most citedLong-term AGN variability and the case of GSN 069

6 citations · 6 across the 2 of their papers we have counts for

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astro-ph2008115 cited

The XMM-Newton long look of NGC 1365: uncovering of the obscured X-ray source

G. Risaliti, M. Salvati, M. Elvis +10

We present an analysis of the extreme obscuration variability observed during an XMM-Newton 5-days continuous monitoring of the AGN in NGC 1365. The source was in a reflection-domi…

astro-ph2008165 cited

A systematic look at the Very High and Low/Hard state of GX 339-4: Constraining the black hole spin with a new reflection model

R. C. Reis, A. C. Fabian, R. Ross +3

We present a systematic study of GX 339-4 in both its very high and low hard states from simultaneous observations made with XMM-Newton and RXTE in 2002 and 2004. The X-ray spectra…

astro-ph200851 cited

Weighing the black holes in ultraluminous X-ray sources through timing

P. Casella, G. Ponti, A. Patruno +3

We describe a new method to estimate the mass of black holes in Ultraluminous X-ray Sources (ULXs). The method is based on the recently discovered ``variability plane'', populated…

astro-ph200893 cited

Initial Measurements of Black Hole Spin in GX 339-4 from Suzaku Spectroscopy

J. M. Miller, C. S. Reynolds, A. C. Fabian +6

We report on a deep Suzaku observation of the stellar-mass black hole GX 339-4 in outburst. A clear, strong, relativistically-shaped iron emission line from the inner accretion dis…

astro-ph200745 cited

Suzaku observations of Markarian 335: evidence for a distributed reflector

J. Larsson, G. Miniutti, A. C. Fabian +3

We report on a 151 ks net exposure Suzaku observation of the Narrow Line Seyfert 1 galaxy Mrk 335. The 0.5-40 keV spectrum contains a broad Fe line, a strong soft excess below abou…

astro-ph200739 cited

Constraints on light bending and reflection from the hard X-ray background

P. Gandhi, A. C. Fabian, T. Suebsuwong +3

Light bending due to strong gravity has recently been invoked to explain variability and flux correlations between different bands in some accreting black holes. A characteristic f…