We review some of the main physical and statistical properties of the X-ray absorber in AGNs. In particular, we review the distribution of the absorbing column density inferred from X-ray observations of various AGN samples. We discuss the location of the X-ray absorber and the relation with the dust absorption at optical and infrared wavelengths. Finally, we shortly review the recent findings on X-ray absorption at high luminosities and at high redshift
The optical classification of a Seyfert galaxy and whether it is considered X-ray absorbed are often...
We explore the relationship between X-ray absorption and optical obscuration within the BAT AGN Spec...
The majority of active galactic nuclei (AGNs) are obscured by large amounts of absorbing m...
Aims. Intrinsic absorption is a fundamental physical property for understanding the evolution of a...
X-ray spectroscopy offers an opportunity to study the complex mixture of emitting and absorbing comp...
Trabajo presentado al XII Scientific Meeting of the Spanish Astronomical Society (SEA), celebrado en...
This talk discusses the unified X-ray/UV absorption models in AGN. I will first review the models an...
Active galactic nuclei (AGN) show evidence for reprocessing gas, outflowing from the accreting black...
I present results of the analysis of ASCA data for 24 type-1 active galactic nuclei. Spectral featur...
In this work the INTEGRAL hard X-ray selected sample of active galactic nuclei (AGN) has been used t...
Resumen del trabajo presentado al XXIX XMM-Newton SSC consortium meeting, celebrado en Madrid (Españ...
ISBN: 92-9092-915-4International audienceIn the 2-10 keV range, the AGN continuum is generally well ...
Aims.We study the hard X-ray luminosity function and absorption distribution of local ($z\lesssim ...
The spectroscopic analysis of 117 serendipitous sources in the HELLAS2XMM 1df (1 degree field) surve...
I review the constraints that X-ray observations impose on the physical properties and the geometric...
The optical classification of a Seyfert galaxy and whether it is considered X-ray absorbed are often...
We explore the relationship between X-ray absorption and optical obscuration within the BAT AGN Spec...
The majority of active galactic nuclei (AGNs) are obscured by large amounts of absorbing m...
Aims. Intrinsic absorption is a fundamental physical property for understanding the evolution of a...
X-ray spectroscopy offers an opportunity to study the complex mixture of emitting and absorbing comp...
Trabajo presentado al XII Scientific Meeting of the Spanish Astronomical Society (SEA), celebrado en...
This talk discusses the unified X-ray/UV absorption models in AGN. I will first review the models an...
Active galactic nuclei (AGN) show evidence for reprocessing gas, outflowing from the accreting black...
I present results of the analysis of ASCA data for 24 type-1 active galactic nuclei. Spectral featur...
In this work the INTEGRAL hard X-ray selected sample of active galactic nuclei (AGN) has been used t...
Resumen del trabajo presentado al XXIX XMM-Newton SSC consortium meeting, celebrado en Madrid (Españ...
ISBN: 92-9092-915-4International audienceIn the 2-10 keV range, the AGN continuum is generally well ...
Aims.We study the hard X-ray luminosity function and absorption distribution of local ($z\lesssim ...
The spectroscopic analysis of 117 serendipitous sources in the HELLAS2XMM 1df (1 degree field) surve...
I review the constraints that X-ray observations impose on the physical properties and the geometric...
The optical classification of a Seyfert galaxy and whether it is considered X-ray absorbed are often...
We explore the relationship between X-ray absorption and optical obscuration within the BAT AGN Spec...
The majority of active galactic nuclei (AGNs) are obscured by large amounts of absorbing m...