activity
20162026
most citedPolarized Blazar X-rays imply particle acceleration in shocks

140 citations · 1.8k across the 102 of their papers we have counts for

collaborators
Showing 2020 · astro-ph.HEShow all

7 papers · 2 filters

astro-ph.HE2020★ 27 cited

Location and energetics of the ultra-fast outflow in PG 1448+273

M. Laurenti, A. Luminari, F. Tombesi +3

Ultra-fast outflows (UFOs) play a key role in the AGN feedback mechanism. It is therefore important to fully characterize their location and energetics. We study the UFO in the lat…

astro-ph.HE2020

Towards precision measurements of accreting black holes using X-ray reflection spectroscopy

Cosimo Bambi, Laura W. Brenneman, Thomas Dauser +14

Relativistic reflection features are commonly observed in the X-ray spectra of accreting black holes. In the presence of high quality data and with the correct astrophysical model,…

astro-ph.HE2020★ 29 cited

The first broadband X-ray view of the narrow line Seyfert 1 Ton S180

G. A. Matzeu, E. Nardini, M. L. Parker +15

We present joint \textit{XMM-Newton} and \textit{NuSTAR} observations of the `bare' narrow line Seyfert 1 Ton S180 (), carried out in 2016 and providing the first hard X-r…

astro-ph.HE2020★ 38 cited

The soft excess of the NLS1 galaxy Mrk 359 studied with an XMM-Newton-NuSTAR monitoring campaign

R. Middei, P. -O. Petrucci, S. Bianchi +7

XMM-Newton and NuSTAR multiple exposures allow us to disentangle the different emission components of active galactic nuclei (AGNs) and to study the evolution of their different sp…

astro-ph.HE2020★ 22 cited

The lively accretion disk in NGC 2992. I. Transient iron K emission lines in the high flux state

A. Marinucci, S. Bianchi, V. Braito +5

We report on one of the brightest flux levels of the Seyfert 2 galaxy NGC 2992 ever observed in X-rays, on May 2019. The source has been monitored every few days from March 26, 201…

astro-ph.HE2020

The Open Universe survey of Swift-XRT GRB fields: a complete sample of HBL blazars

P. Giommi, Y. L. Chang, S. Turriziani +22

We have analysed all the X-ray images centred on Gamma Ray Bursts generated by Swift over the last 15 years using automatic tools that do not require any expertise in X-ray astrono…