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The z < 1.2 optical luminosity function from a sample of ∼410,000 galaxies in Boötes

Beare, Richard; Brown, Michael J. I.; Pimbblet, Kevin; Bian, Fuyan; Lin, Yen-Ting

Authors

Richard Beare

Michael J. I. Brown

Fuyan Bian

Yen-Ting Lin



Abstract

Using a sample of ~410,000 galaxies to a depth of IAB=24 over 8.26 deg2 in the Boötes field (~10 times larger than the z~1 luminosity function (LF) studies in the prior literature), we have accurately measured the evolving B-band LF of red galaxies at z<1.2 and blue galaxies at z<1.0 In addition to the large sample size, we utilize photometry that accounts for the varying angular sizes of galaxies, photometric redshifts verified with spectroscopy, and absolute magnitudes that should have very small random and systematic errors. Our results are consistent with the migration of galaxies from the blue cloud to the red sequence as they cease to form stars and with downsizing in which more massive and luminous blue galaxies cease star formation earlier than fainter less massive ones. Comparing the observed fading of red galaxies with that expected from passive evolution alone, we find that the stellar mass contained within the red galaxy population has increased by a factor of ~3.6 from z~1.1 to z~0.1 The bright end of the red galaxy LF fades with decreasing redshift, with the rate of fading increasing from ~0.2 mag per unit redshift at z = 1.0 to ~0.8 at z = 0.2. The overall decrease in luminosity implies that the stellar mass in individual highly luminous red galaxies increased by a factor of ~2.2 from z = 1.1 to z = 0.1.

Citation

Beare, R., Brown, M. J. I., Pimbblet, K., Bian, F., & Lin, Y. (2015). The z < 1.2 optical luminosity function from a sample of ∼410,000 galaxies in Boötes. The Astrophysical journal, 815(2), https://doi.org/10.1088/0004-637x/815/2/94

Journal Article Type Article
Acceptance Date Nov 4, 2015
Online Publication Date Dec 14, 2015
Publication Date Dec 20, 2015
Deposit Date Dec 8, 2015
Publicly Available Date Nov 23, 2017
Journal The astrophysical journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 815
Issue 2
DOI https://doi.org/10.1088/0004-637x/815/2/94
Keywords Galaxies -- abundances, Galaxies -- evolution, Galaxies -- statistics
Public URL https://hull-repository.worktribe.com/output/382254
Publisher URL http://iopscience.iop.org/article/10.1088/0004-637X/815/2/94;jsessionid=B1EF495E5BF5CB64783112A577F2B0DD.c3.iopscience.cld.iop.org
Additional Information Copy of article first published in: The astrophysical journal, 2015, v.815, issue 2.

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