The e-ASTROGAM mission Exploring the extreme Universe with gamma rays in the MeV - GeV range

De Angelis A, Tatischeff V, Tavani M, Oberlack U, Grenier I, Hanloni L, Walter R, Argan A, Von Ballmoos P, Bulgarelli A, Donnarumma I, Hernanz M, Kuvvetli I, Pearce M, Zdziarski A, Aboudan A, Ajello M, Ambrosi G, Bernard D, Bernardini E, Bonvicini V, Brogna A, Branchesi M, Budtz-Jorgensen C, Bykov A, Campana R, Cardillo M, Coppi P, De Martino D, Diehl R, Doro M, Fioretti V, Funk S, Ghisellini G, Grove E, Hamadache C, Hartmann DH, Hayashida M, Isern J, Kanbach G, Kiener J, Knodlseder J, Labanti C, Laurent P, Limousin O, Longo F, Mannheim K, Marisaldi M, Martinez M, Mazziotta MN, Mcenery J, Mereghetti S, Minervini G, Moiseev A, Morselli A, Nakazawa K, Orleanski P, Paredes JM, Patricelli B, Pevre J, Piano G, Pohl M, Ramarijaona H, Rando R, Reichardt I, Roncadelli M, Silva R, Tavecchio F, Thompson DJ, Turolla R, Ulyanov A, Vacchi A, Wu X, Zoglauer A (2017)

Publication Status: Published

Publication Type: Journal article

Publication year: 2017

Journal

Publisher: SPRINGER

Book Volume: 44

Pages Range: 25-82

Journal Issue: 1

DOI: 10.1007/s10686-017-9533-6

Abstract

e-ASTROGAM ('enhanced ASTROGAM') is a breakthrough Observatory space mission, with a detector composed by a Silicon tracker, a calorimeter, and an anticoincidence system, dedicated to the study of the non-thermal Universe in the photon energy range from 0.3 MeV to 3 GeV - the lower energy limit can be pushed to energies as low as 150 keV, albeit with rapidly degrading angular resolution, for the tracker, and to 30 keV for calorimetric detection. The mission is based on an advanced space-proven detector technology, with unprecedented sensitivity, angular and energy resolution, combined with 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 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 provide unique data of significant interest to a broad astronomical community, complementary to powerful observatories such as LIGO-Virgo-GEO600-KAGRA, SKA, ALMA, E-ELT, TMT, LSST, JWST, Athena, CTA, IceCube, KM3NeT, and the promise of eLISA.

Authors with CRIS profile

Involved external institutions

Polska Akademia Nauk (PAN) / Polish Academy of Sciences Poland (PL) National Aeronautics and Space Administration (NASA) United States (USA) (US) Technical University of Denmark / Danmarks Tekniske Universitet (DTU) Denmark (DK) Institut de Ciències de l'Espai (ICE) Spain (ES) National Institute for Astrophysics / Istituto Nazionale Astrofisica (INAF) Italy (IT) Institut de Recherche en Astrophysique et Planétologie (IRAP) France (FR) University of Geneva / Université de Genève (UNIGE) Switzerland (CH) University College Dublin (UCD) Ireland (IE) University of Paris 7 - Denis Diderot / Université Paris VII Denis Diderot France (FR) Johannes Gutenberg-Universität Mainz (JGU) Germany (DE) National Institute for Nuclear Physics / Istituto Nazionale di Fisica Nucleare (INFN) Italy (IT) National Center for Scientific Research / Centre national de la recherche scientifique (CNRS) France (FR) Julius-Maximilians-Universität Würzburg Germany (DE) Università degli Studi di Trieste Italy (IT) Commissariat à l'énergie atomique France (FR) École Polytechnique - Université Paris-Saclay France (FR) Max-Planck-Institut für extraterrestrische Physik (MPE) / Max Planck Institute for Extraterrestrial Physics Germany (DE) University of Tokyo Japan (JP) Brera Observatory / Osservatorio Astronomico di Brera Italy (IT) University of Padua / Universita degli Studi di Padova Italy (IT) Yale University United States (USA) (US) Ioffe Physical-Technical Institute / Физико-технический институт имени А. Ф. Иоффе РАН Russian Federation (RU) University of Urbino "Carlo Bo" / Università degli Studi di Urbino "Carlo Bo" (UNIURB) Italy (IT) Deutsches Elektronen-Synchrotron DESY Germany (DE) Clemson University United States (USA) (US) Institut de Fisica d'Altes Energies (IFAE) / The Institute for High Energy Physics Spain (ES) University of Bergen / Universitetet i Bergen Norway (NO) Universidade de Coimbra Portugal (PT) Universitat Rovira i Virgili (URV) Spain (ES) Universität Potsdam Germany (DE) Scuola Normale Superiore di Pisa (SNS) Italy (IT) Universitat de Barcelona (UB) / University of Barcelona Spain (ES) Università degli Studi di Roma 'Tor Vergata' Italy (IT) University of California, Berkeley United States (USA) (US) University of Udine / Università degli Studi di Udine Italy (IT) U.S. Naval Research Laboratory United States (USA) (US)

How to cite

APA:

De Angelis, A., Tatischeff, V., Tavani, M., Oberlack, U., Grenier, I., Hanloni, L.,... Zoglauer, A. (2017). The e-ASTROGAM mission Exploring the extreme Universe with gamma rays in the MeV - GeV range. Experimental Astronomy, 44(1), 25-82. https://dx.doi.org/10.1007/s10686-017-9533-6

MLA:

De Angelis, Alessandro, et al. "The e-ASTROGAM mission Exploring the extreme Universe with gamma rays in the MeV - GeV range." Experimental Astronomy 44.1 (2017): 25-82.

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