Appendix I. Observing Programs 2009B and 2010A

Total Page:16

File Type:pdf, Size:1020Kb

Appendix I. Observing Programs 2009B and 2010A Appendix I. Observing Programs 2009B and 2010A GN Scientific Ranking 2009B Band 1 Ref. No. PI Partner(s) Title Instrument(s) Hrs Measuring the Energetics and Ubiquity of GN-2009B-Q-1 Alexander UK NIFS 24 Outflows in z~2 Galaxies Hosting AGN Activity GMOS study of the gamma-ray blazar 3C66A, GN-2009B-Q-2 Andruchow AR GMOS 5.2 its host and environment Constraining the Effects of High Energy GN-2009B-Q-3 Bary US Photons on Proto-Planetary Disk Chemistry Michelle 5.5 and Evolution A search for the WR progenitors of Type Ib/c GN-2009B-Q-4 Bibby UK GMOS 9.4 SNe in the "Supernova Factory" NGC 6946 GN-2009B-Q-5 Bresolin UH The uncertain abundance gradient of M33 GMOS 4.3 GN-2009B-Q-6 Brown US Sedna and the Birth of the Solar System GMOS 3.6 How do small massive galaxies become big GN-2009B-Q-7 Carrasco GS NIRI+AltairLGS 6.7 massive galaxies? Understanding Transition Circumstellar Disks: NIRI+Altair / GN-2009B-Q-8 Cieza UH a search for close companions in Perseus and 10 Taurus-Auriga NIRI+AltairLGS A deep survey of Wolf-Rayet stars in the dwarf GN-2009B-Q-9 Crowther UK GMOS 3.6 irregular galaxy IC10 Probing Stellar Physics at the Bottom of the NIRI+Altair / GN-2009B-Q-10 Dieterich US Main Sequence: Connecting Masses to 8.8 Photospheric Observables NIRI+AltairLGS Probing grain growth in protoplanetary disks: GN-2009B-Q-11 Duchene US scattered light imaging of edge-on disks in the Michelle 3.4 mid-infrared Black Hole Mass and Orbital Structure in GN-2009B-Q-12 Gebhardt US NIFS+AltairLGS 16.5 NGC507 and NGC741 UV and Early-time Studies of the Evolution of GN-2009B-Q-13 Howell UK/US GMOS 8 Type Ia Supernovae Early evolution of photoevaporating GN-2009B-Q-14 Kassis US protoplanetary disks: mid-infrared spectra of Michelle 10.6 the Orion Nebula proplyds Followup observations of MBCs found in GN-2009B-Q-15 Kleyna UH GMOS 5 PanSTARRS1 Searching for the Bottom of the Initial Mass GN-2009B-Q-16 Luhman US NIRI 16 Function HR 8799 and the Search of Jupiter-like Planets GN-2009B-Q-17 Marois GS NIRI+Altair 6 Around Young & Nearby Early-Type Stars. GN-2009B-Q-18 Matheson US CluLeSS: Cluster and Lensed Supernova Search NIRI 11 The dynamics of the Andromeda sub-group: GN-2009B-Q-19 McConnachie CA/US spectroscopy of two new dwarf galaxies GMOS 8 around M31 Echoes of Historic Milky Way Supernovae: GN-2009B-Q-20 Rest CA/US Spectroscopy of the Cas A, Tycho, 3C 58, and GMOS 18 Crab SNe at Maximum Light. GN-2009B-Q-21 Roberts UK Constraining the mass of the black hole within GMOS 18.6 an ultraluminous X-ray source Titan methane weather at Equinox: Seasonal NIFS+Altair / GN-2009B-Q-22 Roe US 6 climate change and surface geology NIRI+Altair ALTAIR Study of Supernovae in Luminous GN-2009B-Q-23 Ryder AU NIRI+AltairLGS 4.5 Infrared Galaxies Spectroscopic follow-up of Ly-alpha blobs at GN-2009B-Q-24 Saito JP GMOS 2 z~3 in the 2 sq. deg. COSMOS field GN-2009B-Q-25 Sheppard US The First Known Equal Sized Plutino Binary GMOS 3 Massive Outflows in Luminous Quasars and GN-2009B-Q-26 Stockton UH GMOS 6 Radio Galaxies Storchi- GN-2009B-Q-27 BR Feeding vs. feedback in nearby active galaxies NIFS+AltairLGS 4 Bergmann AU / CA / Gamma-Ray Bursts: From Progenitors to GN-2009B-Q-28 Fox GS / UK / GMOS / NIRI 30.3 Probes US GN-2009B-Q-29 Tonry UH Spectroscopy of Pan-STARRS Detections GMOS 16 GN-2009B-Q-30 Trujillo GS/US Primordial Solar System Ices NIRI 22 Kinematics and Energetics in Luminous GN-2009B-Q-31 U UH NIFS+AltairLGS 5 Infrared Galaxies The highest-redshift quasars 5.8<z<7.2 in the GN-2009B-Q-32 Warren UK GMOS / NIRI 3 UKIDSS LAS Near-infrared spectroscopy of CFHQS z>6 GN-2009B-Q-33 Willott CA NIRI 22.5 quasars The Gemini Cluster Astrophysics Spectroscopic