We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.

Durham Research Online
You are in:

The evolution of AGN host galaxies : from blue to red and the influence of large-scale structures.

Silverman, J.D. and Mainieri, V. and Lehmer, B.D. and Alexander, D.M. and Bauer, F.E. and Bergeron, J. and Brandt, W.N. and Gilli, R. and Hasinger, G. and Schneider, D.P. and Tozzi, P. and Vignali, C. and Koekemoer, A.M. and Miyaji, T. and Popesso, P. and Rosati, P. and Szokoly, G. (2008) 'The evolution of AGN host galaxies : from blue to red and the influence of large-scale structures.', Astrophysical journal., 675 (2). pp. 1025-1040.


We present an analysis of 109 moderate-luminosity (41.9<=logL0.5-8.0keV<=43.7) AGNs in the Extended Chandra Deep Field-South survey, which is drawn from 5549 galaxies from the COMBO-17 and GEMS surveys having 0.4<=z<=1.1. These obscured or optically weak AGNs facilitate the study of their host galaxies since the AGNs provide an insubstantial amount of contamination to the galaxy light. We find that the color distribution of AGN host galaxies is highly dependent on (1) the strong color-evolution of luminous (MV<-20.7) galaxies, and (2) the influence of ~10 Mpc scale structures. When excluding galaxies within the redshift range 0.63<=z<=0.76, a regime dominated by sources in large-scale structures at z=0.67 and z=0.73, we observe a bimodality in the host galaxy colors. Galaxies hosting AGNs at z>~0.8 preferentially have bluer (rest-frame U-V<0.7) colors than their z<~0.6 counterparts (many of which fall along the red sequence). The fraction of galaxies hosting AGNs peaks in the ``green valley'' (0.5<U-V<1.0) this is primarily due to enhanced AGN activity in the redshift interval 0.63<=z<=0.76. The AGN fraction in this redshift and color interval is 12.8% (compared to its ``field'' value of 7.8%) and reaches a maximum of 14.8% at U-V~0.8. We further find that blue, bulge-dominated (Sérsic index n>2.5) galaxies have the highest fraction of AGN (21%) in our sample. We explore the scenario that the evolution of AGN hosts is driven by galaxy mergers and illustrate that an accurate assessment requires a larger area survey since only three hosts may be undergoing a merger with timescales <~1 Gyr following a starburst phase.

Item Type:Article
Keywords:Galaxies, Active, Evolution, Large-scale structure of universe, Quasars, X-rays.
Full text:(VoR) Version of Record
Download PDF
Publisher Web site:
Publisher statement:© 2008. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
Date accepted:No date available
Date deposited:05 September 2013
Date of first online publication:March 2008
Date first made open access:No date available

Save or Share this output

Look up in GoogleScholar