Published May 1996
| Published + Accepted Version
Journal Article
Open
Autofib Redshift Survey ā I. Evolution of the galaxy luminosity function
Abstract
We present a detailed determination of the rest frame B-band galaxy luminosity function (LF) as a function of redshift and star formation activity from z = 0 to zā 0.75. The data set used for this purpose is a composite sample of over 1700 redshifts spanning a wide range in apparent magnitude, 11.5
Additional Information
Ā© 1996 RAS. Provided by the NASA Astrophysics Data System. Accepted 1995 November 23; Received 1995 November 21; in original form 1995 August 22.; Published: 01 May 1996. We thank Ian Parry, Ray Sharples, Peter Gray and staff at the AAT for their great efforts in making the Autofib instrument a reliable working system. We also thank PATT for their patience and support over many semesters. Keith Taylor and Jeremy Allington-Smith are thanked for their assistance with LDSS-1 and LDSS-2. We acknowledge useful discussions with Len Cowie, Olivier LeFevre, David Koo, Simon Lilly, Steve Maddox and Ron Marzke. RSE and KGB acknowledge financial support from PPARC. JSH thanks the Marshall Aid Commission. MMC acknowledges the assistance of the Australian Academy of Science/Royal Society exchange program.Attached Files
Published - 280-1-235.pdf
Accepted Version - 9512057.pdf
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9512057.pdf
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Additional details
- Eprint ID
- 108374
- Resolver ID
- CaltechAUTHORS:20210309-153603399
- Particle Physics and Astronomy Research Council (PPARC)
- Marshall Aid Commission
- Australian Academy of Science
- Created
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2021-03-10Created from EPrint's datestamp field
- Updated
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2023-04-18Created from EPrint's last_modified field