no code implementations • 4 Feb 2021 • Alessandro De Angelis, Vincent Tatischeff, Andrea Argan, Soren Brandt, Andrea Bulgarelli, Andrei Bykov, Elisa Costantini, Rui Curado da Silva, Isabelle A. Grenier, Lorraine Hanlon, Dieter Hartmann, Margarida Hernanz, Gottfried Kanbach, Irfan Kuvvetli, Philippe Laurent, Mario N. Mazziotta, Julie McEnery, Aldo Morselli, Kazuhiro Nakazawa, Uwe Oberlack, Mark Pearce, Javier Rico, Marco Tavani, Peter von Ballmoos, Roland Walter, Xin Wu, Silvia Zane, Andrzej Zdziarski, Andreas Zoglauer
The energy range between about 100 keV and 1 GeV is of interest for a vast class of astrophysical topics.
Instrumentation and Methods for Astrophysics
no code implementations • 2 Dec 2020 • Daniele Rogantini, Elisa Costantini, Missagh Mehdipour, Lucien Kuiper, Piero Ranalli, Rens Waters
High ionisation lines in the soft X-ray band are generally associated to either interstellar hot gas along the line of sight or to photoionised gas intrinsic to the source.
High Energy Astrophysical Phenomena Astrophysics of Galaxies
