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DIGITAL.CSIC
Article . 2018 . Peer-reviewed
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Astrophysics and Space Science
Article . 1998 . Peer-reviewed
License: Springer Nature TDM
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X-ray Observations of Active Galactic Nuclei in the Cosmological Context

Authors: Barcons, Xavier; Carballo, R.; Carrera, Francisco J.; Ceballos, María Teresa; González-Serrano, José Ignacio; Fabian, Andrew C.; Warwick, R. S.;

X-ray Observations of Active Galactic Nuclei in the Cosmological Context

Abstract

We review recent discoveries of obscured Active Galactic Nuclei at significant redshifts with X-ray observations. Most, if not all, the X-ray luminous galaxies found at faint X-ray fluxes could in fact be obscured AGN, where the obscuring material is also forming stars copiously. Given that AGN of various types appear to dominate the source populations at all X-ray fluxes, we also discuss their clustering properties. Current results imply that the population of X-ray selected AGN is not strongly biased, and therefore X-ray observations can be used to trace the distribution of matter out to redshifts ∼ 2.

Partial financial support for this work was provided by the DGESID under project PB95-0122. ACF thanks the Royal Society for support.

Peer Reviewed

Country
Spain
Keywords

Cluster property, Active galactic nucleus, Cosmological context, Current result, Source population

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
Green