Search Results - "Fanidakis, N."
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Clustering, bias and the accretion mode of X-ray-selected AGN
Published in Monthly notices of the Royal Astronomical Society (11-01-2013)“…We present the spatial clustering properties of 1466 X-ray-selected active galactic nuclei (AGN) compiled from the Chandra Deep Field (CDF) North and South,…”
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The evolution of active galactic nuclei across cosmic time: what is downsizing?
Published in Monthly notices of the Royal Astronomical Society (01-02-2012)“…We use a coupled model of the formation and evolution of galaxies and black holes (BHs) to study the evolution of active galactic nuclei (AGNs) in a cold dark…”
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Grand unification of AGN activity in the ΛCDM cosmology
Published in Monthly notices of the Royal Astronomical Society (01-01-2011)“…We track the coevolution of supermassive black holes (SMBHs) and their host galaxies through cosmic time. The calculation is embedded in the galform…”
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4
The most luminous quasars do not live in the most massive dark matter haloes at any redshift
Published in Monthly notices of the Royal Astronomical Society (21-11-2013)“…Quasars (QSOs) represent the brightest active galactic nuclei (AGN) in the Universe and are thought to indicate the location of prodigiously growing black…”
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Constraints on black hole fuelling modes from the clustering of X-ray AGN
Published in Monthly notices of the Royal Astronomical Society (11-10-2013)“…We present a clustering analysis of X-ray selected active galactic nuclei (AGN) by compiling X-ray samples from the literature and re-estimating the…”
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6
The cluster-scale environment of PKS 2155−304
Published in Monthly notices of the Royal Astronomical Society (01-01-2016)“…PKS 2155-304 is one of the brightest extragalactic source in the X-ray and EUV bands, and is a prototype for the BL Lac class of objects. In this paper, we…”
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7
The clustering amplitude of X-ray-selected AGN at z ∼ 0.8: evidence for a negative dependence on accretion luminosity
Published in Monthly notices of the Royal Astronomical Society (21-04-2016)“…The northern tile of the wide-area and shallow XMM-XXL X-ray survey field is used to estimate the average dark matter halo mass of relatively luminous…”
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Investigating evidence for different black hole accretion modes since redshift z ∼ 1
Published in Monthly notices of the Royal Astronomical Society (01-05-2014)Get full text
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Investigating evidence for different black hole accretion modes since redshift z ~ 1
Published in Monthly notices of the Royal Astronomical Society (01-05-2014)“…Chandra data in the COSMOS, AEGIS-XD and 4 Ms Chandra Deep Field South are combined with multiwavelength photometry available in those fields to determine the…”
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Grand unification of AGN activity in the ΛCDM cosmology: Grand unification of AGN activity
Published in Monthly notices of the Royal Astronomical Society (01-01-2011)Get full text
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12
Grand unification of AGN activity in the ACDM cosmology
Published in Monthly notices of the Royal Astronomical Society (2011)Get full text
Journal Article -
13
Grand unification of AGN activity in the [Lambda]CDM cosmology
Published in Monthly notices of the Royal Astronomical Society (01-01-2011)“…We track the coevolution of supermassive black holes (SMBHs) and their host galaxies through cosmic time. The calculation is embedded in the galform…”
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Journal Article -
14
The Cluster-Scale Environment of PKS 2155-304
Published 06-10-2015“…PKS 2155-304 is one of the brightest extragalactic source in the X-ray and EUV bands, and is a prototype for the BL Lac class of objects. In this paper we…”
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Journal Article -
15
The clustering amplitude of X-ray selected AGN at z=0.8: Evidence for a negative dependence on accretion luminosity
Published 04-02-2016“…The northern tile of the wide-area and shallow XMM-XXL X-ray survey field is used to estimate the average dark matter halo mass of relatively luminous X-ray…”
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16
Clustering, Bias and the Accretion Mode of X-ray selected AGN
Published 28-09-2012“…We present the spatial clustering properties of 1466 X-ray selected AGN compiled from the Chandra CDF-N, CDF-S, eCDF-S, COSMOS and AEGIS fields in the 0.5-8…”
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The VLA-COSMOS 3~GHz Large Project: AGN and host-galaxy properties out to z$\lesssim$6
Published 28-03-2017“…A&A 602, A3 (2017) We explore the multiwavelength properties of AGN host galaxies for different classes of radio-selected AGN out to z$\lesssim$6 via a…”
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18
The most luminous quasars do not live in the most massive dark matter haloes at any redshift
Published 09-05-2013“…Quasars represent the brightest Active Galactic Nuclei (AGN) in the Universe and are thought to indicate the location of prodigiously growing Black Holes…”
Get full text
Journal Article -
19
Constraints on black hole fuelling modes from the clustering of X-ray AGN
Published 09-05-2013“…We present a clustering analysis of X-ray selected AGN by compiling X-ray samples from the literature and re-estimating the dark matter (DM) halo masses of AGN…”
Get full text
Journal Article -
20
Investigating evidence for different black hole accretion modes since redshift z~1
Published 10-02-2014“…Chandra data in the COSMOS, AEGIS-XD and 4Ms CDFS are combined with optical/near-IR photometry to determine the rest-frame U-V vs V-J colours of X-ray AGN…”
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