We have surveyed the optical linear polarimetric properties of 65 soft X-ray selected ROSAT Active Galactic Nuclei (AGN). Most of these sources show low polarization (<1%) and no optical reddening. This is in agreement with the X-ray results suggesting a direct view on the center. However, two of our AGN show polarization as high as 7--8% and high reddening. This optical reddening suggests a high column of dusty gas, but why does this gas not absorb the soft X-rays? We suggest that the dusty gas is actually ionized. There is evidence for these 'warm' absorbers from X-ray absorption features seen in ROSAT and ASCA spectra
We report the results of near infrared observations of 19 soft X-ray selected AGN. The goal of the o...
X-rays are a powerful probe of the physical conditions in the nuclei of active galaxies. We review t...
Active galactic nuclei (AGN) show evidence for reprocessing gas, outflowing from the accreting black...
We have surveyed the optical linear polarization of a completely identified sample of 43 bright soft...
We report the detection of ionized absorption in the ASCA spectrum of the narrow-line Seyfert 1 gala...
Recent ROSAT studies have identified a significant population of Active Galactic Nuclei (AGN) that a...
As a part of this program, we observed three AGN:PKS2251 + 113, PG0043 = 039 and PLH909. Two objects...
We study the properties of warm absorbers in several active galaxies (AGN) and present new candidate...
The ROSAT Deep Surveys in the Lockman Hole have revealed that AGNs are the main contributors (~75%) ...
We analyze the 0.5-10 keV spectra of six Seyfert 2 galaxies observed with the X-ray satellite ASCA: ...
The optical polarization properties of both low- and high-luminosity active galactic nuclei (AGN) a...
We review some of the main physical and statistical properties of the X-ray absorber in AGNs. In par...
We present a sample of twenty-one ROSAT bright active galactic nuclei (AGN), representing a range of...
Observations of warm absorbers provided new ways to study the nuclear environments of AGNs. I discus...
International audienceWe report on the first observation of a radio-quiet Active Galactic Nucleus (A...
We report the results of near infrared observations of 19 soft X-ray selected AGN. The goal of the o...
X-rays are a powerful probe of the physical conditions in the nuclei of active galaxies. We review t...
Active galactic nuclei (AGN) show evidence for reprocessing gas, outflowing from the accreting black...
We have surveyed the optical linear polarization of a completely identified sample of 43 bright soft...
We report the detection of ionized absorption in the ASCA spectrum of the narrow-line Seyfert 1 gala...
Recent ROSAT studies have identified a significant population of Active Galactic Nuclei (AGN) that a...
As a part of this program, we observed three AGN:PKS2251 + 113, PG0043 = 039 and PLH909. Two objects...
We study the properties of warm absorbers in several active galaxies (AGN) and present new candidate...
The ROSAT Deep Surveys in the Lockman Hole have revealed that AGNs are the main contributors (~75%) ...
We analyze the 0.5-10 keV spectra of six Seyfert 2 galaxies observed with the X-ray satellite ASCA: ...
The optical polarization properties of both low- and high-luminosity active galactic nuclei (AGN) a...
We review some of the main physical and statistical properties of the X-ray absorber in AGNs. In par...
We present a sample of twenty-one ROSAT bright active galactic nuclei (AGN), representing a range of...
Observations of warm absorbers provided new ways to study the nuclear environments of AGNs. I discus...
International audienceWe report on the first observation of a radio-quiet Active Galactic Nucleus (A...
We report the results of near infrared observations of 19 soft X-ray selected AGN. The goal of the o...
X-rays are a powerful probe of the physical conditions in the nuclei of active galaxies. We review t...
Active galactic nuclei (AGN) show evidence for reprocessing gas, outflowing from the accreting black...