GN-2009B-Q-34 Wilson CA GMOS 17 Survey (GCLASS) GMOS / NIFS / Catching the LCROSS Impact Excavation of GN-2009B-Q-35 Wooden US NIFS+Altair / 2 Lunar Dust+Ice at K-band with NIFS NIRI+Altair GS Scientific Ranking 2009B Band 1 Ref. No. PI Partner(s) Title Instrument(s) Hrs A Comprehensive Study of Dust Formation GS-2009B-Q-1 Andrews US in Type II Supernovae with HST, Spitzer and GMOS-S 10.2 Gemini Mass calibration and gas physics for ACT SZ GS-2009B-Q-2 Barrientos CL GMOS-S 20 clusters The Supernovae of Gamma-Ray Bursts: GS-2009B-Q-3 Bersier UK GMOS-S 6 Exploring the diversity of stellar explosions GS-2009B-Q-4 Bosch AR Binary Statistics in 30 Doradus GMOS-S 7 Rapid observations of gamma-ray bursts GS-2009B-Q-5 Tanvir AU/CA/CL/UK GMOS-S 13 with Gemini-S Eta Carinae's Continuing Instability and GS-2009B-Q-6 Davidson US GMOS-S 2.5 Recovery -- The 2009 “Event” Searching for the Massive Stars Associated GS-2009B-Q-7 De Buizer US TReCS 6.2 with Methanol Maser Rings (T-ReCS) The optical counterpart of the GS-2009B-Q-8 Gladstone UK GMOS-S 1.7 ultraluminous X-ray source NGC 253 ULX2 GS-2009B-Q-9 Stritzinger CL Early and late phase spectroscopic study of GMOS-S 10 supernovae in the Local Universe by the Chilean Millennium Center for Supernova Studies NICI Imaging of Planetary-Mass Objects in GS-2009B-Q-10 Hayward GS NICI 7 the Orion Nebula UV and Early-time Studies of the Evolution GS-2009B-Q-11 Howell UK/US GMOS-S 8 of Type Ia Supernovae Search for unseen companions around 4 GS-2009B-Q-12 Hoyer CL transiting planets using Transit Timing GMOS-S 23 Variations.(III) GS-2009B-Q-13 Kasliwal US Transients in the Local Universe GMOS-S 5 A NICI Search of Jupiter-like Planets Around GS-2009B-Q-14 Marois CA/GS/UK/US NICI 25.3 HR 8799 and Young & Nearby Stars. CluLeSS: Cluster and Lensed Supernova GS-2009B-Q-15 Matheson US GMOS-S 15.2 Search Spectroscopic Confirmation and Dynamical GS-2009B-Q-16 Mohr US Mass Estimates of South Pole Telescope GMOS-S 42.6 SZE Selected Galaxy Clusters National GS-2009B-Q-17 UK Gemini Outreach Proposal GMOS-S 1 Office The PS1 core-collapse supernova survey: GS-2009B-Q-18 Pastorello UK GMOS-S 5 deaths of very massive stars Mid-IR Observations of the AGN's NGC1808 GS-2009B-Q-19 Pastoriza BR TReCS 3.5 and ngc1365 Constraining the mass of the black hole GS-2009B-Q-20 Roberts UK GMOS-S 29.2 within NGC 1313 X-2 Titan methane weather at Equinox: GS-2009B-Q-21 Roe US Seasonal climate change and surface NICI 4 geology Optical Spectroscopy of the Light Echo GS-2009B-Q-22 Sinnott CA GMOS-S 3 System of SN1987A GS-2009B-Q-23 Smith US IR Variability of Eta Carinae: The 2009 Event Phoenix / TReCS 12 Simultaneity of Accretion and Outflow in GS-2009B-Q-24 Valenti US Phoenix 4.9 Young Stars z=6 quasars to probe the reionization of the GS-2009B-Q-25 Willott CA GMOS-S 6 universe The Gemini Cluster Astrophysics GS-2009B-Q-26 Wilson CA/US GMOS-S 34 Spectroscopic Survey (GCLASS) Atmospheric Transmission Spectroscopy of GS-2009B-Q-27 Wittenmyer AU Phoenix 5.3 WASP-7b Galaxy Formation in Action: Resolving the GS-2009B-Q-28 Yang US Nature of Newly Discovered Lyman-alpha GMOS-S 27.2 Blobs in the Chandra Deep Field South GN Scientific Ranking 2009B Band 2 Ref. No. PI Partner(s) Title Instrument(s) Hrs A Survey for Faint, Close, Low-Mass Tertiaries GN-2009B-Q-36 Allen US NIRI+Altair 14 to Nearby Spectroscopic Binaries GN-2009B-Q-37 Bally US AO Imaging of the Explosive Orion OMC1 NIRI+Altair / 20 Outflow NIRI+AltairLGS Beyond the Biggest and the Brightest: Integral GN-2009B-Q-38 Bandara CA Field Spectroscopy of Gravitationally Lensed NIFS+AltairLGS 12.5 Galaxies with Laser Guided Adaptive Optics Globular cluster systems of lenticular galaxies: GN-2009B-Q-39 Bassino AR GMOS 6.7 looking for clues on the origin of S0s. Spatially Resolving Molecular Hydrogen in NIFS+Altair / GN-2009B-Q-40 Beck US 22.1 Planet-Forming Disks NIRI Exotic Explosions and Eruptions: Exploring a GN-2009B-Q-41 Berger GS/US GMOS 12 New Transient Phase-Space with Pan-STARRS Characterizing the Nature of Hyper-luminous GN-2009B-Q-42 Christensen GS GMOS 4.2 Supernovae Testing the theory of magneto-centrifugal GN-2009B-Q-43 Coffey UK NIFS+Altair 13 ejection from T Tauri disks Searching for the Massive Stars Associated GN-2009B-Q-44 De Buizer US NIRI+AltairLGS 2.3 with Methanol Maser Rings (Altair/NIRI) NIRI / Detecting the progenitors of core collapse GN-2009B-Q-45 Crockett UK/US NIRI+Altair / 10 supernovae - precision astrometry with ALTAIR NIRI+AltairLGS Probing the Bending Mechanism Responsible GN-2009B-Q-46 Gomez GS for the Wide-Angle Tailed Radio Source in GMOS 5.8 Abell 562 Chemistry of the dwarf spheroidal NGC185: GN-2009B-Q-47 Goncalves BR GMOS 2.5 PNe versus its Seyfert 2 classification Post-Outburst Dust Formation in Warm GN-2009B-Q-48 Gorlova US Michelle 2.5 Hypergiant Rho Cassiopeiae GN-2009B-Q-49 GOTO UH A search for high redshift QSOs at 5.8<z<8 GMOS / NIRI 14 Michelle / GN-2009B-Q-50 Hodapp UH NIRI and Michelle photometry of Sigma Ori IRS 3 NIRI+Altair The DODO Survey: Extending a Direct Imaging GN-2009B-Q-51 Hogan GS Search for Planetary Mass Companions to NIRI 15.8 White Dwarfs Uranus Cloud Structure after 2007 equinox - NIFS+Altair / GN-2009B-Q-52 Irwin UK 5 NIFS and NIRI NIRI+Altair The Lithium Depletion Boundary and Age of GN-2009B-Q-53 James UH GMOS 12 the Southern Open Cluster Blanco 1 Determining the low-mass end of the local GN-2009B-Q-54 Krajnovic GS/UK NIFS+AltairLGS 6 Mbh-sigma relation Stellar Populations in the Host Galaxies of GN-2009B-Q-55 Liu US GMOS 27.3 Luminous Obscured Quasars Galaxy Transformation in Groups within the GN-2009B-Q-56 Lu CA GMOS 6.2 Accretion Zone of Clusters Precise ages and masses of free floating GN-2009B-Q-57 Lucas UK NIFS+AltairLGS 15 planetary mass brown dwarfs Further spectroscopic investigations of NGC GN-2009B-Q-58 Mason GS Michelle 2.5 1068 Accretion and Outflow from Young Stellar GN-2009B-Q-59 McGregor
Recommended publications
  • FY08 Technical Papers by GSMTPO Staff
    AURA/NOAO ANNUAL REPORT FY 2008 Submitted to the National Science Foundation July 23, 2008 Revised as Complete and Submitted December 23, 2008 NGC 660, ~13 Mpc from the Earth, is a peculiar, polar ring galaxy that resulted from two galaxies colliding. It consists of a nearly edge-on disk and a strongly warped outer disk. Image Credit: T.A. Rector/University of Alaska, Anchorage NATIONAL OPTICAL ASTRONOMY OBSERVATORY NOAO ANNUAL REPORT FY 2008 Submitted to the National Science Foundation December 23, 2008 TABLE OF CONTENTS EXECUTIVE SUMMARY ............................................................................................................................. 1 1 SCIENTIFIC ACTIVITIES AND FINDINGS ..................................................................................... 2 1.1 Cerro Tololo Inter-American Observatory...................................................................................... 2 The Once and Future Supernova η Carinae...................................................................................................... 2 A Stellar Merger and a Missing White Dwarf.................................................................................................. 3 Imaging the COSMOS...................................................................................................................................... 3 The Hubble Constant from a Gravitational Lens.............................................................................................. 4 A New Dwarf Nova in the Period Gap............................................................................................................
