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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 &dagger  ,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
Affiliation: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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