activity
19972025
most citedOn the X-ray, optical emission line and black hole mass properties of local Seyfert galaxies

352 citations · 1.6k across the 38 of their papers we have counts for

collaborators

38 papers

astro-ph.HE2025

3C403: a candidate neutrino-emitting radio galaxy

Gabriele Bruni, Loredana Bassani, Sergio Alves Garre +12

3C403 is a well-known FRII radio galaxy with jets extending up to kiloparsec scales. We report its identification as the second most significant candidate among more than 150 sourc…

astro-ph.HE2024

The challenge of identifying INTEGRAL sources on the Galactic plane

Raffaella Landi, Loredana Bassani, Gabriele Bruni +6

The International Gamma-ray Astrophysics Laboratory (INTEGRAL) has been surveying the sky above 20 keV since its launch in 2002 providing new insights into the nature of the source…

astro-ph.HE2023

Dealing with broad-band X-ray spectra of faint AGN: a case study

Manuela Molina, Angela Malizia, Loredana Bassani

In this work we analyse 3 average-luminosity hard X-ray selected AGN: ESO 506-G27, IGR J19039+3344 and NGC 7465. They have simultaneous Swift/XRT and NuSTAR data never published be…

astro-ph.HE2021★ 4 cited

Investigating the true nature of three hard X-ray sources

Manuela Molina, Angela Malizia, Nicola Masetti +6

Many of the new high energy sources discovered both by INTEGRAL/IBIS and Swift/BAT have been characterised thanks to extensive, multi-band follow-up campaigns, but there are still…

astro-ph.HE2021★ 2 cited

Multi-wavelength observations of the Galactic X-ray binaries IGR J20155+3827 and Swift J1713.4-4219

F. Onori, M. Fiocchi, N. Masetti +4

In recent years, thanks to the continuous surveys performed by INTEGRAL and Swift satellites, our knowledge of the hard X-ray/soft gamma-ray sky has greatly improved. As a result i…

astro-ph.HE2020★ 24 cited

X-ray absorption in INTEGRAL AGN: Host galaxy inclination

A. Malizia, L. Bassani, J. B. Stephen +2

In this work the INTEGRAL hard X-ray selected sample of AGN has been used to investigate the possible contribution of absorbing material distributed within the host galaxies to the…