MAGIC detection of GRB 201216C at z = 1.1

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dc.contributor.authorAbe, H.
dc.contributor.authorAbe, S.
dc.contributor.authorAcciari, V.A.
dc.contributor.authorAgudo, I.
dc.contributor.authorAniello, T.
dc.contributor.authorAnsoldi, S.
dc.contributor.authorAntonelli, L.A.
dc.contributor.authorArbet Engels, A.
dc.contributor.authorArcaro, C.
dc.contributor.authorArtero, M.
dc.contributor.authorAsano, K.
dc.contributor.authorBaack, D.
dc.contributor.authorBabić, A.
dc.contributor.authorBaquero, A.
dc.contributor.authorBarres de Almeida, U.
dc.contributor.authorBarrio, J.A.
dc.contributor.authorBatković, I.
dc.contributor.authorBaxter, J.
dc.contributor.authorBecerra González, J.
dc.contributor.authorBednarek, W.
dc.contributor.authorBernardini, E.
dc.contributor.authorBernete, J.
dc.contributor.authorBerti, A.
dc.contributor.authorBesenrieder, J.
dc.contributor.authorBigongiari, C.
dc.contributor.authorBiland, A.
dc.contributor.authorBlanch, O.
dc.contributor.authorBonnoli, G.
dc.contributor.authorBošnjak, Ž.
dc.contributor.authorBurelli, I.
dc.contributor.authorBusetto, G.
dc.contributor.authorCampoy-Ordaz, A.
dc.contributor.authorCarosi, A.
dc.contributor.authorCarosi, R.
dc.contributor.authorCarretero-Castrillo, Mar
dc.contributor.authorCastro-Tirado, A.J.
dc.contributor.authorCeribella, G.
dc.contributor.authorChai, Y.
dc.contributor.authorCifuentes, A.
dc.contributor.authorCikota, S.
dc.contributor.authorColombo, Elisabetta
dc.contributor.authorContreras, J.L.
dc.contributor.authorCortina, J.
dc.contributor.authorCovino, S.
dc.contributor.authorD’Amico, G.
dc.contributor.authorD’Elia, V.
dc.contributor.authorDa Vela, P.
dc.contributor.authorDazzi, F.
dc.contributor.authorDe Angelis, A.
dc.contributor.authorDe Lotto, B.
dc.contributor.authorDel Popolo, A.
dc.contributor.authorDelfino, M.
dc.contributor.authorDelgado González, Julio
dc.contributor.authorDelgado Mendez, C.
dc.contributor.authorDepaoli, D.
dc.contributor.authorDi Pierro, F.
dc.contributor.authorDi Venere, L.
dc.contributor.authorDominis Prester, D.
dc.contributor.authorDonini, A.
dc.contributor.authorDorner, D.
dc.contributor.authorDoro, M.
dc.contributor.authorElsaesser, D.
dc.contributor.authorEmery, G.
dc.contributor.authorEscudero, J.
dc.contributor.authorFariña, L.
dc.contributor.authorFattorini, A.
dc.contributor.authorFoffano, L.
dc.contributor.authorFont, L.
dc.contributor.authorFukami, S.
dc.contributor.authorFukazawa, Yugo
dc.contributor.authorGarcía López, R.J.
dc.contributor.authorGarczarczyk, M.
dc.contributor.authorGasparyan, S.
dc.contributor.authorGaug, M.
dc.contributor.authorGiesbrecht Paiva, J.G.
dc.contributor.authorGiglietto, N.
dc.contributor.authorGiordano, F.
dc.contributor.authorGliwny, P.
dc.contributor.authorGodinović, N.
dc.contributor.authorGrau, R.
dc.contributor.authorGreen, D.
dc.contributor.authorGreen, J.G.
dc.contributor.authorHadasch, D.
dc.contributor.authorHahn, A.
dc.contributor.authorHassan, T.
dc.contributor.authorHeckmann, L.
dc.contributor.authorHerrera, J.
dc.contributor.authorHrupec, D.
dc.contributor.authorHütten, M.
dc.contributor.authorImazawa, R.
dc.contributor.authorInada, T.
dc.contributor.authorIotov, R.
dc.contributor.authorIshio, K.
dc.contributor.authorJiménez Martínez, I.
dc.contributor.authorJormanainen, J.
dc.contributor.authorKerszberg, D.
dc.contributor.authorKluge, G.W.
dc.contributor.authorKobayashi, Y.
dc.contributor.authorKouch, P.M.
dc.contributor.authorKubo, H.
dc.contributor.authorKushida, J.
dc.contributor.authorLáinez Lezáun, M.
dc.contributor.authorLamastra, A.
dc.contributor.authorLeone, F.
dc.contributor.authorLindfors, E.
dc.contributor.authorLinhoff, L.
dc.contributor.authorLombardi, S.
dc.contributor.authorLongo, F.
dc.contributor.authorLópez-Coto, R.
dc.contributor.authorLópez-Moya, M.
dc.contributor.authorLópez-Oramas, A.
dc.contributor.authorLoporchio, S.
dc.contributor.authorLorini, A.
dc.contributor.authorLyard, E.
dc.contributor.authorMachado de Oliveira Fraga, B.
dc.contributor.authorMajumdar, P.
dc.contributor.authorMakariev, M.
dc.contributor.authorManeva, G.
dc.contributor.authorMang, N.
dc.contributor.authorManganaro, M.
dc.contributor.authorMangano, S.
