MAGIC 望远镜对红移 $z=1.1$ 处 GRB 201216C 的探测
高能天体物理现象
2024-07-03 v1
摘要
伽马射线暴（GRBs）是发生于宇宙学距离上的爆发性暂现事件，在多个能段以电磁辐射形式释放大量能量。我们报道了 MAGIC 望远镜对长伽马射线暴 GRB~201216C 的探测。该源位于 ，因此是迄今在甚高能段探测到的最远源。GRB~201216C 高于 \SI{70}{\GeV} 的发射与多波段数据在同步辐射与同步自康普顿（SSC）情形下一并建模。我们发现 SSC 能很好地解释从光学到甚高能波段的宽波段数据。对于晚期射电数据，需另一分量来解释观测到的发射。与先前在甚高能段探测到的伽马射线暴不同，GRB~201216C 的模型强烈倾向于星风状介质。模型参数值与以往对截至 GeV 能段探测到的伽马射线暴余辉研究所得相近。
引用
@article{arxiv.2310.06473,
title = {MAGIC detection of GRB 201216C at $z=1.1$},
author = {H. Abe and S. Abe and V. A. Acciari and I. Agudo and T. Aniello and S. Ansoldi and L. A. Antonelli and A. Arbet Engels and C. Arcaro and M. Artero and K. Asano and D. Baack and A. Babić and A. Baquero and U. Barres de Almeida and J. A. Barrio and I. Batković and J. Baxter and J. Becerra González and W. Bednarek and E. Bernardini and J. Bernete and A. Berti and J. Besenrieder and C. Bigongiari and A. Biland and O. Blanch and G. Bonnoli and Ž. Bošnjak and I. Burelli and G. Busetto and A. Campoy-Ordaz and A. Carosi and R. Carosi and M. Carretero-Castrillo and A. J. Castro-Tirado and G. Ceribella and Y. Chai and A. Cifuentes and S. Cikota and E. Colombo and J. L. Contreras and J. Cortina and S. Covino and G. D'Amico and V. D'Elia and P. Da Vela and F. Dazzi and A. De Angelis and B. De Lotto and A. Del Popolo and M. Delfino and J. Delgado and C. Delgado Mendez and D. Depaoli and F. Di Pierro and L. Di Venere and D. Dominis Prester and A. Donini and D. Dorner and M. Doro and D. Elsaesser and G. Emery and J. Escudero and L. Fariña and A. Fattorini and L. Foffano and L. Font and S. Fukami and Y. Fukazawa and R. J. García López and M. Garczarczyk and S. Gasparyan and M. Gaug and J. G. Giesbrecht Paiva and N. Giglietto and F. Giordano and P. Gliwny and N. Godinović and R. Grau and D. Green and J. G. Green and D. Hadasch and A. Hahn and T. Hassan and L. Heckmann and J. Herrera and D. Hrupec and M. Hütten and R. Imazawa and T. Inada and R. Iotov and K. Ishio and I. Jiménez Martínez and J. Jormanainen and D. Kerszberg and G. W. Kluge and Y. Kobayashi and P. M. Kouch and H. Kubo and J. Kushida and M. Láinez Lezáun and A. Lamastra and F. Leone and E. Lindfors and L. Linhoff and S. Lombardi and F. Longo and R. López-Coto and M. López-Moya and A. López-Oramas and S. Loporchio and A. Lorini and E. Lyard and B. Machado de Oliveira Fraga and P. Majumdar and M. Makariev and G. Maneva and N. Mang and M. Manganaro and S. Mangano and K. Mannheim and M. Mariotti and M. Martínez and A. Mas-Aguilar and D. Mazin and S. Menchiari and S. Mender and S. Mićanović and D. Miceli and T. Miener and J. M. Miranda and R. Mirzoyan and M. Molero González and E. Molina and H. A. Mondal and A. Moralejo and D. Morcuende and C. Nanci and L. Nava and V. Neustroev and M. Nievas Rosillo and C. Nigro and L. Nikolić and K. Nilsson and K. Nishijima and T. Njoh Ekoume and K. Noda and S. Nozaki and Y. Ohtani and A. Okumura and J. Otero-Santos and S. Paiano and M. Palatiello and D. Paneque and R. Paoletti and J. M. Paredes and L. Pavletić and D. Pavlović and M. Persic and M. Pihet and G. Pirola and F. Podobnik and P. G. Prada Moroni and E. Prandini and G. Principe and C. Priyadarshi and W. Rhode and M. Ribó and J. Rico and C. Righi and N. Sahakyan and T. Saito and K. Satalecka and F. G. Saturni and B. Schleicher and K. Schmidt and F. Schmuckermaier and J. L. Schubert and T. Schweizer and A. Sciaccaluga and J. Sitarek and V. Sliusar and D. Sobczynska and A. Spolon and A. Stamerra and J. Strišković and D. Strom and M. Strzys and Y. Suda and S. Suutarinen and H. Tajima and M. Takahashi and R. Takeishi and F. Tavecchio and P. Temnikov and K. Terauchi and T. Terzić and M. Teshima and L. Tosti and S. Truzzi and A. Tutone and S. Ubach and J. van Scherpenberg and M. Vazquez Acosta and S. Ventura and V. Verguilov and I. Viale and C. F. Vigorito and V. Vitale and I. Vovk and R. Walter and M. Will and T. Yamamoto and A. Gomboc and N. Jordana-Mitjans and A. Melandri and C. G. Mundell and M. Shrestha and I. A. Steele},
journal= {arXiv preprint arXiv:2310.06473},
year = {2024}
}
备注
13 pages, 6 figures, 2 tables. Accepted for publication in Monthly Notices of the Royal Astronomical Society