15.252 10.491 9.587 M5.0 V 17.9 442 151412.0−374406 228.550305 −37.735131 −19.2 −22.6 15.434 11.325 10.489 M4.0 V 40.4 443 151534.7−252701 228.894895 −25.450461 −25.6 −31.3 15.649 11.230 10.358 M4.5 V 31.5 444 151602.2−323202 229.009216 −32.534153 −13.9 −11.0 15.356 11.427 10.547 M4.0 V 42.3 445 151607.9−242008 229.032988 −24.335621 −25.2 −27.4 14.982 10.952 10.027 M4.0 V 34.0 446 151634.8−350030 229.145345 −35.008365 −18.1 −28.7 14.908 10.983 10.108 M4.0 V 34.5 447 151750.6+114335 229.461005 11.726459 −27.1 −21.9 15.402 11.387 10.507 M4.0 V 41.5 448 151945.6−022359 229.940033 −2.399934 +51.2 −149.6 15.659 11.350 10.511 M4.5 V 33.3 449 152012.7−355925 230.053122 −35.990471 +64.1 −239.0 16.523 11.472 10.639 M5.5 V 22.1 450 152045.4−075614 230.189264 −7.937260 −69.3 −70.9 14.481 10.346 9.435 M4.5 V 21.0 451 152229.6−230938 230.623548 −23.160749 −20.5 −26.3 15.347 11.354 10.431 M4.0 V 40.9 452 152448.3−311908 231.201421 −31.318930 −23.6 −27.7 15.657 11.456 10.610 M4.5 V 34.9 453 152452.4+284701 231.218570 28.783760 +11.1 +6.3 15.519 11.473 10.610 M4.0 V 43.2 454 152502.3+060443 231.259713 6.078775 +60.5 −24.1 14.969 11.050 10.192 M4.0 V 35.6 455 152559.7+114607 231.499075 11.768828 −136.6 −40.6 15.223 11.242 10.413 M4.0 V 38.9 456 152623.3+330529 231.597402 33.091575 −116.2 −69.4 15.915 11.383 10.520 M5.0 V 27.0 457 152726.4−334356 231.860179 −33.732308 −19.0 −33.3 15.389 11.385 10.504 M4.0 V 41.5 458 152732.4−023623 231.885139 −2.606485 +47.4 −5.6 15.404 11.394 10.523 M4.0 V 41.7 459 152756.4−193750 231.985047 −19.630679 +9.2 −3.1 15.474 11.375 10.471 M4.0 V 41.3 460 152806.3−325801 232.026497 −32.966964 −28.2 −24.0 15.456 11.330 10.499 M4.5 V 33.0 461 152809.0−125847 232.037784 −12.979782 −28.7 −24.4 15.351 10.921 10.042 M4.5 V 27.3 462 152817.8−211751 232.074503 −21.297696 +260.6 −248.4 15.688 11.487 10.630 M4.5 V 35.5 463 152857.5−371427 232.239904 −37.240904 +82.1 −129.2 15.097 11.167 10.321 M4.0 V 37.5 464 153013.7−140144 232.557286 −14.028960 −46.3 −8.5 16.178 11.243 10.396 M5.5 V 19.9 465 153021.8−135846 232.590995 −13.979665 −163.0 −385.8 15.389 11.445 10.576 M4.0 V 42.7 466 153109.3−165430 232.788754 −16.908592 −17.6 −33.0 16.005 11.223 10.371 M5.0 V 25.1 467 153116.7+344126 232.819720 34.690684 −101.3 +39.8 14.640 10.732 9.881 M4.0 V 30.7 468 153122.1−031900 232.842364 −3.316854 −103.4 +17.9 14.966 11.033 10.199 M4.0 V 35.3 469 153139.0−104244 232.912756 −10.712242 +127.8 −16.6 15.116 11.156 10.334 M4.0 V 37.4 470 153140.8+021042 232.920411 2.178397 +14.6 −529.2 15.680 11.427 10.523 M4.5 V 34.5 471 153159.7−351755 232.998753 −35.298726 +16.6 −127.3 15.470 11.337 10.474 M4.5 V 33.1 472 153258.1−044534 233.242408 −4.759701 −20.0 −16.2 16.098 11.311 10.418 M5.0 V 26.2 473 153307.1−092507 233.279663 −9.418887 −75.7 −72.3 15.068 11.129 10.325 M4.0 V 36.9 474 153348.6−291126 233.452500 −29.190765 +8.3 −60.2 16.344 11.105 10.272 M5.5 V 18.7 475 153444.6−280026 233.686218 −28.007253 −37.2 −41.9 14.260 10.332 9.422 M4.0 V 25.6 476 153454.8−072143 233.728474 −7.362144 +1.4 −14.6 15.097 10.862 9.988 M4.5 V 26.6 477 153510.7−384130 233.794599 −38.691681 −18.1 −27.0 14.999 11.087 10.222 M4.0 V 36.2 478 153546.3−341317 233.943333 −34.221503 −17.5 −18.7 15.471 11.456 10.630 M4.0 V 42.9

37 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

479 153654.4−292857 234.226860 −29.482671 −78.8 −23.7 15.528 11.427 10.566 M4.0 V 42.3 480 153758.2+054724 234.492884 5.790197 +3.9 −68.0 15.874 11.436 10.585 M4.5 V 34.6 481 153830.8−314458 234.628379 −31.749488 −23.1 −27.1 15.632 11.457 10.520 M4.5 V 35.0 482 153845.2+380413 234.688581 38.070438 −70.7 −14.8 15.376 11.408 10.557 M4.0 V 41.9 483 154007.7+103318 235.032164 10.555094 −0.4 −141.3 15.266 10.999 10.107 M4.5 V 28.3 484 154018.0−041211 235.075225 −4.203163 −16.8 −20.9 15.808 11.439 10.551 M4.5 V 34.7 485 154316.1−251902 235.817183 −25.317430 −8.6 −20.4 16.053 11.344 10.454 M5.0 V 26.6 486 154541.8−051531 236.424435 −5.258766 −15.8 −25.4 14.562 10.501 9.599 M4.0 V 27.6 487 154609.7−344828 236.540590 −34.807847 −64.3 +60.0 15.283 11.321 10.437 M4.0 V 40.3 488 154707.7+153409 236.782214 15.569352 −68.2 −28.9 15.592 11.467 10.589 M4.5 V 35.1 489 154734.9−275342 236.895674 −27.895163 +102.8 +7.0 16.010 11.217 10.346 M5.0 V 25.1 490 154736.7−312642 236.902963 −31.445083 −38.7 −51.0 15.034 11.023 10.083 M4.0 V 35.1 491 154833.6+080302 237.140095 8.050729 −5.0 −111.9 15.404 11.123 10.215 M4.5 V 30.0 492 154910.6−352307 237.294439 −35.385380 −18.6 −28.2 16.670 11.383 10.414 M5.5 V 21.2 493 154919.7−225729 237.332289 −22.958251 −12.8 −30.3 14.824 10.534 9.536 M4.5 V 22.9 494 155105.4−285623 237.772565 −28.939854 −15.6 −25.8 15.376 11.227 10.344 M4.5 V 31.5 495 155233.4−231119 238.139415 −23.188724 −25.5 −13.1 15.322 11.231 10.297 M4.0 V 38.7 496 155358.7−231543 238.494923 −23.262172 −10.9 −17.0 15.511 11.070 10.086 M4.5 V 29.3 497 155443.7+001422 238.682249 0.239630 −76.3 −83.7 15.281 11.113 10.302 M4.5 V 29.8 498 155450.4−052147 238.710041 −5.363172 +145.7 −119.9 14.387 10.327 9.378 M4.0 V 25.5 499 155500.2−234508 238.751016 −23.752396 −37.2 −39.1 14.984 10.815 9.922 M4.5 V 26.0 500 155501.9−275453 238.758144 −27.914793 −18.1 −26.5 15.047 11.112 10.240 M4.0 V 36.6 501 155518.9+314650 238.828874 31.780804 −45.6 +26.2 15.225 11.294 10.421 M4.0 V 39.8 502 155556.6−371615 238.985972 −37.270898 −9.9 −25.8 15.343 11.382 10.525 M4.0 V 41.5 503 155603.4−364355 239.014214 −36.732111 −30.0 −40.4 14.527 10.448 9.633 M4.0 V 27.0 504 155612.1−235407 239.050671 −23.902161 −19.7 −28.8 15.383 11.128 10.230 M4.5 V 30.0 505 155625.1−201615 239.104605 −20.271101 −13.4 −24.1 15.694 10.820 9.857 M5.5 V 16.4 506 155625.2−262828 239.105208 −26.474639 −27.6 −32.9 15.289 11.244 10.336 M4.0 V 38.9 507 155701.0−150115 239.254190 −15.021038 +25.3 −18.9 14.925 10.700 9.818 M4.5 V 24.7 508 155703.6−230448 239.265362 −23.080155 −12.1 −22.8 15.508 11.145 10.213 M4.5 V 30.3 509 155711.6−362801 239.298614 −36.467177 −20.8 −45.4 15.625 11.416 10.604 M4.5 V 34.3 510 155749.3+124516 239.455532 12.754595 −19.9 +8.9 15.336 11.311 10.426 M4.0 V 40.1 511 155758.3−340548 239.492998 −34.096919 −144.8 −52.4 15.140 11.234 10.392 M4.0 V 38.7 512 155803.1−343305 239.512957 −34.551461 +9.5 −26.8 15.123 10.951 10.029 M4.5 V 27.7 513 155924.1−211631 239.850619 −21.275481 −15.8 −29.5 15.473 11.323 10.358 M4.5 V 32.9 514 155938.0−260323 239.908624 −26.056565 −72.2 −10.0 15.582 11.142 10.246 M4.5 V 30.2 515 160357.6−175510 240.990094 −17.919564 −2.6 −14.3 15.634 11.435 10.457 M4.5 V 34.6 516 160424.4−364618 241.101780 −36.771940 −25.9 −22.4 15.720 11.346 10.501 M4.5 V 33.2 517 160607.2−022052 241.530128 −2.347796 −173.4 +205.8 14.880 10.837 9.977 M4.0 V 32.3 518 160616.4−361800 241.568670 −36.300042 −1.9 −62.9 15.179 11.031 10.140 M4.5 V 28.7 519 160638.0−272755 241.658473 −27.465414 −8.4 −13.7 14.705 10.708 9.758 M4.0 V 30.4 520 160734.9−273616 241.895668 −27.604638 −14.7 −22.7 15.436 11.400 10.446 M4.0 V 41.8 521 160758.5−062108 241.993768 −6.352357 −211.0 +45.2 15.678 11.448 10.513 M4.5 V 34.8 522 160826.9+171843 242.112138 17.312193 +33.6 −27.2 15.768 11.448 10.576 M4.5 V 34.8 523 160838.6+253452 242.161041 25.581184 −65.9 −82.7 15.287 11.245 10.433 M4.0 V 38.9 524 160842.5−273330 242.177308 −27.558413 −25.7 −28.6 15.288 11.297 10.419 M4.0 V 39.9 525 160849.8+002455 242.207729 0.415410 −94.7 +16.4 15.402 11.325 10.475 M4.0 V 40.4 526 160856.9−283557 242.237290 −28.599321 −14.6 −23.2 14.638 10.560 9.632 M4.0 V 28.4

38 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

527 160905.2−080946 242.271935 −8.163008 −111.2 −34.7 14.836 10.345 9.386 M5.0 V 16.8 528 160920.6−222205 242.335972 −22.368285 −8.9 −23.3 15.290 10.498 9.499 M5.0 V 18.0 529 160931.0−204146 242.379549 −20.696133 −18.5 −25.7 15.861 11.129 10.138 M5.0 V 24.1 530 161003.1−272839 242.512967 −27.477691 −11.1 −23.5 14.812 10.773 9.837 M4.0 V 31.3 531 161009.5−194720 242.539611 −19.789078 −10.8 −28.1 15.878 11.446 10.490 M4.5 V 34.8 532 161014.4−195137 242.560215 −19.860466 −12.6 −29.4 15.251 11.214 10.234 M4.0 V 38.4 533 161133.7−202736 242.890674 −20.460152 −15.5 −23.8 15.120 11.214 10.217 M4.0 V 38.4 534 161208.1−254758 243.033905 −25.799473 −16.4 −33.5 15.219 11.304 10.312 M4.0 V 40.0 535 161212.3+380320 243.051441 38.055814 −223.4 +24.8 15.224 11.104 10.211 M4.5 V 29.7 536 161317.8−371819 243.324167 −37.305349 +1.2 +10.4 15.057 11.119 10.254 M4.0 V 36.7 537 161318.8−274402 243.328723 −27.734101 −9.8 −31.1 14.482 10.492 9.623 M4.0 V 27.5 538 161320.8−175752 243.336702 −17.964508 +10.7 −27.2 14.964 10.816 9.871 M4.5 V 26.0 539 161321.2−175748 243.338481 −17.963576 +5.7 −19.8 14.983 11.010 10.045 M4.0 V 34.9 540 161324.5−272613 243.352393 −27.437004 −16.4 −34.3 14.736 10.687 9.780 M4.0 V 30.1 541 161335.2+011558 243.396920 1.266125 +49.0 +4.4 15.340 11.294 10.362 M4.0 V 39.8 542 161356.6−245756 243.485946 −24.965814 −15.2 −21.6 15.071 11.142 10.150 M4.0 V 37.1 543 161455.1−301453 243.729760 −30.248194 −11.1 −11.2 14.343 10.408 9.523 M4.0 V 26.5 544 161500.1−300823 243.750518 −30.139935 −8.5 −52.2 15.695 11.477 10.574 M4.5 V 35.3 545 161555.6−124624 243.981984 −12.773342 −171.7 +0.4 15.614 11.245 10.346 M4.5 V 31.7 546 161556.6−211218 243.986147 −21.205124 −12.8 −26.2 15.937 11.366 10.397 M5.0 V 26.8 547 161658.8−313638 244.245317 −31.610678 −129.8 −99.0 13.394 9.329 8.475 M4.0 V 16.1 548 161703.3−214102 244.264042 −21.684039 −22.4 −23.8 15.967 10.971 10.047 M5.5 V 17.6 549 161709.4−004842 244.289380 −0.811933 −50.3 −90.7 14.777 10.783 9.891 M4.0 V 31.5 550 161721.7−214438 244.340727 −21.743989 −7.5 −21.8 15.375 11.209 10.259 M4.5 V 31.2 551 161829.1−303911 244.621568 −30.653130 −9.5 −24.4 15.281 10.898 10.011 M4.5 V 27.0 552 161841.8−183239 244.674523 −18.544436 −15.7 −35.2 15.175 11.023 10.082 M4.5 V 28.6 553 161852.7−225954 244.719943 −22.998349 −7.1 −22.1 15.265 11.101 10.103 M4.5 V 29.7 554 161854.1+263743 244.725762 26.628755 +94.4 −32.4 15.382 11.365 10.504 M4.0 V 41.1 555 161902.1−213809 244.758920 −21.636096 −13.2 −27.2 15.238 11.324 10.402 M4.0 V 40.4 556 161926.6−282007 244.861167 −28.335472 −11.2 −33.4 14.719 10.774 9.876 M4.0 V 31.3 557 161926.9−122221 244.862188 −12.372726 −1.5 −20.7 14.666 10.716 9.763 M4.0 V 30.5 558 161934.4−315005 244.893720 −31.834866 −17.5 −27.3 15.077 11.076 10.162 M4.0 V 36.0 559 161947.1−220311 244.946259 −22.053125 −11.0 −31.2 15.766 11.491 10.545 M4.5 V 35.5 560 161948.3−221251 244.951524 −22.214409 −16.3 −28.7 15.174 11.273 10.321 M4.0 V 39.4 561 161955.0−150616 244.979365 −15.104481 −40.5 −17.5 14.772 10.864 10.014 M4.0 V 32.7 562 162027.5−271739 245.114957 −27.294236 −16.7 −23.3 15.288 11.164 10.234 M4.5 V 30.6 563 162027.6−210017 245.115134 −21.004894 −12.0 +3.5 15.036 10.887 9.947 M4.5 V 26.9 564 162036.4−212312 245.151668 −21.386708 −14.9 −28.0 15.308 10.942 10.016 M4.5 V 27.6 565 162118.2−194518 245.326248 −19.755174 −15.8 −27.6 15.167 11.213 10.333 M4.0 V 38.3 566 162155.0−215204 245.479442 −21.867890 −15.9 −18.9 15.452 11.372 10.402 M4.0 V 41.3 567 162206.5−212709 245.527408 −21.452507 −16.3 −25.4 15.010 11.107 10.129 M4.0 V 36.5 568 162229.7−151513 245.624064 −15.253673 −10.1 −24.0 15.270 11.361 10.430 M4.0 V 41.1 569 162247.2−323149 245.697005 −32.530551 +3.0 −21.1 15.319 11.375 10.512 M4.0 V 41.3 570 162321.6−214644 245.840185 −21.779086 −151.4 −147.5 15.285 10.791 9.866 M5.0 V 20.6 571 162329.3+000041 245.872192 0.011449 −110.3 −89.7 15.215 11.139 10.249 M4.0 V 37.1 572 162343.3+164839 245.930829 16.811098 −81.8 −59.3 15.020 11.031 10.230 M4.0 V 35.3 573 162416.4−321213 246.068419 −32.203637 −16.9 −168.7 13.321 9.150 8.154 M4.5 V 12.1 574 162555.4−272124 246.480872 −27.356751 −7.4 −33.1 15.060 10.857 9.975 M4.5 V 26.5

