Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 607164.0, MPI für Astronomie / Publikationen_mpia
On the occupation of X-ray-selected galaxy groups by radio active galactic nuclei since z = 1.3
Authors:Smolčić, V.; Finoguenov, A.; Zamorani, G.; Schinnerer, E.; Tanaka, M.; Giodini, S.; Scoville, N.
Date of Publication (YYYY-MM-DD):2011
Journal Abbrev.:Monthly Notices of the Royal Astronomical Society
Volume:416
Issue / Number:1
Start Page:L31
End Page:L35
Audience:Not Specified
Abstract / Description:Previous clustering analysis of low-power radio active galactic nuclei (AGNs) has indicated that they preferentially live in massive groups. The X-ray surveys of the Cosmic Evolution Survey (COSMOS) field have achieved a sensitivity at which these groups are directly detected out to z = 1.3. Making use of the surveys Chandra, XMM-Newton and VLA-COSMOS, we identify radio AGN members [1023.6≲ L1.4 GHz/(W Hz-1) ≲ 1025] of galaxy groups (1013.2≲ M200/M&sun;≲ 1014.4; 0.1 < z < 1.3) and study (i) the radio-AGN-X-ray group occupation statistics as a function of group mass; and (ii) the distribution of radio AGNs within the groups. We find that radio AGNs are preferentially associated with galaxies close to the centre (<0.2r200). Compared to our control sample of group members matched in stellar mass and colour to the radio-AGN host galaxies, we find a significant enhancement of radio-AGN activity associated with 1013.6≲ M200/M&sun;≲ 1014 haloes. We present the first direct measurement of the halo occupation distribution (HOD) for radio AGNs, based on the total mass function of galaxy groups hosting radio AGNs. Our results suggest a possible deviation from the usually assumed power-law HOD model. We also find an overall increase in the fraction of radio AGNs in galaxy groups (<1r200), relative to that in all environments. Based on observations with the National Radio Astronomy Observatory which is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc., and with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA.
Free Keywords:cosmology: observations; galaxies: active; radio continuum: galaxies
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://cdsads.u-strasbg.fr/abs/2011MNRAS.416L..31S
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.