MAGIC detection of GRB 201216C at z = 1.1

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.; Pierro, F. Di; Venere, L. Di; 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.; de Oliveira Fraga, B. Machado; 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.

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Katsuaki Asano
Abe et al., 2023

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Oxford University Press, Monthly Notices of the Royal Astronomical Society, 3(527), p. 5856-5867, 2023

DOI: 10.1093/mnras/stad2958

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@article{Abe2023,
  abstract = {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.},
  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 Pierro, F. Di and Venere, L. Di and Prester, D. Dominis 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 de Oliveira Fraga, B. Machado 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 Rosillo, M. Nievas 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 Moroni, P. G. Prada 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 Acosta, M. Vazquez 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.},
  doi = {10.1093/mnras/stad2958},
  journal = {Monthly Notices of the Royal Astronomical Society},
  month = {oct},
  pages = {5856-5867},
  title = {MAGIC detection of GRB 201216C at z = 1.1},
  url = {https://oadoi.org/10.1093/mnras/stad2958},
  volume = {527},
  year = {2023}
}

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MAGIC detection of GRB 201216C at z = 1.1

Journal article published in 2023 by H. Abe, S. Abe, V. A. Acciari, I. Agudo, T. Aniello, S. Ansoldi, L. A. Antonelli, A. Arbet Engels, C. Arcaro, M. Artero, K. Asano

, D. Baack, A. Babić, A. Baquero, U. Barres de Almeida and other authors. H. Abe, S. Abe, V. A. Acciari, I. Agudo, T. Aniello, S. Ansoldi, L. A. Antonelli, A. Arbet Engels, C. Arcaro, M. Artero, K. Asano

, D. Baack, A. Babić, A. Baquero, U. Barres de Almeida, J. A. Barrio, I. Batković, J. Baxter, J. Becerra González, W. Bednarek, E. Bernardini, J. Bernete, A. Berti

, J. Besenrieder, C. Bigongiari, A. Biland, O. Blanch, G. Bonnoli, Ž. Bošnjak, I. Burelli, G. Busetto, A. Campoy-Ordaz, A. Carosi, R. Carosi, M. Carretero-Castrillo, A. J. Castro-Tirado, G. Ceribella, Y. Chai, A. Cifuentes, S. Cikota, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, G. D’Amico, V. D’Elia, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, A. Del Popolo, M. Delfino, J. Delgado, C. Delgado Mendez, D. Depaoli, F. Di Pierro, L. Di Venere, D. Dominis Prester, A. Donini, D. Dorner, M. Doro, D. Elsaesser, G. Emery, J. Escudero

, L. Fariña, A. Fattorini, L. Foffano, L. Font, S. Fukami

, Y. Fukazawa, R. J. García López, M. Garczarczyk, S. Gasparyan, M. Gaug, J. G. Giesbrecht Paiva, N. Giglietto, F. Giordano, P. Gliwny, N. Godinović, R. Grau, D. Green, J. G. Green, D. Hadasch, A. Hahn, T. Hassan, L. Heckmann, J. Herrera, D. Hrupec, M. Hütten, R. Imazawa, T. Inada, R. Iotov, K. Ishio, I. Jiménez Martínez, J. Jormanainen, D. Kerszberg, G. W. Kluge, Y. Kobayashi, P. M. Kouch, H. Kubo, J. Kushida, M. Láinez Lezáun, A. Lamastra, F. Leone, E. Lindfors, L. Linhoff, S. Lombardi, F. Longo, R. López-Coto, M. López-Moya, A. López-Oramas, S. Loporchio

, A. Lorini, E. Lyard, B. Machado de Oliveira Fraga, P. Majumdar, M. Makariev, G. Maneva, N. Mang, M. Manganaro, S. Mangano, K. Mannheim, M. Mariotti, M. Martínez, A. Mas-Aguilar, D. Mazin, S. Menchiari, S. Mender, S. Mićanović, D. Miceli, T. Miener, J. M. Miranda, R. Mirzoyan, M. Molero González, E. Molina, H. A. Mondal, A. Moralejo, D. Morcuende, C. Nanci, L. Nava

, V. Neustroev, M. Nievas Rosillo, C. Nigro, L. Nikolić, K. Nilsson, K. Nishijima, T. Njoh Ekoume, K. Noda, S. Nozaki, Y. Ohtani, A. Okumura, J. Otero-Santos, S. Paiano, M. Palatiello, D. Paneque, R. Paoletti, J. M. Paredes, L. Pavletić, D. Pavlović, M. Persic, M. Pihet, G. Pirola, F. Podobnik, P. G. Prada Moroni, E. Prandini, G. Principe, C. Priyadarshi, W. Rhode, M. Ribó, J. Rico, C. Righi, N. Sahakyan, T. Saito, K. Satalecka, F. G. Saturni, B. Schleicher, K. Schmidt, F. Schmuckermaier, J. L. Schubert, T. Schweizer, A. Sciaccaluga, J. Sitarek, V. Sliusar, D. Sobczynska, A. Spolon, A. Stamerra, J. Strišković, D. Strom, M. Strzys, Y. Suda

, S. Suutarinen

, H. Tajima, M. Takahashi, R. Takeishi, F. Tavecchio, P. Temnikov, K. Terauchi, T. Terzić, M. Teshima, L. Tosti, S. Truzzi, A. Tutone, S. Ubach, J. van Scherpenberg, M. Vazquez Acosta, S. Ventura, V. Verguilov, I. Viale, C. F. Vigorito, V. Vitale, I. Vovk, R. Walter, M. Will, T. Yamamoto, A. Gomboc, N. Jordana-Mitjans, A. Melandri

, C. G. Mundell, M. Shrestha, I. A. Steele

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Abstract

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.

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MAGIC detection of GRB 201216C at z = 1.1

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