activity
19982016
most citedUniversal spectral shape of high accretion rate AGN

141 citations · 855 across the 31 of their papers we have counts for

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astro-ph2006★ 17 cited

Thermal instability in X-ray photoionized media in Active Galactic Nuclei: Influence on the gas structure and spectral features

A. C. Goncalves, S. Collin, A. -M. Dumont +1

A photoionized gas in thermal equilibrium can display a thermal instability, with 3 or more solutions in the multi-branch region of the S-shape curve giving the temperature versus…

astro-ph2006★ 33 cited

A new model for the Warm Absorber in NGC 3783: a single medium in total pressure equilibrium

A. C. Goncalves, S. Collin, A. -M. Dumont +4

(Abridged) Many active galactic nuclei exhibit X-ray features typical of the highly ionized gas called "Warm Absorber" (WA). Such a material appears to be stratified, displaying zo…

astro-ph2006

The puzzle of the soft X-ray excess in AGN: absorption or reflection?

L. Chevallier, S. Collin, A. -M. Dumont +4

The 2-10 keV continuum of AGN is generally well represented by a single power law. However, at smaller energies the continuum displays an excess with respect to the extrapolation o…

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,…

astro-ph2005★ 51 cited

The role of absorption and reflection in the soft X-ray excess of Active Galactic Nuclei : 1. Preliminary results

Loïc Chevallier, Suzy Collin, Anne-Marie Dumont +4

The 2-10 keV continuum of AGN is well represented by a single power law, generally attributed to a hot comptonizing medium, such as a corona above the accretion disk. At smaller en…

astro-ph2005

X-ray Variability of Active Galactic Nuclei and the Flare Model

R. W. Goosmann, B. Czerny, A. -M. Dumont +4

Short-term variability of X-ray spectra has been reported for several Active Galactic Nuclei. Significant X-ray flux variations are observed within time scales down to 10^4 -- 10^5…