Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/220456
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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