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The galaxy cluster mid-infrared luminosity function at 1.3 < z

Wylezalek, D.; Vernett, Joel; De Breuck, C.; Stern, Daniel; Brodwin, Mark; Galametz, A.; Gonzalez, Anthony H.; Jarvis, Matt; Hatch, Nina A.; Seymour, Nick; Stanford, Spencer A,

Authors

D. Wylezalek

Joel Vernett

C. De Breuck

Daniel Stern

Mark Brodwin

A. Galametz

Anthony H. Gonzalez

Matt Jarvis

Nina A. Hatch

Nick Seymour

Spencer A, Stanford



Abstract

We present 4.5 μm luminosity functions for galaxies identified in 178 candidate galaxy clusters at 1.3 1.3. The luminosity functions are derived for different redshift and richness bins, and the IRAC imaging reaches depths of m∗ + 2, allowing us to measure the faint end slopes of the luminosity functions. We find that α = −1 describes the luminosity function very well in all redshift bins and does not evolve significantly. This provides evidence that the rate at which the low mass galaxy population grows through star formation gets quenched and is replenished by in-falling field galaxies does not have a major net effect on the shape of the luminosity function. Our measurements for m∗ are consistent with passive evolution models and high formation redshifts (zf ∼ 3). We find a slight trend toward fainter m∗ for the richest clusters, implying that the most massive clusters in our sample could contain older stellar populations, yet another example of cosmic downsizing. Modeling shows that a contribution of a star-forming population of up to 40% cannot be ruled out. This value, found from our targeted survey, is significantly lower than the values found for slightly lower redshift, z ∼ 1, clusters found in wide-field surveys. The results are consistent with cosmic downsizing, as the clusters studied here were all found in the vicinity of RLAGNs—which have proven to be preferentially located in massive dark matter halos in the richest environments at high redshift—and they may therefore be older and more evolved systems than the general protocluster population.

Citation

Wylezalek, D., Vernett, J., De Breuck, C., Stern, D., Brodwin, M., Galametz, A., …Stanford, S. A. (in press). The galaxy cluster mid-infrared luminosity function at 1.3 < z. Astrophysical Journal, 786(1), https://doi.org/10.1088/0004-637X/786/1/17

Journal Article Type Article
Acceptance Date Mar 7, 2014
Online Publication Date Apr 10, 2014
Deposit Date Sep 28, 2016
Publicly Available Date Sep 28, 2016
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 786
Issue 1
DOI https://doi.org/10.1088/0004-637X/786/1/17
Keywords galaxies; clusters; formation; high-redshift; luminosity function
Public URL http://eprints.nottingham.ac.uk/id/eprint/37218
Publisher URL http://iopscience.iop.org/article/10.1088/0004-637X/786/1/17/meta
Copyright Statement Copyright information regarding this work can be found at the following address: http://eprints.nottingh.../end_user_agreement.pdf

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Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf





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