activity
20122024
most citedBlack hole feedback in the luminous quasar PDS 456

277 citations · 1.4k across the 33 of their papers we have counts for

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Showing 2018 · astro-ph.HEShow all

6 papers · 2 filters

astro-ph.HE2018

A deep X-ray view of the bare AGN Ark 120. VI. Geometry of the hot corona from spectroscopic and polarization signatures

A. Marinucci, D. Porquet, F. Tamborra +9

The spectral shape of the hard X-ray continuum of Active Galactic Nuclei (AGN) can be ascribed to inverse Compton scattering of optical/UV seed photons from the accretion disc by a…

astro-ph.HE2018

Towards an informed quest for accretion disc winds in quasars: the intriguing case of Ton 28

Emanuele Nardini, Elisabeta Lusso, Susanna Bisogni

We report on the detection of a blueshifted Fe K absorption feature in two consecutive XMM-Newton observations of the luminous blue quasar Ton 28, at the 4 cumulative significan…

astro-ph.HE2018

Resolving the X-ray obscuration in a low flux observation of the quasar PDS 456

James Reeves, Valentina Braito, Emanuele Nardini +5

Simultaneous XMM-Newton, NuSTAR and HST observations, performed in March 2017, of the nearby () luminous quasar PDS 456 are presented. PDS 456 had a low X-ray flux compare…

astro-ph.HE2018

Spectral and polarimetric signatures of X-ray eclipses in AGN

E. S. Kammoun, F. Marin, M. Dovciak +3

X-ray observations of active galactic nuclei (AGN) show variability on timescales ranging from a few hours up to a few days. Some of this variability may be associated with occulta…

astro-ph.HE2018

Tracking the Iron K line and the Ultra Fast Outflow in NGC 2992 at different accretion states

A. Marinucci, S. Bianchi, V. Braito +3

The Seyfert 2 galaxy NGC 2992 has been monitored eight times by XMM-Newton in 2010 and then observed again in 2013, while in 2015 it was simultaneously targeted by Swift and NuSTAR…

astro-ph.HE2018

Testing the accuracy of reflection-based supermassive black hole spin measurements in AGN

E. S. Kammoun, E. Nardini, G. Risaliti

X-ray reflection is a very powerful method to assess the spin of supermassive black holes (SMBHs) in active galactic nuclei (AGN), yet this technique is not universally accepted. I…