activity
20102016
most citedBlack hole feedback in the luminous quasar PDS 456

277 citations · 1.2k across the 16 of their papers we have counts for

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16 papers

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★ 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…

astro-ph.HE2015★ 16 cited

The Chandra/HETG view of NGC 1365 in a Compton-thick state

E. Nardini, J. Gofford, J. N. Reeves +3

We present the analysis of a Chandra High-Energy Transmission Grating (HETG) observation of the local Seyfert galaxy NGC 1365. The source, well known for its dramatic X-ray spectra…

astro-ph.HE2015★ 1 cited

The Suzaku view of highly-ionised outflows in AGN: II -- Location, energetics and scalings with Bolometric Luminosity

J. Gofford, J. N. Reeves, D. E. McLaughlin +4

Ongoing studies with XMM-Newton have shown that powerful accretion disc winds, as revealed through highly-ionised Fe\,K-shell absorption at E>=6.7 keV, are present in a significant…

astro-ph.HE2015★ 277 cited

Black hole feedback in the luminous quasar PDS 456

E. Nardini, J. N. Reeves, J. Gofford +17

The evolution of galaxies is connected to the growth of supermassive black holes in their centers. During the quasar phase, a huge luminosity is released as matter falls onto the b…

astro-ph.HE2014★ 164 cited

Ultra-fast outflows in radio-loud active galactic nuclei

F. Tombesi, F. Tazaki, R. F. Mushotzky +5

Recent X-ray observations show absorbing winds with velocities up to mildly-relativistic values of the order of ~0.1c in a limited sample of 6 broad-line radio galaxies. They are o…