activity
19962023
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 4.2k across the 75 of their papers we have counts for

collaborators

77 papers

astro-ph.HE2023★ 9 cited

Two-temperature accretion flows around strongly magnetized stars and their spectral analysis

Shilpa Sarkar, Kuldeep Singh, Indranil Chattopadhyay +1

We investigate two-temperature accretion flows onto strongly magnetized compact stars. Matter is accreted in the form of an accretion disc upto the disc radius (), where…

astro-ph.HE2021★ 3 cited

Exploring the MeV Sky with a Combined Coded Mask and Compton Telescope: The Galactic Explorer with a Coded Aperture Mask Compton Telescope (GECCO)

Elena Orlando, Eugenio Bottacini, Alexander Moiseev +33

The sky at MeV energies is currently poorly explored. Here we present an innovative mission concept that builds on and improves past and currently proposed missions at such energie…

astro-ph.IM2021

INTEGRAL reloaded: spacecraft, instruments and ground system

Erik Kuulkers, Carlo Ferrigno, Peter Kretschmar +85

ESA's INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) was launched on 17 Oct 2002 at 06:41 CEST. Since then, it has been providing long, uninterrupted observations (up t…

astro-ph.IM2021★ 54 cited

Gamma-ray Astrophysics in the MeV Range: the ASTROGAM Concept and Beyond

Alessandro De Angelis, Vincent Tatischeff, Andrea Argan +26

The energy range between about 100 keV and 1 GeV is of interest for a vast class of astrophysical topics. In particular, (1) it is the missing ingredient for understanding extreme…

astro-ph.HE2021★ 24 cited

Potential origin of the state-dependent high-energy tail in the black hole microquasar Cygnus X-1 as seen with INTEGRAL

F. Cangemi, T. Beuchert, T. Siegert +8

0.1-10 MeV observations of the black hole microquasar Cygnus X-1 have shown the presence of a spectral feature in the form of a power law in addition to the standard black body and…

astro-ph.IM2020★ 3 cited

Origin of the in-orbit instrumental background of the Hard X-ray Imager onboard Hitomi

Kouichi Hagino, Hirokazu Odaka, Goro Sato +43

Understanding and reducing the in-orbit instrumental backgrounds are essential to achieving high sensitivity in hard X-ray astronomical observations. The observational data of the…