papers

Publications (12)

astro-ph.HE2026

Polarization properties of thermal accretion disk emission. I. Direct radiation

L. Marra, J. Podgorný, R. Taverna +4

The X-ray polarimetric observing window re-opening is shedding new light on our current understanding of compact accreting sources. This is true, in particular, for stellar-mass bl…

astro-ph.GA2018

Thick turbulent gas disks with magnetocentrifugal winds in active galactic nuclei - Model infrared emission and optical polarization

B. Vollmer, M. Schartmann, L. Burtscher +4

(Abridged) Infrared high-resolution imaging and interferometry have shown that the dust distribution is frequently elongated along the polar direction of an AGN. To explain these f…

astro-ph2004

Flare-induced fountains and buried flares in AGN

B. Czerny, R. Goosmann

We discuss the local physical changes at the surface of an AGN accretion disk after the onset of a magnetic flare. The X-ray irradiation by a flare creates a hot spot at the disk s…

astro-ph.GA2017

Constraining the geometry and kinematics of the quasar broad emission line region using gravitational microlensing. I. Models and simulations

L. Braibant, D. Hutsemékers, D. Sluse +1

Recent studies have shown that line profile distortions are commonly observed in gravitationally lensed quasar spectra. We investigate the effect of gravitational microlensing on q…

astro-ph.IM2015

The Microchannel X-ray Telescope on Board the SVOM Satellite

D. Gotz, C. Adami, S. Basa +18

We present the Micro-channel X-ray Telescope (MXT), a new narrow-field (about 1°) telescope that will be flying on the Sino-French SVOM mission dedicated to Gamma-Ray Burst scienc…

astro-ph.GA2016

Understanding Active Galactic Nuclei using near-infrared high angular resolution polarimetry II: Preliminary results

F. Marin, L. Grosset, R. Goosmann +5

In this second research note of a series of two, we present the first near-infrared results we obtained when modeling Active Galactic Nuclei (AGN). Our first proceedings showed the…

astro-ph.GA2019

Constraining the geometry and kinematics of the quasar broad emission line region using gravitational microlensing. II. Comparing models with observations in the lensed quasar HE0435-1223

D. Hutsemékers, L. Braibant, D. Sluse +1

The quadruply lensed quasar HE0435-1223 shows a clear microlensing effect that affects differently the blue and red wings of the H line profile in its image D. To interpret the…

astro-ph.HE2026

X-ray polarization of reflected thermal emission

J. Podgorný, M. Dovčiak, R. Goosmann +5

We compute rest-frame reflection spectra and the corresponding energy-dependent linear polarization degree and angle for (un)polarized single-temperature blackbody spectra impingin…

astro-ph.GA2018

AGN Black hole mass estimates using polarization in broad emission Lines

Đ. Savić, R. Goosmann, L. Č. Popović +2

The innermost regions in active galactic nuclei (AGNs) were not being spatially resolved so far but spectropolarimetry can provide us insight about their hidden physics and the geo…

astro-ph2005

Radio Quiet AGN

B. Czerny, R. Goosmann, V. Karas +1

Active Galactic Nuclei are powered by accretion onto massive black holes. Although radio-quiet objects are not as spectacular sources of very high energy photons as radio-loud ones…

astro-ph.HE2011

The flare model for X-ray variability of NGC 4258

T. Trzesniewski, B. Czerny, V. Karas +4

We study the variability mechanism of active galactic nuclei (AGN) within the framework of the flare model. To this end we examine the case of Seyfert/LINER galaxy NGC 4258, which…

astro-ph2005

Modeling the Warm Absorber in AGN

A. Rozanska, R. Goosmann, A. -M. Dumont +1

We present a wide grid of models for the structure and transmission properties of warm absorbers in active galactic nuclei (AGN). Contrary to commonly used constant density models,…