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The e-ASTROGAM gamma-ray space observatory for the multimessenger astronomy of the 2030s

Tatischeff, V. (author)
De Angelis, A. (author)
Tavani, M. (author)
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Grenier, I. (author)
Oberlack, U. (author)
Hanlon, L. (author)
Walter, R. (author)
Argan, A. (author)
Von Ballmoos, P. (author)
Bulgarelli, A. (author)
Donnarumma, I. (author)
Hernanz, M. (author)
Kuvvetli, I. (author)
Mallamaci, M. (author)
Pearce, Mark, 1970- (author)
KTH,Partikel- och astropartikelfysik
Zdziarski, A. (author)
Aboudan, A. (author)
Ajello, M. (author)
Ambrosi, G. (author)
Bernard, D. (author)
Bernardini, E. (author)
Bonvicini, V. (author)
Brogna, A. (author)
Branchesi, M. (author)
Budtz-Jorgensen, C. (author)
Bykov, A. (author)
Campana, R. (author)
Cardillo, M. (author)
Marisaldi, Mario (author)
Zoglauer, A. (author)
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 (creator_code:org_t)
SPIE - International Society for Optical Engineering, 2018
2018
English.
In: Proceedings of SPIE - The International Society for Optical Engineering. - : SPIE - International Society for Optical Engineering. - 9781510619517
  • Conference paper (peer-reviewed)
Abstract Subject headings
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  • e-ASTROGAM is a concept for a breakthrough observatory space mission carrying a γ-ray telescope dedicated to the study of the non-thermal Universe in the photon energy range from 0.15 MeV to 3 GeV. The lower energy limit can be pushed down to energies as low as 30 keV for gamma-ray burst detection with the calorimeter. The mission is based on an advanced space-proven detector technology, with unprecedented sensitivity, angular and energy resolution, combined with remarkable polarimetric capability. Thanks to its performance in the MeV-GeV domain, substantially improving its predecessors, e-ASTROGAM will open a new window on the non-thermal Universe, making pioneering observations of the most powerful Galactic and extragalactic sources, elucidating the nature of their relativistic outflows and their effects on the surroundings. With a line sensitivity in the MeV energy range one to two orders of magnitude better than previous and current generation instruments, e-ASTROGAM will determine the origin of key isotopes fundamental for the understanding of supernova explosion and the chemical evolution of our Galaxy. The mission will be a major player of the multiwavelength, multimessenger time-domain astronomy of the 2030s, and provide unique data of significant interest to a broad astronomical community, complementary to powerful observatories such as LISA, LIGO, Virgo, KAGRA, the Einstein Telescope and the Cosmic Explorer, IceCube-Gen2 and KM3NeT, SKA, ALMA, JWST, E-ELT, LSST, Athena, and the Cherenkov Telescope Array.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

Compton and pair creation telescope
Gamma-ray astronomy
gamma-ray polarization
high-energy astrophysical phenomena
space mission
time-domain astronomy
Cosmology
Observatories
Space telescopes
Supernovae
Astrophysical phenomena
Gamma ray polarization
Pair creation
Space missions
Time domain
Gamma rays

Publication and Content Type

ref (subject category)
kon (subject category)

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