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@ARTICLE{Abe:620273,
      author       = {Abe, H. and Abe, S. and Acciari, V. A. and Agudo, I. and
                      Aniello, T. and Ansoldi, S. and Antonelli, L. A. and Engels,
                      A. Arbet and Arcaro, C. and Artero, M. and Asano, K. and
                      Baack, D. and Babić, A. and Baquero, A. and de Almeida, U.
                      Barres and Barrio, J. A. and Batković, I. and Baxter, J.
                      and González, J. Becerra and Bednarek, W. and Bernardini,
                      E. and Bernete, J. and Berti, A. and Besenrieder, J. and
                      Bigongiari, C. and Biland, A. and Blanch, O. and Bonnoli, G.
                      and Bošnjak, Ž. and Burelli, I. and Busetto, G. and
                      Campoy-Ordaz, A. and Carosi, A. and Carosi, R. and
                      Carretero-Castrillo, M. and Castro-Tirado, A. J. and
                      Ceribella, G. and Chai, Y. and Cifuentes, A. and Cikota, S.
                      and Colombo, E. and Contreras, J. L. and Cortina, J. and
                      Covino, S. and D'Amico, G. and D'Elia, V. and Da Vela, P.
                      and Dazzi, F. and De Angelis, A. and De Lotto, B. and Del
                      Popolo, A. and Delfino, M. and Delgado, J. and Mendez, C.
                      Delgado and Depaoli, D. and Di Pierro, F. and Di Venere, L.
                      and Dominis Prester, D. and Donini, A. and Dorner, D. and
                      Doro, M. and Elsaesser, D. and Emery, G. and Escudero, J.
                      and Fariña, L. and Fattorini, A. and Foffano, L. and Font,
                      L. and Fukami, S. and Fukazawa, Y. and López, R. J. García
                      and Garczarczyk, M. and Gasparyan, S. and Gaug, M. and
                      Paiva, J. G. Giesbrecht and Giglietto, N. and Giordano, F.
                      and Gliwny, P. and Godinović, N. and Grau, R. and Green, D.
                      and Green, J. G. and Hadasch, D. and Hahn, A. and Hassan, T.
                      and Heckmann, L. and Herrera, J. and Hrupec, D. and Hütten,
                      M. and Imazawa, R. and Inada, T. and Iotov, R. and Ishio, K.
                      and Martínez, I. Jiménez and Jormanainen, J. and
                      Kerszberg, D. and Kluge, G. W. and Kobayashi, Y. and Kouch,
                      P. M. and Kubo, H. and Kushida, J. and Lezáun, M. Láinez
                      and Lamastra, A. and Leone, F. and Lindfors, E. and Linhoff,
                      L. and Lombardi, S. and Longo, F. and López-Coto, R. and
                      López-Moya, M. and López-Oramas, A. and Loporchio, S. and
                      Lorini, A. and Lyard, E. and Fraga, B. Machado de Oliveira
                      and Majumdar, P. and Makariev, M. and Maneva, G. and Mang,
                      N. and Manganaro, M. and Mangano, S. and Mannheim, K. and
                      Mariotti, M. and Martínez, M. and Mas-Aguilar, A. and
                      Mazin, D. and Menchiari, S. and Mender, S. and Mićanović,
                      S. and Miceli, D. and Miener, T. and Miranda, J. M. and
                      Mirzoyan, R. and González, M. Molero and Molina, E. and
                      Mondal, H. A. and Moralejo, A. and Morcuende, D. and Nanci,
                      C. and Nava, L. and Neustroev, V. and Nievas Rosillo, M. and
                      Nigro, C. and Nikolić, L. and Nilsson, K. and Nishijima, K.
                      and Ekoume, T. Njoh and Noda, K. and Nozaki, S. and Ohtani,
                      Y. and Okumura, A. and Otero-Santos, J. and Paiano, S. and
                      Palatiello, M. and Paneque, D. and Paoletti, R. and Paredes,
                      J. M. and Pavletić, L. and Pavlović, D. and Persic, M. and
                      Pihet, M. and Pirola, G. and Podobnik, F. and Prada Moroni,
                      P. G. and Prandini, E. and Principe, G. and Priyadarshi, C.
                      and Rhode, W. and Ribó, M. and Rico, J. and Righi, C. and
                      Sahakyan, N. and Saito, T. and Satalecka, K. and Saturni, F.
                      G. and Schleicher, B. and Schmidt, K. and Schmuckermaier, F.
                      and Schubert, J. L. and Schweizer, T. and Sciaccaluga, A.
                      and Sitarek, J. and Sliusar, V. and Sobczynska, D. and
                      Spolon, A. and Stamerra, A. and Strišković, J. and Strom,
                      D. and Strzys, M. and Suda, Y. and Suutarinen, S. and
                      Tajima, H. and Takahashi, M. and Takeishi, R. and Tavecchio,
                      F. and Temnikov, P. and Terauchi, K. and Terzić, T. and
                      Teshima, M. and Tosti, L. and Truzzi, S. and Tutone, A. and
                      Ubach, S. and van Scherpenberg, J. and Vazquez Acosta, M.
                      and Ventura, S. and Verguilov, V. and Viale, I. and
                      Vigorito, C. F. and Vitale, V. and Vovk, I. and Walter, R.
                      and Will, M. and Yamamoto, T. and Gomboc, A. and
                      Jordana-Mitjans, N. and Melandri, A. and Mundell, C. G. and
                      Shrestha, M. and Steele, I. A.},
      title        = {{MAGIC} detection of {GRB} 201216{C} at $z$ = 1.1},
      issn         = {1365-2966},
      reportid     = {PUBDB-2025-00107, arXiv:2310.06473},
      year         = {2023},
      note         = {13 pages, 6 figures, 2 tables. Accepted for publication in
                      Monthly Notices of the 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.},
      keywords     = {gamma ray: burst (INSPIRE) / radiation: electromagnetic
                      (INSPIRE) / VHE (INSPIRE) / MAGIC (INSPIRE) / redshift
                      (INSPIRE) / gamma ray: emission (INSPIRE) / Compton
                      scattering (INSPIRE) / GeV (INSPIRE) / synchrotron (INSPIRE)
                      / optical (INSPIRE) / astroparticle physics (autogen) /
                      radiation mechanisms: non-thermal (autogen) / gamma-ray
                      burst: individual: GRB 201216C (autogen) / gamma-ray bursts
                      (autogen)},
      cin          = {$Z_CTAS$},
      ddc          = {520},
      cid          = {$I:(DE-H253)Z_CTAS-20210408$},
      pnm          = {611 - Fundamental Particles and Forces (POF4-611)},
      pid          = {G:(DE-HGF)POF4-611},
      experiment   = {EXP:(DE-H253)CTA-20150101},
      typ          = {PUB:(DE-HGF)25},
      eprint       = {2310.06473},
      howpublished = {arXiv:2310.06473},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2310.06473;\%\%$},
      doi          = {10.1093/mnras/stad2958},
      url          = {https://bib-pubdb1.desy.de/record/620273},
}