dc.contributor.authorMannheim, K.
dc.contributor.authorMariotti, M.
dc.contributor.authorMartínez, M.
dc.contributor.authorMas-Aguilar, A.
dc.contributor.authorMazin, D.
dc.contributor.authorMenchiari, S.
dc.contributor.authorMender, S.
dc.contributor.authorMićanović, S.
dc.contributor.authorMiceli, D.
dc.contributor.authorMiener, T.
dc.contributor.authorMiranda, J.M.
dc.contributor.authorMirzoyan, R.
dc.contributor.authorMolero González, M.
dc.contributor.authorMolina, Edgar
dc.contributor.authorMondal, H.A.
dc.contributor.authorMoralejo, A.
dc.contributor.authorMorcuende, D.
dc.contributor.authorNanci, C.
dc.contributor.authorNava, L.
dc.contributor.authorNeustroev, V.
dc.contributor.authorNievas Rosillo, M.
dc.contributor.authorNigro, C.
dc.contributor.authorNikolić, L.
dc.contributor.authorNilsson, K.
dc.contributor.authorNishijima, K.
dc.contributor.authorNjoh Ekoume, T.
dc.contributor.authorNoda, K.
dc.contributor.authorNozaki, S.
dc.contributor.authorOhtani, Y.
dc.contributor.authorOkumura, A.
dc.contributor.authorOtero-Santos, J.
dc.contributor.authorPaiano, S.
dc.contributor.authorPalatiello, M.
dc.contributor.authorPaneque, D.
dc.contributor.authorPaoletti, R.
dc.contributor.authorParedes i Poy, Josep Maria
dc.contributor.authorPavletić, L.
dc.contributor.authorPavlović, D.
dc.contributor.authorPersic, M.
dc.contributor.authorPihet, M.
dc.contributor.authorPirola, G.
dc.contributor.authorPodobnik, F.
dc.contributor.authorPrada Moroni, P.G.
dc.contributor.authorPrandini, E.
dc.contributor.authorPrincipe, G.
dc.contributor.authorPriyadarshi, C.
dc.contributor.authorRhode, W.
dc.contributor.authorRibó Gomis, Marc
dc.contributor.authorRico, J.
dc.contributor.authorRighi, C.
dc.contributor.authorSahakyan, N.
dc.contributor.authorSaito, T.
dc.contributor.authorSatalecka, K.
dc.contributor.authorSaturni, F.G.
dc.contributor.authorSchleicher, B.
dc.contributor.authorSchmidt, K.
dc.contributor.authorSchmuckermaier, F.
dc.contributor.authorSchubert, J.L.
dc.contributor.authorSchweizer, T.
dc.contributor.authorSciaccaluga, A.
dc.contributor.authorSitarek, J.
dc.contributor.authorSliusar, V.
dc.contributor.authorSobczynska, D.
dc.contributor.authorSpolon, A.
dc.contributor.authorStamerra, A.
dc.contributor.authorStrišković, J.
dc.contributor.authorStrom, D.
dc.contributor.authorStrzys, M.
dc.contributor.authorSuda, Y.
dc.contributor.authorSuutarinen, S.
dc.contributor.authorTajima, H.
dc.contributor.authorTakahashi, M.
dc.contributor.authorTakeishi, R.
dc.contributor.authorTavecchio, F.
dc.contributor.authorTemnikov, P.
dc.contributor.authorTerauchi, K.
dc.contributor.authorTerzić, T.
dc.contributor.authorTeshima, M.
dc.contributor.authorTosti, L.
dc.contributor.authorTruzzi, S.
dc.contributor.authorTutone, A.
dc.contributor.authorUbach, S.
dc.contributor.authorvan Scherpenberg, J.
dc.contributor.authorVazquez Acosta, M.
dc.contributor.authorVentura, Salvador
dc.contributor.authorVerguilov, V.
dc.contributor.authorViale, I.
dc.contributor.authorVigorito, C.F.
dc.contributor.authorVitale, V.
dc.contributor.authorVovk, I.
dc.contributor.authorWalter, R.
dc.contributor.authorWill, M.
dc.contributor.authorYamamoto, T.
dc.contributor.authorGomboc, A.
dc.contributor.authorJordana-Mitjans, N.
dc.contributor.authorMelandri, A.
dc.contributor.authorMundell, C.G.
dc.contributor.authorShrestha, M.
dc.contributor.authorSteele, I.A.
dc.date.accessioned2025-04-14T16:22:01Z
dc.date.available2025-04-14T16:22:01Z
dc.date.issued2024-01-01
dc.date.updated2025-04-14T16:22:02Z
dc.description.abstractGamma-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.
dc.format.extent12 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec743765
dc.identifier.issn0035-8711
dc.identifier.urihttps://hdl.handle.net/2445/220456
dc.language.isoeng
dc.publisherRoyal Astronomical Society
dc.relation.isformatofReproducció del document publicat a: https://doi.org/10.1093/mnras/stad2958
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society, 2024, vol. 527, num.3, p. 5856-5867
dc.relation.urihttps://doi.org/10.1093/mnras/stad2958
dc.rights(c) Abe, H. et al., 2024
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationAstrofísica
dc.subject.classificationEsclat de raigs gamma
dc.subject.classificationFísica de partícules
dc.subject.otherAstrophysics
dc.subject.otherGamma ray bursts
dc.subject.otherParticle physics
dc.titleMAGIC detection of GRB 201216C at z = 1.1
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion

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