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All-Sky-ASTROGAM: The MeV Gamma-Ray Companion to Multimessenger Astronomy

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arxiv 1905.07806 v1 pith:X3LCY3DZ submitted 2019-05-19 astro-ph.HE astro-ph.IM

All-Sky-ASTROGAM: The MeV Gamma-Ray Companion to Multimessenger Astronomy

V. Tatischeff , A. De Angelis , M. Tavani , U. Oberlack , R. Walter , G. Ambrosi , A. Argan , P. von Ballmoos
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S. Brandt A. Bulgarelli A. Bykov S. Ciprini D. Dominis Prester V. Fioretti I. Grenier L. Hanlon D. H. Hartmann M. Hernanz J. Isern G. Kanbach I. Kuvvetli P. Laurent M.N. Mazziotta J. McEnery S. Mereghetti A. Meuris A. Morselli K. Nakazawa M. Pearce R. Rando J. Rico R. Curado da Silva A. Ulyanov X. Wu A. Zdziarski A. Zoglauer
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classification astro-ph.HE astro-ph.IM
keywords gamma-rayall-sky-astrogammissionactiveagencyalmostastronomyastrophysical
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All-Sky-ASTROGAM is a gamma-ray observatory operating in a broad energy range, 100 keV to a few hundred MeV, recently proposed as the "Fast" (F) mission of the European Space Agency for a launch in 2028 to an L2 orbit. The scientific payload is composed of a unique gamma-ray imaging monitor for astrophysical transients, with very large field of view (almost 4$\pi$ sr) and optimal sensitivity to detect bright and intermediate flux sources (gamma-ray bursts, active galactic nuclei, X-ray binaries, supernovae and novae) at different timescales ranging from seconds to months. The mission will operate in a maturing gravitational wave and multi-messenger epoch, opening up new and exciting synergies.

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