학술논문

Multi-messenger and transient astrophysics with the Cherenkov Telescope Array
Document Type
Working Paper
Author
Bošnjak, Ž.Brown, A. M.Carosi, A.Chernyakova, M.Cristofari, P.Longo, F.López-Oramas, A.Santander, M.Satalecka, K.Schüssler, F.Sergijenko, O.Stamerra, A.Agudo, I.Batista, R. AlvesAmato, E.Anguner, E. O.Antonelli, L. A.Backes, M.Balazs, CsabaBaroncelli, L.Tjus, J. BeckerBigongiari, C.Bissaldi, E.Boisson, C.Bolmont, J.Böttcher, M.Bordas, P.Braiding, C.Bregeon, J.Bucciantini, N.Bulgarelli, A.Burton, M.Cangemi, F.Caraveo, P.Cardillo, M.Caroff, S.Casanova, S.Chaty, S.Coelho, J. G.Cotter, G.D'Aì, A.D'Ammando, F.Pino, E. M. de Gouveia Daldella Volpe, D.de Martino, D.Di Girolamo, T.Di Piano, A.Djannati-Ataï, A.Dwarkadas, V.Wilhelmi, E. de OnaAnjos, R. C. DosEmery, G.Fedorova, E.Fegan, S.Fiasson, A.Fioretti, V.Filipovic, M. D.Gaggero, D.Galanti, G.Gasparrini, D.Ghirlanda, G.Goldoni, P.Granot, J.Green, J. G.Heller, M.Hnatyk, B.Hnatyk, R.Horan, D.Hovatta, T.Inoue, S.Jamrozy, M.Kantzas, D.Khélifi, B.Komin, N.Lamastra, A.La Palombara, N.Lenain, J. P.Lindfors, E.Liodakis, I.Lombardi, S.Lucarelli, F.Luque-Escamilla, P. L.Majumdar, P.Marcowith, A.Markoff, S.Marti, J.Martinez, M.Mazin, D.McKeague, S.Mereghetti, S.Mestre, E.Montaruli, T.Morlino, G.Morselli, A.Mundell, C.Murach, T.Nava, L.Nayerhoda, A.Nicastro, L.Niemiec, J.Nikolajuk, M.Olmi, B.Ong, R.Orienti, M.Osborne, J. P.Paredes, Josep M.Pareschi, G.Parmiggiani, N.Patricelli, B.Pe'er, A.Piano, G.Pühlhofer, G.Punch, M.Reimer, O.Ribó, M.Rodriguez, G.Rodriguez, J.Romano, P.Romeo, G.Roncadelli, M.Rowell, G.Rudak, B.Sadeh, I.Greus, F. SalesaSaturni, F. G.Sawangwit, U.Seglar-Arroyo, M.Shellard, R. C.Sol, H.Starling, R.Stolarczyk, T.Tagliaferri, G.Tavecchio, F.Tibaldo, L.Testa, V.Vercellone, S.Viana, A.Vink, J.Vitale, V.Vergani, S. D.Vorobiov, S.Wierzcholska, A.Yang, L.Zavrtanik, D.Zhdanov, V.
Source
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
Abstract
The discovery of gravitational waves, high-energy neutrinos or the very-high-energy counterpart of gamma-ray bursts has revolutionized the high-energy and transient astrophysics community. The development of new instruments and analysis techniques will allow the discovery and/or follow-up of new transient sources. We describe the prospects for the Cherenkov Telescope Array (CTA), the next-generation ground-based gamma-ray observatory, for multi-messenger and transient astrophysics in the decade ahead. CTA will explore the most extreme environments via very-high-energy observations of compact objects, stellar collapse events, mergers and cosmic-ray accelerators.
Comment: Submitted to ASTRONET roadmap on behalf of the CTA consortium