39 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

575 162627.8−262515 246.616093 −26.420926 −14.6 −25.2 14.932 10.841 9.845 M4.0 V 32.3 576 162632.7−262259 246.636497 −26.383066 −18.6 −27.0 16.685 11.452 10.490 M5.5 V 21.9 577 162639.9−051409 246.666408 −5.235908 −47.9 +0.0 15.493 11.440 10.573 M4.0 V 42.6 578 162853.1−204452 247.221606 −20.747966 −18.2 −22.9 14.545 10.572 9.576 M4.0 V 28.5 579 162908.7−253424 247.286426 −25.573338 −18.7 −29.8 15.123 11.021 10.132 M4.0 V 35.1 580 162933.7−333219 247.390517 −33.538642 −31.0 −43.4 15.807 11.415 10.537 M4.5 V 34.3 581 162956.6−265918 247.485960 −26.988487 −19.4 −25.1 15.512 11.393 10.437 M4.5 V 33.9 582 163018.3−312222 247.576633 −31.372788 −36.7 +12.7 15.937 11.449 10.573 M5.0 V 27.9 583 163051.3+472643 247.714060 47.445484 −56.4 +7.2 14.898 10.944 10.078 M4.0 V 33.9 584 163105.7−272546 247.774135 −27.429512 −9.3 −24.2 15.597 11.461 10.527 M4.5 V 35.0 585 163151.3−271338 247.964149 −27.227434 −19.6 −32.2 15.372 11.396 10.525 M4.0 V 41.7 586 163156.6−284612 247.986146 −28.770246 −11.9 −21.6 15.497 11.430 10.495 M4.0 V 42.4 587 163411.1−250737 248.546478 −25.127127 −3.6 −24.9 16.111 10.878 9.968 M5.5 V 16.8 588 163431.3−061831 248.630503 −6.308740 +56.7 −16.1 14.857 10.935 10.100 M4.0 V 33.7 589 163435.1−265803 248.646389 −26.967563 −10.0 −19.7 16.053 11.467 10.477 M5.0 V 28.1 590 163458.0−225720 248.741873 −22.955792 −17.2 −31.9 15.456 11.296 10.349 M4.5 V 32.5 591 163654.8−145909 249.228560 −14.986014 −1.6 −25.5 15.132 10.771 9.840 M4.5 V 25.5 592 163716.3+220012 249.318263 22.003529 +298.1 −49.6 15.157 11.237 10.395 M4.0 V 38.8 593 163721.3+150356 249.339075 15.065723 −39.8 +52.8 15.420 11.376 10.477 M4.0 V 41.3 594 163856.3+243559 249.734806 24.599775 +116.1 +44.5 15.426 11.348 10.474 M4.0 V 40.8 595 163941.6+104958 249.923402 10.832959 +4.8 −19.6 14.481 10.475 9.608 M4.0 V 27.3 596 164009.1−303655 250.038295 −30.615532 −7.2 −34.1 15.150 11.248 10.382 M4.0 V 39.0 597 164049.9−261653 250.208039 −26.281566 +3.5 −34.0 16.694 11.282 10.386 M6.0 V 15.6 598 164109.9−225444 250.291400 −22.912362 +207.6 −793.2 15.182 11.157 10.317 M4.0 V 37.4 599 164153.9−294943 250.474606 −29.828622 −22.8 −36.4 15.412 11.447 10.605 M4.0 V 42.7 600 164220.2−293903 250.584535 −29.650851 −6.5 −31.4 15.450 11.493 10.675 M4.0 V 43.6 601 164226.9−294116 250.612410 −29.687814 −6.1 −26.6 15.448 11.207 10.332 M4.5 V 31.2 602 164410.4+144307 251.043737 14.718695 −48.7 −54.2 15.474 11.235 10.379 M4.5 V 31.6 603 164420.5+011526 251.085717 1.257428 −25.3 +34.6 15.506 11.374 10.529 M4.5 V 33.7 604 164528.9−250247 251.370667 −25.046570 −7.4 −26.7 15.383 11.214 10.274 M4.5 V 31.3 605 164603.7−182656 251.515685 −18.449126 −7.9 −34.1 15.988 11.188 10.218 M5.0 V 24.7 606 164627.1−182441 251.613305 −18.411552 −115.9 −85.8 15.445 11.407 10.529 M4.0 V 41.9 607 164745.2−152642 251.938548 −15.445246 −11.8 −14.9 15.748 11.079 10.119 M5.0 V 23.5 608 164929.9−015503 252.374660 −1.917569 −68.4 −32.4 15.311 11.258 10.396 M4.0 V 39.1 609 164935.5−001409 252.398026 −0.236093 −9.9 −39.4 15.175 11.182 10.334 M4.0 V 37.8 610 164954.7−104444 252.478036 −10.745772 +95.0 −91.2 14.863 10.945 10.035 M4.0 V 33.9 611 165003.8−282352 252.516220 −28.397889 −7.9 −32.8 15.229 11.258 10.389 M4.0 V 39.1 612 165040.6+304543 252.669252 30.762017 +98.8 −75.2 15.919 11.331 10.434 M5.0 V 26.4 613 165042.7−111757 252.678155 −11.299438 +26.3 −268.7 15.244 11.333 10.464 M4.0 V 40.5 614 165351.3+120527 253.463908 12.090911 −3.8 −4.9 16.187 11.155 10.329 M5.5 V 19.1 615 165558.7−062552 253.994709 −6.431138 +44.7 +42.3 15.530 11.375 10.549 M4.5 V 33.7 616 165815.5−184500 254.564603 −18.750225 −3.3 −24.9 16.020 11.425 10.543 M5.0 V 27.6 617 170042.1−092535 255.175695 −9.426627 −235.0 −220.0 14.899 10.793 9.871 M4.0 V 31.6 618 170127.8−202454 255.366243 −20.415168 −21.0 −24.1 15.209 11.012 10.175 M4.5 V 28.5 619 170229.5+134101 255.622935 13.683805 +0.3 +88.7 16.108 11.398 10.493 M5.0 V 27.2 620 170324.5−022723 255.852280 −2.456636 −41.1 +15.0 15.324 11.332 10.496 M4.0 V 40.5 621 170604.9−213217 256.520560 −21.538272 +160.0 +167.8 15.798 11.421 10.531 M4.5 V 34.4 622 170849.0+194309 257.204406 19.719354 −62.2 +48.7 15.013 11.043 10.186 M4.0 V 35.5

40 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

623 171458.7−020850 258.744923 −2.147431 −79.4 +128.2 15.448 11.478 10.623 M4.0 V 43.3 624 171616.8−091200 259.070123 −9.200109 −33.7 −5.4 15.204 11.274 10.414 M4.0 V 39.4 625 171640.4−130335 259.168475 −13.059816 −79.6 −103.1 14.956 10.958 10.030 M4.0 V 34.1 626 172130.7−150617 260.378009 −15.104926 −14.8 −42.8 15.191 11.263 10.424 M4.0 V 39.2 627 172251.3−153539 260.713928 −15.594433 −4.6 −25.2 14.753 10.685 9.821 M4.0 V 30.1 628 172330.3+371601 260.876373 37.267099 −139.1 +38.0 15.444 11.498 10.643 M4.0 V 43.7 629 172537.6+204725 261.406939 20.790309 −20.1 +88.9 15.623 11.362 10.474 M4.5 V 33.5 630 172904.2+412225 262.267892 41.373791 −116.9 −31.1 15.757 11.166 10.304 M5.0 V 24.5 631 172932.7+093107 262.386382 9.518868 −22.9 −40.9 15.065 10.937 10.096 M4.5 V 27.5 632 172951.3+093337 262.464150 9.560368 −23.1 −41.1 14.352 10.414 9.471 M4.0 V 26.5 633 173103.7+142913 262.765665 14.486983 −3.3 +42.2 15.604 11.266 10.396 M4.5 V 32.0 634 173107.2−023918 262.780220 −2.655036 −48.1 −17.2 14.323 10.315 9.420 M4.0 V 25.4 635 173645.4+050856 264.189527 5.149159 −6.1 −27.9 15.481 11.210 10.368 M4.5 V 31.2 636 173803.7+125321 264.515617 12.889334 +18.3 +76.9 14.791 10.756 9.858 M4.0 V 31.1 637 174105.6+301355 265.273663 30.232106 −42.8 +74.7 15.175 11.243 10.360 M4.0 V 38.9 638 174148.8+150156 265.453440 15.032379 +54.1 −373.3 15.096 10.873 10.028 M4.5 V 26.7 639 174225.8−001135 265.607592 −0.193104 +110.0 −197.6 15.720 11.410 10.486 M4.5 V 34.2 640 174225.8−001137 265.607865 −0.193611 +110.0 −197.6 15.367 11.410 10.486 M4.0 V 42.0 641 174250.3−071102 265.709930 −7.183927 +39.9 −23.2 15.467 11.304 10.451 M4.5 V 32.6 642 174549.1+100449 266.454798 10.080409 +99.0 +3.1 15.458 11.484 10.624 M4.0 V 43.4 643 174814.3+133747 267.059614 13.629873 −63.5 −85.3 14.779 10.334 9.458 M4.5 V 20.8 644 174919.2+475605 267.330218 47.934815 −408.7 +86.5 16.438 11.214 10.285 M5.5 V 19.7 645 175156.2+014220 267.984409 1.705564 −9.1 −1.5 15.168 10.997 10.164 M4.5 V 28.3 646 180113.4+094837 270.306047 9.810524 −13.4 −39.5 14.286 10.294 9.369 M4.0 V 25.1 647 180309.1+195907 270.788256 19.985379 −11.2 +83.9 14.604 10.655 9.758 M4.0 V 29.7 648 180422.4+094840 271.093732 9.811386 +36.8 +21.9 15.491 11.263 10.369 M4.5 V 32.0 649 181024.2+412545 272.600882 41.429216 −105.8 +53.7 15.064 11.132 10.185 M4.0 V 36.9 650 181037.0+075609 272.654525 7.936084 −94.1 −45.2 14.980 11.012 10.127 M4.0 V 35.0 651 181636.3+063857 274.151450 6.649169 +16.4 −11.7 15.673 11.069 10.216 M5.0 V 23.4 652 182001.9+162556 275.008117 16.432288 −125.8 −48.6 16.381 11.450 10.531 M5.5 V 21.9 653 182856.2+345639 277.234514 34.944307 −20.9 −9.8 14.743 10.665 9.792 M4.0 V 29.8 654 182917.5+240842 277.323172 24.145190 +15.2 +89.3 14.777 10.858 9.981 M4.0 V 32.6 655 183001.3−372648 277.505499 −37.446867 −10.2 −42.9 15.407 11.344 10.455 M4.0 V 40.7 656 183013.1−323822 277.554870 −32.639491 +55.5 −34.6 15.680 11.443 10.596 M4.5 V 34.7 657 183547.5+202939 278.948249 20.494421 +47.1 −36.5 15.851 11.489 10.649 M4.5 V 35.5 658 183801.5+341806 279.506315 34.301712 +59.5 +72.3 16.561 11.419 10.526 M5.5 V 21.6 659 184032.4−401058 280.135392 −40.182925 −111.8 −167.1 15.028 11.028 10.154 M4.0 V 35.2 660 184150.9−294130 280.462222 −29.691846 +12.4 −61.7 14.537 10.620 9.718 M4.0 V 29.2 661 184245.2+255129 280.688375 25.858293 −10.4 −16.3 15.470 11.389 10.536 M4.0 V 41.6 662 184249.7−321247 280.707251 −32.213058 −673.3 −498.6 13.451 9.544 8.679 M4.0 V 17.8 663 184251.4−360729 280.714227 −36.124927 −2.3 −15.5 15.188 11.255 10.394 M4.0 V 39.1 664 184610.8+333305 281.545105 33.551627 +88.2 +79.3 15.079 10.989 10.104 M4.0 V 34.6 665 184813.1−371248 282.054735 −37.213552 +17.7 −17.2 14.987 11.049 10.197 M4.0 V 35.6 666 185409.2−262139 283.538435 −26.361054 +3.9 −52.0 15.690 11.441 10.628 M4.5 V 34.7 667 185523.2−240031 283.847062 −24.008813 +42.8 −44.5 15.797 11.312 10.440 M5.0 V 26.2 668 185933.3+341614 284.889044 34.270817 −1.5 −5.6 14.727 10.700 9.848 M4.0 V 30.3 669 185955.9+432359 284.982935 43.399788 +351.4 +396.6 14.749 10.727 9.831 M4.0 V 30.7 670 190047.2−364747 285.197076 −36.796430 −12.9 −12.8 15.901 11.373 10.391 M5.0 V 26.9

41 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

671 190105.0+305716 285.270972 30.954685 −6.5 −12.1 13.062 9.023 8.041 M4.0 V 14.0 672 190206.3−242119 285.526303 −24.355290 +37.7 −75.9 15.703 11.335 10.448 M4.5 V 33.1 673 190259.2−202239 285.746880 −20.377616 −96.5 +43.4 13.687 9.738 8.889 M4.0 V 19.4 674 190307.6−193955 285.782056 −19.665414 −14.2 −62.4 14.982 11.048 10.097 M4.0 V 35.5 675 190333.0−384706 285.887527 −38.785267 +39.8 −110.5 14.793 10.674 9.727 M4.5 V 24.4 676 190543.4−271125 286.431140 −27.190543 +15.0 −47.6 16.291 11.152 10.259 M5.5 V 19.1 677 190715.9−283429 286.816334 −28.574824 +4.3 −33.8 15.392 11.370 10.492 M4.0 V 41.2 678 190937.6+392326 287.407046 39.390634 +6.2 +129.7 15.351 11.328 10.433 M4.0 V 40.4 679 191045.5−131804 287.689898 −13.301131 +49.3 −93.1 14.601 10.614 9.794 M4.0 V 29.1 680 191202.7−193637 288.011481 −19.610335 +18.9 −43.5 15.494 11.415 10.505 M4.0 V 42.1 681 191226.5−182812 288.110573 −18.470018 +73.7 −85.0 15.455 11.317 10.455 M4.5 V 32.8 682 191500.8−284758 288.753354 −28.799677 +13.6 −54.3 15.367 10.856 9.961 M5.0 V 21.2 683 192004.7−371654 290.019934 −37.281674 +28.2 +21.3 15.616 11.446 10.543 M4.5 V 34.8 684 192118.6−323844 290.327755 −32.645606 +153.3 −47.4 14.744 10.506 9.638 M4.5 V 22.6 685 192250.4−241114 290.710014 −24.187495 +23.8 −212.0 14.966 10.875 10.027 M4.0 V 32.8 686 192325.1+393434 290.854954 39.576179 +16.3 −51.7 14.959 10.834 10.006 M4.5 V 26.2 687 192621.8+481457 291.591110 48.249355 −125.8 −39.1 15.502 11.427 10.597 M4.0 V 42.3 688 192656.5−252502 291.735518 −25.417395 −50.5 +5.8 15.610 11.400 10.532 M4.5 V 34.1 689 192820.8−362010 292.086736 −36.336289 +2.5 −15.8 15.974 11.169 10.290 M5.0 V 24.5 690 193358.2−073312 293.492693 −7.553596 +38.9 −24.6 15.267 11.261 10.391 M4.0 V 39.2 691 193620.0+354736 294.083602 35.793454 +156.5 +89.5 14.488 10.427 9.523 M4.0 V 26.7 692 193759.6−152647 294.498708 −15.446564 +62.9 −16.6 15.381 11.125 10.229 M4.5 V 30.0 693 194122.7−240243 295.344947 −24.045479 +43.9 −36.1 15.382 11.449 10.593 M4.0 V 42.7 694 194126.5−113740 295.360499 −11.627786 +109.8 −52.1 15.446 11.414 10.558 M4.0 V 42.1 695 194221.2−062024 295.588367 −6.340185 +59.8 −162.1 14.890 10.575 9.706 M4.5 V 23.3 696 194347.0−193956 295.946058 −19.665692 −120.8 −132.7 14.783 10.761 9.861 M4.0 V 31.1 697 194515.3−060222 296.313978 −6.039535 +159.1 −66.3 15.074 11.144 10.283 M4.0 V 37.1 698 194550.8−081504 296.461806 −8.251310 +4.1 −21.2 15.716 11.225 10.237 M5.0 V 25.1 699 194913.7+055306 297.307281 5.885146 +116.8 −2.1 14.555 10.651 9.799 M4.0 V 29.6 700 194934.4−130430 297.393589 −13.075168 +54.6 −25.9 14.600 10.620 9.761 M4.0 V 29.2 701 195157.6−282503 297.990358 −28.417684 +3.3 −116.8 15.405 11.484 10.652 M4.0 V 43.4 702 195311.7+375728 298.298829 37.957816 −7.2 −2.1 13.780 9.116 8.224 M5.0 V 9.5 703 195341.0−061310 298.420913 −6.219453 +173.8 +40.6 15.464 11.485 10.678 M4.0 V 43.5 704 195546.6−021237 298.944428 −2.210546 −193.4 +15.1 15.117 11.131 10.142 M4.0 V 36.9 705 200311.7−064214 300.798789 −6.703891 +36.0 +1.8 14.682 10.745 9.909 M4.0 V 30.9 706 200635.8−153307 301.649323 −15.552096 −142.1 −71.1 15.225 10.635 9.738 M5.0 V 19.2 707 200740.7−024047 301.919855 −2.679813 +11.1 −27.5 15.518 11.289 10.306 M4.5 V 32.4 708 200822.6−011432 302.094302 −1.242479 +21.7 +19.8 15.614 11.347 10.438 M4.5 V 33.2 709 200837.8−254526 302.157790 −25.757264 +37.3 −56.0 15.226 10.899 10.066 M4.5 V 27.0 710 201019.1−371855 302.579981 −37.315313 +26.8 −102.9 15.583 11.488 10.674 M4.0 V 43.5 711 201104.5+215210 302.768789 21.869689 −65.0 +10.3 15.580 11.181 10.278 M4.5 V 30.8 712 201225.1−244905 303.104853 −24.818229 −9.0 +33.1 15.197 11.163 10.321 M4.0 V 37.5 713 201243.6+441357 303.181980 44.232554 +39.8 +39.4 15.400 11.404 10.539 M4.0 V 41.9 714 201458.7−345505 303.744625 −34.918201 −138.1 +49.5 14.386 10.325 9.472 M4.0 V 25.5 715 201822.7+000507 304.594990 0.085508 +61.5 −114.0 16.370 11.387 10.447 M5.5 V 21.3 716 202120.3+413920 305.334857 41.655727 −3.0 −3.9 14.515 10.597 9.620 M4.0 V 28.9 717 202152.4−363521 305.468695 −36.589303 +63.2 −44.9 14.895 10.956 10.017 M4.0 V 34.1 718 202328.2+082802 305.867861 8.467379 +105.4 −4.1 15.537 11.492 10.685 M4.0 V 43.6

42 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

719 202331.9+392033 305.883222 39.342652 −26.7 +26.6 15.137 11.153 10.157 M4.0 V 37.3 720 202334.1+114217 305.892088 11.704907 +45.5 −139.6 14.984 10.937 10.135 M4.0 V 33.8 721 202433.7+410126 306.140646 41.024166 −4.0 −6.3 15.068 11.001 10.010 M4.0 V 34.8 722 202527.1−194803 306.363195 −19.800965 +42.2 −28.9 14.284 10.042 9.149 M4.5 V 18.2 723 202753.8+484510 306.974506 48.752963 +236.2 −5.0 15.026 11.037 10.189 M4.0 V 35.4 724 202839.9+275521 307.166523 27.922651 −4.5 −15.9 15.274 11.235 10.304 M4.0 V 38.7 725 202840.2−175035 307.167815 −17.843065 −14.3 −16.7 14.880 10.641 9.788 M4.5 V 24.0 726 202856.4−042040 307.235401 −4.344714 +193.4 +74.1 15.366 10.955 10.090 M4.5 V 27.7 727 203015.8+352821 307.566186 35.472511 −3.9 −10.4 15.259 11.320 10.327 M4.0 V 40.3 728 203034.8+411532 307.645002 41.259104 −0.3 −3.9 14.907 10.997 10.046 M4.0 V 34.7 729 203039.1+380823 307.663318 38.139734 −1.7 −3.4 15.070 11.135 10.155 M4.0 V 37.0 730 203114.3+260450 307.809681 26.080719 −86.6 +19.0 14.611 10.555 9.739 M4.0 V 28.3 731 203128.2+403256 307.867878 40.549035 −3.4 −4.0 14.820 10.506 9.508 M4.5 V 22.6 732 203129.7+411751 307.873923 41.297549 +0.2 −4.9 15.411 11.384 10.402 M4.0 V 41.5 733 203131.2+410111 307.880164 41.019948 +0.4 −0.5 13.656 9.714 8.804 M4.0 V 19.2 734 203135.5−280517 307.897955 −28.088123 +61.4 −19.3 14.949 10.988 10.097 M4.0 V 34.6 735 203142.1+404755 307.925684 40.798716 +109.8 +55.7 15.332 11.303 10.448 M4.0 V 40.0 736 203211.4+403220 308.047916 40.539025 −3.1 −1.3 15.204 10.885 9.888 M4.5 V 26.9 737 203213.8+410052 308.057719 41.014604 −1.1 −1.3 15.321 11.353 10.372 M4.0 V 40.9 738 203237.6+401249 308.156876 40.213662 −3.7 −4.0 15.212 11.231 10.290 M4.0 V 38.7 739 203240.3+415049 308.168027 41.847005 −2.5 −1.2 15.102 11.135 10.154 M4.0 V 37.0 740 203242.8+404135 308.178596 40.693239 +0.3 −0.7 14.849 10.643 9.682 M4.5 V 24.0 741 203244.8+405411 308.186714 40.903275 −2.0 −3.6 15.417 11.487 10.495 M4.0 V 43.5 742 203259.1+404755 308.246574 40.798644 −2.5 −3.4 15.234 11.206 10.240 M4.0 V 38.2 743 203301.0+405242 308.254282 40.878369 −4.9 −2.6 14.943 10.977 10.007 M4.0 V 34.4 744 203303.8+404519 308.265975 40.755500 −4.0 −0.5 15.001 10.971 10.082 M4.0 V 34.3 745 203306.2+404710 308.276169 40.786383 −0.6 −3.8 15.042 10.910 9.931 M4.5 V 27.2 746 203311.2+143017 308.296828 14.504965 −12.7 −50.3 15.343 11.062 10.167 M4.5 V 29.1 747 203336.6+403318 308.402540 40.555170 −0.1 −5.4 14.726 10.614 9.632 M4.5 V 23.7 748 203339.7+405714 308.415590 40.954091 −0.2 −3.1 15.378 11.469 10.557 M4.0 V 43.1 749 203409.1+411524 308.538212 41.256907 −1.0 −1.6 15.342 11.414 10.416 M4.0 V 42.1 750 203441.1+412934 308.671475 41.492859 −2.8 −1.3 15.294 11.084 10.099 M4.5 V 29.4 751 203454.8+412521 308.728596 41.422545 −1.5 −3.0 15.220 10.998 10.014 M4.5 V 28.3 752 203506.0+021816 308.775340 2.304620 −99.3 −29.8 14.413 10.279 9.371 M4.5 V 20.3 753 203508.6+404801 308.786205 40.800292 −0.7 −7.6 15.431 11.424 10.452 M4.0 V 42.3 754 203521.7+415143 308.840721 41.862000 +1.8 −3.8 14.501 10.483 9.494 M4.0 V 27.4 755 203532.7−312952 308.886341 −31.497809 −1.9 −129.7 15.562 11.346 10.371 M4.5 V 33.2 756 203558.6+275202 308.994222 27.867318 +35.5 −20.6 14.871 10.510 9.633 M4.5 V 22.6 757 203756.5+394010 309.485580 39.669627 −1.2 −6.8 14.971 10.939 9.947 M4.0 V 33.8 758 203907.1+245747 309.779952 24.963154 +6.7 −149.4 15.455 11.362 10.503 M4.0 V 41.1 759 203941.2−113603 309.921965 −11.601030 +101.5 −145.2 15.520 11.392 10.505 M4.5 V 33.9 760 203948.2+414706 309.951011 41.785226 −7.3 −4.7 14.462 10.481 9.511 M4.0 V 27.4 761 204002.4+405516 310.010348 40.921162 −0.5 −8.3 14.842 10.899 9.992 M4.0 V 33.2 762 204005.1−235504 310.021489 −23.918004 +9.8 −121.1 15.242 11.247 10.402 M4.0 V 39.0 763 204407.5−011551 311.031551 −1.264271 +137.6 −16.3 15.016 11.028 10.152 M4.0 V 35.2 764 204643.8+244205 311.682610 24.701622 +84.6 −8.3 15.312 10.978 10.158 M4.5 V 28.0 765 204727.9+014257 311.866516 1.716071 +109.8 +17.5 15.295 11.321 10.423 M4.0 V 40.3 766 204906.4−263927 312.276893 −26.657542 −22.3 −1.5 14.772 10.861 10.011 M4.0 V 32.6