    [Show full text]
  • XMM–Newton Observations of NGC 3268 in the Antlia Galaxy Cluster: Characterization of a Hidden Group of Galaxies at Z ≈ 0.41
    MNRAS 00, 1 (2018) doi:10.1093/mnras/sty1401 Advance Access publication 2018 May 28 XMM–Newton observations of NGC 3268 in the Antlia Galaxy Cluster: characterization of a hidden group of galaxies at z ≈ 0.41 I. D. Gargiulo,1,4‹ F. Garc´ıa,2,3,4,5 J. A. Combi,2,3,4 J. P. Caso1,2,4 and L. P. Bassino1,2,4 1Instituto de Astrof´ısica de La Plata (CCT La Plata, CONICET, UNLP), Paseo del Bosque s/n, B1900FWA La Plata, Argentina 2Facultad de Ciencias Astronomicas´ y Geof´ısicas, Universidad Nacional de La Plata, Paseo del Bosque, B1900FWA La Plata, Argentina 3Instituto Argentino de Radioastronom´ıa (CCT-La Plata, CONICET; CICPBA), C.C. No. 5, 1894 Villa Elisa, Argentina 4Consejo Nacional de Investigaciones Cient´ıficas y Tecnicas,´ Rivadavia 1917, Ciudad Autonoma´ de Buenos Aires, C1033AAJ Buenos Aires, Argentina 5Laboratoire AIM (UMR 7158 CEA/DRF-CNRS-Universite´ Paris Diderot), Irfu/Departament´ d’Astrophysique, Centre de Saclay, F-91191 Gif-sur-Yvette, France Accepted 2018 May 25. Received 2018 May 25; in original form 2016 December 1 ABSTRACT We report on a detailed X-ray study of the extended emission of the intracluster medium (ICM) around NGC 3268 in the Antlia Cluster of galaxies, together with a characterization of an extended source in the field, namely a background cluster of galaxies at z ≈ 0.41, which was previously accounted as an X-ray point source. The spectral properties of the extended emission of the gas present in Antlia were studied using data from the XMM–Newton satellite, complemented with optical images of Cerro Tololo Inter-American Observatory (CTIO) Blanco telescope, to attain for associations of the optical sources with the X-ray emission.
    [Show full text]
  • The Puzzling Nature of Dwarf-Sized Gas Poor Disk Galaxies
    Dissertation submitted to the Department of Physics Combined Faculties of the Astronomy Division Natural Sciences and Mathematics University of Oulu Ruperto-Carola-University Oulu, Finland Heidelberg, Germany for the degree of Doctor of Natural Sciences Put forward by Joachim Janz born in: Heidelberg, Germany Public defense: January 25, 2013 in Oulu, Finland THE PUZZLING NATURE OF DWARF-SIZED GAS POOR DISK GALAXIES Preliminary examiners: Pekka Heinämäki Helmut Jerjen Opponent: Laura Ferrarese Joachim Janz: The puzzling nature of dwarf-sized gas poor disk galaxies, c 2012 advisors: Dr. Eija Laurikainen Dr. Thorsten Lisker Prof. Heikki Salo Oulu, 2012 ABSTRACT Early-type dwarf galaxies were originally described as elliptical feature-less galax- ies. However, later disk signatures were revealed in some of them. In fact, it is still disputed whether they follow photometric scaling relations similar to giant elliptical galaxies or whether they are rather formed in transformations of late- type galaxies induced by the galaxy cluster environment. The early-type dwarf galaxies are the most abundant galaxy type in clusters, and their low-mass make them susceptible to processes that let galaxies evolve. Therefore, they are well- suited as probes of galaxy evolution. In this thesis we explore possible relationships and evolutionary links of early- type dwarfs to other galaxy types. We observed a sample of 121 galaxies and obtained deep near-infrared images. For analyzing the morphology of these galaxies, we apply two-dimensional multicomponent fitting to the data. This is done for the first time for a large sample of early-type dwarfs. A large fraction of the galaxies is shown to have complex multicomponent structures.
