Portal de Periódicos da CAPES

Science with e-ASTROGAM

2018; Elsevier BV; Volume: 19; Linguagem: Inglês

10.1016/j.jheap.2018.07.001

2214-4056

A. De Angelis, V. Tatischeff, I. A. Grenier, J. McEnery, M. Mallamaci, M. Tavani, U. Oberlack, L. Hanlon, R. Walter, A. Argan, P. von Ballmoos, A. Bulgarelli, A. Bykov, M. Hernanz, G. Kanbach, I. Kuvvetli, M. Pearce, A. A. Zdziarski, J. M. Conrad, G. Ghisellini, A. K. Harding, J. Isern, M. D. Leising, F. Longo, G. M. Madejski, M. Martı́nez, M. N. Mazziotta, J. M. Paredes, M. Pohl, R. Rando, M. Razzano, A. Aboudan, M. Ackermann, Andrea Addazi, M. Ajello, C. Albertus, J. M. Alvarez, G. Ambrosi, Sonia Antón, L. A. Antonelli, A. Babić, B. Baibussinov, Matteo Balbo, L. Baldini, Ş. Balman, Cosimo Bambi, U. Barres de Almeida, J. A. Barrio, Richard Bartels, D. Bastieri, W. Bednarek, D. Bernard, E. Bernardini, T. Bernasconi, B. Bertucci, A. Biland, E. Bissaldi, Markus Boettcher, V. Bonvicini, V. Bosch‐Ramon, E. Bottacini, V. Bozhilov, T. Bretz, M. Branchesi, Vedran Brdar, Torsten Bringmann, A. Brogna, Clark Jorgensen, G. Busetto, S. Buson, M. Busso, A. Caccianiga, S. Camera, R. Campana, P. A. Caraveo, M. Cardillo, P. Carlson, Sébastien Célestin, Marina Cermeño, A. Chen, C. C. Cheung, E. Churazov, S. Ciprini, A. Coc, S. Colafrancesco, A. Coleiro, W. Collmar, P. Coppi, R. M. Curado da Silva, S. Cutini, F. D’Ammando, B. De Lotto, D. de Martino, Alessandra De Rosa, M. Del Santo, L. Delgado, R. Diehl, Stefano Dietrich, A.D. Dolgov, A. Domínguez, D. Dominis Prester, I. Donnarumma, D. Dorner, M. Doro, Maíra Dutra, D. Elsäesser, M. Fabrizio, A. Fernández-Barral, V. Fioretti, Luca Foffano, V. Formato, N. Fornengo, L. Foschini, A. Franceschini, A. Franckowiak, S. Funk, F. Fuschino, Daniele Gaggero, Giorgio Galanti, F. Gargano, D. Gasparrini, R. D. Gehrz, Filippo Giammaria Praticò, N. Giglietto, P. Giommi, F. Giordano, M. Giroletti, G. Ghirlanda, N. Godinović, C. Gouiffès, J. E. Grove, C. Hamadache, D. H. Hartmann, M. Hayashida, Andrzej Hryczuk, P. Jean, T. J. Johnson, J. José, S. Kaufmann, B. Khélifi, J. Kiener, J. Knödlseder, Merlin Kole, Joachim Kopp, V. Kozhuharov, C. Labanti, S. Lalkovski, Philippe Laurent, Olivier Limousin, M. Linares, E. Lindfors, M. Lindner, Jia Liu, S. Lombardi, F. Loparco, R. López-Coto, Marcos López, B. Lott, P. Lubrano, D. Malyshev, N. Mankuzhiyil, K. Mannheim, M. J. M. Marchã, Antonino Marcianò, B. Marcote, M. Mariotti, M. Marisaldi, S. McBreen, S. Mereghetti, Alexander Merle, R. Mignani, G. Minervini, A. A. Moiseev, A. Morselli, Flávia Luisa L. Moura, K. Nakazawa, Lara Nava, D. Nieto, M. Orienti, M. Orio, E. Orlando, P. Orleański, S. Paiano, R. Paoletti, Alessandro Papitto, Mario Pasquato, B. Patricelli, M. Ángeles Pérez-García, M. Persic, G. Piano, A. Pichel, M. Pimenta, C. Pittori, T. A. Porter, Juri Poutanen, E. Prandini, Nikos Prantzos, N. Produit, Stefano Profumo, F. S. Queiroz, S. Rainò, Are Raklev, Marco Regis, I. Reichardt, Yoel Rephaeli, J. Rico, Werner Rodejohann, G. Rodriguez Fernandez, M. Roncadelli, L. Roso, A. C. Rovero, R. Ruffini, G. Sala, M. Sánchez‐Conde, A. Santangelo, P. M. Saz Parkinson, T. Sbarrato, A. Shearer, R.C. Shellard, Kathleen Short, Thomas Siegert, Clarissa Siqueira, P. Spinelli, A. Stamerra, S. Starrfield, A. W. Strong, Inga Strümke, F. Tavecchio, Roberto Taverna, T. Terzić, D. J. Thompson, O. Tibolla, D. F. Torres, R. Turolla, A. Ulyanov, A. Ursi, A. Vacchi, Jeriek Van den Abeele, G. Vankova-Kirilova, C. Venter, F. Verrecchia, P. Vincent, Xiao-Ping Wang, Christoph Weniger, X. Wu, G. Zaharijaš, L. Zampieri, Silvia Zane, S. Zimmer, Andreas Zoglauer, the eASTROGAM collaboration,

Dark Matter and Cosmic Phenomena

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 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 LISA.