43 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

767 204924.9+432746 312.353832 43.463022 +26.6 −52.8 15.784 11.095 10.154 M5.0 V 23.7 768 205023.0+253133 312.595845 25.526046 +1.5 −106.8 15.130 11.078 10.216 M4.0 V 36.0 769 205131.0−154857 312.879179 −15.815947 +24.5 −54.4 15.403 11.219 10.338 M4.5 V 31.3 770 205202.7+164359 313.011305 16.733215 +0.0 −33.0 15.152 11.135 10.216 M4.0 V 37.0 771 205431.8+005128 313.632902 0.857888 +62.2 −16.6 14.727 10.752 9.922 M4.0 V 31.0 772 205715.4+284153 314.314268 28.698058 +91.2 −123.4 14.820 10.542 9.685 M4.5 V 22.9 773 210229.9−073544 315.624843 −7.595655 +78.3 −126.5 15.519 11.362 10.506 M4.5 V 33.5 774 210702.8+363829 316.761688 36.641455 +0.6 −3.9 15.390 11.364 10.533 M4.0 V 41.1 775 210802.6+481654 317.011115 48.281938 −2.2 +4.7 15.220 11.299 10.305 M4.0 V 39.9 776 210935.4−151858 317.397531 −15.316224 +119.3 −198.4 15.622 11.476 10.598 M4.5 V 35.3 777 211047.1+271141 317.696300 27.194830 +41.6 −23.2 15.398 11.379 10.550 M4.0 V 41.4 778 211145.4+371003 317.939416 37.167577 −2.1 −83.9 15.034 11.017 10.162 M4.0 V 35.0 779 211546.2−130246 318.942767 −13.046228 +31.6 −60.7 15.433 11.099 10.234 M4.5 V 29.7 780 211637.2+464516 319.155172 46.754465 −7.7 +8.7 16.013 11.464 10.615 M5.0 V 28.1 781 211757.1+460130 319.488199 46.025097 +31.8 −44.8 13.698 9.673 8.807 M4.0 V 18.9 782 211905.3+452530 319.772269 45.425215 −119.8 −67.7 15.504 11.209 10.297 M4.5 V 31.2 783 211929.6+023115 319.873673 2.520866 +127.8 +52.1 15.027 10.984 10.105 M4.0 V 34.5 784 212230.5−333855 320.627318 −33.648629 +31.9 −89.4 14.758 10.455 9.566 M4.5 V 22.0 785 212610.2+280856 321.542517 28.148976 +80.7 +5.0 15.186 11.246 10.347 M4.0 V 38.9 786 213249.5−300849 323.206666 −30.147073 −30.8 +1.4 14.848 10.869 9.968 M4.0 V 32.7 787 213428.2−184029 323.617518 −18.674969 +83.1 −13.9 14.990 11.041 10.156 M4.0 V 35.4 788 213502.8−301347 323.761805 −30.229986 +26.5 −0.9 15.664 11.485 10.636 M4.5 V 35.4 789 213739.4+365941 324.414319 36.994945 +9.2 −17.8 15.719 11.478 10.541 M4.5 V 35.3 790 213847.5+050451 324.698185 5.081033 +52.8 −42.9 14.684 10.721 9.872 M4.0 V 30.6 791 213901.7+070034 324.757475 7.009516 +74.2 −51.3 15.296 11.264 10.373 M4.0 V 39.3 792 214219.1+104129 325.579874 10.691643 +78.4 −93.3 15.020 10.912 10.026 M4.0 V 33.4 793 214504.9+020821 326.270529 2.139190 +31.2 −45.9 14.937 10.991 10.139 M4.0 V 34.6 794 214605.6−251538 326.523558 −25.260571 +84.1 −136.9 14.971 11.026 10.177 M4.0 V 35.2 795 214746.6+102947 326.944263 10.496548 −114.2 −106.8 15.183 11.259 10.431 M4.0 V 39.2 796 215008.8−043100 327.536800 −4.516673 +250.1 −6.1 15.255 11.130 10.277 M4.5 V 30.1 797 215016.9−391743 327.570586 −39.295555 +128.0 −56.8 15.404 11.443 10.538 M4.0 V 42.6 798 215140.0+321605 327.916742 32.268261 +226.5 −9.6 14.539 10.589 9.714 M4.0 V 28.8 799 215354.2+032454 328.475835 3.415273 +60.4 −19.8 14.985 11.067 10.165 M4.0 V 35.9 800 215517.3−004623 328.822430 −0.773139 +64.0 −52.3 15.094 10.977 10.090 M4.5 V 28.0 801 215534.4−024117 328.893512 −2.688312 +152.5 +18.4 15.428 11.175 10.289 M4.5 V 30.7 802 215718.8−352020 329.328705 −35.338911 +187.1 −92.4 14.571 10.631 9.800 M4.0 V 29.3 803 220159.8+330506 330.499438 33.085176 +64.9 +58.5 15.292 11.083 10.169 M4.5 V 29.4 804 220214.8+203615 330.561985 20.604329 +133.3 +19.4 15.111 11.095 10.236 M4.0 V 36.3 805 220258.5+124515 330.744140 12.754296 +25.4 −141.8 15.310 11.396 10.544 M4.0 V 41.7 806 220346.7−093841 330.944646 −9.644760 +155.9 +4.8 14.935 10.925 10.069 M4.0 V 33.6 807 220559.0+355057 331.496100 35.849433 +130.6 −63.6 15.155 11.139 10.256 M4.0 V 37.1 808 220625.8+213944 331.607745 21.662229 +122.8 +3.4 14.710 10.769 9.943 M4.0 V 31.3 809 220653.3+165500 331.722368 16.916819 +104.5 +3.3 14.979 10.954 10.105 M4.0 V 34.0 810 221213.2−004519 333.055197 −0.755306 +68.6 +8.8 14.890 10.966 10.147 M4.0 V 34.2 811 221705.9+294631 334.274963 29.775410 +81.2 +10.9 15.368 11.421 10.532 M4.0 V 42.2 812 221706.0+254128 334.275358 25.691376 +23.5 −18.4 15.409 11.418 10.552 M4.0 V 42.1 813 221828.2+185521 334.617915 18.922523 −101.1 +110.5 15.033 10.867 10.059 M4.5 V 26.6 814 221921.3−161154 334.839161 −16.198513 −15.6 −381.2 15.258 11.254 10.349 M4.0 V 39.1

44 Table A1: (continued).

0 No. CMC15 α(J2000) δ(J2000) µα cos δ µδ r JKs SpT d [deg] [deg] [mas/a] [mas/a] [mag] [mag] [mag] [pc]

815 222041.6+275504 335.173534 27.917794 +101.2 +98.4 14.702 10.707 9.875 M4.0 V 30.4 816 222831.0+464004 337.129306 46.667896 +61.1 −23.4 15.480 11.240 10.375 M4.5 V 31.6 817 222944.3−182313 337.434706 −18.387173 +112.7 −61.0 14.782 10.677 9.787 M4.0 V 30.0 818 223638.2+301130 339.159196 30.191794 +14.3 −107.8 15.697 11.457 10.542 M4.5 V 35.0 819 223913.1+185632 339.804738 18.942289 −42.1 −54.4 15.024 10.785 9.929 M4.5 V 25.7 820 224424.8+001359 341.103462 0.233257 +6.9 −102.0 15.343 11.136 10.317 M4.5 V 30.2 821 225606.4−111706 344.026923 −11.285220 +139.8 −34.0 15.245 11.324 10.417 M4.0 V 40.4 822 225810.6−390549 344.544418 −39.097003 −46.4 −50.2 14.726 10.711 9.812 M4.0 V 30.4 823 225847.5+185449 344.698265 18.913614 +7.5 −86.1 14.855 10.828 9.998 M4.0 V 32.1 824 230226.0−250842 345.608351 −25.145031 −36.8 +11.2 15.021 11.021 10.157 M4.0 V 35.1 825 230341.7+282947 345.923978 28.496600 −25.8 +79.2 15.134 10.707 9.823 M4.5 V 24.8 826 230642.9+132051 346.679020 13.347693 +48.8 −99.2 15.528 11.329 10.477 M4.5 V 33.0 827 230800.6+243704 347.002636 24.618004 −28.0 −43.7 15.191 11.265 10.434 M4.0 V 39.3 828 230837.9+483900 347.157937 48.650121 +106.4 −4.7 14.930 10.976 10.128 M4.0 V 34.4 829 231028.3+431820 347.618246 43.305755 +33.9 −8.4 15.599 11.323 10.505 M4.5 V 32.9 830 231524.9−040910 348.853895 −4.152822 −98.0 −131.7 14.670 10.602 9.671 M4.0 V 28.9 831 231732.4+094156 349.385347 9.699145 +141.4 +70.0 15.644 11.466 10.658 M4.5 V 35.1 832 232028.4+394648 350.118477 39.780268 +50.0 −3.4 15.499 11.275 10.427 M4.5 V 32.2 833 232246.0−034344 350.691955 −3.728940 +65.0 −46.1 15.512 11.317 10.484 M4.5 V 32.8 834 232330.7−280714 350.878318 −28.120824 +109.2 −125.2 15.603 11.409 10.506 M4.5 V 34.2 835 232416.9−152223 351.070553 −15.373100 +196.1 −51.6 16.144 11.190 10.196 M5.5 V 19.4 836 232604.1−103725 351.517122 −10.623807 +158.3 +6.8 15.411 11.145 10.192 M4.5 V 30.3 837 232904.3+032911 352.268309 3.486482 +78.7 −46.0 15.633 11.111 10.188 M5.0 V 23.9 838 232954.1−122233 352.475701 −12.375953 +253.6 +140.4 14.682 10.711 9.870 M4.0 V 30.4 839 232959.4+022834 352.497739 2.476162 −14.6 −56.9 15.272 11.360 10.532 M4.0 V 41.0 840 233129.7+403252 352.873892 40.548023 +54.1 −15.2 15.427 11.448 10.636 M4.0 V 42.7 841 233536.8−060536 353.903395 −6.093351 +77.0 −35.5 15.166 11.178 10.313 M4.0 V 37.7 842 233556.4−002332 353.985340 −0.392284 +231.4 +28.1 15.179 11.062 10.157 M4.5 V 29.1 843 234109.0−363818 355.287893 −36.638405 +85.9 −87.9 15.312 11.074 10.219 M4.5 V 29.3 844 234152.0−025629 355.466693 −2.941636 +101.6 −74.1 14.665 10.500 9.645 M4.5 V 22.5 845 234208.6+010918 355.536075 1.155213 +23.7 −82.1 14.192 10.194 9.313 M4.0 V 24.0 846 234622.9+261901 356.595582 26.317213 +34.8 −10.9 15.409 11.337 10.492 M4.0 V 40.6 847 234803.8+225539 357.015951 22.927686 −68.0 −81.7 15.033 10.903 10.011 M4.5 V 27.1 848 234851.3+064307 357.214124 6.718849 −71.8 −90.2 14.749 10.529 9.721 M4.5 V 22.8 849 235325.6−184440 358.356691 −18.744697 +106.0 −83.2 16.153 11.236 10.384 M5.5 V 19.9

45 Table A2: Previously known M-dwarf candidates (in Simbad and/or in Lepine+11).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

1 000000.3−153448 +246.3 +71.0 14.565 10.474 9.627 G 273−196 2 000022.7+375803 +253.9 −69.0 15.090 11.006 10.139 G 171−35 3 000115.7+065935 −445.1 −85.8 15.857 11.286 10.418 NLTT 58776 4 000457.6−170937 +145.6 −13.6 16.015 10.997 10.084 2MASS J00045753−1709369 5 000530.0−253101 +272.4 −147.0 13.750 9.433 8.493 G 266−39 6 000639.2−070535 −104.0 +87.9 14.087 9.831 8.958 2MASS J00063925−0705354 7 000706.4+355642 −205.0 −107.7 15.587 11.476 10.598 LP 240−27 8 000853.9+205024 −266.2 −270.2 12.882 8.870 8.010 GJ 3010 9 000853.9+282148 +146.3 +48.3 15.350 11.234 10.309 2MASS J00085390+2821484 10 000855.2+491856 +350.2 +203.0 15.727 10.864 9.980 LP 191−43 11 000959.9−063201 +252.3 +0.5 15.212 11.157 10.277 LP 644−53 12 001202.6+020623 +303.7 +64.7 14.518 10.590 9.721 LP 584−75 13 001213.4+302844 +52.7 −25.9 14.216 10.242 9.410 2MASS J00121341+3028443 14 001319.5+273330 +16.3 −116.4 14.418 10.431 9.581 2MASS J00131951+2733310 15 001458.2+021307 +314.3 −110.7 15.450 11.411 10.535 LP 584−88 16 001518.8+434434 +218.1 +26.6 15.201 11.218 10.396 LP 192−46 17 001715.8−321954 +201.8 −4.5 14.696 10.641 9.734 2MASS J00171571−3219539 18 001914.0−145511 +286.4 +18.7 15.147 10.876 9.944 2MASS J00191396−1455113 19 001939.3+195104 +70.3 −48.9 14.927 10.926 10.078 2MASS J00193931+1951050 20 001943.0+195111 +69.8 −49.8 14.695 10.718 9.864 2MASS J00194303+1951117 21 002010.7−054345 +294.9 +35.3 15.971 11.499 10.507 LP 645−4 22 002116.5+184355 +679.6 −78.9 16.127 11.320 10.420 LHS 1060 23 002158.1+313715 +291.1 +240.1 15.855 11.450 10.563 LP 292−71 24 002327.9+241824 −270.3 +127.5 13.684 9.753 8.867 G 131−62 25 002434.9+300229 +585.9 +7.4 13.984 9.776 8.892 GJ 3033 26 002602.6+394723 +226.2 +25.5 15.413 10.990 10.102 LP 193−488 27 002706.8+494152 +361.1 −230.1 13.637 9.733 8.852 LHS 6007 28 002716.4+473103 +13.5 +7.0 15.115 11.103 10.253 2MASS J00271665+4731006 29 002801.0+145641 +165.5 −400.6 15.489 11.427 10.563 LP 465−21 30 002814.4−322756 +103.5 −50.3 14.485 10.121 9.278 2MASS J00281434−3227556 31 002854.8−273333 +167.7 +38.6 14.701 10.759 9.899 2MASS J00285473−2733337 32 003253.1−043407 +73.6 −156.6 13.349 9.276 8.350 2MASS J00325313−0434068 33 003322.3+144806 +273.9 −72.0 15.533 11.258 10.406 LP 465−43 34 003543.1+023313 +158.0 −176.8 15.432 10.517 9.543 NLTT 1930 35 003544.1−054112 −3.1 −262.4 15.361 10.667 9.711 LP 645−53 36 003555.5+102835 +1088.4 −388.7 14.623 10.222 9.367 LHS 117 37 003630.2−005441 +401.5 −195.6 14.995 10.996 10.136 LP 585−58 38 003800.8+402623 −72.3 +6.2 15.863 11.405 10.456 V* HI And 39 003804.7−325849 +247.9 −186.5 15.771 10.813 9.951 G 267−143 40 003903.4+133016 +87.6 −79.4 14.869 10.937 10.064 [SLS2012] PYC J00390+1330 41 003933.8+145434 +327.9 +25.0 13.844 9.826 8.946 G 32−37B 42 004236.0−161923 −143.0 +247.1 14.578 10.306 9.477 UCAC3 148−1626 43 004339.4−112608 +309.9 +14.7 15.567 11.234 10.343 LP 705−93 44 004420.7+090734 +814.8 −5.8 13.424 9.501 8.621 LHS 1137 45 004435.1−185704 +279.7 +184.0 15.314 11.274 10.426 LP 766−10 46 004556.7+334711 +260.4 +16.4 14.704 10.183 9.314 G 132−25 47 004641.4+485141 −198.5 −73.7 15.541 11.339 10.432 LP 150−44 48 004957.2+070838 +160.2 +3.2 15.317 11.413 10.578 2MASS J00495723+0708382

46 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

49 005017.5+083734 +64.7 −35.9 13.801 9.745 8.897 [ZEH2003] RX J0050.2+0837 2 50 005026.9−260713 +205.2 +18.0 15.368 11.306 10.434 2MASS J00502687−2607132 51 005448.1+273103 +340.0 +7.9 14.335 10.340 9.454 G 69−32 52 005453.5+174457 +181.2 +9.0 15.450 11.148 10.267 LP 406−35 53 005726.0+293234 +246.2 +12.1 15.544 11.447 10.570 LP 294−24 54 005801.1+391911 −102.6 +34.1 13.598 9.561 8.680 2MASS J00580115+3919111 55 005907.4+410223 +239.6 +43.4 15.473 11.377 10.508 NLTT 3228 56 005908.2+375239 +205.6 +1.0 14.610 10.688 9.837 2MASS J00590821+3752399 57 010013.9+340405 +226.5 +4.9 15.918 11.498 10.623 NLTT 3286 58 010014.1−073107 +83.9 −318.4 15.269 11.256 10.385 LP 646−49 59 010226.8+410143 −153.8 −119.7 13.999 10.084 9.257 2MASS J01022695+4101442 60 010630.6−251649 +366.3 −208.8 15.146 11.156 10.304 LP 826−539 61 010630.7+301711 +218.5 +5.5 15.613 11.225 10.353 LP 294−50 62 010812.2+002756 −239.3 −346.9 14.186 10.112 9.166 G 1−47 63 010918.8−243024 +277.5 −186.8 13.910 9.940 9.066 GJ 2021 64 011030.3−112644 +180.0 −321.7 14.781 10.703 9.804 G 270−165 65 011123.5+164830 +333.0 −262.3 14.823 10.861 10.028 G 34−8 66 011125.4+152621 +181.9 −129.9 13.658 9.082 8.208 GJ 3076 67 011212.0+054126 +129.2 −190.1 15.317 11.320 10.485 NLTT 3994 68 011303.6−343819 +129.9 −65.6 14.317 10.413 9.588 GEN\# +6.10050038 69 011513.4+224052 +275.5 −418.7 14.787 10.573 9.718 LHS 1221 70 011514.9+414305 +214.5 −47.8 15.201 11.094 10.210 LP 194−43 71 011550.2+470202 +198.6 −20.1 14.151 10.210 9.308 ** FMR 42 72 012210.3+220902 +237.0 −152.7 12.375 8.412 7.537 G 34−23 73 012227.3+192616 +146.7 −24.4 15.722 11.492 10.589 2MASS J01222732+1926170 74 012258.4+125203 +3.1 −1.9 12.680 7.546 6.642 V* U Psc 75 012315.0+025712 −340.6 −372.3 16.289 11.389 10.449 NLTT 4612 76 012331.6−234542 −197.7 −222.2 15.453 11.166 10.312 LP 827−167 77 012430.7−335502 +184.5 −128.8 14.771 10.555 9.682 GJ 2022 C 78 012619.5+300520 +259.8 +43.3 15.878 11.249 10.342 NLTT 4779 79 012854.6−264246 +74.9 +128.2 16.226 11.462 10.557 [PS78] 219 80 012942.6−082358 +117.6 −69.6 15.529 10.655 9.771 2MASS J01294256−0823580 81 013029.1−351202 +250.2 −306.4 15.194 11.275 10.433 2MASS J01302899−3512002 82 013128.6+250549 −153.7 −180.2 15.764 11.423 10.620 NLTT 5044 83 013410.5+125752 −157.1 −53.7 14.684 10.692 9.850 2MASS J01341058+1257530 84 013638.6+450014 +15.3 +34.3 15.533 11.382 10.560 2MASS J01363862+4500152 85 013707.0+421611 −262.9 −141.1 15.546 11.415 10.506 NLTT 5383 86 013836.9+172618 +325.1 +23.0 15.416 11.402 10.547 NLTT 5483 87 013921.8−393610 +120.0 −237.9 13.723 9.209 8.274 SIPS J0139−3936 88 013935.7+162729 −153.9 −117.2 14.831 10.800 9.967 LP 408−34 89 014115.9+301610 +747.2 −248.1 15.562 11.166 10.315 LHS 1280 90 014340.2−114925 +57.9 −182.7 15.456 11.369 10.561 LP 708−336 91 014353.3+001432 +40.2 −156.1 16.522 11.169 10.258 2MASS J01435333+0014323 92 014605.1+413049 +217.5 −37.1 14.611 10.669 9.760 2MASS J01460505+4130493 93 014751.8+105218 +212.7 −25.6 15.479 11.232 10.364 NLTT 5985 94 014901.6+251218 +411.6 +49.3 14.913 10.672 9.773 G 94−16 95 015027.1−185137 −227.2 +242.3 15.543 11.484 10.665 LP 768−566 96 015105.2−305754 +102.2 +302.6 14.908 10.942 10.141 LP 884−94

