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19972009
most citedCAIXA: a Catalogue of AGN In the XMM-Newton Archive I. Spectral analysis

253 citations · 1.4k across the 37 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-ph20085 cited

XMM-Newton observation of MACHO 104.20906.960: a dwarf nova candidate with a 2 h period

A. A. Nucita, S. Carpano, F. De Paolis +3

The binaries known as cataclysmic variables are particular binary systems in which the primary star (a white dwarf) accretes material from a secondary via Roche-lobe mechanism. Usu…

astro-ph2008253 cited

CAIXA: a Catalogue of AGN In the XMM-Newton Archive I. Spectral analysis

Stefano Bianchi, Matteo Guainazzi, Giorgio Matt +2

We present CAIXA, a Catalogue of AGN In the XMM-Newton Archive. It consists of all the radio-quiet X-ray unobscured ( cm) Active Galactic Nuclei…

astro-ph200877 cited

A BLR origin for the iron K line in NGC7213

Stefano Bianchi, Fabio La Franca, Giorgio Matt +5

The X-ray spectrum of NGC7213 is known to present no evidence for Compton reflection, a unique result among bright Seyfert 1s. The observed neutral iron K line, therefore, canno…

astro-ph200858 cited

The Seyfert 1 Galaxy Mrk 335 at a very low flux state: mapping the soft X-ray photoionised gas

A. L. Longinotti, A. Nucita, M. Santos-Lleo +1

This paper reports on an XMM-Newton observation of the Seyfert 1 Galaxy Mrk 335 performed as a Target of Opportunity when the source was in an unusually low flux state. The low lev…

astro-ph2008175 cited

Chandra unveils a binary Active Galactic Nucleus in Mrk463

Stefano Bianchi, Marco Chiaberge, Enrico Piconcelli +2

We analyse Chandra, XMM-Newton and HST data of the double-nucleus Ultraluminous Infrared Galaxy (ULIRG), Mrk463. The Chandra detection of two luminous ($\mathrm{L}_\mathrm{2-10 keV…