Context. The obscured accretion phase in black hole growth is a crucial ingredient in many models linking the active galactic nuclei (AGN) activity with the evolution of their host galaxy. At present, a complete census of obscured AGN is still missing, although several attempts in this direction have been carried out recently, mostly in the hard X-rays and at mid-infrared wavelengths. Aims. The purpose of this work is to assess whether the [Ne
In order to study the evolution of the relative fraction of obscured active galactic nuclei (AGNs), ...
Most bulge-dominated galaxies host black holes (BH) with masses that tightly correlate with the mass...
Context. The diffuse cosmic X-ray background (CXB) is the sum of the emission of discrete sources, m...
none8siContext. The obscured accretion phase in black hole growth is a crucial ingredient in many mo...
Recent models of super-massive black hole (SMBH) and host galaxy joint evolution predict the presenc...
Obscured AGN are a crucial ingredient to understand the full growth history of super massive black h...
It is widely accepted that black holes at the centres of galaxies grow to become ‘super’massive thro...
Resumen del trabajo presentado al Spanish X-ray Astronomy, celebrado en Santander del 3 al 5 de juno...
Our current understanding of the evolution of obscured accretion onto supermassive black holes is re...
Highly obscured active galactic nuclei (AGN) are common in nearby galaxies, but are difficult to obs...
As it is well established that almost all galaxies host a central supermassive black hole (SMBH), it...
Heavily obscured, Compton thick (CT, NH> 1024 cm-2) active galactic nuclei (AGN) may represent an im...
The rapid development of new observational capabilities provides the ability to detect both the obsc...
In order to study the evolution of the relative fraction of obscured active galactic nuclei (AGNs), ...
Most bulge-dominated galaxies host black holes (BH) with masses that tightly correlate with the mass...
Context. The diffuse cosmic X-ray background (CXB) is the sum of the emission of discrete sources, m...
none8siContext. The obscured accretion phase in black hole growth is a crucial ingredient in many mo...
Recent models of super-massive black hole (SMBH) and host galaxy joint evolution predict the presenc...
Obscured AGN are a crucial ingredient to understand the full growth history of super massive black h...
It is widely accepted that black holes at the centres of galaxies grow to become ‘super’massive thro...
Resumen del trabajo presentado al Spanish X-ray Astronomy, celebrado en Santander del 3 al 5 de juno...
Our current understanding of the evolution of obscured accretion onto supermassive black holes is re...
Highly obscured active galactic nuclei (AGN) are common in nearby galaxies, but are difficult to obs...
As it is well established that almost all galaxies host a central supermassive black hole (SMBH), it...
Heavily obscured, Compton thick (CT, NH> 1024 cm-2) active galactic nuclei (AGN) may represent an im...
The rapid development of new observational capabilities provides the ability to detect both the obsc...
In order to study the evolution of the relative fraction of obscured active galactic nuclei (AGNs), ...
Most bulge-dominated galaxies host black holes (BH) with masses that tightly correlate with the mass...
Context. The diffuse cosmic X-ray background (CXB) is the sum of the emission of discrete sources, m...