47 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

97 015257.3+083326 +90.8 −57.7 13.496 9.238 8.358 EM* StHA 10 98 015330.7+014755 +414.8 +50.3 15.380 10.786 9.879 G 159−9 99 015349.5+031322 +344.1 +34.5 14.689 10.587 9.701 G 159−10 100 015349.6+442728 +243.7 −98.0 14.756 10.416 9.547 G 133−48 101 015350.7−103214 +617.3 −271.8 14.876 10.454 9.649 LHS 1311 102 015407.9−153623 +90.0 −289.1 13.741 9.807 8.899 WT 1243 103 015645.7+303328 +219.2 −12.5 14.449 10.323 9.449 NLTT 6496 104 015754.7+285701 +70.8 −240.5 15.196 11.286 10.458 LP 296−59 105 015845.3+404944 +396.8 −70.8 15.017 10.704 9.811 LP 196−17 106 020244.3+133433 +455.6 −91.1 13.669 9.652 8.802 GJ 3129 107 020341.8−012847 +279.8 +30.0 16.082 11.418 10.529 2MASS J02034172−0128474 108 020501.3+323545 +285.2 −88.4 14.667 10.504 9.684 G 133−63 109 020707.9−181008 +105.5 −106.9 14.659 10.698 9.749 2MASS J02070786−1810077 110 020812.2+150842 +191.1 −41.9 14.220 10.052 9.196 NLTT 7084 111 020904.5+434126 +180.0 −31.4 15.763 10.819 9.974 LP 196−29 112 021044.6−093825 +225.3 +5.6 14.555 10.649 9.806 LP 709−44 113 021113.6+205822 +262.1 −13.4 15.537 11.405 10.528 NLTT 7239 114 021135.6−115332 −123.6 −160.9 15.587 11.232 10.375 LP 709−50 115 021138.3+080350 +229.7 −330.8 15.547 11.312 10.389 NLTT 7268 116 021151.6−035403 −13.8 −136.4 15.242 10.680 9.732 2MASS J02115166−0354022 117 021159.9+322145 +520.7 −231.2 15.067 10.778 9.842 LHS 1352 118 021320.6+364850 +28.2 +46.8 13.490 9.367 8.518 2MASS J02132062+3648506 119 021412.6−035744 +508.2 −153.6 15.741 10.481 9.485 LP 649−72 120 021621.3−220047 −115.8 +243.0 16.197 11.308 10.401 LP 829−41 121 021705.0−300621 +46.3 −30.2 14.670 10.578 9.717 WISE J021705.03−300621.9 122 021710.1+352631 +553.6 −263.0 15.301 9.983 9.011 GJ 3147 123 022022.2−080826 −202.3 −213.7 14.997 10.848 10.033 LP 650−215 124 022046.2+025837 +150.2 −288.0 14.070 10.064 9.202 GJ 3153 125 022153.3+281114 +126.9 −75.4 15.044 11.097 10.263 2MASS J02215334+2811145 126 022206.2+365145 +409.9 −142.5 16.426 11.388 10.439 2MASS J02220614+3651466 127 022315.9+291327 −163.0 −316.7 15.338 11.068 10.158 G 36−14 128 022401.4−103904 −369.2 −342.4 15.382 11.465 10.594 LHS 1399 129 022408.6−243416 +159.2 +56.4 15.241 10.981 10.089 2MASS J02240858−2434163 130 022547.5+243523 +210.2 −21.8 15.701 11.384 10.545 G 94−65 131 022731.3+193525 +183.4 −148.9 15.565 11.210 10.307 2MASS J02273126+1935260 132 023139.3+445638 +94.9 −52.4 13.923 9.970 9.133 2MASS J02313926+4456387 133 023503.2+410441 +179.7 −55.3 15.369 11.373 10.522 LP 197−24 134 023514.9+024753 +130.5 −221.2 13.981 10.030 9.144 G 76−8 135 023644.1+224025 −42.6 −374.3 14.597 10.081 9.194 G 36−26 136 023729.7+002127 +507.2 −165.3 14.463 10.547 9.689 GJ 3172 137 023746.1−070550 +63.8 −429.4 14.952 10.639 9.832 LHS 1427 138 023917.6−264919 +29.8 −213.4 13.652 9.601 8.749 LP 886−73 139 024011.1+422847 +134.4 −35.1 14.934 10.991 10.150 1RXS J024011.3+422846 140 024115.2−043218 +351.6 −63.4 13.129 9.199 8.246 G 75−35 141 024127.2−304915 +89.8 −25.8 15.372 11.127 10.256 WISE J024127.29−304915.1 142 024422.7+105734 +44.8 +45.1 14.724 10.301 9.452 UCAC3 202−9347 143 024541.3+445702 +409.9 −126.3 15.754 11.168 10.217 GJ 3179 B 144 024820.4+235219 +186.2 −25.6 14.999 10.847 9.965 2MASS J02482042+2352191

48 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

145 025131.1+241314 +61.1 −141.8 15.507 11.456 10.516 2MASS J02513113+2413154 146 025151.1+443409 +168.4 −111.4 15.601 11.307 10.426 2MASS J02515114+4434093 147 025243.4+332234 +159.1 −149.5 15.282 11.287 10.456 LP 298−43 148 025603.9−003633 +258.3 +69.6 14.829 10.421 9.567 LP 591−156 149 025613.9+235909 +75.5 −168.5 14.200 9.977 9.072 2MASS J02561395+2359105 150 025700.0+464214 +43.3 −81.0 15.432 11.415 10.588 [SLS2012] PYC J02570+4642 151 025946.4+385535 +230.8 −91.4 14.753 10.411 9.517 G 134−63 152 030133.2+325122 +337.2 −117.2 14.820 10.829 9.944 G 37−23 153 030138.7+322049 −319.4 −136.7 15.812 11.460 10.568 2MASS J03013889+3220498 154 030444.1+220321 +37.8 −49.3 14.913 10.486 9.655 2MASS J03044407+2203212 155 030615.0+120554 +226.7 −2.0 15.661 11.288 10.425 LP 471−50 156 030626.2+171329 +208.6 −25.8 14.858 10.925 10.066 LP 411−54 157 030732.1−063649 +195.9 −398.0 14.747 10.462 9.552 G 77−24 158 030746.8+245755 +228.1 −126.5 14.260 10.132 9.267 LP 355−27 159 030839.5−384436 +75.8 −7.2 15.153 11.249 10.418 WISE J030839.55−384436.3 160 030904.6+003112 −19.5 −224.6 15.012 10.785 9.835 NLTT 10023 161 031002.1−133413 −57.0 −292.8 14.966 10.990 10.082 LP 712−11 162 031053.4+005309 +276.1 −319.9 14.928 11.008 10.112 NLTT 10130 163 031115.4+010630 +110.3 −21.5 15.553 10.682 9.755 2MASS J03111547+0106307 164 031130.4+431126 +7.2 −232.3 14.456 10.526 9.624 NLTT 10125 165 031142.4−153719 +90.4 −153.6 15.875 11.448 10.558 LP 772−14 166 031203.9+111851 +1.5 −32.7 15.034 10.996 10.134 2MASS J03120387+1118513 167 031323.0+044629 −173.6 +458.0 13.273 8.775 7.833 V* CD Cet 168 031412.5+284038 +310.8 −751.3 16.128 10.993 10.092 LHS 1516 169 031437.2−094017 −270.7 −160.5 15.577 11.452 10.577 WT 1361 170 031718.2−194018 +519.0 −216.4 14.967 10.980 10.169 LHS 1524 171 031806.0−202231 +12.6 −38.2 14.362 10.396 9.471 2MASS J03180602−2022297 172 031856.7−343317 +47.7 −1.6 14.802 10.839 9.996 WISE J031856.73−343317.6 173 032105.5−052638 +69.6 +21.5 15.177 11.031 10.219 LHS 1536 174 032158.0−163614 −49.0 −244.5 15.131 11.200 10.346 LP 772−46 175 032339.1+054115 +79.8 −71.7 13.939 9.867 9.013 PM I03236+0541 176 032436.2+215018 +127.6 −42.0 15.309 11.290 10.398 LP 356−751 177 032640.3+051335 +59.0 −92.6 14.989 10.966 10.129 [SLS2012] PYC J03266+0513 178 032644.9+191439 −2.7 −153.8 14.299 10.123 9.252 GJ 3225 179 032730.8+221238 −39.0 −53.0 14.055 10.044 9.194 2MASS J03273084+2212382 180 033235.7+284355 +51.5 −72.1 13.448 9.357 8.473 2MASS J03323578+2843554 181 033351.3+060842 +315.4 +214.7 15.491 11.331 10.516 NLTT 11229 182 033410.5+220421 +312.9 +106.6 15.606 11.355 10.475 2MASS J03341053+2204213 183 033556.9−103057 +115.5 −144.0 14.872 10.970 10.136 LP 713−10 184 033608.7+311838 +117.6 −136.3 13.365 9.187 8.315 2MASS J03360868+3118398 185 033631.4−261958 +85.1 −26.1 15.619 10.675 9.763 WISE J033631.50−261958.1 186 033640.8+032919 +116.5 −123.0 13.245 9.295 8.444 GJ 3237 187 033901.6−243406 +69.5 −17.2 14.914 10.898 9.968 WISE J033901.64−243406.1 188 034033.5−023934 +105.2 −44.7 15.604 11.470 10.616 LP 593−39 189 034043.7−145213 +142.7 −128.8 15.274 11.284 10.414 LP 773−24 190 034143.8+182406 +23.9 −42.2 14.412 10.484 9.643 2MASS J03414386+1824061 191 034231.8+121622 +203.2 −24.1 14.189 10.157 9.275 2MASS J03423180+1216225 192 034236.9+221230 +64.9 −85.7 16.835 11.227 10.320 Cl* Melotte 22 MT 32

49 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

193 034247.0−242746 +23.1 −372.7 14.893 10.929 10.042 CD−24 1826B 194 034253.2+232649 +176.7 −61.2 14.267 10.202 9.316 V* LR Tau 195 034322.1−093349 +400.5 +302.5 14.009 9.799 8.854 LHS 1582 196 034335.5+262130 +173.3 −61.2 14.716 10.772 9.903 2MASS J03433551+2621311 197 034420.8+074154 −158.7 +11.6 14.185 10.191 9.380 2MASS J03442081+0741549 198 034659.5+152416 +222.5 −25.0 14.889 10.733 9.851 LP 473−26 199 034758.8+232904 −62.5 −137.8 15.792 11.347 10.492 Cl* Melotte 22 MT 88 200 035047.0+481235 +71.0 −102.5 14.532 10.572 9.694 V* MR Per 201 035059.5+141401 +65.7 −74.1 14.809 10.241 9.380 2MASS J03505949+1414017 202 035100.7+141339 +64.5 −77.5 13.405 9.436 8.579 2MASS J03510078+1413398 203 035241.7+170103 +436.7 −651.6 13.145 8.933 8.053 Wolf 227 204 035336.7+311224 +143.1 −72.0 14.531 10.456 9.582 LP 301−63 205 035616.3−391521 +69.6 −13.9 14.824 10.460 9.602 WISE J035616.31−391521.8 206 035630.4+241718 +29.6 −48.0 15.640 11.160 10.289 V* V692 Tau 207 035646.6+362441 +128.8 −84.0 14.949 10.981 10.102 LP 248−7 208 035719.9+410742 −204.8 −31.3 16.174 10.903 9.949 2MASS J03571999+4107426 209 035849.1+123022 +255.3 −309.1 13.717 9.757 8.877 G 7−14 210 035915.0+163951 +141.4 −27.4 15.263 11.269 10.382 LP 414−25 211 035945.1+215147 +275.0 −205.8 15.152 11.092 10.243 LP 357−99 212 040059.5+142045 +132.0 −20.9 14.633 10.693 9.826 Cl* Melotte 25 REIDA 477 213 040253.1+182426 +133.4 −36.8 14.717 10.770 9.913 Cl* Melotte 25 REID 42 214 040324.8+082450 +21.7 −120.8 14.773 10.647 9.775 [SLS2012] PYC J04034+0824 215 040427.0+202430 +120.3 −41.8 15.290 11.210 10.325 2MASS J04042701+2024303 216 040620.6+190138 +107.8 −26.6 15.473 11.341 10.471 217 040703.3+201650 +170.3 −46.6 15.617 11.450 10.556 Cl* Melotte 25 REID 64 218 040708.1+145956 +58.7 −158.0 14.909 10.986 10.107 2MASS J04070817+1459562 219 040730.6−400529 +282.6 +35.9 15.489 11.330 10.418 2MASS J04073043−4005291 220 040855.5−312855 −366.3 +303.1 13.831 9.775 8.823 LP 889−37 221 040922.2+054626 +221.9 −126.1 15.353 10.708 9.740 NLTT 12648 222 041233.0+210343 −0.3 −23.6 14.900 10.891 9.939 2MASS J04123300+2103433 223 041234.8+352959 −163.6 +96.1 14.977 10.642 9.790 2MASS J04123491+3529592 224 041247.3+222326 +118.4 −47.8 15.079 11.061 10.165 225 041305.6+151451 +126.3 −21.4 15.372 11.303 10.444 Cl* Melotte 25 VA 50 226 041326.6−013921 +138.3 −6.4 13.298 9.375 8.504 2MASS J04132663−0139211 227 041447.3+280305 +10.6 −31.6 15.572 10.796 9.917 2MASS J04144739+2803055 228 041534.5+193559 +215.4 −46.8 14.937 10.787 9.911 LP 414−139 229 041627.9+205328 +6.0 −17.9 15.228 11.054 10.085 2MASS J04162791+2053285 230 041632.0+460635 −169.0 −118.2 15.523 11.422 10.546 2MASS J04163215+4606360 231 041643.3+164919 +101.5 −23.6 15.090 11.161 10.275 Cl* Melotte 25 LH 247 232 041718.5+084921 +129.2 −377.0 13.225 9.030 8.182 GJ 3270 233 041739.7+122453 +122.7 −16.5 14.731 10.746 9.868 Cl* Melotte 25 VA 112 234 041818.5+221322 +91.3 −8.1 16.240 11.170 10.207 2MASS J04181854+2213229 235 041833.8+182152 +113.7 −44.9 15.591 11.490 10.601 LP 414−158 236 041835.9+173057 +63.3 −68.9 15.321 11.352 10.504 Cl* Melotte 25 VA 139 237 041903.1+193239 +124.2 −44.8 14.822 10.904 10.009 238 041920.8+043650 +135.4 −291.4 14.335 10.427 9.565 G 82−11 239 041935.4+282721 +5.9 −28.8 15.793 10.954 9.971 V* FR Tau 240 042039.1+271731 +4.0 −31.0 14.689 10.497 9.560 USNO−B1.0 1172−00072216

50 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

241 042109.3+275036 +1.8 −28.8 16.149 11.229 10.358 2MASS J04210934+2750368 242 042119.7+120237 +109.1 −9.7 15.819 11.361 10.483 Cl* Melotte 25 VA 208 243 042123.4+105202 +93.4 −10.4 15.020 11.049 10.190 2MASS J04212344+1052021 244 042135.5+165339 +138.7 −42.6 14.898 10.783 9.915 Cl* Melotte 25 LH 199 245 042233.5+390043 +598.2 −611.6 14.602 10.473 9.670 LHS 1667 246 042239.8+150344 +63.7 −31.7 14.968 10.917 10.062 Cl* Melotte 25 HAN 269 247 042254.1+243953 +5.0 −22.3 14.606 9.648 8.651 2MASS J04225416+2439538 248 042259.2+255913 +33.6 −249.6 13.593 9.645 8.786 G 8−31 249 042306.1+234602 +215.7 −175.1 15.383 11.135 10.233 LP 358−167 250 042312.4+154246 +110.0 −29.2 15.323 11.241 10.356 LP 415−35 251 042409.4+150515 +174.4 −66.9 14.541 10.303 9.472 V* IO Tau 252 042420.2+304433 −141.3 −186.1 15.404 11.451 10.617 NLTT 13166 253 042421.5+370620 +47.3 −57.6 14.191 10.191 9.340 2MASS J04242150+3706208 254 042445.0+270144 +4.6 −30.6 15.528 11.340 10.458 2MASS J04244506+2701447 255 042515.5+282927 +14.6 −28.8 16.775 11.258 10.328 2MASS J04251550+2829275 256 042519.2+370508 +402.4 +5.8 15.505 10.972 10.096 2MASS J04251914+3705083 257 042530.5−095549 +86.5 +356.0 16.216 11.471 10.572 LP 715−12 258 042547.0+173240 +103.3 −28.9 15.348 11.189 10.316 Cl* Melotte 25 LH 135 259 042604.3+170714 +111.1 −36.9 14.927 10.887 9.987 2MASS J04260431+1707145 260 042613.6+465945 +145.4 −125.4 15.419 11.001 10.118 LP 156−58 261 042621.7+180000 +103.8 −33.1 15.226 11.119 10.253 SDSS J042621.75+180000.8 262 042632.6−304804 −64.8 −472.4 13.475 9.303 8.411 LHS 5094 263 042703.1+240615 +108.1 −48.1 15.479 11.489 10.574 LP 358−268 264 042724.1+140707 +101.2 −17.0 15.352 11.401 10.529 2MASS J04272407+1407072 265 042745.6−332742 +47.5 −1.3 15.429 11.263 10.395 WISE J042745.66−332742.6 266 042929.7+261652 +4.4 −32.1 15.305 10.340 9.388 V* FW Tau 267 043025.3+395057 +269.8 −566.8 13.132 9.113 8.246 V* V546 Per 268 043052.1−011246 +129.8 +33.8 15.706 11.403 10.527 2MASS J04305207−0112471 269 043115.7+104215 +96.4 −9.6 14.493 10.535 9.676 1RXS J043115.6+104217 270 043115.7+182006 +11.4 −19.9 15.466 11.210 10.304 2MASS J04311578+1820072 271 043123.8+241052 +4.3 −20.9 14.068 9.729 8.768 V* V927 Tau 272 043226.2+182752 +9.5 −21.0 15.980 11.117 10.173 2MASS J04322627+1827521 273 043241.0+180923 +10.4 −23.6 15.659 11.311 10.341 2MASS J04324107+1809239 274 043331.5−021101 +229.5 −261.6 16.278 11.475 10.630 2MASS J04333153−0211010 275 043334.0+204445 +452.7 −324.9 13.828 9.769 8.960 GJ 3296 276 043341.7+175040 +11.0 −16.8 15.720 11.274 10.313 Cl* Melotte 25 LH 48 277 043348.2+422706 +210.4 −201.3 15.439 11.462 10.544 LP 201−54 278 043423.8+205257 +21.3 −225.2 15.231 11.021 10.138 LP 415−213 279 043431.2+172220 +5.9 −22.5 15.344 11.205 10.234 2MASS J04343128+1722201 280 043437.7+190604 −195.6 −66.3 15.270 10.610 9.710 LP 415−217 281 043459.2+173337 +4.2 −30.4 15.719 10.634 9.717 Cl* Melotte 25 LH 27 282 043506.1+130804 +21.0 −49.3 15.029 10.953 10.102 Cl* Melotte 25 LH 3 283 043513.1+172549 +12.4 −25.3 15.178 11.000 10.058 Cl* Melotte 25 LH 19 284 043513.1+225920 +94.5 −48.5 15.571 11.127 10.250 V* EZ Tau 285 043524.6+104452 +111.8 −8.3 15.492 11.179 10.282 286 043528.4+152357 +96.2 −31.4 15.426 11.320 10.438 Cl* Melotte 25 VA 763 287 043547.7+252343 +2.9 −21.6 14.645 10.272 9.331 2MASS J04354778+2523436 288 043649.1+045110 +279.8 −106.6 15.840 11.254 10.418 NLTT 13616

