activity
20152021
most citedA deep X-ray view of the bare AGN Ark120. IV. XMM-Newton and NuSTAR spectra dominated by two temperature (warm, hot) Comptonization processes

99 citations · 261 across the 6 of their papers we have counts for

collaborators

14 papers

astro-ph.HE202117 cited

Hard X-ray selected giant radio galaxies -- III. The LOFAR view

G. Bruni, M. Brienza, F. Panessa +12

Giant radio galaxies (GRGs), with extended structures reaching hundreds of kpc, are among the most spectacular examples of ejection of relativistic plasma from super-massive black…

astro-ph.HE2020

Soft gamma-ray selected giant radio galaxies: an update

L. Bassani, F. Ursini, A. Malizia +9

We present an update on the sample of soft gamma-ray selected giant radio galaxies (GRGs) extracted from INTEGRAL/IBIS and Swift/BAT surveys; it includes 8 new sources and one cand…

astro-ph.GA2020

A broadband X-ray view of the NLSy1 1E 0754.6+392.8

R. Middei, F. Tombesi, F. Vagnetti +8

The soft X-ray band of many active galactic nuclei (AGNs) is affected by obscuration due to partially ionised matter crossing our line of sight. In this context, two past XMM-Newto…

astro-ph.HE202099 cited

Radiation spectra of warm and optically thick coronae in AGN

P. -O. Petrucci, D. Gronkiewicz, A. Rozanska +9

A soft X-ray excess above the 2-10 keV power law extrapolation is generally observed in AGN X-ray spectra. Presently there are two competitive models to explain it: blurred ionized…

astro-ph.HE2019

The coronal temperature of NGC 4388 and NGC 2110 measured with INTEGRAL

F. Ursini, L. Bassani, A. Malizia +4

We aim to measure the physical properties of the hot X-ray corona of two active galactic nuclei, NGC 4388 and NGC 2110. We analysed the hard X-ray (20-300 keV) INTEGRAL spectrum in…

astro-ph.GA2019

Probing restarting activity in hard X-ray selected giant radio galaxies

G. Bruni, F. Ursini, F. Panessa +13

With their sizes larger than 0.7 Mpc, Giant Radio Galaxies (GRGs) are the largest individual objects in the Universe. To date, the reason why they reach such enormous extensions is…