All-Sky-ASTROGAM: The MeV Gamma-Ray Companion to Multimessenger Astronomy. (arXiv:1905.07806v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Tatischeff_V/0/1/0/all/0/1">V. Tatischeff</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Angelis_A/0/1/0/all/0/1">A. De Angelis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tavani_M/0/1/0/all/0/1">M. Tavani</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Oberlack_U/0/1/0/all/0/1">U. Oberlack</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Walter_R/0/1/0/all/0/1">R. Walter</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ambrosi_G/0/1/0/all/0/1">G. Ambrosi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Argan_A/0/1/0/all/0/1">A. Argan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ballmoos_P/0/1/0/all/0/1">P. von Ballmoos</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Brandt_S/0/1/0/all/0/1">S. Brandt</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bulgarelli_A/0/1/0/all/0/1">A. Bulgarelli</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bykov_A/0/1/0/all/0/1">A. Bykov</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ciprini_S/0/1/0/all/0/1">S. Ciprini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Prester_D/0/1/0/all/0/1">D. Dominis Prester</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Fioretti_V/0/1/0/all/0/1">V. Fioretti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Grenier_I/0/1/0/all/0/1">I. Grenier</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hanlon_L/0/1/0/all/0/1">L. Hanlon</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hartmann_D/0/1/0/all/0/1">D. H. Hartmann</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hernanz_M/0/1/0/all/0/1">M. Hernanz</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Isern_J/0/1/0/all/0/1">J. Isern</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kanbach_G/0/1/0/all/0/1">G. Kanbach</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kuvvetli_I/0/1/0/all/0/1">I. Kuvvetli</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Laurent_P/0/1/0/all/0/1">P. Laurent</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mazziotta_M/0/1/0/all/0/1">M.N. Mazziotta</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+McEnery_J/0/1/0/all/0/1">J. McEnery</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mereghetti_S/0/1/0/all/0/1">S. Mereghetti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Meuris_A/0/1/0/all/0/1">A. Meuris</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Morselli_A/0/1/0/all/0/1">A. Morselli</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Nakazawa_K/0/1/0/all/0/1">K. Nakazawa</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pearce_M/0/1/0/all/0/1">M. Pearce</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rando_R/0/1/0/all/0/1">R. Rando</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rico_J/0/1/0/all/0/1">J. Rico</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Silva_R/0/1/0/all/0/1">R. Curado da Silva</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ulyanov_A/0/1/0/all/0/1">A. Ulyanov</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wu_X/0/1/0/all/0/1">X. Wu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zdziarski_A/0/1/0/all/0/1">A. Zdziarski</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zoglauer_A/0/1/0/all/0/1">A. Zoglauer</a>

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.

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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