51 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

289 043702.2+423041 +162.0 −204.1 15.241 11.075 10.206 2MASS J04370219+4230427 290 043732.1+164531 +87.7 −26.9 14.852 10.633 9.723 291 043802.4−055614 −70.5 −182.6 13.834 9.730 8.818 LP 655−43 292 043809.4+111905 +85.9 −9.6 15.565 11.410 10.529 293 043810.5+154917 +97.5 −25.8 15.368 11.384 10.526 294 043904.5+233319 −0.9 −24.6 14.852 10.479 9.617 2MASS J04390453+2333199 295 043905.7+233811 +8.8 −23.2 15.954 11.338 10.475 WISE J043905.72+233811.1 296 043933.6+413249 +442.9 +129.9 15.163 11.128 10.266 2MASS J04393348+4132488 297 043951.6+193934 +89.3 −42.0 15.627 11.365 10.441 298 044033.1−073119 −32.8 −315.7 14.518 10.473 9.579 2MASS J04403324−0731177 299 044104.2+255755 +2.0 −22.8 15.948 10.947 9.952 Haro 6−32 300 044145.6+230158 −1.5 −21.8 14.718 10.738 9.854 [TLM2010] 2M J044145 B 301 044159.0−135604 +285.9 +30.5 15.373 11.428 10.602 LP 715−44 302 044320.2+294006 +4.6 −33.4 15.201 10.402 9.408 Haro 6−36 303 044443.7+182429 +84.0 −42.2 14.513 10.561 9.655 LP 415−2037 304 044505.7+432432 +372.9 −633.9 14.899 10.840 9.960 LP 201−108 305 044609.1+064500 +91.0 +4.4 14.518 10.395 9.522 RX J0446.1+0644 306 044615.2+184629 +95.2 −36.7 15.234 11.087 10.188 LP 416−26 307 044617.7−062302 +263.4 −220.8 15.143 11.049 10.234 LP 656−8 308 044627.1+173735 +91.2 −31.5 15.619 11.467 10.618 LP 416−471 309 044642.6+245903 +0.9 −27.3 16.175 11.261 10.338 2MASS J04464260+2459034 310 044712.2+203810 +83.9 −95.6 13.574 9.380 8.507 2MASS J04471225+2038109 311 044749.6+124129 +69.0 −14.6 15.342 11.337 10.455 LP 476−631 312 044801.0−260301 +166.1 +78.3 14.990 10.773 9.936 LP 835−18 313 044857.8+364822 −1.2 −368.0 15.617 10.867 9.955 2MASS J04485783+3648237 314 044859.5+153617 +85.7 −24.9 15.147 11.001 10.131 315 045050.3+260728 +24.8 −54.7 16.657 9.152 8.305 LHS 1705 316 045051.0+220720 +631.4 −433.5 14.504 9.896 8.977 LHS 1706 317 045128.9+103247 +120.6 −405.1 15.417 11.388 10.505 NLTT 14060 318 045203.8−105822 −354.3 −213.2 15.464 10.502 9.606 LP 716−10 319 045229.3+093028 +164.0 −351.5 15.388 11.294 10.449 NLTT 14097 320 045336.0−283535 +25.9 +0.0 14.394 10.174 9.301 UCAC3 123−12808 321 045357.0+091558 +91.8 −1.4 15.345 11.308 10.445 322 045435.3+083020 +135.6 −191.4 15.582 11.334 10.384 NLTT 14154 323 045545.3+301938 +6.1 −29.8 15.804 11.440 10.462 2MASS J04554535+3019389 324 045651.4−165530 +9.4 −439.2 15.275 11.330 10.502 LP 776−31 325 045703.2+333156 −78.2 −336.2 16.322 11.396 10.408 2MASS J04570322+3331584 326 050305.6+212235 +94.1 −140.9 14.029 9.750 8.888 LP 359−186 327 050414.7+110324 −63.2 +192.6 13.139 9.144 8.311 GJ 3326 328 050505.9+441403 +92.8 −29.3 14.115 9.829 9.017 PM I05050+4414 329 050612.9+043926 +34.2 −92.5 12.847 8.909 8.067 RX J0506.2+0439 330 050616.7+244610 −0.6 −21.1 14.822 10.792 9.815 2MASS J05061674+2446102 331 050647.8+074201 −174.9 −205.5 15.532 11.448 10.600 NLTT 14509 332 050711.3+143001 +16.4 −76.1 15.173 10.571 9.664 [SLS2012] PYC J05071+1430 333 050714.4+373042 −105.5 −8.0 14.713 10.284 9.397 2MASS J05071449+3730421 334 050827.3−210144 +36.5 −15.3 14.189 9.716 8.833 2MASS J05082729−2101444 335 050919.4−134841 +278.0 −22.7 15.545 10.929 10.025 LP 717−3 336 051453.6−330429 +176.7 +144.6 14.310 10.089 9.171 LTT 2215

52 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

337 051517.1+090735 +79.5 −306.6 15.556 11.462 10.633 NLTT 14744 338 051517.5+233625 +36.7 −71.5 14.561 10.186 9.306 2MASS J05151753+2336260 339 051622.7+244522 +32.7 −105.3 14.991 10.651 9.746 [SLS2012] PYC J05163+2445 340 051836.6−284204 −38.4 +435.7 15.139 10.873 10.014 LP 892−32 341 051842.0+303500 +5.4 −29.4 15.050 10.649 9.749 342 051955.0−281749 +8.9 +264.4 15.498 11.356 10.530 LP 892−36 343 052349.0+223238 +226.7 −305.4 14.844 10.703 9.850 GJ 1078 344 052419.1−160115 +20.5 −36.7 13.031 8.668 7.807 2MASS J05241914−1601153 345 052425.7+192206 −14.2 −35.2 13.769 9.464 8.564 2MASS J05242572+1922070 346 052623.6+100341 +32.9 −217.2 14.907 10.468 9.655 NLTT 15056 347 052753.4+312753 −66.2 −146.2 15.421 11.426 10.535 2MASS J05275344+3127540 348 052848.2+112054 −95.9 −66.4 14.178 10.174 9.331 V* V441 Ori 349 052944.6−323914 +150.5 +100.3 13.148 9.215 8.316 2MASS J05294468−3239141 350 053157.8−030336 +5.4 −54.4 13.798 9.452 8.538 PM I05319-0303W 351 053700.7+233044 +2.4 −45.6 15.942 11.435 10.543 352 054025.7+244806 +1.6 −400.1 14.172 8.978 8.039 V* V780 Tau 353 054053.8+085418 −17.5 −35.8 14.995 10.455 9.589 2MASS J05405390+0854183 354 054304.6−263538 +68.5 +199.5 14.606 10.568 9.717 LP 837−16 355 054307.8+443946 −119.1 −108.3 14.729 10.819 9.993 2MASS J05430792+4439470 356 054458.0−245610 +220.6 −140.1 14.842 10.761 9.846 LP 837−20 357 055011.7+093949 +259.4 +240.1 15.159 11.186 10.333 2MASS J05501174+0939492 358 055246.8+032101 +174.8 −78.8 15.143 11.136 10.223 2MASS J05524682+0321016 359 055344.0+315052 +83.7 −124.1 14.884 10.711 9.859 2MASS J05534403+3150526 360 055405.1−024822 +28.7 −253.9 15.142 10.723 9.806 LP 658−71 361 055543.7+465056 +8.4 −534.7 15.028 11.089 10.274 ** LDS 3680 362 055817.2−043802 +81.3 −217.9 15.329 11.113 10.312 LP 659−4 363 055850.2−030832 +25.1 −204.5 15.584 11.404 10.591 LP 659−6 364 055853.3+212100 +55.7 −444.2 14.561 9.968 9.066 LHS 6097 365 055919.5−091833 +42.9 +65.5 14.955 10.975 10.124 2MASS J05591958−0918340 366 060156.4+403206 −16.8 −188.2 15.491 11.238 10.384 2MASS J06015642+4032074 367 060229.2+495153 +58.9 −855.5 13.812 9.350 8.435 LHS 1809 368 060433.8+412645 +52.0 −91.5 15.185 11.044 10.221 2MASS J06043383+4126465 369 060438.8+074154 +82.4 −207.5 15.049 10.636 9.784 2MASS J06043887+0741545 370 060524.8−161805 +328.7 +134.1 14.666 10.492 9.662 LP 779−17 371 060731.8+471225 −6.2 −7.8 13.736 9.723 8.887 2MASS J06073185+4712266 372 061022.4+223419 +38.7 −161.0 15.598 10.644 9.746 NLTT 16144 373 061156.0+332549 +129.1 −407.7 14.282 10.163 9.345 LHS 6100 374 061222.4−080716 −103.0 +1.9 16.525 11.201 10.270 2MASS J06122246−0807162 375 061237.8−082622 −198.7 −155.3 14.971 10.861 9.961 LP 659−20 376 061955.6+165025 −19.0 −103.2 14.841 10.840 10.020 [SLS2012] PYC J06199+1650 377 061957.4+202218 +60.9 −207.2 14.741 10.740 9.885 G 104−33 378 062015.3−002339 −51.4 −121.9 15.359 11.307 10.434 LP 600−8 379 062051.7+314511 −71.2 −432.3 15.553 11.362 10.462 2MASS J06205178+3145134 380 062136.4+322237 +65.7 −194.7 15.332 11.041 10.155 2MASS J06213640+3222390 381 062150.4+155413 +36.3 +30.5 15.420 11.389 10.553 2MASS J06215046+1554140 382 062351.2+454003 −28.8 −285.8 14.795 10.348 9.437 LP 160−22 383 062728.1+212922 +132.1 −210.8 15.447 11.225 10.354 2MASS J06272815+2129225 384 063038.6−020550 −204.4 −52.0 14.731 10.729 9.857 WD 0628−020

53 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

385 063038.7−020553 −77.6 −213.3 14.904 10.729 9.857 UCAC3 176−39422 386 063150.7+412944 −7.7 −211.3 14.205 9.680 8.805 GJ 3396 387 063220.2−094329 −11.1 −57.0 13.781 9.848 8.984 PM I06323-0943 388 063529.8−040318 −287.8 +180.0 13.752 9.272 8.307 PM I06354-0403 389 063636.9+061910 +69.5 +138.2 16.318 11.242 10.321 2MASS J06363696+0619102 390 063755.4+085859 −7.6 −340.3 15.105 11.163 10.262 2MASS J06375540+0858594 391 063756.6−371131 −47.6 +116.7 14.436 10.326 9.509 1RXS J063756.9−371132 392 064058.0+494429 +2.3 −164.2 15.390 10.743 9.862 2MASS J06405810+4944304 393 064206.9+094640 −16.0 −110.4 15.556 11.398 10.496 Cl* NGC 2264 SBL 513 394 064334.6+164135 −215.8 +39.7 13.737 9.776 8.888 G 110−14 395 064417.9+412815 +76.4 −400.5 15.720 11.233 10.327 2MASS J06441792+4128179 396 064641.0−215016 −190.4 −42.8 16.364 11.220 10.354 LP 839−29 397 064707.1+443945 +102.8 +47.5 15.009 10.846 10.036 2MASS J06470710+4439458 398 064859.8+382116 −126.4 −170.7 14.812 10.833 9.919 LP 254−29 399 065631.0+440154 +182.3 −684.6 13.889 9.923 9.073 LHS 1883 400 070006.8−190124 +155.0 −74.7 13.350 9.029 8.091 PM I07001-1901 401 070110.6+155827 −17.5 −179.8 15.457 11.375 10.499 2MASS J07011069+1558280 402 070136.5−143717 −229.4 +215.8 15.664 11.252 10.321 2MASS J07013658−1437185 403 070155.2+441715 −106.5 −167.9 15.508 11.285 10.362 2MASS J07015525+4417163 404 070434.4+165726 +7.8 −211.0 14.702 10.521 9.639 2MASS J07043449+1657273 405 070640.4+262459 −58.9 −152.6 15.120 10.847 9.948 NLTT 17409 406 071111.5+432956 +350.2 −572.8 15.431 9.979 9.126 2MASS J07111138+4329590 407 071114.7+102758 +120.7 −128.8 15.527 11.112 10.215 NLTT 17513 408 071251.0+370733 +449.3 −119.1 15.121 11.114 10.265 2MASS J07125105+3707340 409 071442.3−400938 −20.9 −10.7 14.635 10.453 9.596 1RXS J071441.9−400939 410 071617.9+330909 −103.5 −439.4 13.805 9.763 8.879 GJ 1096 411 072011.3+152354 −226.9 −252.3 15.422 11.110 10.236 2MASS J07201139+1523554 412 072217.4+085156 −160.4 −62.1 14.729 10.603 9.753 2MASS J07221747+0851566 413 072418.7+382058 +30.0 −51.9 14.900 10.957 10.117 1RXS J072418.7+382101 414 072421.1−312557 −56.0 +28.8 13.732 9.788 8.889 2MASS J07242124−3125577 415 072851.1−301554 −221.7 −274.4 13.143 8.896 8.062 GJ 2060 C 416 073129.4+024908 −194.3 −508.2 16.180 11.166 10.237 2MASS J07312949+0249084 417 073326.7−274904 −94.4 −49.2 15.290 11.009 10.080 2MASS J07332681−2749041 418 073505.8+100028 −252.7 +208.2 15.380 11.178 10.326 2MASS J07350593+1000283 419 073554.6+333345 −48.9 −232.4 15.524 11.309 10.446 LP 256−34 420 073625.1+070442 −18.4 −281.1 12.555 8.180 7.282 GJ 3454 421 073847.2+492525 +43.0 −496.5 15.421 10.632 9.701 LP 162−47 422 074119.3+123938 −25.8 −159.2 15.405 11.498 10.643 2MASS J07411937+1239390 423 074440.1+033308 −347.3 −448.8 10.563 6.581 5.698 V* YZ CMi 424 074540.3+493148 −101.6 −174.8 16.137 11.404 10.472 NLTT 18368 425 074636.4−253702 −8.3 −3.6 12.185 7.745 6.935 426 075151.3+053257 −64.2 −66.1 14.034 9.966 9.089 LHS 1950 427 075154.6−000012 +248.8 −742.6 12.537 8.496 7.661 ** LDS 6210 428 075544.6−274206 −255.5 +100.1 15.517 11.404 10.523 2MASS J07554477−2742068 429 075830.4+153000 −84.0 −118.4 14.428 10.429 9.561 GJ 3469 B 430 075852.7+121205 −0.4 −13.2 15.077 10.650 9.839 2MASS J07585271+1212058 431 081048.0+010911 +52.9 +192.2 14.993 10.623 9.744 NLTT 19068 432 081852.9+212703 −170.8 +5.2 14.734 10.676 9.832 2MASS J08185301+2127034

54 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

433 082012.9+092014 −158.0 −387.4 14.419 10.465 9.565 LHS 6145 434 082156.8+174856 −444.1 +163.4 15.073 10.902 10.037 LHS 2002 435 082426.7+255536 −196.4 −138.4 14.689 10.618 9.705 NLTT 19450 436 082430.9+390053 −233.1 −141.1 15.831 11.088 10.137 LP 209−2 437 082458.9+414725 +244.4 −5.6 14.700 10.753 9.876 LP 209−4 438 082924.1−041618 +93.1 −387.3 15.195 11.281 10.404 LP 665−17 439 082949.1+264632 −201.1 −547.9 14.274 8.235 7.260 V* DX Cnc 440 082955.6+163902 +115.7 +95.4 15.305 11.229 10.404 2MASS J08295564+1639016 441 083046.3−041340 +44.7 +33.4 15.535 11.242 10.376 1RXS J083046.4−041344 442 083123.2−102955 −592.9 −322.1 14.309 10.070 9.136 LHS 2024 443 083519.8+140833 −132.3 −79.4 13.335 9.163 8.282 2MASS J08351992+1408333 444 083606.3+170046 +60.9 −307.7 14.721 10.815 9.987 LP 425−244 445 083720.4−281958 +149.4 −184.4 14.856 10.727 9.888 2MASS J08372042−2819575 446 084012.1−364157 −188.4 +45.3 15.107 11.154 10.320 2MASS J08401227−3641577 447 084127.2+023726 −264.5 −169.4 15.889 11.351 10.451 NLTT 20048 448 084908.5+393625 −382.2 −335.5 15.123 10.584 9.640 LHS 2052 449 085117.5+460602 −356.4 +21.8 15.704 11.363 10.496 LP 164−63 450 085147.1+331519 −72.7 −157.8 15.637 11.417 10.567 2MASS J08514713+3315206 451 085240.8+281858 −491.6 −237.3 12.500 8.560 7.666 * rho Cnc B 452 085559.5+065203 −188.7 −97.2 15.350 11.358 10.453 NLTT 20552 453 085619.5+123948 −44.8 −253.5 13.792 9.585 8.708 G 41−8 454 085929.2+291818 −6.1 −83.0 15.584 10.775 9.836 LP 312−51 455 090023.4+215004 −53.8 −337.6 15.203 9.436 8.437 LHS 2090 456 090320.9+054014 −50.2 −381.6 16.141 10.766 9.832 NLTT 20861 457 090440.2−121914 +91.0 −683.8 14.907 10.746 9.893 LHS 2098 458 090543.3−084159 +283.9 −180.8 15.107 10.828 9.961 2MASS J09054323−0841581 459 090729.2+330443 −704.1 −151.5 15.525 11.308 10.482 LHS 2107 460 090848.5+465552 +103.1 −278.0 15.039 11.068 10.233 LP 165−26 461 090848.8+115141 −453.3 +191.4 14.651 10.739 9.899 LHS 5144 462 090907.9+224741 −81.2 −71.8 14.656 10.474 9.616 2MASS J09090798+2247413 463 090950.2−141401 −130.2 +74.7 15.305 11.067 10.176 2MASS J09095024−1414013 464 091000.6+090138 −353.2 −38.3 14.790 10.597 9.765 G 46−23 465 091339.9+185913 −162.8 −268.4 14.949 10.997 10.087 LP 427−15 466 091402.1+482041 −115.7 −109.9 15.966 11.454 10.582 2MASS J09140220+4820417 467 091536.2−103548 −396.2 −186.0 13.107 8.605 7.733 LHS 6167 468 091650.7+244855 −70.9 −123.3 14.819 10.466 9.603 2MASS J09165078+2448559 469 091752.2+211718 −70.9 −73.5 15.492 11.437 10.530 SDSS J091752.21+211718.2 470 091759.4−182329 −38.9 −211.9 16.171 11.423 10.509 LP 787−17 471 091841.3+264551 −194.4 −352.5 15.950 11.269 10.291 GJ 3549 B 472 091918.8+383116 −244.8 −42.7 13.878 9.924 9.059 GJ 1122 A 473 091918.9+383123 −194.5 +452.7 14.074 10.048 9.150 GJ 1122 B 474 092148.9+433027 −294.1 −115.5 13.342 9.431 8.490 GJ 3554 475 092246.4−154725 +433.6 −254.4 15.299 10.965 10.051 LHS 2132 476 092418.0−400513 +140.3 −204.9 14.489 10.464 9.602 2MASS J09241790−4005120 477 092439.6+034623 −200.3 −37.3 15.040 11.055 10.173 NLTT 21687 478 092645.0+085741 +156.4 −99.4 14.529 10.350 9.436 2MASS J09264503+0857421 479 092855.6−072214 −150.0 −712.8 14.398 10.370 9.537 LHS 2146 480 092903.6−242904 −213.9 −139.7 16.079 10.841 9.910 2MASS J09290378−2429041

