The density of extremely red objects around high-z radio-loud AGN
Abstract
We present the results of a K-band imaging survey of 40 arcmin^{2} in fields around 14 radio-loud AGN (6 radio galaxies and 8 quasars) with z>1.5. The survey, 80% complete to K<19.2 and complemented by R-band imaging, aimed at investigating whether extremely red objects (EROs) are present in excess around high-z AGN, and to study the environment of z>1.5 radio galaxies and radio-loud quasars. At the differential galaxy counts in our fields suggest a systematic excess over the general field counts. At K<19.2, we find an excess of galaxies with R-K>6 compared to the general field. Consistently, we also find that the R-K colour distribution of all the galaxies in the AGN fields are significantly redder than the colour distribution of the field galaxies. On the other hand, the distribution of the R-K colours is undistinguishable from that of galaxies taken from literature fields around radio-loud quasars at 1<z<2. We discuss the main implications of our findings and we compare the possible scenarios which could explain our results.
Keywords
Cite
@article{arxiv.astro-ph/0006019,
title = {The density of extremely red objects around high-z radio-loud AGN},
author = {A. Cimatti and D. Villani and L. Pozzetti and S. di Serego Alighieri},
journal= {arXiv preprint arXiv:astro-ph/0006019},
year = {2015}
}
Comments
10 pages, 6 figures, MNRAS, in press