    [Show full text]
  • Naming the Extrasolar Planets
    Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named.
    [Show full text]
  • Early-Type Galaxies in the Antlia Cluster: Catalogue and Isophotal Analysis
    MNRAS 477, 1760–1771 (2018) doi:10.1093/mnras/sty611 Advance Access publication 2018 March 7 Early-type galaxies in the Antlia cluster: catalogue and isophotal analysis Juan P. Calderon,´ 1,2,3‹ Lilia P. Bassino,1,2,3 Sergio A. Cellone1,3,4 and Mat´ıas Gomez´ 5 1Consejo Nacional de Investigaciones Cient´ıficas y Tecnicas,´ Rivadavia 1917, Buenos Aires, Argentina 2Instituto de Astrof´ısica de La Plata (CCT La Plata - CONICET - UNLP), La Plata, Argentina 3Facultad de Ciencias Astronomicas´ y Geof´ısicas, Universidad Nacional de La Plata, Paseo del Bosque, B1900FWA La Plata, Argentina Downloaded from https://academic.oup.com/mnras/article-abstract/477/2/1760/4924514 by Universidad Andres Bello user on 28 May 2019 4Complejo Astronomico´ El Leoncito (CONICET - UNLP - UNC - UNSJ), San Juan, Argentina 5Departamento de Ciencias F´ısicas, Facultad de Ciencias Exactas, Universidad Andres Bello, Santiago, Chile Accepted 2018 February 26. Received 2018 February 26; in original form 2017 December 14 ABSTRACT We present a statistical isophotal analysis of 138 early-type galaxies in the Antlia cluster, located at a distance of ∼ 35 Mpc. The observational material consists of CCD images of four 36 × 36 arcmin2 fields obtained with the MOSAIC II camera at the Blanco 4-m telescope at Cerro Tololo Interamerican Observatory. Our present work supersedes previous Antlia studies in the sense that the covered area is four times larger, the limiting magnitude is MB ∼−9.6 mag, and the surface photometry parameters of each galaxy are derived from Sersic´ model fits extrapolated to infinity. In a companion previous study we focused on the scaling relations obtained by means of surface photometry, and now we present the data, on which the previous paper is based, the parameters of the isophotal fits as well as an isophotal analysis.
    [Show full text]
  • Galaxy Populations in the Antlia Cluster – I
    Mon. Not. R. Astron. Soc. 386, 2311–2322 (2008) doi:10.1111/j.1365-2966.2008.13211.x Galaxy populations in the Antlia cluster – I. Photometric properties of early-type galaxies Anal´ıa V. Smith Castelli,1,2† Lilia P. Bassino,1,2† Tom Richtler,3† Sergio A. Cellone,1,2† Cristian Aruta‡ and Leopoldo Infante4† 1Facultad de Ciencias Astronomicas´ y Geof´ısicas, Universidad Nacional de La Plata, Paseo del Bosque, B1900FWA La Plata, Argentina 2 Instituto de Astrof´ısica de la Plata (CONICET-UNLP) Downloaded from https://academic.oup.com/mnras/article-abstract/386/4/2311/1467775 by guest on 18 December 2018 3Departamento de F´ısica, Universidad de Concepcion,´ Casilla 160-C, Concepcion,´ Chile 4Departamento de Astronom´ıa y Astrof´ısica, Pontificia Universidad Catolica´ de Chile, Casilla 306, Santiago 22, Chile Accepted 2008 March 7. Received 2008 March 6; in original form 2007 November 16 ABSTRACT We present the first colour–magnitude relation (CMR) of early-type galaxies in the central region of the Antlia cluster, obtained from CCD wide-field photometry in the Washington photometric system. Integrated (C − T1) colours, T1 magnitudes, and effective radii have been measured for 93 galaxies (i.e. the largest galaxies sample in the Washington system till now) from the FS90 Antlia Group catalogue. Membership of 37 objects can be confirmed through new radial velocities and data collected from the literature. The resulting colour– magnitude diagram shows that early-type FS90 galaxies that are spectroscopically confirmed Antlia members or that were considered as definite members by FS90, follow a well-defined σ ∼ .
