Volume 336, Issue 3 pp. 907-931

The 2dF Galaxy Redshift Survey: the bJ-band galaxy luminosity function and survey selection function

Peder Norberg

Peder Norberg

Department of Physics, University of Durham, Science Laboratories, South Road, Durham DH1 3LE

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Shaun Cole

Shaun Cole

Department of Physics, University of Durham, Science Laboratories, South Road, Durham DH1 3LE

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Carlton M. Baugh

Corresponding Author

Carlton M. Baugh

Department of Physics, University of Durham, Science Laboratories, South Road, Durham DH1 3LE

E-mail: [email protected]Search for more papers by this author
Carlos S. Frenk

Carlos S. Frenk

Department of Physics, University of Durham, Science Laboratories, South Road, Durham DH1 3LE

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Ivan Baldry

Ivan Baldry

Department of Physics & Astronomy, Johns Hopkins University, 3400 North Charles Street Baltimore, MD 21218–2686, USA

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Joss Bland-Hawthorn

Joss Bland-Hawthorn

Anglo-Australian Observatory, PO Box 296, Epping, NSW 2121, Australia

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Terry Bridges

Terry Bridges

Anglo-Australian Observatory, PO Box 296, Epping, NSW 2121, Australia

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Russell Cannon

Russell Cannon

Anglo-Australian Observatory, PO Box 296, Epping, NSW 2121, Australia

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Matthew Colless

Matthew Colless

Research School of Astronomy & Astrophysics, The Australian National University, Weston Creek, ACT 2611, Australia

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Chris Collins

Chris Collins

Astrophysics Research Institute, Liverpool John Moores University, 12 Quays House, Egerton Wharf, Birkenhead L14 1LD

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Warrick Couch

Warrick Couch

Department of Astrophysics, University of New South Wales, Sydney, NSW 2052, Australia

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Nicholas J. G. Cross

Nicholas J. G. Cross

Department of Physics & Astronomy, Johns Hopkins University, 3400 North Charles Street Baltimore, MD 21218–2686, USA

School of Physics and Astronomy, North Haugh, St Andrews, Fife KY16 9SS

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Gavin Dalton

Gavin Dalton

Department of Physics, Keble Road, Oxford OX1 3RH

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Roberto De Propris

Roberto De Propris

Department of Astrophysics, University of New South Wales, Sydney, NSW 2052, Australia

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Simon P. Driver

Simon P. Driver

Research School of Astronomy & Astrophysics, The Australian National University, Weston Creek, ACT 2611, Australia

School of Physics and Astronomy, North Haugh, St Andrews, Fife KY16 9SS

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George Efstathiou

George Efstathiou

Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA

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Richard S. Ellis

Richard S. Ellis

Department of Astronomy, California Institute of Technology, Pasadena, CA 91125, USA

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Karl Glazebrook

Karl Glazebrook

Department of Physics & Astronomy, Johns Hopkins University, 3400 North Charles Street Baltimore, MD 21218–2686, USA

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Carole Jackson

Carole Jackson

Research School of Astronomy & Astrophysics, The Australian National University, Weston Creek, ACT 2611, Australia

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Ofer Lahav

Ofer Lahav

Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA

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Ian Lewis

Ian Lewis

Department of Physics, Keble Road, Oxford OX1 3RH

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Stuart Lumsden

Stuart Lumsden

Department of Physics & Astronomy, E C Stoner Building, Leeds LS2 9JT

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Steve Maddox

Steve Maddox

School of Physics and Astronomy, University of Nottingham, University Park, Nottingham NG7 2RD

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Darren Madgwick

Darren Madgwick

Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA

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John A. Peacock

John A. Peacock

Institute of Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ

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Bruce A. Peterson

Bruce A. Peterson

Research School of Astronomy & Astrophysics, The Australian National University, Weston Creek, ACT 2611, Australia

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Will Sutherland

Will Sutherland

Institute of Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ

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Keith Taylor

Keith Taylor

Anglo-Australian Observatory, PO Box 296, Epping, NSW 2121, Australia

Department of Astronomy, California Institute of Technology, Pasadena, CA 91125, USA

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(The 2dFGRS Team)

(The 2dFGRS Team)

Department of Physics, University of Durham, Science Laboratories, South Road, Durham DH1 3LE

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First published: 25 October 2002
Citations: 158

Abstract

We use more than 110 500 galaxies from the 2dF Galaxy Redshift Survey (2dFGRS) to estimate the bJ-band galaxy luminosity function at redshift z= 0, taking account of evolution, the distribution of magnitude measurement errors and small corrections for incompleteness in the galaxy catalogue. Throughout the interval −16.5 > Murn:x-wiley:00358711:media:MNR5831:tex2gif-sub-4− 5 log10h > −22, the luminosity function is accurately described by a Schechter function with Murn:x-wiley:00358711:media:MNR5831:tex2gif-sub-7− 5 log10h=−19.66 ± 0.07, α=−1.21 ± 0.03 and Φ= (1.61 ± 0.08) × 10−2h3 Mpc−3, giving an integrated luminosity density of ρL= (1.82 ± 0.17) × 108h L Mpc−3 (assuming an Ω0= 0.3, Λ0= 0.7 cosmology). The quoted errors have contributions from the accuracy of the photometric zero-point, from large-scale structure in the galaxy distribution and, importantly, from the uncertainty in the appropriate evolutionary corrections. Our luminosity function is in excellent agreement with, but has much smaller statistical errors than, an estimate from the Sloan Digital Sky Survey (SDSS) data when the SDSS data are accurately translated to the bJ band and the luminosity functions are normalized in the same way. We use the luminosity function, along with maps describing the redshift completeness of the current 2dFGRS catalogue, and its weak dependence on apparent magnitude, to define a complete description of the 2dFGRS selection function. Details and tests of the calibration of the 2dFGRS photometric parent catalogue are also presented.

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