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arxiv: 2106.03621 · v1 · pith:XN7NBBRRnew · submitted 2021-06-07 · 🌌 astro-ph.HE

Multi-messenger and transient astrophysics with the Cherenkov Telescope Array

\v{Z}. Bo\v{s}njak , A. M. Brown , A. Carosi , M. Chernyakova , P. Cristofari , F. Longo , A. L\'opez-Oramas , M. Santander
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K. Satalecka F. Sch\"ussler O. Sergijenko A. Stamerra I. Agudo R. Alves Batista E. Amato E. O. Anguner L. A. Antonelli M. Backes Csaba Balazs L. Baroncelli J. Becker Tjus C. Bigongiari E. Bissaldi C. Boisson J. Bolmont M. B\"ottcher P. Bordas C. Braiding J. Bregeon N. Bucciantini A. Bulgarelli M. Burton F. Cangemi P. Caraveo M. Cardillo S. Caroff S. Casanova S. Chaty J. G. Coelho G. Cotter A. D'A\`i F. D'Ammando E. M. de Gouveia Dal Pino D. della Volpe D. de Martino T. Di Girolamo A. Di Piano A. Djannati-Ata\"i V. Dwarkadas E. de Ona Wilhelmi R. C. Dos Anjos G. Emery E. Fedorova S. Fegan A. Fiasson V. Fioretti M.D. Filipovic D. Gaggero G. Galanti D. Gasparrini G.Ghirlanda P. Goldoni J. Granot J. G. Green M. Heller B. Hnatyk R. Hnatyk D. Horan T. Hovatta S. Inoue M. Jamrozy D. Kantzas B. Kh\'elifi N. Komin A. Lamastra N. La Palombara J. P. Lenain E. Lindfors I. Liodakis S. Lombardi F. Lucarelli P. L. Luque-Escamilla P. Majumdar A. Marcowith S. Markoff J. Marti M. Martinez D. Mazin S. McKeague S. Mereghetti E. Mestre T. Montaruli G. Morlino A. Morselli C. Mundell T. Murach L. Nava A. Nayerhoda L. Nicastro J. Niemiec M. Nikolajuk B. Olmi R. Ong M. Orienti J.P. Osborne Josep M. Paredes G. Pareschi N. Parmiggiani B. Patricelli A. Pe'er G. Piano G. P\"uhlhofer M. Punch O. Reimer M. Rib\'o G. Rodriguez J. Rodriguez P. Romano G. Romeo M. Roncadelli G. Rowell B. Rudak I. Sadeh F. Salesa Greus F. G. Saturni U. Sawangwit M. Seglar-Arroyo R. C. Shellard H. Sol R. Starling T. Stolarczyk G. Tagliaferri F. Tavecchio L. Tibaldo V. Testa S. Vercellone A. Viana J. Vink V. Vitale S. D. Vergani S. Vorobiov A. Wierzcholska L. Yang D. Zavrtanik V. Zhdanov (on behalf of the CTA Consortium)
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classification 🌌 astro-ph.HE
keywords transientastrophysicsarraycherenkovdiscoverygamma-rayhigh-energymulti-messenger
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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.

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