On the occupation of X-ray selected galaxy groups by radio AGN since z=1.3

Details On the occupation of X-ray selected galaxy groups by radio AGN since z=1.3 On the occupation of X-ray selected galaxy groups by radio AGN since z=1.3

2011-08-15

arxiv.org/abs/1108.2952v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

5 pages, 4 figures, accepted for publication in MNRAS Letters

Scientific paper

Previous clustering analysis of low-power radio AGN has indicated that they preferentially live in massive groups. The X-ray surveys of the COSMOS field have achieved a sensitivity at which these groups are directly detected out to z=1.3. Making use of Chandra-, XMM- and VLA-COSMOS surveys we identify radio AGN members (10**23.6 < L_1.4GHz/(W/Hz) < 10**25) of galaxy groups (10**13.2 < M_200/M_sun < 10**14.4; 0.1

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