Title: | MAGIC detection of GRB 201216C at z = 1.1 |
Author: | Abe, H. Abe, S. Acciari, V.A. Agudo, I. Aniello, T. Ansoldi, S. Antonelli, L.A. Arbet Engels, A. Arcaro, C. Artero, M. Asano, K. Baack, D. Babić, A. Baquero, A. Barres de Almeida, U. Barrio, J.A. Batković, I. Baxter, J. Becerra González, J. Bednarek, W. Bernardini, E. Bernete, J. Berti, A. Besenrieder, J. Bigongiari, C. Biland, A. Blanch, O. Bonnoli, G. Bošnjak, Ž. Burelli, I. Busetto, G. Campoy-Ordaz, A. Carosi, A. Carosi, R. Carretero-Castrillo, Mar Castro-Tirado, A.J. Ceribella, G. Chai, Y. Cifuentes, A. Cikota, S. Colombo, Elisabetta Contreras, J.L. Cortina, J. Covino, S. D’Amico, G. D’Elia, V. Da Vela, P. Dazzi, F. De Angelis, A. De Lotto, B. Del Popolo, A. Delfino, M. Delgado González, Julio Delgado Mendez, C. Depaoli, D. Di Pierro, F. Di Venere, L. Dominis Prester, D. Donini, A. Dorner, D. Doro, M. Elsaesser, D. Emery, G. Escudero, J. Fariña, L. Fattorini, A. Foffano, L. Font, L. Fukami, S. Fukazawa, Yugo García López, R.J. Garczarczyk, M. Gasparyan, S. Gaug, M. Giesbrecht Paiva, J.G. Giglietto, N. Giordano, F. Gliwny, P. Godinović, N. Grau, R. Green, D. Green, J.G. Hadasch, D. Hahn, A. Hassan, T. Heckmann, L. Herrera, J. Hrupec, D. Hütten, M. Imazawa, R. Inada, T. Iotov, R. Ishio, K. Jiménez Martínez, I. Jormanainen, J. Kerszberg, D. Kluge, G.W. Kobayashi, Y. Kouch, P.M. Kubo, H. Kushida, J. Láinez Lezáun, M. Lamastra, A. Leone, F. Lindfors, E. Linhoff, L. Lombardi, S. Longo, F. López-Coto, R. López-Moya, M. López-Oramas, A. Loporchio, S. Lorini, A. Lyard, E. Machado de Oliveira Fraga, B. Majumdar, P. Makariev, M. Maneva, G. Mang, N. Manganaro, M. Mangano, S. Mannheim, K. Mariotti, M. Martínez, M. Mas-Aguilar, A. Mazin, D. Menchiari, S. Mender, S. Mićanović, S. Miceli, D. Miener, T. Miranda, J.M. Mirzoyan, R. Molero González, M. Molina, Edgar Mondal, H.A. Moralejo, A. Morcuende, D. Nanci, C. Nava, L. Neustroev, V. Nievas Rosillo, M. Nigro, C. Nikolić, L. Nilsson, K. Nishijima, K. Njoh Ekoume, T. Noda, K. Nozaki, S. Ohtani, Y. Okumura, A. Otero-Santos, J. Paiano, S. Palatiello, M. Paneque, D. Paoletti, R. Paredes i Poy, Josep Maria Pavletić, L. Pavlović, D. Persic, M. Pihet, M. Pirola, G. Podobnik, F. Prada Moroni, P.G. Prandini, E. Principe, G. Priyadarshi, C. Rhode, W. Ribó Gomis, Marc Rico, J. Righi, C. Sahakyan, N. Saito, T. Satalecka, K. Saturni, F.G. Schleicher, B. Schmidt, K. Schmuckermaier, F. Schubert, J.L. Schweizer, T. Sciaccaluga, A. Sitarek, J. Sliusar, V. Sobczynska, D. Spolon, A. Stamerra, A. Strišković, J. Strom, D. Strzys, M. Suda, Y. Suutarinen, S. Tajima, H. Takahashi, M. Takeishi, R. Tavecchio, F. Temnikov, P. Terauchi, K. Terzić, T. Teshima, M. Tosti, L. Truzzi, S. Tutone, A. Ubach, S. van Scherpenberg, J. Vazquez Acosta, M. Ventura, Salvador Verguilov, V. Viale, I. Vigorito, C.F. Vitale, V. Vovk, I. Walter, R. Will, M. Yamamoto, T. Gomboc, A. Jordana-Mitjans, N. Melandri, A. Mundell, C.G. Shrestha, M. Steele, I.A. |
Keywords: | Astrofísica Esclat de raigs gamma Física de partícules Astrophysics Gamma ray bursts Particle physics |
Issue Date: | 1-Jan-2024 |
Publisher: | Royal Astronomical Society |
Abstract: | Gamma-ray bursts (GRBs) are explosive transient events occurring at cosmological distances, releasing a large amount of energy as electromagnetic radiation over several energy bands. We report the detection of the long GRB 201216C by the MAGIC telescopes. The source is located at z = 1.1 and thus it is the farthest one detected at very high energies. The emission above 70 GeV of GRB 201216C is modelled together with multiwavelength data within a synchrotron and synchrotron self-Compton (SSC) scenario. We find that SSC can explain the broad-band data well from the optical to the very-high-energy band. For the late-time radio data, a different component is needed to account for the observed emission. Differently from previous GRBs detected in the very-high-energy range, the model for GRB 201216C strongly favours a wind-like medium. The model parameters have values similar to those found in past studies of the afterglows of GRBs detected up to GeV energies. |
Note: | Reproducció del document publicat a: https://doi.org/10.1093/mnras/stad2958 |
It is part of: | Monthly Notices of the Royal Astronomical Society, 2024, vol. 527, num.3, p. 5856-5867 |
URI: | https://hdl.handle.net/2445/220456 |
Related resource: | https://doi.org/10.1093/mnras/stad2958 |
ISSN: | 0035-8711 |
Appears in Collections: | Articles publicats en revistes (Física Quàntica i Astrofísica) Articles publicats en revistes (Institut de Ciències del Cosmos (ICCUB))
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