activity
20032025
most citedThe 4th IBIS/ISGRI soft gamma-ray survey catalog

236 citations · 903 across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.IM2025

The X-ray Integral Field Unit at the end of the Athena reformulation phase

Philippe Peille, Didier Barret, Edoardo Cucchetti +279

The Athena mission entered a redefinition phase in July 2022, driven by the imperative to reduce the mission cost at completion for the European Space Agency below an acceptable ta…

astro-ph.GA2025

3D MC I: X-ray Tomography Begins to Unravel the 3-D Structure of a Molecular Cloud in our Galaxy's Center

Samantha W. Brunker, Cara Battersby, Danya Alboslani +5

Astronomers have used observations of the Galactic gas and dust via infrared, microwave, and radio to study molecular clouds in extreme environments such as the Galactic center. Mo…

astro-ph.HE2019★ 18 cited

Constraining the cosmic ray spectrum in the vicinity of the supernova remnant W28: from sub-GeV to multi-TeV energies

V. H. M. Phan, S. Gabici, G. Morlino +4

Supernova remnants interacting with molecular clouds are ideal laboratories to study the acceleration of particles at shock waves and their transport and interactions in the surrou…

astro-ph.HE2014★ 1 cited

The reflection of two past outbursts of Sagittarius A* observed by Chandra during the last decade

Maïca Clavel, R. Terrier, A. Goldwurm +4

The supermassive black hole at the Galactic center, Sagittarius A*, has experienced periods of higher activity in the past. The reflection of these past outbursts is observed in th…

astro-ph.HE2011★ 25 cited

Extended hard X-ray emission from the Vela pulsar wind nebula

Fabio Mattana, Diego Götz, Régis Terrier +8

The nebula powered by the Vela pulsar is one of the best examples of an evolved pulsar wind nebula, allowing to access the particle injection history and the interaction with the s…

astro-ph.HE2010

Molecular clouds: X-ray mirrors of the Galactic nuclear activity

Gabriele Ponti, Regis Terrier, Andrea Goldwurm +2

We present the result of a study of the X-ray emission from the Galactic Centre Molecular Clouds (MC), within 15 arcmin from Sgr A*. We use XMM-Newton data spanning about 8 years.…