activity
20092026
most citedSuzaku observations of 'bare' active galactic nuclei

297 citations · 4.6k across the 139 of their papers we have counts for

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Showing 2016Show all

6 papers · 1 filter

astro-ph.HE2016★ 20 cited

X-ray flaring in PDS 456 observed in a high-flux state

G. A. Matzeu, J. N. Reeves, E. Nardini +3

We present an analysis of a \,ks (net exposure) \textit{Suzaku} observation, carried out in 2007, of the nearby () luminous (L\,erg\,s)…

astro-ph.HE2016★ 31 cited

A deep X-ray view of the bare AGN Ark 120. II. Evidence for Fe K emission transients

E. Nardini, D. Porquet, J. N. Reeves +3

We report on the results from a large observational campaign on the bare Seyfert galaxy Ark 120, jointly carried out in 2014 with XMM-Newton, Chandra, and NuSTAR. The fortunate lin…

astro-ph.HE2016★ 28 cited

A deep X-ray view of the bare AGN Ark 120. I. Revealing the Soft X-ray Line Emission

James Reeves, Delphine Porquet, Valentina Braito +3

The Seyfert 1 galaxy, Ark 120, is a prototype example of the so-called class of bare nucleus AGN, whereby there is no known evidence for the presence of ionized gas along the direc…

astro-ph.HE2016★ 3 cited

Broadband short term variability of the quasar PDS 456

G. A. Matzeu, J. N. Reeves, E. Nardini +4

We present a detailed analysis of a recent ks net exposure \textit{Suzaku} observation, carried out in 2013, of the nearby () luminous (L erg…

astro-ph.HE2016★ 47 cited

Discovery of Broad Soft X-ray Absorption Lines from the Quasar Wind in PDS 456

James Reeves, Valentina Braito, Emanuele Nardini +5

High resolution soft X-ray spectroscopy of the prototype accretion disk wind quasar, PDS 456, is presented. Here, the XMM-Newton RGS spectra are analyzed from the large 2013-2014 X…

astro-ph.HE2016★ 67 cited

Short term X-ray spectral variability of the quasar PDS 456 observed in a low flux state

Gabriele A. Matzeu, James N. Reeves, Emanuele Nardini +4

We present an analysis of the 2013 Suzaku campaign on the nearby luminous quasar PDS 456, covering a total duration of ~1 Ms and a net exposure of 455 ks. During these observations…