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A multi-wavelength approach to the properties of extremely red galaxy populations. I, contribution to the star formation rate density and active galactic nucleus content

Messias, H.; Afonso, J.; Hopkins, A.; Mobasher, B.; Dominici, T.; Alexander, D.M.

A multi-wavelength approach to the properties of extremely red galaxy populations. I, contribution to the star formation rate density and active galactic nucleus content Thumbnail


Authors

H. Messias

J. Afonso

A. Hopkins

B. Mobasher

T. Dominici



Abstract

We present a multi-wavelength analysis of the properties of extremely red galaxy (ERG) populations, selected in the GOODS-South/Chandra Deep Field South field. By using all the photometric and spectroscopic information available on large deep samples of extremely red objects (EROs; 645 sources), IRAC EROs (IEROs; 294 sources), and distant red galaxies (DRGs; 350 sources), we derive redshift distributions, identify active galactic nucleus (AGN)-powered and star formation (SF)-powered galaxies, and, using the radio observations of this field, estimate robust (AGN- and dust-unbiased) SF rate densities (\dot{ρ}_{*}) for these populations. We also investigate the properties of "pure" (galaxies that conform to only one of the three ERG criteria considered) and "combined" (galaxies that verify all three criteria) sub-populations. Overall, a large number of AGNs are identified (up to ~30%, based on X-rays and mid-infrared criteria), the majority of which are type-2 (obscured) objects. Among ERGs with no evidence for AGN activity, we identify sub-populations covering a wide range of average SF rates, from below 10 M sun yr-1 to as high as 200 M sun yr-1. Applying a redshift separation (1 <= z < 2 and 2 <= z <= 3), we find significant evolution (an increase of a factor of 2 or higher) of \dot{ρ}_{*} for EROs and DRGs, while none is observed for IEROs. The former populations can contribute more than 20% to the global \dot{ρ}_{*} at 2 <= z <= 3. The emission from AGN activity is typically not strong in the ERG population, with AGNs increasing the average radio luminosity of ERG sub-populations by, nominally, less than 20%. AGNs are common, however, and, if no discrimination is attempted, this could significantly increase the \dot{ρ}_{*} estimate (by over 100% in some cases). Thus, and while the contribution of star-forming processes to the radio luminosity in galaxies with AGN remains uncertain, a comprehensive identification of AGNs in these populations is necessary to obtain meaningful results.

Journal Article Type Article
Publication Date Aug 1, 2010
Deposit Date Apr 8, 2013
Publicly Available Date Sep 5, 2013
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 719
Issue 1
Pages 790-802
DOI https://doi.org/10.1088/0004-637x/719/1/790
Keywords Galaxies, Active, High-redshift, Starburst.
Public URL https://durham-repository.worktribe.com/output/1459529

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Copyright Statement
© 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.






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