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The HIPASS catalogue – III. Optical counterparts and isolated dark galaxies
M. T. Doyle 1★ , M. J. Drinkwater 1 , D. J. Rohde 1 , K. A. Pimbblet 1 , M. Read 2 , M. J. Meyer 3,4 , M. A. Zwaan 5 , E. Ryan-Weber 3,6 , J. Stevens 3 , B. S. Koribalski 7 , R. L. Webster 3 , L. Staveley-Smith 7 , D. G. Barnes 3 , M. Howlett 8 , V. A. Kilborn 8,9 , M. Waugh 3 , M. J. Pierce 8 , R. Bhathal 10 , W. J. G. de Blok 11 , M. J. Disney 11 , R. D. Ekers 7 , K. C. Freeman 12 , D. A. Garcia 11 , B. K. Gibson 8 , J. Harnett 13 , P. A. Henning 14 , H. Jerjen 12 , M. J. Kesteven 7 , P. M. Knezek 15 , S. Mader 7 , M. Marquarding 7 , R. F. Minchin 11 , J. O'Brien 12 , T. Oosterloo 16 , R. M. Price 14 , M. E. Putman 17 , S. D. Ryder 18 , E. M. Sadler 19 , I. M. Stewart 20 , F. Stootman 10 and A. E. Wright 7
  1 Department of Physics, University of Queensland, Brisbane, QLD 4072, Australia   2 WFAU, Institute for Astronomy, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ   3 School of Physics, University of Melbourne, VIC 3010, Australia   4 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore MD 21218, USA   5 European Southern Observatory, Karl-Schwarzschild-Str.2, 85748 Garching b. Munchen, Germany   6 Institute of Astronomy, University of Cambridge, Madingly Road, Cambridge CB3 0HA   7 Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia   8 Centre for Astrophysics and Supercomputing, Swinburne University of Technology, PO Box 218, Hawthorn, VIC 3122 Australia   9 Jodrell Bank Observatory, University of Manchester, Macclesfield, Cheshire SK11 9DL   10 Department of Physics, University of Western Sydney Macarthur, PO Box 555, Campbelltown, NSW 2560, Australia   11 School of Physics and Astronomy, Cardiff University, The Parade, Cardiff CF24 3YB   12 Research School of Astronomy and Astrophysics, Mount Stromlo Observatory, Cotter Road, Weston, ACT 2611, Australia   13 University of Technology Sydney, Broadway NSW 2007, Australia   14 Institute for Astrophysics, University of New Mexico, 800 Yale Blvd, NE, Albuquerque, NM 87131, USA   15 WIYN, Inc. 950 North Cherry Avenue, Tucson, AZ 85719 USA   16 ASTRON, PO Box 2, 7990 AA Dwingeloo, the Netherlands   17 Department of Astronomy, University of Michigan, Ann Arbor, MI 48109   18 Anglo-Australian Observatory, PO Box 296, Epping, NSW 1710, Australia   19 School of Physics, University of Sydney, NSW 2006, Australia   20 Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH
Correspondence to   E-mail: mtdoyle@physics.uq.edu.au
Copyright 2005 RAS
KEYWORDS
methods: data analysis • catalogues • surveys • galaxies: photometry • radio lines: galaxies

ABSTRACT

Abstract1 INTRODUCTION2 SELECTION OF OPTICAL COUNTERPARTS3 THE OPTICAL HICAT CATALOGUE, HOPCAT4 RESULTSSUPPLEMENTARY MATERIAL

We present the largest catalogue to date of optical counterparts for H i radio-selected galaxies, HOPCAT. Of the 4315 H i radio-detected sources from the H i Parkes All Sky Survey (HIPASS) catalogue, we find optical counterparts for 3618 (84 per cent) galaxies. Of these, 1798 (42 per cent) have confirmed optical velocities and 848 (20 per cent) are single matches without confirmed velocities. Some galaxy matches are members of galaxy groups. From these multiple galaxy matches, 714 (16 per cent) have confirmed optical velocities and a further 258 (6 per cent) galaxies are without confirmed velocities. For 481 (11 per cent), multiple galaxies are present but no single optical counterpart can be chosen and 216 (5 per cent) have no obvious optical galaxy present. Most of these 'blank fields' are in crowded fields along the Galactic plane or have high extinctions.

Isolated 'dark galaxy' candidates are investigated using an extinction cut of  ABj < 1 mag  and the blank-fields category. Of the 3692 galaxies with an  ABj  extinction <1 mag, only 13 are also blank fields. Of these, 12 are eliminated either with follow-up Parkes observations or are in crowded fields. The remaining one has a low surface brightness optical counterpart. Hence, no isolated optically dark galaxies have been found within the limits of the HIPASS survey.


Accepted 2005 April 27. Received 2005 April 7

DIGITAL OBJECT IDENTIFIER (DOI)
10.1111/j.1365-2966.2005.09159.x About DOI

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