    [Show full text]
  • Cold Gas, Star Formation, and Substructure in the Nearby Antlia Cluster
    University of Groningen KAT-7 science verification Hess, Kelley M.; Jarrett, T. H.; Carignan, Claude; Passmoor, Sean S.; Goedhart, Sharmila Published in: Monthly Notices of the Royal Astronomical Society DOI: 10.1093/mnras/stv1372 IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below. Document Version Publisher's PDF, also known as Version of record Publication date: 2015 Link to publication in University of Groningen/UMCG research database Citation for published version (APA): Hess, K. M., Jarrett, T. H., Carignan, C., Passmoor, S. S., & Goedhart, S. (2015). KAT-7 science verification: Cold gas, star formation, and substructure in the nearby Antlia Cluster. Monthly Notices of the Royal Astronomical Society, 452(2), 1617-1636. https://doi.org/10.1093/mnras/stv1372 Copyright Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons). The publication may also be distributed here under the terms of Article 25fa of the Dutch Copyright Act, indicated by the “Taverne” license. More information can be found on the University of Groningen website: https://www.rug.nl/library/open-access/self-archiving-pure/taverne- amendment. Take-down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal.
    [Show full text]
  • Catalogue of Excitation Classes P for 750 Galactic Planetary Nebulae
    Catalogue of Excitation Classes p for 750 Galactic Planetary Nebulae Name p Name p Name p Name p NeC 40 1 Nee 6072 9 NeC 6881 10 IC 4663 11 NeC 246 12+ Nee 6153 3 NeC 6884 7 IC 4673 10 NeC 650-1 10 Nee 6210 4 NeC 6886 9 IC 4699 9 NeC 1360 12 Nee 6302 10 Nee 6891 4 IC 4732 5 NeC 1501 10 Nee 6309 10 NeC 6894 10 IC 4776 2 NeC 1514 8 NeC 6326 9 Nee 6905 11 IC 4846 3 NeC 1535 8 Nee 6337 11 Nee 7008 11 IC 4997 8 NeC 2022 12 Nee 6369 4 NeC 7009 7 IC 5117 6 NeC 2242 12+ NeC 6439 8 NeC 7026 9 IC 5148-50 6 NeC 2346 9 NeC 6445 10 Nee 7027 11 IC 5217 6 NeC 2371-2 12 Nee 6537 11 Nee 7048 11 Al 1 NeC 2392 10 NeC 6543 5 Nee 7094 12 A2 10 NeC 2438 10 NeC 6563 8 NeC 7139 9 A4 10 NeC 2440 10 NeC 6565 7 NeC 7293 7 A 12 4 NeC 2452 10 NeC 6567 4 Nee 7354 10 A 15 12+ NeC 2610 12 NeC 6572 7 NeC 7662 10 A 20 12+ NeC 2792 11 NeC 6578 2 Ie 289 12 A 21 1 NeC 2818 11 NeC 6620 8 IC 351 10 A 23 4 NeC 2867 9 NeC 6629 5 Ie 418 1 A 24 1 NeC 2899 10 Nee 6644 7 IC 972 10 A 30 12+ NeC 3132 9 NeC 6720 10 IC 1295 10 A 33 11 NeC 3195 9 NeC 6741 9 IC 1297 9 A 35 1 NeC 3211 10 NeC 6751 9 Ie 1454 10 A 36 12+ NeC 3242 9 Nee 6765 10 IC1747 9 A 40 2 NeC 3587 8 NeC 6772 9 IC 2003 10 A 41 1 NeC 3699 9 NeC 6778 9 IC 2149 2 A 43 2 NeC 3918 9 NeC 6781 8 IC 2165 10 A 46 2 NeC 4071 11 NeC 6790 4 IC 2448 9 A 49 4 NeC 4361 12+ NeC 6803 5 IC 2501 3 A 50 10 NeC 5189 10 NeC 6804 12 IC 2553 8 A 51 12 NeC 5307 9 NeC 6807 4 IC 2621 9 A 54 12 NeC 5315 2 NeC 6818 10 Ie 3568 3 A 55 4 NeC 5873 10 NeC 6826 11 Ie 4191 6 A 57 3 NeC 5882 6 NeC 6833 2 Ie 4406 4 A 60 2 NeC 5879 12 NeC 6842 2 IC 4593 6 A
    [Show full text]
  • Suzaku X-Ray Observations of the Nearest Non-Cool Core Cluster, Antlia: Dynamically Young but with Remarkably Relaxed Outskirts
