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19972026
most citedCompton reflection and iron fluorescence in BeppoSAX observations of Seyfert type 1 galaxies

217 citations · 1k across the 20 of their papers we have counts for

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20 papers

astro-ph.HE2026★ 2 cited

A XRISM view of the iron line complex in NGC 1068: Rethinking the prototypical Compton-thick AGN

S. Bianchi, B. Vander Meulen, E. Bertola +32

We analyze a XRISM/Resolve observation of NGC1068, focusing on the Fe K and Fe K fluorescent lines and on the Fe XXV and Fe XXVI emission complexes. Line centroid energies, i…

astro-ph.CO2013★ 43 cited

A Chandra view of the clumpy reflector at the heart of the Circinus galaxy

A. Marinucci, G. Miniutti, S. Bianchi +2

We present a spectral and imaging analysis of the X-ray reflecting structure at the heart of the Circinus galaxy, investigating the innermost regions surrounding the central black…

astro-ph.HE2010★ 46 cited

Suzaku observations of hard X-ray selected Seyfert 2 galaxies

A. Comastri, K. Iwasawa, R. Gilli +4

We present Suzaku observations of five hard X-ray selected nearby Seyfert 2 galaxies. All the sources were clearly detected with the pin Hard X-ray Detector up to several tens of k…

astro-ph2004

Transmission- to reflection-dominated transition in Seyfert 2 galaxies: the XMM-Newton view

M. Guainazzi, P. Rodriguez-Pascual, A. C. Fabian +3

In this paper we present the current status of a XMM-Newton program to observe an optically-defined, complete and unbiased sample of Compton-thick Seyfert 2 galaxies. The main goal…

astro-ph2003★ 25 cited

Chandra and XMM-Newton observations of Tololo 0109-383

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

We present and discuss Chandra and XMM-Newton observations of the Seyfert 2 galaxy and Compton-thick absorbed source, Tololo~0109-383. The hard X-ray emission (i.e. above 2 k…

astro-ph2002★ 217 cited

Compton reflection and iron fluorescence in BeppoSAX observations of Seyfert type 1 galaxies

G. C. Perola, G. Matt, M. Cappi +5

A sample of nine bright Seyfert 1 and NELG type galaxies, observed with BeppoSAX, is analyzed to assess on a truly broad band basis (0.1-200 keV) the issue of the spectral contribu…