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The cosmological significance of low surface brightness galaxies found in a deep blind neutral hydrogen survey
Authors:R F Minchin  M J Disney  Q A Parker  P J Boyce  W J G de Blok  G D Banks †  R D Ekers  K C Freeman  D A Garcia  B K Gibson  M Grossi  R F Haynes  P M Knezek  R H Lang  D F Malin  R M Price  M Putman  I M Stewart  A E Wright
Institution:School of Physics and Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3YB;Department of Physics, Macquarie University, Sydney, NSW 2109, Australia;Planning Division, Cardiff University, Park Place, Cardiff CF10 3UA;Australia Telescope National Facility, PO Box 76, Epping, NSW 1710, Australia;Research School of Astronomy and Astrophysics, Mount Stromlo Observatory, Cotter Road, Weston, ACT 2611, Australia;Centre for Astrophysics and Supercomputing, Swinburne University of Technology, PO Box 218, Hawthorn, Victoria 3122, Australia;School of Mathematics and Physics, University of Tasmania, Hobart, Tasmania 7001, Australia;WIYN Consortium Inc., 950 North Cherry Avenue, Tucson, AZ 85719, USA;Anglo-Australian Observatory, PO Box 296, Epping, NSW 1710, Australia;Department of Physics and Astronomy, University of New Mexico, 800 Yale Boulevard NE, Albuquerque, NM 87131, USA;Department of Astronomy, University of Michigan, Ann Arbor, MI 48108, USA;Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH
Abstract:
Keywords:surveys  galaxies: fundamental parameters  galaxies: luminosity function  mass function  radio lines: galaxies
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