activity
19982012
most citedOn the X-ray, optical emission line and black hole mass properties of local Seyfert galaxies

352 citations · 739 across the 14 of their papers we have counts for

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Showing 2005Show all

6 papers · 1 filter

astro-ph2005

A very deep Chandra observation of the Perseus cluster: shocks, ripples and conduction

A. C. Fabian, J. S. Sanders, G. B. Taylor +4

We present the first results from a very deep Chandra X-ray observation of the core of the Perseus cluster of galaxies. A pressure map reveals a clear thick band of high pressure a…

astro-ph2005

A search for changing-look AGN in the Grossan catalog

S. Bianchi, M. Guainazzi, G. Matt +4

We observed with XMM-Newton 4 objects selected from the Grossan catalog, with the aim to search for new 'changing-look' AGN. The sample includes all the sources which showed in sub…

astro-ph2005

X-rays from the Type II quasar in the hyperluminous infrared galaxy IRAS F15307+3252

K. Iwasawa, C. S. Crawford, A. C. Fabian +1

We report the detection of X-ray emission from the hyperluminous infrared galaxy IRAS F15307+3252 at z=0.93 and its properties obtained from XMM-Newton observations. Although the X…

astro-ph2005

Molecular Gas and Nuclear Activity in Radio Galaxies Detected by IRAS

A. S. Evans, J. M. Mazzarella, J. A. Surace +3

This paper reports the latest results from a millimeter-wave (CO) spectroscopic survey of IRAS-detected radio galaxies with L_1.4GHz ~ 10^23-28 W/Hz in the redshift range z ~ 0.02-…

astro-ph2005

X-ray reflection in the Seyfert galaxy 1H0419-577 revealing strong relativistic effects in the vicinity of a Kerr black hole

A. C. Fabian, G. Miniutti, K. Iwasawa +1

We report results obtained from six XMM-Newton observations of the Seyfert galaxy 1H 0419-577. Here we show that the X-ray spectrum and variability are well described by a two-comp…

astro-ph2005

The XMM-Newton view of Mrk3 and IXO30

Stefano Bianchi, Giovanni Miniutti, Andrew C. Fabian +1

We present the analysis of the XMM-Newton EPIC pn spectrum of the Seyfert 2 galaxy, Mrk3. We confirm that the source is dominated by a pure Compton reflection component and an iron…