55 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

481 092910.9+255808 −1046.4 −268.2 15.611 10.906 9.958 LHS 269 482 093248.2+265943 −93.5 +285.9 14.976 10.356 9.472 HD 82443B 483 094102.0+220127 +485.4 −530.2 13.631 9.627 8.813 LHS 2171 484 094332.1+444521 −76.5 −85.0 15.384 11.456 10.597 2MASS J09433219+4445224 485 094423.9+163641 +50.5 −285.9 15.539 11.470 10.583 LP 428−32 486 094454.0−122054 −345.3 +50.8 13.074 8.496 7.601 2MASS J09445422−1220544 487 094558.2−325328 −299.3 +155.4 13.396 9.204 8.279 2MASS J09455843−3253299 488 094627.6−122859 −179.2 −148.9 16.211 11.266 10.349 LP 728−23 489 094747.1+283748 +141.4 −247.9 15.254 11.164 10.216 LP 314−66 490 095009.0+305213 −192.6 −38.2 15.000 10.708 9.870 2MASS J09500916+3052140 491 095104.5+355808 −75.2 +187.5 14.810 10.577 9.690 LP 261−75 492 095135.7+404333 −133.7 −146.8 15.592 11.326 10.462 NLTT 22760 493 095319.6+073650 −206.3 +18.4 15.515 11.355 10.449 2MASS J09531969+0736501 494 095355.1+205647 −209.4 +388.1 13.361 9.208 8.326 GJ 3571 495 095506.6+342039 −33.9 −244.3 15.308 11.359 10.470 LP 261−109 496 095757.9+114828 −434.5 −159.1 14.073 10.092 9.176 LHS 6179 497 095856.4+055759 −179.5 −71.2 14.036 9.937 9.039 NLTT 23096 498 095900.4−300743 −34.7 −6.6 15.820 11.466 10.600 2MASS J09590058−3007441 499 100050.2+315545 −535.9 −423.6 15.537 10.261 9.275 * 20 LMi B 500 100146.9+272438 +101.7 −280.5 15.269 11.007 10.068 LP 315−23 501 100242.4+145912 +127.2 −244.8 13.561 9.649 8.803 G 43−23 502 100249.0+482731 −330.6 −273.9 14.754 9.963 9.005 LHS 6180 503 100336.4+331912 +76.7 −147.2 15.379 11.392 10.487 2MASS J10033638+3319126 504 100516.3+170325 −154.3 −185.6 15.358 11.130 10.256 NLTT 23347 505 100652.0−124654 −107.6 +2.1 13.841 9.749 8.902 2MASS J10065210−1246543 506 100704.1+352656 −318.1 −70.4 16.068 11.433 10.532 NLTT 23417 507 100800.9−143626 −369.3 −96.1 15.102 10.603 9.666 LP 729−33 508 101209.0−312445 +273.6 +623.8 12.807 8.848 7.993 2MASS J10120908−3124451 509 101320.8+464725 −248.3 −82.3 15.756 10.873 9.982 LP 167−17 510 101453.0+212345 −192.4 −223.9 13.752 9.725 8.881 G 54−19 511 101510.8+284146 +364.7 −149.5 14.663 10.737 9.823 G 118−45 512 101811.9−202820 −385.1 +114.2 14.803 10.586 9.707 NLTT 23954 513 101813.6−202840 −392.2 +114.0 13.244 8.999 8.145 NLTT 23956 514 101836.0−114303 −344.6 −251.3 15.457 11.079 10.223 LP 729−55 515 102119.0+080426 −138.6 −93.2 14.934 10.789 9.934 NLTT 24099 516 102128.7+171243 −255.4 +44.2 15.512 11.230 10.356 LP 430−7 517 102213.4+264720 −287.8 −266.7 15.409 11.338 10.510 LP 316−89 518 102351.9+435333 +170.5 −2.1 14.553 10.039 9.127 2MASS J10235185+4353332 519 102502.7−090515 −424.9 −336.9 14.903 10.985 10.180 LHS 2258 520 102845.7−283037 −65.5 −11.1 15.684 10.953 10.026 2MASS J10284580−2830374 521 103232.9+063007 −235.3 −190.1 15.024 10.507 9.544 NLTT 24622 522 103425.7+461822 −420.4 −102.2 15.754 11.265 10.324 GJ 3611 B 523 103507.8−073238 −113.1 −316.0 15.591 11.189 10.358 LP 670−16 524 103832.5−071054 −31.2 +16.9 9.960 5.643 4.780 HD 92200 525 104144.1−311156 +355.1 −270.1 15.512 11.041 10.162 LP 904−51 526 104241.3−241603 +244.5 +136.3 15.642 10.277 9.338 NLTT 25128 527 104514.7+494129 +17.1 −217.8 15.193 11.125 10.219 NLTT 25223 528 104551.7−230901 −245.1 −141.5 14.456 10.044 9.176 LP 849−6

56 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

529 104712.4+402643 −294.8 −37.5 16.760 11.384 10.399 ** LDS 4016 530 104900.5+474553 −477.0 −183.9 15.255 11.112 10.205 LHS 2313 531 105032.6−132612 −237.1 +46.9 15.029 11.086 10.215 LP 731−65 532 105214.2+055509 −699.4 −58.3 14.159 9.834 8.941 GJ 3631 533 105310.4+415538 −243.2 +7.4 15.407 11.459 10.580 LP 213−82 534 105646.2+324627 −154.5 −75.4 14.782 10.653 9.817 2MASS J10564633+3246278 535 105703.7+221719 −158.1 −137.3 15.925 11.287 10.350 LP 373−35 536 105746.5+045332 +254.0 +183.3 15.389 11.134 10.238 NLTT 25837 537 105827.9−104630 −189.5 −76.0 13.792 9.512 8.640 LP 731−76 538 105906.1+301511 −531.0 −308.1 14.772 10.543 9.651 GJ 3635 539 110007.4+211450 −182.3 −36.0 15.206 11.107 10.251 2MASS J11000752+2114505 540 110032.8+064131 −284.1 −44.9 15.078 11.123 10.248 [ZEH2003] RX J1100.5+0641 5 541 110035.4+372849 −716.6 −246.8 14.746 10.659 9.746 LHS 2340 542 110050.4+120410 +123.7 −119.5 15.284 10.676 9.782 GJ 3636 543 110229.3+283400 −213.4 −19.9 15.294 11.191 10.333 LP 317−39 544 110354.0+241747 −533.4 −409.9 16.342 11.430 10.502 LHS 2345 545 110425.3−174809 +363.9 −311.2 15.206 10.826 9.867 LHS 5186 546 110506.8−221254 −65.4 −352.3 15.169 10.703 9.820 LP 849−51 547 110533.4+321352 +125.9 +99.3 16.020 11.408 10.498 LP 263−71 548 110750.2−342103 +23.5 −246.8 14.329 10.262 9.407 2MASS J11075025−3421003 549 110849.3+395512 −328.2 −159.1 15.272 10.747 9.842 LP 214−42 550 110953.2−241459 −11.1 +30.1 14.416 10.144 9.260 2MASS J11095327−2414594 551 111128.1−265503 −89.8 −19.0 15.386 10.331 9.453 1RXS J111128.1−265501 552 111212.4+251957 +259.5 −36.2 15.446 11.335 10.523 LP 374−7 553 111238.6+033845 +240.6 −34.7 15.355 11.098 10.243 NLTT 26626 554 111556.7+184159 −162.7 −10.7 15.560 11.428 10.551 2MASS J11155672+1841593 555 111859.5−351140 −94.8 −162.7 15.164 11.146 10.225 2MASS J11185965−3511385 556 111930.6+464141 +304.7 −611.5 15.028 10.087 9.199 LHS 2395 557 111948.0−163237 −357.3 +54.1 15.097 10.645 9.786 LP 792−14 558 112212.0−113216 −319.0 −19.0 16.243 11.475 10.587 2MASS J11221219−1132159 559 112242.8+375548 +245.3 +11.3 16.600 11.284 10.323 LP 264−45 560 112307.8+255336 −1009.1 −327.5 14.552 10.294 9.459 LHS 302 561 112404.3+380810 +123.8 −13.8 13.836 9.928 9.089 2MASS J11240434+3808108 562 112453.2+132253 −17.1 −50.4 15.726 11.043 10.070 2MASSI J1124532+132253 563 112500.4+431938 −524.1 −207.5 14.450 10.377 9.470 LHS 2403 564 112528.6−190154 +141.9 −168.0 14.729 10.673 9.789 LP 792−59 565 112931.7+094113 −93.4 −294.9 14.952 10.954 10.072 NLTT 27533 566 113123.9+053028 −321.4 +69.3 15.428 11.474 10.575 NLTT 27628 567 113218.2−301951 −88.5 −29.8 16.074 9.641 8.765 NAME SSS 113218−3019 568 113223.0+181622 −363.9 +49.3 14.137 10.175 9.338 2MASS J11322300+1816223 569 113241.1−265209 −101.3 −38.6 14.487 9.837 9.012 V* V549 Hya 570 113456.6+181707 −249.2 −429.3 14.681 10.533 9.703 G 56−47 571 113931.5−243900 −12.8 +177.4 15.338 11.353 10.443 LP 851−68 572 113933.7−304000 −88.7 −25.9 14.330 9.985 9.118 2MASS J11393382−3040002 573 114333.0−074549 −152.4 +38.8 15.053 10.899 10.065 2MASS J11433308−0745491 574 114742.1+001506 −305.9 −95.3 16.350 11.189 10.235 GJ 3686 B 575 114744.3+004816 +605.6 −1219.2 10.455 6.505 5.654 V* FI Vir 576 114825.9−380927 +12.1 +52.4 15.749 11.124 10.180 2MASSW J1148259−380927

57 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

577 114849.4+185653 +24.3 −304.9 15.093 10.876 10.030 LP 433−58 578 115155.3−013132 +145.4 −153.3 14.897 10.544 9.643 LP 613−62 579 115206.6+034119 −1.0 +229.9 15.317 11.397 10.526 LHS 2466 580 115257.9+242845 −321.1 +77.3 13.875 9.937 9.016 G 121−28 581 115745.5−014902 +397.7 −204.7 15.302 10.905 10.024 2MASS J11574552−0149023 582 120027.4−340537 −54.8 −15.4 13.767 9.606 8.723 2MASS J12002750−3405371 583 120028.2−000612 −102.8 −80.2 15.446 11.287 10.372 2MASS J12002826−0006123 584 120412.5+051412 −187.9 −151.8 14.764 10.217 9.317 NLTT 29470 585 120446.3+022400 −203.0 −1.0 15.797 11.401 10.567 NLTT 29510 586 120513.9−253349 +189.3 −215.1 15.387 11.470 10.606 LP 852−6 587 120546.6−184934 −14.6 −312.7 15.457 11.199 10.317 ** WNO 54B 588 120617.4+123024 −182.2 +22.8 15.031 11.127 10.240 2MASS J12061746+1230249 589 120624.9+001602 +39.4 −127.5 14.393 10.348 9.475 2MASS J12062495+0016025 590 120818.2−210106 +36.5 −274.2 15.843 11.115 10.231 LP 794−23 591 120843.8−113346 +245.7 −325.6 15.710 11.000 10.175 LP 734−29 592 120906.7+473604 +587.4 −297.2 14.360 10.239 9.346 LHS 2516 593 120906.8+473534 +587.1 −297.8 15.383 11.095 10.225 LHS 2517 594 121028.4−131025 +242.8 −348.4 13.202 9.292 8.412 LP 734−34 595 121314.9−210831 −373.0 +128.9 14.973 11.071 10.240 LP 794−38 596 121408.6−234516 +38.8 +84.7 13.245 9.067 8.234 2MASS J12140866−2345172 597 121416.5+003726 −956.8 −278.4 13.035 8.456 7.540 GJ 1154 598 121731.6+251826 +26.6 −69.5 15.431 11.395 10.494 2MASS J12173161+2518272 599 121837.8−202407 −324.6 +34.5 14.927 10.891 10.033 LP 794−49 600 121841.9−060912 +106.7 −31.5 14.135 10.117 9.280 2MASS J12184187−0609123 601 121847.1+294448 −207.2 −413.8 15.593 11.021 10.089 LP 320−359 602 121948.7−233205 −221.6 −25.0 14.526 10.489 9.580 LP 52−34 603 122004.9−181259 −241.3 +50.2 14.858 10.564 9.623 LP 794−53 604 122126.6+303837 −198.3 −262.0 14.632 10.057 9.169 G 148−47 605 122127.0+303835 −110.9 −310.3 14.479 10.057 9.169 G 148−48 606 122203.9−062913 +52.4 −329.0 15.180 10.987 10.118 LP 675−4 607 122229.4+400337 −169.9 +8.2 14.917 10.966 10.121 2MASS J12222948+4003372 608 122250.5−040446 −188.9 −334.1 13.716 9.662 8.825 G 13−33 609 122501.0+232316 −136.0 −304.4 15.694 11.456 10.619 LP 376−62 610 122520.6−174946 −119.0 −14.4 15.175 10.894 9.993 2MASS J12252074−1749468 611 122651.3−331612 −66.2 −25.9 15.361 10.691 9.783 2MASS J12265135−3316124 612 122657.3+270053 +88.6 −245.2 14.343 10.197 9.320 V* CX Com 613 122702.0−254502 −298.9 −256.6 14.946 10.837 9.928 LP 852−50 614 122850.5−083424 −169.5 −82.4 15.552 11.449 10.624 LP 675−62 615 122945.2−284731 −99.4 −24.0 15.741 11.129 10.269 LP 909−5 616 122954.3−052722 −717.2 −408.2 13.527 8.818 7.962 LHS 2567 617 123124.1−063801 +449.2 −226.0 15.398 11.328 10.434 LHS 5217 618 123317.3+090115 −1756.9 +211.8 11.804 6.995 6.042 Wolf 424 619 123405.0+134545 +58.6 −156.7 15.185 11.217 10.373 2MASS J12340501+1345458 620 123517.2+131806 +93.8 +203.2 17.170 11.225 10.365 NLTT 31198 621 123548.9−395024 −50.4 −27.0 13.737 9.790 8.943 TWA 11C 622 123628.5+351200 −351.6 −117.4 13.153 9.113 8.261 G 123−45 623 123943.5+253045 −179.9 −152.2 14.296 10.242 9.394 GJ 3739 624 124016.8+125359 −259.8 −1.1 15.749 11.460 10.554 LP 495−235

58 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

625 124128.9+190500 +68.6 −305.4 14.284 10.368 9.477 G 59−34 626 124229.6+250341 +22.7 +16.2 14.728 10.734 9.790 LP 377−54 627 124400.6−111030 −483.7 −155.3 13.582 9.516 8.674 LHS 5226 628 124422.7+042123 +32.6 +7.5 15.079 10.788 9.958 LHS 2619 629 124853.4+120432 +229.8 −145.5 15.308 11.400 10.570 2MASS J12485345+1204326 630 125431.9+445934 −650.2 −267.9 15.332 10.874 9.986 LHS 2650 631 125450.7+115914 −267.7 −396.5 15.013 10.509 9.621 LP 496−48 632 125750.6+375950 +43.6 +79.1 15.146 10.948 10.002 LHS 2655 633 125923.9+074354 −680.4 +2.0 15.324 10.740 9.838 LHS 2657 634 130033.3+225540 +51.4 −13.4 15.119 11.016 10.184 V* KZ Com 635 130033.4+054108 −942.4 +225.4 12.744 8.553 7.660 Wolf 461 636 130040.1−201045 −291.1 −153.1 14.822 10.814 9.918 LP 796−24 637 130425.8+140510 −245.7 −28.0 15.293 11.231 10.374 NLTT 32773 638 130523.7+211208 −193.3 +45.5 15.257 11.323 10.481 LP 378−405 639 130650.3+305052 +173.8 −475.0 14.802 10.226 9.315 LHS 2674a 640 130710.9+150431 +59.0 −169.7 15.789 11.363 10.459 NLTT 32923 641 130720.7−101946 −359.1 −45.5 15.040 10.908 10.019 LP 736−27 642 130841.1+090658 −200.6 −128.0 15.379 11.267 10.326 NLTT 33004 643 130934.9+285906 −348.6 −197.8 13.520 9.476 8.612 GJ 1167 A 644 131012.4+474517 −634.1 −612.4 13.822 9.584 8.687 LHS 2686 645 131121.5+283240 −410.9 −448.0 15.287 10.841 9.966 LHS 2691 646 131151.7+252050 −454.0 −164.4 15.030 10.736 9.843 LHS 5240 647 131420.3+132000 −242.4 −176.1 15.082 9.754 8.794 NLTT 33370 648 131551.1+400608 +135.1 −85.7 14.608 10.696 9.841 2MASS J13155111+4006086 649 131634.5−273913 −125.5 −143.0 15.714 11.479 10.611 LP 910−62 650 132017.4−022413 +75.8 −201.0 14.559 10.636 9.817 LP 617−34 651 132138.0+395948 −40.5 +41.3 14.614 10.608 9.767 LP 218−84 652 132154.0−142409 −218.2 +78.3 13.757 9.817 8.985 LP 737−51 653 132426.3−105222 −25.4 −32.2 15.381 11.388 10.532 654 132440.8+005932 −115.0 −439.1 13.879 9.976 9.091 LHS 6253 655 132657.9+150542 +58.8 +11.1 15.274 11.079 10.166 LP 437−81 656 132726.7−334546 +33.8 −15.5 17.236 9.680 8.833 LHS 5246 657 132909.8+111837 −71.3 −190.4 14.376 10.452 9.485 NLTT 34250 658 133002.6−084226 −1117.6 −471.3 13.694 9.599 8.749 BD−07 3632B 659 133031.0+190934 −506.3 −1289.1 14.129 10.065 9.221 LHS 355 660 133239.0+305906 −199.1 −81.2 13.687 9.620 8.762 ** LDS 1392 661 133328.0+123850 −87.5 −344.5 15.057 11.107 10.267 LP 498−6 662 133600.0+402412 +35.8 +29.8 14.858 10.717 9.823 2MASS J13360002+4024118 663 133840.9−113208 +144.1 −88.7 13.664 9.714 8.814 UCAC3 157−131101 664 133915.9+092236 +84.3 −314.9 14.514 10.526 9.629 NLTT 34786 665 133938.6−205818 −142.6 −118.8 15.364 11.406 10.580 LP 798−75 666 134019.0+471228 +285.2 −486.2 14.767 10.685 9.864 LHS 2777 667 134341.6−400229 +222.6 −108.5 14.328 10.137 9.248 2MASS J13434146−4002292 668 134618.5+071337 +107.0 −115.6 14.689 10.726 9.792 2MASS J13461853+0713382 669 134809.1+042916 −168.5 −66.9 15.089 10.746 9.839 NLTT 35270 670 134813.3+233648 −1479.1 +118.3 14.692 10.082 9.179 LHS 362 671 134840.8−051710 +244.8 −464.2 14.244 10.329 9.403 LHS 2804 672 134848.6+040601 −3.8 −182.5 13.690 9.755 8.882 Wolf 1494

