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 R...
Context. Finding active galactic nuclei (AGN) behind the Magellanic Clouds (MCs) is difficult becaus...
Most active galactic nuclei (AGN) are 'obscured', i.e. the nucleus is hiding behind a screen of abso...
We present a multiwavelength study of seven active galactic nuclei (AGN) at spectroscopic redshift &...
In order to study the evolution of the relative fraction of obscured active galactic nuclei (AGNs), ...
We study the incidence of nuclear obscuration on a complete sample of 1310 active galactic nuclei (A...
We present a structural study of 182 obscured active galactic nuclei (AGNs) at z ≤1.5, selected in t...
The Two Micron All Sky Survey is finding previously unidentified, luminous, red, active galactic nuc...
The rapid development of new observational capabilities provides the ability to detect both the obsc...
We use Chandra data to study the incidence and properties of active galactic nuclei (AGNs) in 16 int...
International audienceWe present a structural study of 182 obscured Active Galactic Nuclei (AGNs) at...
Recent models of super-massive black hole (SMBH) and host galaxy joint evolution predict the presenc...
Aims: The co-evolution of host galaxies and the active black holes which reside in their centre is o...
International audienceX-ray observations of galaxy clusters are impacted by the presence of active g...
Context. Finding active galactic nuclei (AGN) behind the Magellanic Clouds (MCs) is difficult becaus...
Most active galactic nuclei (AGN) are 'obscured', i.e. the nucleus is hiding behind a screen of abso...
We present a multiwavelength study of seven active galactic nuclei (AGN) at spectroscopic redshift &...
In order to study the evolution of the relative fraction of obscured active galactic nuclei (AGNs), ...
We study the incidence of nuclear obscuration on a complete sample of 1310 active galactic nuclei (A...
We present a structural study of 182 obscured active galactic nuclei (AGNs) at z ≤1.5, selected in t...
The Two Micron All Sky Survey is finding previously unidentified, luminous, red, active galactic nuc...
The rapid development of new observational capabilities provides the ability to detect both the obsc...
We use Chandra data to study the incidence and properties of active galactic nuclei (AGNs) in 16 int...
International audienceWe present a structural study of 182 obscured Active Galactic Nuclei (AGNs) at...
Recent models of super-massive black hole (SMBH) and host galaxy joint evolution predict the presenc...
Aims: The co-evolution of host galaxies and the active black holes which reside in their centre is o...
International audienceX-ray observations of galaxy clusters are impacted by the presence of active g...
Context. Finding active galactic nuclei (AGN) behind the Magellanic Clouds (MCs) is difficult becaus...
Most active galactic nuclei (AGN) are 'obscured', i.e. the nucleus is hiding behind a screen of abso...
We present a multiwavelength study of seven active galactic nuclei (AGN) at spectroscopic redshift &...