Start Over

MAGIC detection of GRB 201216C at $z=1.1$

Authors :: Abe, H.
Abe, S.
Acciari, V. A.
Agudo, I.
Aniello, T.
Ansoldi, S.
Antonelli, L. A.
Engels, A. Arbet
Arcaro, C.
Artero, M.
Asano, K.
Baack, D.
Babić, A.
Baquero, A.
de Almeida, U. Barres
Barrio, J. A.
Batković, I.
Baxter, J.
González, J. Becerra
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, M.
Castro-Tirado, A. J.
Ceribella, G.
Chai, Y.
Cifuentes, A.
Cikota, S.
Colombo, E.
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, J.
Mendez, C. Delgado
Depaoli, D.
Di Pierro, F.
Di Venere, L.
Prester, D. Dominis
Donini, A.
Dorner, D.
Doro, M.
Elsaesser, D.
Emery, G.
Escudero, J.
Fariña, L.
Fattorini, A.
Foffano, L.
Font, L.
Fukami, S.
Fukazawa, Y.
López, R. J. García
Garczarczyk, M.
Gasparyan, S.
Gaug, M.
Paiva, J. G. Giesbrecht
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.
Martínez, I. Jiménez
Jormanainen, J.
Kerszberg, D.
Kluge, G. W.
Kobayashi, Y.
Kouch, P. M.
Kubo, H.
Kushida, J.
Lezáun, M. Láinez
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.
Fraga, B. Machado de Oliveira
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.
González, M. Molero
Molina, E.
Mondal, H. A.
Moralejo, A.
Morcuende, D.
Nanci, C.
Nava, L.
Neustroev, V.
Rosillo, M. Nievas
Nigro, C.
Nikolić, L.
Nilsson, K.
Nishijima, K.
Ekoume, T. Njoh
Noda, K.
Nozaki, S.
Ohtani, Y.
Okumura, A.
Otero-Santos, J.
Paiano, S.
Palatiello, M.
Paneque, D.
Paoletti, R.
Paredes, J. M.
Pavletić, L.
Pavlović, D.
Persic, M.
Pihet, M.
Pirola, G.
Podobnik, F.
Moroni, P. G. Prada
Prandini, E.
Principe, G.
Priyadarshi, C.
Rhode, W.
Ribó, M.
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.
Acosta, M. Vazquez
Ventura, S.
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.
Source :: Monthly Notices of the Royal Astronomical Society, Volume 527, Issue 3, January 2024, Pages 5856-5867
Publication Year :: 2023
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 \SI{70}{\GeV} of GRB~201216C is modelled together with multi-wavelength data within a synchrotron and synchrotron-self Compton (SSC) scenario. We find that SSC can explain the broadband 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 favors 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.<br />Comment: 13 pages, 6 figures, 2 tables. Accepted for publication in Monthly Notices of the Royal Astronomical Society

Subjects :: Astrophysics - High Energy Astrophysical Phenomena

Details

Database :: arXiv
Journal :: Monthly Notices of the Royal Astronomical Society, Volume 527, Issue 3, January 2024, Pages 5856-5867
Publication Type :: Report
Accession number :: edsarx.2310.06473
Document Type :: Working Paper
Full Text :: https://doi.org/10.1093/mnras/stad2958