59 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

673 135028.0+052736 −127.2 −116.0 15.451 11.237 10.339 2MASS J13502806+0527368 674 135035.8+033038 −804.9 −112.0 14.699 10.685 9.789 LHS 2811 675 135157.0−175849 −110.9 −17.2 14.913 10.823 9.927 LP 798−49 676 135620.4−280350 −507.8 −86.3 14.444 10.480 9.565 LHS 2826 677 135816.0−120258 −335.9 +41.2 13.808 9.728 8.887 LP 739−2 678 135820.7+110049 +197.9 −483.3 15.328 10.830 9.988 LHS 2831 679 140035.3+213301 −405.6 −145.5 15.172 11.074 10.270 G 150−56 680 140133.1+122726 −453.1 −420.9 14.945 11.004 10.191 LHS 2844 681 140223.4+430059 −132.0 +92.8 15.177 11.037 10.126 2MASS J14022347+4300591 682 140536.9−320840 +81.0 −204.4 14.669 10.701 9.800 LP 912−48 683 140555.9−164332 −185.6 −57.5 14.627 10.721 9.857 LP 799−63 684 140651.4+313346 +53.4 −375.1 15.159 10.893 10.038 LP 324−70 685 140735.4−060051 −305.9 −684.4 15.154 10.880 9.973 LHS 2862 686 140931.9+413808 −219.3 +73.3 15.189 10.706 9.848 LP 220−50 687 140951.6+072425 −192.0 −49.9 15.409 11.087 10.140 NLTT 36435 688 141304.7−120127 −619.7 −381.3 13.248 9.040 8.163 V* GQ Vir 689 141320.5+002304 +76.7 −160.4 14.845 10.741 9.880 2MASS J14132052+0023047 690 141415.2+284724 +209.9 −287.5 15.312 10.935 10.075 LP 325−4 691 141545.7+062505 +249.0 −128.5 14.663 10.681 9.771 NLTT 36747 692 141702.7+314246 −582.7 −147.4 12.489 8.443 7.609 GJ 3839 693 141707.3+085136 −139.4 +17.9 13.229 9.109 8.198 PM I14171+0851 694 141929.5+025436 −199.6 −146.5 14.328 9.954 9.072 NLTT 36959 695 142036.4+313004 −207.4 −63.5 15.092 10.786 9.907 LP 325−24 696 142052.7+365717 −1353.2 +226.6 15.642 11.054 10.254 LHS 370 697 142055.4+121806 −383.5 −138.0 14.882 10.912 10.036 2MASS J14205545+1218068 698 142219.9+235235 −248.8 +40.6 14.818 10.516 9.647 LP 381−49 699 142243.3+162446 −188.9 +39.3 14.416 10.303 9.452 NLTT 37131 700 142307.7−221710 −273.1 −464.4 14.303 10.402 9.504 LHS 2906 701 142323.7−145533 −164.0 +306.9 15.397 11.062 10.191 LP 740−6 702 142343.7+142651 +331.5 −548.8 16.521 11.218 10.256 LHS 2909 703 142513.1−162455 −368.6 +20.0 16.485 11.477 10.488 LP 800−58 704 142524.1+213151 −220.3 +105.8 15.507 11.034 10.144 NLTT 37289 705 142534.6+254005 −51.3 −15.5 16.640 11.083 10.105 2MASS J14253465+2540050 706 142649.7−325649 +104.0 −18.1 15.339 11.181 10.292 2MASS J14264969−3256489 707 142756.0−002231 +528.3 −85.6 13.324 9.305 8.403 GJ 1183 A 708 142756.4−002219 −276.1 +251.2 13.422 9.345 8.461 I14279-002En 709 142804.1+135613 −360.2 −491.1 16.647 11.014 10.026 LHS 2919 710 142831.5+455433 −873.5 +105.2 16.177 11.336 10.434 LHS 2921 711 142837.9+405704 +216.3 −177.0 15.277 11.354 10.516 LP 221−118 712 142959.5+293401 −232.0 −471.1 14.014 10.072 9.238 LHS 2925 713 143104.4−030716 −335.0 +15.8 14.274 10.212 9.327 714 143152.8−151551 +153.1 −86.1 15.245 11.115 10.273 LP 740−58 715 143153.5−134611 −157.9 −198.6 15.323 11.247 10.375 LP 740−25 716 143208.4+081131 −512.2 +28.1 14.993 10.108 9.166 LHS 2935 717 143331.3+341747 −98.4 −36.1 16.674 11.451 10.554 NDWFS J143331.4+341747 718 143345.6−312441 −27.3 −28.7 15.304 11.310 10.422 2MASS J14334561−3124412 719 143404.7−182411 −503.7 +26.4 13.729 9.580 8.708 LHS 5273 720 143718.4+265259 −225.3 +87.2 15.143 11.022 10.125 LP 325−68

60 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

721 143723.8−024250 −360.1 −28.1 15.261 11.312 10.500 LP 620−41 722 144158.7−164902 −195.7 −260.0 14.271 10.225 9.390 2MASS J14415883−1649008 723 144347.0−130715 −6.3 +4.7 10.463 6.539 5.570 HD 129603 724 144414.9−271725 −264.9 −42.6 14.994 10.891 10.036 LP 858−20 725 144433.3+364159 −49.2 −108.8 14.680 10.727 9.871 2MASS J14443334+3642002 726 144440.0−221447 −113.6 −334.4 14.701 10.569 9.644 LP 858−23 727 144600.8+463323 +481.2 −399.5 14.061 10.138 9.308 LHS 2973 728 145158.0+025912 −75.1 −159.1 15.234 11.277 10.440 2MASS J14515804+0259130 729 145337.1+113412 +73.8 −724.6 14.700 10.577 9.652 LHS 2995 730 145410.4−204129 −105.6 −277.6 14.362 10.256 9.348 LP 801−25 731 145627.1+175459 −849.2 +494.8 15.134 10.742 9.852 LHS 3001 732 145925.0+361832 −123.9 +76.1 14.292 10.257 9.377 2MASS J14592508+3618321 733 150049.9−153308 −385.6 −134.7 15.508 11.494 10.545 LP 741−28 734 151012.0+462405 +389.9 −398.1 14.542 10.629 9.810 LHS 3031 735 151315.8−113333 −62.9 −69.0 15.292 11.260 10.392 2MASS J15131587−1133329 736 151411.5+030046 +149.1 −72.0 15.507 11.252 10.343 2MASS J15141149+0300467 737 151416.8−095839 −127.0 −126.3 13.589 9.665 8.780 PM I15142-0958 738 151628.0−210216 −213.0 −194.5 15.668 11.478 10.594 LP 802−13 739 151640.6+391048 −209.5 −60.1 16.361 10.796 9.813 LP 222−65 740 151655.7−003711 −119.3 −190.9 13.884 9.960 9.105 2MASS J15165576−0037116 741 151831.4+203628 +10.1 +94.8 14.786 10.119 9.268 2MASS J15183145+2036279 742 151907.8+142447 −81.0 −29.4 15.055 11.024 10.200 2MASS J15190781+1424478 743 151921.1+340342 −168.4 −202.5 14.669 10.460 9.537 2MASS J15192126+3403431 744 152115.9+394516 −438.4 +182.0 15.737 10.732 9.745 NLTT 40017 745 152332.6+220326 −21.5 −283.0 15.384 11.172 10.325 NLTT 40109 746 152351.1+172757 −399.7 −1261.2 13.116 9.105 8.279 LHS 396 747 152419.6+201125 −144.2 +95.8 15.057 11.033 10.154 2MASS J15241967+2011252 748 152543.5+311211 +20.0 −245.8 15.096 10.651 9.699 NLTT 40208 749 152724.1+371415 −142.2 +121.5 15.073 11.043 10.239 2MASS J15272423+3714148 750 152725.4+173132 +10.7 −183.5 15.577 11.370 10.511 LP 442−53 751 152745.0−090135 +25.1 −307.5 14.473 10.552 9.632 GJ 586 C 752 152902.8+464623 −118.3 −21.9 14.075 9.942 9.114 2MASS J15290296+4646240 753 152944.0+425247 +423.7 −617.9 13.571 9.587 8.719 LHS 3075 754 153030.3+092601 −185.4 +182.8 14.431 9.569 8.661 NLTT 40406 755 153109.5−350457 −46.9 −32.6 14.669 10.718 9.797 2MASS J15310958−3504571 756 153154.1+285109 −545.7 +34.1 13.681 9.673 8.820 GJ 3910 757 153340.4−391747 −47.4 −68.5 13.743 9.837 9.021 [SZB2012] 75 758 153427.0+152832 −123.6 −191.0 14.866 10.773 9.950 LP 443−16 759 153450.8+180012 −221.5 −325.5 14.958 10.595 9.713 LP 443−17 760 153507.5−065522 −9.7 −16.2 14.607 10.571 9.705 761 153535.7+291257 −203.0 +167.6 15.269 11.126 10.249 2MASS J15353572+2912577 762 154554.4−044823 −528.6 −282.9 16.078 11.341 10.426 LHS 3112 763 154623.3+310254 −320.2 +250.3 15.880 11.135 10.264 LP 328−40 764 154715.1+014921 −231.1 −53.4 15.932 10.637 9.667 NLTT 41186 765 154740.6+224116 −180.9 −29.5 13.589 9.543 8.647 2MASS J15474070+2241165 766 155009.7−202912 −190.9 −308.0 14.927 10.896 9.999 LP 803−37 767 155042.6−035846 −19.5 −26.8 15.313 10.447 9.470 768 155051.4+182538 −21.2 −262.2 14.958 10.848 9.957 NLTT 41333

61 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

769 155244.6−262315 +213.7 −455.5 15.773 10.258 9.315 LHS 5303 770 155531.7+351203 −231.7 +156.2 13.034 8.928 8.041 G 180−11A 771 155836.2−234802 −13.9 −16.0 15.055 11.110 10.192 UCAC3 133−177729 772 155918.3−221043 −12.7 −26.3 15.573 11.044 10.073 2MASS J15591839−2210430 773 155929.2+232139 −329.7 +513.0 14.918 10.975 10.066 LHS 3140 774 160015.6−223158 −7.4 −28.2 15.285 11.365 10.442 2MASS J16001567−2231580 775 160110.3−222227 −13.8 −29.7 15.116 10.732 9.758 2MASS J16011037−2222276 776 160113.9−251628 −13.0 −15.5 15.370 11.357 10.419 777 160121.5−223726 −10.6 −20.2 15.154 11.026 10.052 2MASS J16012156−2237265 778 160123.7−241948 −46.3 −54.8 16.078 11.448 10.541 2MASS J16012373−2419483 779 160127.7+211613 −62.9 −89.5 14.675 10.772 9.832 [SLS2012] PYC J16014+2116 780 160129.8−224838 −9.8 −31.5 15.835 11.480 10.490 2MASS J16012985−2248386 781 160144.4+302741 −140.8 +125.7 14.537 10.427 9.540 GJ 3936 B 782 160158.9−224037 −20.3 −26.6 15.375 11.350 10.434 2MASS J16015894−2240368 783 160241.6+013158 −139.9 −536.9 16.136 10.887 10.033 2MASS J16024164+0131580 784 160350.0−180545 −5.3 −23.8 16.417 11.489 10.499 2MASS J16035008−1805459 785 160413.1+233138 −160.6 +12.7 14.373 9.971 9.065 2MASS J16041322+2331386 786 160419.9−061648 −68.7 −862.7 14.983 10.452 9.548 LHS 3149 787 160451.5−210417 −13.4 −28.0 15.806 11.283 10.341 2MASS J16045155−2104169 788 160501.7−241133 −8.1 −18.5 14.980 10.845 9.914 2MASS J16050179−2411327 789 160628.7−200357 −19.3 −32.0 15.824 11.442 10.464 2MASS J16062872−2003571 790 160629.3−240723 −325.9 +207.6 14.288 10.364 9.511 LP 861−22 791 160633.7+405422 −719.3 +160.6 16.135 11.050 10.072 LHS 3154 792 160728.5−240754 −15.8 −30.3 15.381 11.139 10.247 2MASS J16072853−2407543 793 160744.4−203603 −10.0 −20.9 14.194 10.076 9.077 2MASS J16074449−2036030 794 160758.7−244132 −5.9 −23.9 14.909 10.752 9.828 2MASS J16075875−2441319 795 160843.0−190051 −11.8 −26.0 15.584 11.245 10.268 2MASS J16084309−1900519 796 160903.9−193945 −7.8 −35.1 15.468 11.338 10.369 2MASS J16090397−1939456 797 160959.3−180009 −11.0 −26.3 15.630 11.306 10.343 2MASS J16095933−1800090 798 161001.8−234943 −11.0 −21.7 15.387 11.062 10.134 2MASS J16100184−2349432 799 161021.5−194132 −5.0 −2.8 14.946 10.826 9.860 2MASS J16102152−1941318 800 161026.3−193951 −10.8 −29.9 15.813 11.314 10.402 2MASS J16102639−1939513 801 161036.2+094715 +1.4 −584.3 15.700 11.331 10.502 LHS 3162 802 161058.3−063134 −51.1 −189.2 16.776 11.348 10.371 LP 684−33 803 161116.6−193910 −14.4 −25.4 14.483 10.525 9.547 2MASS J16111662−1939103 804 161248.2+110417 −331.7 +325.7 15.551 11.362 10.510 NLTT 42255 805 161310.2−190413 −7.7 −32.1 14.709 10.628 9.647 2MASS J16131023−1904131 806 161411.5−142131 +116.6 −168.1 14.727 10.128 9.234 G 153−36 807 161530.3−325102 −228.1 −220.7 14.175 10.272 9.421 LP 917−23 808 161554.8−231514 −7.2 −15.8 15.345 11.275 10.329 2MASS J16155487−2315146 809 161620.1−234414 −13.7 −29.4 15.434 11.079 10.187 2MASS J16162012−2344141 810 161910.5+195726 +17.9 −9.8 15.184 10.967 10.156 NLTT 42501 811 162107.4+150431 −326.7 +94.4 15.204 11.270 10.440 LP 445−8 812 162141.2−221205 −14.9 −29.1 15.191 10.909 9.941 WSB 10 813 162357.2−262024 −7.4 −20.8 15.282 11.188 10.235 1AXG J162356−2620 814 162524.0+485416 −230.5 +309.5 14.765 10.823 9.971 G 202−47 815 162619.7+364056 −194.1 +852.8 15.720 11.430 10.535 LHS 3196 816 162648.0−172335 −330.5 −411.7 13.707 9.548 8.682 GJ 3954

62 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

817 162944.2−244121 −9.0 −20.9 14.455 10.082 9.144 2MASS J16294427−2441218 818 162949.3+163624 +27.3 +22.5 13.596 9.589 8.777 2MASS J16294932+1636245 819 163019.3+124955 −140.2 −185.3 15.044 10.925 10.035 NLTT 42951 820 163035.6+051020 −213.8 +24.9 15.245 11.332 10.476 NLTT 42959 821 163118.7+405152 −148.3 +310.3 14.073 9.461 8.506 GJ 3959 822 163123.8+220741 +16.9 −156.4 15.123 11.187 10.337 2MASS J16312383+2207426 823 163226.7−285312 +60.1 −82.2 14.746 10.791 9.970 1RXS J163226.4−285313 824 163425.1+475028 −477.7 −55.0 14.847 10.743 9.862 LHS 6308 825 163605.8−044013 −417.7 −64.2 15.493 11.053 10.183 LP 685−36 826 163701.4+353543 −197.3 −509.9 15.898 11.135 10.240 LHS 3227 827 164005.9+004218 +176.0 −157.5 13.056 9.116 8.209 GJ 3967 828 164049.0−272521 +51.7 −185.7 15.720 11.479 10.589 2MASS J16404898−2725204 829 164134.9+042711 −111.5 −358.6 15.629 11.497 10.636 NLTT 43373 830 164205.9−170958 −323.1 −421.4 15.316 11.123 10.244 LHS 3237 831 164214.9+415942 −132.3 −265.3 14.525 10.500 9.618 G 203−21 832 164543.3+044440 −86.0 −470.9 15.274 10.713 9.791 LHS 5321 833 164631.4+343453 −382.7 −389.5 15.951 10.533 9.606 LHS 3241 834 165057.9+222706 +30.3 +397.1 13.426 9.136 8.309 GJ 3976 835 165109.9+355507 −71.5 +171.7 14.297 10.334 9.488 LP 276−29 836 165221.1+400619 +22.3 +201.2 15.187 11.267 10.466 LP 226−3 837 165633.5−204638 −193.1 −188.7 16.593 11.299 10.368 2MASS J16563362−2046373 838 165904.0+382259 +70.2 −30.4 15.380 11.058 10.190 2MASS J16590404+3822593 839 170335.8+081814 −101.3 −346.2 15.454 11.374 10.490 2MASS J17033581+0818146 840 170359.6+011423 +0.5 −0.7 13.710 9.275 8.407 V* V371 Oph 841 170712.5+413644 −160.3 +105.9 14.792 10.690 9.826 LP 226−38 842 170740.8+072206 −493.5 −375.2 13.439 9.284 8.419 GJ 1210 843 171146.1+402901 +249.1 +82.1 15.098 11.074 10.271 G 203−50 844 171518.9+045750 +578.4 −746.2 14.086 9.750 8.782 GJ 1214 845 171744.0+114011 −345.5 −416.9 14.405 9.817 8.931 LHS 3277 846 171855.8+364223 +64.1 −409.5 15.317 11.374 10.533 2MASS J17185585+3642246 847 171932.7−123005 −82.3 −519.7 15.407 11.273 10.453 2MASS J17193275−1230032 848 171952.9+263003 −234.1 +358.5 12.342 8.229 7.351 Ross 867 849 172042.5+420506 +155.1 −215.9 13.840 9.895 9.000 G 203−60 850 172102.7+125844 −247.9 +136.1 15.347 11.064 10.170 LP 507−15 851 172154.5+212547 −154.5 +268.9 13.248 9.344 8.492 GJ 4003 852 172441.7+042248 +143.1 −192.8 15.189 10.794 9.847 NLTT 44733 853 172635.7+203125 −53.1 −27.4 15.595 11.044 10.140 NLTT 44801 854 172811.0−014357 +100.4 −159.7 13.858 9.889 9.010 2MASS J17281105−0143569 855 173103.9+350408 −95.3 +163.5 14.856 10.863 9.959 2MASS J17310397+3504074 856 173145.1+305604 +35.2 −225.2 14.962 10.926 10.067 LP 332−33 857 173314.3+255704 −79.9 −326.7 15.279 11.272 10.387 NLTT 45038 858 173353.1+165512 −108.6 −133.1 13.700 8.895 7.995 2MASS J17335314+1655129 859 173408.6−084952 −188.2 −317.9 15.240 10.905 10.055 LP 688−3 860 173540.8+085641 +61.8 +20.6 14.969 10.871 10.015 [SLS2012] PYC J17356+0856 861 173807.1−085537 −17.6 −301.0 15.532 11.100 10.180 LP 688−8 862 174629.3−084237 −37.6 −424.6 12.194 8.198 7.353 Wolf 1473 863 175135.5+374936 −93.2 +346.9 15.433 10.442 9.496 LP 278−42 864 175530.6−045542 +66.8 +40.0 14.600 10.696 9.784 2MASS J17553063−0455424

