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相关论文: Clustering of X-ray selected Active Galactic Nucle…

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We measure the clustering of X-ray, radio, and mid-IR-selected active galactic nuclei (AGN) at 0.2 < z < 1.2 using multi-wavelength imaging and spectroscopic redshifts from the PRIMUS and DEEP2 redshift surveys, covering 7 separate fields…

We investigate the clustering properties of ~1550 broad-line active galactic nuclei (AGNs) at <z>=0.25 detected in the ROSAT All-Sky Survey (RASS) through their measured cross-correlation function with ~46,000 Luminous Red Galaxies (LRGs)…

宇宙学与河外天体物理 · 物理学 2010-03-26 Mirko Krumpe , Takamitsu Miyaji , Alison L. Coil

This is the fifth paper in a series of investigations of the clustering properties of luminous, broad-emission-line active galactic nuclei (AGN) identified in the ROSAT All-Sky Survey (RASS) and Sloan Digital Sky Survey (SDSS). In this work…

We measure the clustering of non-quasar X-ray AGN at z=0.7-1.4 in the AEGIS field. Using the cross-correlation of 113 Chandra-selected AGN, with a median log L_X=42.8 erg s^-1, with ~5,000 DEEP2 galaxies, we find that the X-ray AGN are fit…

We present a measurement of the fraction of cluster galaxies hosting X-ray bright Active Galactic Nuclei (AGN) as a function of clustercentric distance scaled in units of $r_{500}$. Our analysis employs high quality Chandra X-ray and Subaru…

宇宙学与河外天体物理 · 物理学 2015-06-17 S. Ehlert , A. von der Linden , S. W. Allen , W. N. Brandt , Y. Q. Xue , B. Luo , A. Mantz , R. G. Morris , D. Applegate , P. Kelly

We present a detailed description of the first direct measurement of the spatial correlation function of X-ray selected AGN. This result is based on an X-ray flux-limited sample of 219 AGN discovered in the contiguous 80.7 deg^2 region of…

天体物理学 · 物理学 2009-11-10 C. R. Mullis , J. P. Henry , I. M. Gioia , H. Boehringer , U. G. Briel , W. Voges , J. P. Huchra

We present the results of a new analysis of the X-ray selected Active Galactic Nuclei (AGN) population in the vicinity of 135 of the most massive galaxy clusters in the redshift range of 0.2 < z < 0.9 observed with Chandra. With a sample of…

星系天体物理 · 物理学 2015-06-22 S. Ehlert , S. W. Allen , W. N. Brandt , R. E. A. Canning , B. Luo , A. Mantz , R. G. Morris , A. von der Linden , Y. Q. Xue

Clustering properties of two samples of X-ray selected AGNs are compared with IR/Optical galactic samples. These are the Einstein Observatory Extended Medium Sensitivity Survey: EMSS; and a sample of 654 ROSAT detected radio quasars. The…

天体物理学 · 物理学 2019-08-17 E. Ghaffarsedeh , J. Quenby

This is the third paper in a series that reports on our investigation of the clustering properties of AGNs identified in the ROSAT All-Sky Survey (RASS) and Sloan Digital Sky Survey (SDSS). In this paper, we extend the redshift range to…

宇宙学与河外天体物理 · 物理学 2015-05-30 Mirko Krumpe , Takamitsu Miyaji , Alison L. Coil , Hector Aceves

The incidence and properties of Active Galactic Nuclei (AGN) in the field, groups, and clusters can provide new information about how these objects are triggered and fueled, similar to how these environments have been employed to study…

宇宙学与河外天体物理 · 物理学 2014-11-20 Timothy J. Arnold , Paul Martini , John S. Mulchaey , Angela Berti , Tesla E. Jeltema

The clustering of active galactic nuclei (AGN) sheds light on their typical large (Mpc-scale) environments, which can constrain the growth and evolution of supermassive black holes. Here we measure the clustering of luminous X-ray-selected…

星系天体物理 · 物理学 2020-03-11 M. C. Powell , C. M. Urry , N. Cappelluti , J. T. Johnson , S. M. LaMassa , T. T. Ananna , K. E. Kollmann

X-ray surveys facilitate investigations of the environment of AGNs. Deep Chandra observations revealed that the AGNs source surface density rises near clusters of galaxies. The natural extension of these works is the measurement of spatial…

天体物理学 · 物理学 2009-11-11 N. Cappelluti , H. Boehringer , P. Schuecker , E. Pierpaoli , C. R. Mullis , I. M. Gioia , J. P. Henry

We have analysed the angular clustering of X-ray selected active galactic nuclei (AGN) in different flux-limited sub-samples of the Chandra Deep Field North (CDF-N) and South (CDF-S) surveys. We find a strong dependence of the clustering…

天体物理学 · 物理学 2017-03-22 M. Plionis , M. Rovilos , S. Basilakos , I. Georgantopoulos , F. Bauer

X-ray surveys facilitate investigations of the environment of AGNs. Deep Chandra observations revealed that the AGNs source surface density rises near clusters of galaxies. The natural extension of these works is the measurement of spatial…

天体物理学 · 物理学 2007-05-23 N. Cappelluti , H. Boehringer , P. Schuecker , E. Pierpaoli , C. R. Mullis , I. M. Gioia , J. P. Henry

A sample of 198 soft X--ray selected active galactic nuclei (AGN) from the ROSAT International X--ray Optical Survey (RIXOS), is used to investigate the X--ray luminosity function and its evolution. RIXOS, with a flux limit of 3E-14 erg s-1…

In order to test active galactic nucleus (AGN) unification and evolutionary models, we measured the AGN clustering properties as a function of AGN obscuration defined in terms of hydrogen column density, $N_{\rm H}$. In addition to…

The clustering properties of moderate luminosity ($L_X = \rm 10^{41} - 10^{44} \, erg \,s^{-1}$) X-ray selected AGN at $z\approx0.1$ are explored. X-ray sources in the redshift interval $0.03<z<0.2$ are selected from a serendipitous XMM…

宇宙学与河外天体物理 · 物理学 2015-05-30 Georgios Mountrichas , Antonis Georgakakis

We aim to study the effect of environment on the presence and fuelling of Active Galactic Nuclei (AGN) in massive galaxy clusters. We explore the use of different AGN detection techniques with the goal of selecting AGN across a broad range…

星系天体物理 · 物理学 2015-06-05 Alison J. Klesman , Vicki L. Sarajedini
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