    Suzaku X-ray Observations of the Nearest Non-Cool Core Cluster, Antlia: Dynamically Young but with Remarkably Relaxed Outskirts Jimmy A. Irwin – University of Alabama et al. Deposited 12/04/2018 Citation of published version: Wong, K. et al. (2016): Suzaku X-ray Observations of the Nearest Non-Cool Core Cluster, Antlia: Dynamically Young but with Remarkably Relaxed Outskirts. The Astrophysical Journal, 829(1). DOI: 10.3847/0004-637X/829/1/49 © 2016. The American Astronomical Society. All rights reserved. The Astrophysical Journal, 829:49 (21pp), 2016 September 20 doi:10.3847/0004-637X/829/1/49 © 2016. The American Astronomical Society. All rights reserved. SUZAKU X-RAY OBSERVATIONS OF THE NEAREST NON-COOL CORE CLUSTER, ANTLIA: DYNAMICALLY YOUNG BUT WITH REMARKABLY RELAXED OUTSKIRTS Ka-Wah Wong1,2, Jimmy A. Irwin3, Daniel R. Wik4,5, Ming Sun6, Craig L. Sarazin7, Yutaka Fujita8, and Thomas H. Reiprich9 1 Eureka Scientific, Inc., 2452 Delmer Street Suite 100, Oakland, CA 94602-3017, USA; [email protected] 2 Department of Physics and Astronomy, Minnesota State University, Mankato, MN 56001, USA 3 Department of Physics and Astronomy, University of Alabama, Box 870324, Tuscaloosa, AL 35487, USA 4 Astrophysics Science Division, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA 5 The Johns Hopkins University, Homewood Campus, Baltimore, MD 21218, USA 6 Physics Department, University of Alabama in Huntsville, Huntsville, AL 35899, USA 7 Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904-4325, USA 8 Department of Earth and Space Science, Graduate School of Science, Osaka University, Toyonaka, Osaka 560-0043, Japan 9 Argelander Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, D-53121, Germany Received 2016 February 18; revised 2016 June 17; accepted 2016 July 10; published 2016 September 21 ABSTRACT We present the results of seven Suzaku mosaic observations (>200 ks in total) of the nearest non-cool core cluster, the Antlia Cluster (or Group), beyond its degree-scale virial radius in its eastern direction.
    [Show full text]
  • Integral Field Spectroscopy of Planetary Nebulae with MUSE
    galaxies Article Integral Field Spectroscopy of Planetary Nebulae with MUSE Jeremy R. Walsh 1,* and Ana Monreal-Ibero 2,3 1 European Southern Observatory, 85748 Garching, Germany 2 Instituto de Astrofísica de Canarias (IAC), E-38205 La Laguna, Tenerife, Spain; [email protected] 3 Dpto. Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain * Correspondence: [email protected] Received: 27 February 2020; Accepted: 29 March 2020; Published: 3 April 2020 Abstract: The Multi-Unit Spectroscopic Explorer (MUSE) is a large integral field unit mounted on the ESO Very Large Telescope. Its spatial (60 arcsecond field) and wavelength (4800–9300Å) coverage is well suited to detailed imaging spectroscopy of extended planetary nebulae, such as in the Galaxy. An overview of the capabilities of MUSE applied to Planetary Nebulae (PNe) is provided together with the specific advantages and disadvantages. Some examples of archival MUSE observations of PNe are provided. MUSE datacubes for two targets (NGC 3132 and NGC 7009) are analyzed in detail, and they are used to show the advances achievable for planetary nebula studies. Prospects for further MUSE observations of PNe and a broader analysis of existing datasets are outlined. Keywords: optical spectroscopy; integral field spectroscopy; planetary nebulae; emission lines; physical conditions; abundances; kinematics 1. Overview of MUSE The Multi-Unit Spectroscopic Explorer (MUSE) is a large field-of-view (∼60 × 6000) optical integral field spectrometer mounted on the European Southern Observatory (ESO) Very Large Telescope (VLT), currently on Unit Telescope 4 (Yepun). The field is divided into 24 slices, and each is sent to a separate integral field unit (IFU) that divides the sub-field into 48 mini slits, which are all fed to one of the 24 identical spectrometers [1].
