The density of extremely red objects around high-z radio-loud active galactic nuclei

被引:0
|
作者
Cimatti, A
Villani, D
Pozzetti, L
Alighieri, SD
机构
[1] Osservatorio Astrofis Arcetri, I-50125 Florence, Italy
[2] Univ Florence, Dipartimento Astron, I-50125 Florence, Italy
关键词
galaxies : active; galaxies : evolution; galaxies : formation; galaxies : photometry; galaxies : statistics;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of a K-band imaging survey of 40 arcmin(2) in fields around 14 radio-loud active galactic nuclei (AGN), comprising six radio galaxies and eight quasars, with z > 1.5. The survey, which is 80 per cent complete to K < 19.2 mag and complemented by R-band imaging, aimed at investigating whether extremely red objects are present in excess around high-z AGN, and to study the environment of z > 1.5 radio galaxies and radio-loud quasars. At 18 < K < 19 mag, the differential galaxy counts in our fields suggest a systematic excess over the general field counts. At K < 19.2 mag we find an excess of galaxies with R - K > 6 in comparison with the general field. Consistently, we also find that the R - K colour distribution of all the galaxies in the AGN fields is significantly redder than the;colour distribution of the field galaxies. On the other hand, the distribution of the R - K colours is indistinguishable 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 that could explain our results.
引用
收藏
页码:453 / 461
页数:9
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