63 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

865 175549.7+384213 −293.7 +33.8 15.611 11.473 10.591 LP 278−50 866 175652.1+190555 −242.2 −216.2 14.866 10.625 9.740 2MASS J17565213+1905558 867 180233.9+363045 −86.9 −242.0 15.161 11.077 10.251 LP 278−58 868 180246.2+373101 +180.1 −1139.2 14.257 9.720 8.887 LHS 457 869 180918.0+270626 +58.3 +226.7 14.407 10.461 9.572 NLTT 46025 870 181152.2+322521 −150.5 +326.1 14.872 10.885 10.024 G 206−16 871 181155.4+322547 −153.4 +322.6 15.945 11.498 10.581 NLTT 46103 872 181534.7+395259 +15.4 −147.8 14.644 10.665 9.812 2MASS J18153472+3953004 873 181835.4−371013 −32.8 −114.3 13.949 9.778 8.924 [SZB2012] 103 874 182757.8+372416 −3.0 +335.5 15.244 11.182 10.337 LP 279−37 875 183055.2+473601 −26.2 +330.9 15.760 11.258 10.384 LP 182−4 876 183202.9+203057 −50.7 −208.3 14.569 10.653 9.756 LSPM J1832+2030S 877 183948.4+164849 +135.1 −96.8 16.219 11.425 10.528 2MASS J18394841+1648497 878 184107.0−375011 +6.9 −5.9 10.035 5.909 4.998 V* U CrA 879 184237.1+311105 −238.3 −328.9 15.228 11.152 10.273 G 206−41 880 184607.4−325008 +20.2 −131.6 15.919 11.429 10.549 2MASS J18460763−3250107 881 185233.7+453833 +208.2 +466.8 14.419 10.493 9.673 LHS 3420 882 185639.7−370721 −0.2 −24.5 16.281 10.990 10.046 2MASS J18563974−3707205 883 185659.2−401143 +20.2 −205.4 14.784 10.607 9.729 2MASS J18565922−4011415 884 190201.0+411403 +34.4 +210.9 15.576 11.411 10.513 2MASS J19020105+4114024 885 190712.7+441607 +116.1 +172.0 14.592 10.447 9.559 LP 230−29 886 191228.1+382615 +280.3 −180.3 16.069 11.201 10.311 2MASS J19122805+3826161 887 191306.1−231206 +167.9 −357.4 16.339 11.434 10.516 2MASS J19130608−2312052 888 191731.5+283314 −2.9 −220.9 15.331 10.758 9.923 2MASS J19173151+2833147 889 191941.0+412748 +82.8 −187.8 16.069 11.259 10.374 LP 230−40 890 192434.9−344239 +20.8 −65.8 13.653 9.670 8.785 2MASS J19243494−3442392 891 192752.7−281117 +63.0 −97.7 14.215 9.687 8.786 LHS 5348 892 193104.6−030617 +207.2 +478.8 16.100 11.147 10.228 2MASS J19310458−0306186 893 193530.4−072940 −2.6 −18.1 13.450 8.640 7.672 TYC 5156−662−1 894 193823.3+002104 −10.0 −1.3 14.803 9.829 9.004 895 194212.8−204548 −12.5 −134.0 13.597 9.598 8.756 2MASS J19421282−2045477 896 194307.3+451810 +122.2 +269.3 16.256 11.331 10.380 2MASS J19430726+4518089 897 194453.9−233800 +319.6 −167.3 13.442 9.169 8.265 LP 869−26 898 194822.5−082253 −445.5 −379.2 15.866 11.120 10.191 2MASS J19482268−0822520 899 195354.5+442452 +49.3 −507.0 12.801 7.791 6.854 ** GIC 159 900 195723.7−123351 −92.4 −522.6 14.770 10.212 9.318 GJ 773 B 901 195751.8−105305 −395.0 −291.9 13.743 9.730 8.843 LP 754−8 902 200428.4−335611 +74.9 −105.8 13.982 10.042 9.170 2MASS J20042845−3356105 903 200430.8−234204 +128.3 −342.8 12.468 8.559 7.701 LP 870−65 904 200457.0+032107 −102.8 −332.1 14.559 10.052 9.181 2MASS J20045709+0321076 905 201040.2+404008 +295.9 −92.5 14.755 10.795 9.941 G 209−18 906 201055.5−253512 +5.4 +3.4 14.214 10.217 9.352 LHS 3528 907 201117.4−291758 +104.7 −81.5 15.604 10.937 10.015 2MASS J20111744−2917584 908 201249.3−313024 +178.8 −412.9 14.452 10.481 9.572 LP 926−43 909 201259.9+011258 −12.3 +65.7 15.114 10.486 9.585 2MASS J20125995+0112584 910 201314.0+150031 −3.7 −4.2 12.614 8.577 7.613 V* V586 Aql 911 201455.5+394326 −4.9 −136.4 14.447 10.297 9.457 2MASS J20145550+3943272 912 201741.2−182036 +219.8 −155.0 15.479 11.468 10.571 LP 814−43

64 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

913 201902.8+220521 −3.6 +3.6 12.217 7.333 6.399 HD 346301B 914 201909.2+143816 −84.6 −341.8 15.736 11.440 10.588 LP 515−4 915 202214.6+403002 −34.7 −14.7 10.537 6.590 5.600 TYC 3156−1652−1 916 202235.8−122254 −4.5 +2.9 10.423 5.991 5.127 HD 193802 917 202322.1+080014 +30.0 −225.3 14.518 10.318 9.407 2MASS J20232212+0800149 918 202438.7+393030 −4.0 −4.3 13.179 9.213 8.247 2MASS J20243873+3930300 919 202616.4+373301 −402.5 +358.6 14.353 10.409 9.440 2MASS J20261645+3733012 920 202910.5+160120 −56.4 +148.9 15.285 11.258 10.382 2MASS J20291058+1601202 921 202948.3+094120 +697.6 +209.9 12.496 8.228 7.307 GJ 791.2 922 202958.6+205434 −133.6 −214.0 14.981 11.051 10.199 2MASS J20295868+2054344 923 203001.9+002355 +120.5 +11.1 13.904 9.911 9.093 I20300+0023 924 203235.3+355835 +126.7 +119.1 15.304 11.340 10.493 2MASS J20323532+3558353 925 203238.4+404044 −1.7 −3.5 12.406 8.347 7.383 [CPR2002] A25 926 203243.8+404217 −2.2 −2.9 14.168 10.231 9.292 SDSS J203243.87+404217.1 927 203256.4+411207 −0.4 −1.6 15.050 11.074 10.092 2MASS J20325647+4112075 928 203302.9+404725 −0.9 −2.6 11.449 7.251 6.274 [CPR2002] A20 929 203311.2+404233 −19.3 −1.1 13.072 9.084 8.105 [CPR2002] A22 930 203315.7+282344 −247.5 −295.5 13.904 9.963 9.097 G 210−26 931 203337.6−255652 +55.4 −75.3 14.251 9.712 8.877 2MASS J20333759−2556521 932 203346.7−373345 +76.1 −112.4 15.756 10.848 9.957 2MASS J20334670−3733443 933 203417.1+410630 −2.7 −2.6 14.191 10.121 9.141 2MASS J20341716+4106305 934 203817.1+402105 −2.0 −6.3 14.057 10.046 9.098 2MASS J20381712+4021059 935 203846.0−210645 −206.8 +60.3 15.331 10.973 10.115 LP 871−38 936 204033.9+152959 +1320.4 +657.4 12.778 8.641 7.749 LHS 495 937 204110.9+180005 +143.1 +61.4 16.022 11.331 10.422 2MASS J20411094+1800050 938 204147.4+493848 +157.5 +50.5 14.772 10.416 9.541 2MASS J20414744+4938482 939 204245.2−050018 +233.9 +110.9 16.721 11.449 10.539 LP 695−372 940 204323.9+044555 +465.5 −146.7 14.687 10.083 9.136 LHS 5358 941 204522.1+350815 +376.6 +122.5 14.838 10.497 9.623 2MASS J20452209+3508146 942 204611.9+221956 +158.4 +35.0 15.315 11.399 10.528 2MASS J20461188+2219562 943 205113.6−132916 +651.2 −170.8 15.566 11.424 10.612 2MASS J20511351−1329161 944 205231.4−014709 −88.8 −53.5 15.005 10.896 10.070 LP 636−16 945 205309.1−013304 +354.6 −218.7 15.044 10.659 9.793 2MASS J20530910−0133039 946 205323.8−041637 +190.9 −442.9 15.738 11.420 10.549 LP 696−13 947 205333.0+103701 −490.8 −448.7 13.343 9.348 8.481 LHS 3593 948 205500.8+035529 +42.1 −82.1 15.533 11.498 10.669 [SLS2012] PYC J20550+0355 949 205912.6−342735 +289.9 −244.4 15.431 11.349 10.490 2MASS J20591244−3427335 950 210009.0+433108 +133.6 +13.0 15.860 11.292 10.377 951 210133.3+395703 −151.0 +7.5 15.470 10.990 10.116 2MASS J21013344+3957037 952 210246.1+345435 +235.3 −253.7 13.990 9.846 9.001 G 211−9 953 210251.5−070248 +78.7 −56.7 15.102 11.135 10.256 2MASS J21025150−0702487 954 210312.9+220832 +170.9 +63.8 15.403 11.356 10.477 2MASS J21031292+2208318 955 210343.5+171648 +208.0 +21.1 14.961 10.976 10.095 G 144−57 956 210435.5+021159 −17.4 −316.9 15.408 11.386 10.432 NLTT 50464 957 210603.2+221848 −21.2 −198.2 15.970 11.311 10.377 2MASS J21060322+2218480 958 210616.6+443702 −26.8 −135.0 15.239 10.969 10.128 959 210954.6+472904 +417.9 +153.9 15.802 11.487 10.633 2MASS J21095447+4729043 960 211004.6−192030 +83.8 −91.2 12.524 8.428 7.552 BPS CS 22898−0066

65 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

961 211031.0−271052 +64.6 −69.3 16.213 11.200 10.236 2MASS J21103096−2710513 962 211031.5−271058 +43.0 −58.5 14.624 10.296 9.411 2MASS J21103147−2710578 963 211113.6−224819 −41.1 −342.4 14.064 9.987 9.121 LP 873−9 964 211124.1−094034 −31.0 −343.5 15.791 10.937 9.950 LP 757−92 965 211540.8+165716 +39.7 −17.4 15.294 11.342 10.491 2MASS J21154087+1657161 966 211807.1+482812 +2.1 −2.8 15.277 11.264 10.279 IRAS 21163+4815 967 212133.8−243322 −95.1 −27.3 15.066 11.061 10.183 2MASS J21213394−2433226 968 212243.0+085325 +259.4 −273.8 15.378 11.407 10.598 NLTT 51136 969 212336.2−261400 +37.7 −272.7 15.164 11.226 10.355 LP 873−38 970 212342.7+271236 +155.5 +78.9 15.785 11.427 10.524 2MASS J21234270+2712357 971 212432.4+400400 +545.4 +441.0 15.272 10.339 9.431 2MASS J21243234+4003599 972 212700.8+351801 +207.5 −8.4 15.467 11.484 10.641 2MASS J21270079+3518011 973 212923.3−185509 −33.2 −185.6 16.105 11.263 10.301 LP 817−54 974 212953.9+491843 −0.7 −6.6 15.356 10.909 10.077 Cl* NGC 7092 PLAT 2080 975 213118.8−094726 +28.3 −218.1 11.390 7.316 6.379 Wolf 922 976 213429.4−184037 +80.5 −15.4 14.076 10.046 9.188 2MASS J21342935−1840372 977 213517.5+463315 −163.1 −415.6 15.421 11.297 10.460 LHS 6379 978 213627.2+250009 +254.0 +107.6 15.153 11.003 10.159 2MASS J21362714+2500088 979 213740.1+013713 +77.3 −65.6 12.788 8.802 7.884 GSC 00543−00620 980 214146.9−270456 +142.6 −274.7 14.963 10.699 9.786 LP 930−22 981 214225.2−262405 −39.7 −309.1 15.691 11.321 10.465 LP 874−18 982 214229.6+232912 +3.9 −357.0 15.343 11.211 10.305 NLTT 51901 983 214309.8+074504 +421.3 −14.5 15.747 11.325 10.506 NLTT 51917 984 214407.9+170437 +258.6 −6.2 14.301 10.078 9.193 G 126−30 985 214717.4−044440 +245.3 −10.6 13.504 9.416 8.501 PM I21472-0444 986 214901.7+015646 +129.3 +91.0 15.251 11.340 10.451 NLTT 52157 987 214932.7−073801 +155.7 −79.4 15.712 11.473 10.617 LP 698−49 988 215009.3+055810 +151.0 −17.1 14.755 10.657 9.771 2MASS J21500933+0558102 989 215127.0−012714 +213.5 +19.0 16.237 11.282 10.385 LP 638−50 990 215148.3+133615 +173.4 −118.2 13.275 9.311 8.423 LP 518−58 991 215311.9−255957 −431.4 −17.8 16.054 11.479 10.593 LP 874−37 992 215517.4−004547 +64.5 −53.7 15.172 11.092 10.197 2MASS J21551741−0045478 993 215524.2−023824 +154.5 +30.9 14.820 10.663 9.809 2MASS J21552420−0238247 994 215619.7−102017 −305.1 −261.2 13.920 9.925 9.086 LP 758−62 995 215655.2−015409 +1280.2 +615.9 14.066 9.880 9.026 LHS 516 996 215712.7−090327 +176.1 −124.8 14.428 10.142 9.239 LP 759−6 997 215814.4−210427 +205.8 −30.5 15.437 11.444 10.611 LP 874−66 998 220118.3+434820 +21.8 −22.8 14.715 10.530 9.642 2MASS J22011804+4348240 999 220421.5+150552 +647.1 +503.5 15.651 10.867 9.981 2MASS J22042147+1505517 1000 220509.4−124046 +374.6 −148.4 15.124 10.981 10.147 LP 759−23 1001 220609.7−072337 +175.3 −217.0 15.537 10.674 9.759 LP 699−32 1002 220748.5+053910 +457.1 +120.4 15.462 11.155 10.242 LHS 5381 1003 220850.3+114413 +90.5 −50.9 13.869 9.901 9.037 PM I22088+114 1004 221124.1+405958 −89.6 +68.0 14.371 9.725 8.790 2MASS J22112417+4059587 1005 221203.5+164108 +463.6 −69.4 15.663 11.431 10.556 2MASS J22120345+1641093 1006 221554.8+232101 −111.8 −193.3 16.082 10.985 10.115 NLTT 53354 1007 221636.4+131122 +175.0 +89.7 15.309 11.364 10.545 LP 519−50 1008 221736.4−114521 +8.2 −17.7 15.644 11.421 10.549 UCAC3 157−291252

66 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

1009 221813.7−371350 +195.1 −38.9 15.764 11.410 10.509 LP 983−134 1010 222601.2−151813 +277.3 −49.0 16.326 11.456 10.561 LP 820−19 1011 222729.4+384724 +159.0 +69.2 15.155 11.251 10.374 NLTT 53909 1012 223019.8+041010 −121.0 −289.6 14.611 10.518 9.688 NLTT 54021 1013 223219.4−141835 −196.5 −9.8 15.249 11.227 10.351 LP 760−33 1014 223423.2−165945 +501.3 +0.9 15.733 11.231 10.317 LHS 3831 1015 223447.1+275754 −132.9 −68.2 15.661 11.192 10.367 2MASS J22344716+2757542 1016 223455.2+175201 −428.9 +12.8 15.676 11.415 10.583 LP 460−43 1017 223635.3−024050 −375.5 −443.0 15.767 11.416 10.548 LHS 3834 1018 224318.9−092742 −60.3 −219.8 15.903 11.498 10.635 LP 760−66 1019 224323.1−242453 +203.6 −238.5 14.299 10.250 9.408 LP 876−8 1020 224323.2+220818 +390.0 +1.3 14.315 10.143 9.258 GJ 4292 1021 224329.3+455514 +250.9 −63.2 14.826 10.902 10.028 2MASS J22432928+4555150 1022 224500.1−331526 +173.2 −125.3 12.740 8.681 7.793 V* TX PsA 1023 224637.6+033248 +141.3 −71.5 15.351 11.376 10.491 2MASS J22463761+0332484 1024 224655.9+143714 +336.3 +53.2 15.816 11.418 10.521 LP 521−15 1025 224822.5+123210 +501.3 −13.0 16.178 11.193 10.232 LHS 3856 1026 224854.5+181958 −24.7 −132.8 13.897 9.957 9.119 2MASS J22485459+1819592 1027 224908.3−285121 −173.2 −234.7 13.300 9.342 8.474 LP 932−83 1028 225016.4−295217 −278.1 −393.0 15.342 11.281 10.448 LP 932−7 1029 225055.1+495913 +106.4 −12.0 13.859 9.804 8.920 PM I22509+4959 1030 225135.2−110406 +359.8 −145.7 14.400 9.996 9.130 CCDM J22516−1104P 1031 225135.3−110407 +359.8 −145.7 14.575 9.996 9.130 CCDM J22516−1104A 1032 225205.3−153250 +338.4 +11.4 14.369 10.236 9.370 LP 821−27 1033 225349.7−172135 +32.5 +43.2 15.201 11.188 10.318 2MASS J22534969−1721358 1034 225626.3−110937 +391.2 +272.5 14.410 10.496 9.626 LP 761−6 1035 225820.1+431255 +140.9 −15.1 15.389 11.211 10.319 2MASS J22582006+4312551 1036 225832.0+101458 +163.9 −169.3 14.980 10.391 9.499 NLTT 55442 1037 225914.8+373639 +96.2 −28.9 14.638 10.378 9.535 2MASS J22591479+3736395 1038 230123.9−264946 +262.3 +30.2 14.669 10.739 9.881 LP 933−37 1039 230252.4+433815 −137.4 −6.9 13.264 9.316 8.453 2MASS J23025250+4338157 1040 230407.7−170757 +256.3 −260.4 15.405 11.477 10.638 LP 821−55 1041 230803.4+223251 +286.7 +74.1 14.725 10.681 9.745 G 128−33 1042 230825.5+481338 +163.6 −129.2 15.094 11.098 10.163 2MASS J23082543+4813393 1043 231054.8+453045 −27.1 −262.5 15.586 10.844 9.896 UCAC3 272−282107 1044 231216.7+141427 −127.7 −95.3 15.115 10.908 10.060 2MASS J23121677+1414279 1045 231347.3+211729 +246.3 −35.5 16.124 11.421 10.443 RX J2313.7+2117 1046 231522.0−134619 +301.9 −256.5 14.696 10.737 9.903 LP 762−36 1047 231554.5−062746 +320.5 −48.8 16.337 11.111 10.228 LP 702−50 1048 232038.3+082110 +26.3 −125.4 15.114 10.843 9.885 SDSS J232038.38+082110.4 1049 232113.0+302309 +167.4 +117.2 14.610 10.630 9.802 LP 346−8 1050 232121.9+433807 +196.0 +59.8 15.719 11.457 10.581 LP 238−45 1051 232400.0+283403 +723.6 −80.3 15.216 10.920 10.058 LHS 3940 1052 232641.3−150431 −43.3 −87.1 13.933 9.986 9.112 UCAC3 150−396327 1053 232744.2−304540 +78.0 −72.9 14.493 10.486 9.664 GR* 411 1054 233011.3−023722 +101.7 −77.3 15.090 10.648 9.768 2MASS J23301129−0237227 1055 233038.0−331827 −104.1 −49.7 14.288 10.184 9.317 GR* 422 1056 233045.3+072627 +485.5 +267.5 15.003 10.821 9.974 LHS 3962

67 Table A2: (continued).

0 No. CMC15 µα cos δ µδ r JKs Name [mas/a] [mas/a] [mag] [mag] [mag]

1057 233144.9−024439 +95.1 −73.3 13.888 9.507 8.667 V* AF Psc 1058 233147.6−062551 −27.7 −164.1 13.860 9.844 8.907 2MASS J23314763−0625502 1059 233201.3+005243 −133.8 −324.7 15.411 11.230 10.355 NLTT 57142 1060 233541.3+061120 +555.1 +270.1 15.443 11.088 10.169 GJ 4345 1061 233607.5+105154 +293.2 −314.3 15.414 11.197 10.339 NLTT 57353 1062 233623.7−104144 +240.5 −91.8 14.769 10.654 9.772 G 273−80 1063 233736.0+162203 +16.7 +32.3 15.333 10.479 9.616 LP 463−23 1064 233910.6+305711 +253.3 +58.8 15.738 11.200 10.286 NLTT 57522 1065 234022.3+343314 +533.8 +93.8 15.269 10.572 9.681 LHS 3997 1066 234139.4−063551 +284.8 −93.0 14.518 10.323 9.396 LP 703−42 1067 234252.6+304921 −341.9 −299.2 13.766 9.637 8.814 GJ 1288 1068 234400.7+224202 +214.2 −292.4 15.640 11.444 10.582 LP 402−78 1069 234437.5+304824 +149.0 +0.9 15.209 11.198 10.383 2MASS J23443752+3048248 1070 234617.0+133602 +160.4 −243.1 15.425 11.465 10.564 LP 523−40 1071 234619.3−115644 +224.1 −128.9 15.097 10.665 9.755 G 273−133 1072 234720.6+423809 +12.9 +208.0 15.498 10.947 10.121 LP 239−52 1073 234721.6−122036 −306.2 −146.5 15.194 10.675 9.763 2MASS J23472176−1220358 1074 234824.1+283434 +366.1 −48.1 15.261 11.320 10.425 LP 347−12 1075 235223.5−144125 +416.7 −257.6 14.679 10.436 9.554 LHS 4032 1076 235232.3−341307 +137.4 −135.3 15.509 11.310 10.422 2MASS J23523223−3413068 1077 235359.4+282815 +399.0 +123.2 14.641 10.568 9.731 G 130−21 1078 235640.9−145230 +214.3 +72.9 14.082 9.998 9.110 G 273−177 1079 235810.8+035323 +278.8 +42.8 15.894 11.462 10.583 NLTT 58585 1080 235919.8+324123 −175.0 −245.8 14.518 10.451 9.555 G 130−31

68 Appendix B: Application for Observing Time

Attached the application for observing time of CAHA 2015 in an independent .pdf file.

69