    [Show full text]
  • 7.5 X 11.5.Doubleline.P65
    Cambridge University Press 978-0-521-75618-1 - High Energy Astrophysics, Third Edition Malcolm S. Longair Index More information Name index Abell, George, 99, 101 Cappelluti, Nico, 729 Abraham, Robert, 733 Carter, Brandon, 434 Abramovitz, Milton, 206, 209 Caswell, James, 226 Adams, Fred, 353, 369 Cavaliere, Alfonso, 110 Amsler, Claude, 275 Cesarsky, Catherine, 187, 189 Anderson, Carl, 29, 30, 163 Challinor, Anthony, 115, 259 Arnaud, Monique, 110 Chandrasekhar, Subrahmanyan, 302, 429, 434, Arnett, David, 386 455 Arzoumanian, Zaven, 420 Charlot, Stephane,´ 729, 730, 747 Auger, Pierre, 29 Chwolson, O., 117 Cimatti, Andrea, 736, 748 Babbedge, T., 740 Clayton, Donald, 386 Backer, Donald, 417, 418 Clemmow, Phillip, 267 Bahcall, John, 55, 57, 58 Colless, Matthew, 108, 109 Bahcall, Neta, 105 Compton, Arthur, 231 Balbus, Steven, 455 Cordes, James, 420 Band, David, 264 Cowie, Lennox, 733, 736, 743, 745 Barger, Amy, 745 Cox, Donald, 357 Beckwith, Steven, 737, 744 Becquerel, Henri, 146 Damon, Paul, 297 Bekefi, George, 193 Davies, Rodney, 376 Bell(-Burnell), Jocelyn, 19, 406 Davis, Leverett, 373 Bennett, Charles, 16 Davis, Raymond, 32, 54, 55 Bethe, Hans, 57, 163, 166, 175 de Vaucouleurs, Gerard,´ 77, 78 Bignami, Giovanni, 197 Dermer, Charles, 505 Binney, James, 106, 153 Deubner, Franz-Ludwig, 51 Blaauw, Adriaan, 754 Diehl, Roland, 287 Blackett, Patrick, 29 Dirac, Adrian, 29 Blain, Andrew, 743 Djorgovski, George, 88 Bland-Hawthorn, Jonathan, 733 Dougherty, John, 267 Blandford, Roger, 251 Draine, Bruce, 351, 372, 373, 375, Blumenthal, George, 163, 175,
    [Show full text]
  • Index to JRASC Volumes 61-90 (PDF)
    THE ROYAL ASTRONOMICAL SOCIETY OF CANADA GENERAL INDEX to the JOURNAL 1967–1996 Volumes 61 to 90 inclusive (including the NATIONAL NEWSLETTER, NATIONAL NEWSLETTER/BULLETIN, and BULLETIN) Compiled by Beverly Miskolczi and David Turner* * Editor of the Journal 1994–2000 Layout and Production by David Lane Published by and Copyright 2002 by The Royal Astronomical Society of Canada 136 Dupont Street Toronto, Ontario, M5R 1V2 Canada www.rasc.ca — [email protected] Table of Contents Preface ....................................................................................2 Volume Number Reference ...................................................3 Subject Index Reference ........................................................4 Subject Index ..........................................................................7 Author Index ..................................................................... 121 Abstracts of Papers Presented at Annual Meetings of the National Committee for Canada of the I.A.U. (1967–1970) and Canadian Astronomical Society (1971–1996) .......................................................................168 Abstracts of Papers Presented at the Annual General Assembly of the Royal Astronomical Society of Canada (1969–1996) ...........................................................207 JRASC Index (1967-1996) Page 1 PREFACE The last cumulative Index to the Journal, published in 1971, was compiled by Ruth J. Northcott and assembled for publication by Helen Sawyer Hogg. It included all articles published in the Journal during the interval 1932–1966, Volumes 26–60. In the intervening years the Journal has undergone a variety of changes. In 1970 the National Newsletter was published along with the Journal, being bound with the regular pages of the Journal. In 1978 the National Newsletter was physically separated but still included with the Journal, and in 1989 it became simply the Newsletter/Bulletin and in 1991 the Bulletin. That continued until the eventual merger of the two publications into the new Journal in 1997.
    [Show full text]