Accès ouvert déclaré
2026
preprint
VHE gamma-ray intranight variability from BL Lacertae during the extreme flaring state of 2022
K. Abe, S. Abe, A. Abhishek, Fernando Acero, Arnau Aguasca-Cabot, I. Agudo, Cyril Martin Alispach, D. Ambrosino, F. Ambrosino, L. A. Antonelli, C. Aramo, Axel Arbet-Engels, Cornelia Arcaro, T. T. H. Arnesen, P. Aubert, Ali Baktash, Matteo Balbo, Aya Bamba, A. Baquero Larriva, U. Barres de Almeida, J. A. Barrio, L. Barrios Jiménez, Ivana Batković, J. Baxter, J. Becerra González, J. Bernete, A. Berti, E. Bissaldi, O. Blanch, G. Bonnoli, P. Bordas, A. Briscioli, G. Brunelli, J. Buces, A. Bulgarelli, Irene Burelli, L. Burmistrov, M. Cardillo, Sami Caroff, A. Carosi, R. Carraro, Francesco Cassol, Davide Cerasole, A. Cerviño Cortínez, Y. Chai, G. Chon, L. Chytka, G. M. Cicciari, J. L. Contreras, J. Cortina, H. Costantini, M. Croisonnier, M. Dalchenko, G. D'Amico, P. Da Vela, F. Dazzi, A. De Angelis, M. de Bony de Lavergne, R. Del Burgo, Carmen Delgado, J. Delgado Mengual, D. della Volpe, B. De Lotto, L. del Peral, R. de Menezes, G. De Palma, V. de Souza, C. Díaz, L. Di Bella, Ambra Di Piano, F. Di Pierro, R. Di Tria, L. Di Venere, D. Dominis Prester, A. Donini, D. Dorner, Laura Eisenberger, D. Elsässer, G. Emery, L. Feligioni, F. Ferrarotto, A. Fiasson, L. Foffano, Y. Fukazawa, S. Gallozzi, R. Garcia López, S. Garcia Soto, C. Gasbarra, D. Gasparrini, J. Giesbrecht Paiva, N. Giglietto, F. Giordano, N. Godinovic, T. Gradetzke, R. Grau, J. Green, G. Grolleron, S. Gunji, P. Günther, Jonas Hackfeld, D. Hadasch, M. Hashizume, T. Hassan, K. Hayashi, L. Heckmann, M. Heller, J. Herrera Llorente, Nagisa Hiroshima, D. Hoffmann, D. Horns, Julien Houles, Dario Hrupec, R. Imazawa, T. Inada, S. Inoue, K. Ioka, M. Iori, T. Itokawa, A. Iuliano, J. Jahanvi, I. Jimenez Martinez, J. Jimenez Quiles, I. Jorge Rodrigo, Jakub Jurýšek, M. Kagaya, V. Karas, H. Katagiri, D. Kerszberg, Takuto Kiyomoto, Y. Kobayashi, K. Kohri, Paula Kornecki, H. Kubo, J. Kushida, Bastien Lacave, M. Lainez, A. Lamastra, L. Lemoigne, M. Linhoff, S. Lombardi, F. Longo, R. López-Coto, A. López-Oramas, S. Loporchio, J. Lozano Bahilo, F. Lucarelli, H. Luciani, P. L. Luque-Escamilla, M. Makariev, M. Mallamaci, D. Mandat, K. Mannheim, F. Marini, M. Mariotti, Patricia Márquez, G. Marsella, J. Martí, O. Martinez, G. Martínez, M. Martínez, M. Massa, D. Mazin, J. Méndez-Gallego, S. Menon, E. Mestre Guillen, Davide Miceli, T. Miener, J. M. Miranda, M. Molero Gonzalez, E. Molina, T. Montaruli, Abelardo Moralejo, Alessandro Morselli, Víctor Moya, A. L. Müller, H. Muraishi, S. Nagataki, T. Nakamori, A. Neronov, D. Nieto Castaño, M. Nievas Rosillo, L. Nikolic, K. Noda, V. Novotny, S. Nozaki, M. Ohishi, Y. Ohtani, A. Okumura, R. Orito, L. Orsini, J. Otero-Santos, P. Ottanelli, M. Palatiello, Gabriele Panebianco, D. Paneque, R. Paoletti, J. M. Paredes, M. Pech, Mario Pecimotika, M. Peresano, F. Perrotta, Felix Pfeifle, Marine Pihet, Gian Pietro Pirola, C. Plard, F. Podobnik, M. Polo, C. Pozo-Gonzaléz, E. Prandini, S. Rainò, R. Rando, W. Rhode, M. Ribó, G. Rodriguez Fernandez, M. D. Rodríguez Frías, A. Roy, A. Ruina, E. Ruiz-Velasco, T. Saito, S. Sakurai, D. A. Sanchez, H. Sano, E. Santos Moura, T. Šarić, Y. Sato, F. G. Saturni, V. Savchenko, F. Schiavone, F. Schussler, T. Schweizer, M. Seglar Arroyo, G. Silvestri, A. Simongini, J. Sitarek, Vitalii Sliusar, I. Sofia, Jelena Strišković, M. Strzys, Y. Suda, A. Sunny, H. Tajima, M. Takahashi, Ryuji Takeishi, S. J. Tanaka, Dai Tateishi, T. Tavernier, P. Temnikov, Y. Terada, Kenta Terauchi, T. Terzić, M. Teshima, Martin Tluczykont, T. Tomura, D. F. Torres, F. Tramonti, P. Travnicek, G. Tripodo, Antonio Tutone, Martin Vacula, M. Vázquez Acosta, G. Verna, Ilaria Viale, A. Viana, Alessandro Vigliano, C. F. Vigorito, Elisa Visentin, V. Vitale, Georgios Gerasimos Voutsinas, I. Vovk, T. Vuillaume, R. Walter, T. Yamamoto, R. Yamazaki, Y. Yao, T. Yoshida, T. Yoshikoshi, W. Zhang, N. Zywucka, the CTAO-LST collaboration, F. J. Aceituno, J. A. Acosta-Pulido, V. Casanova, J. Escudero Pedrosa, V. Fallah Ramazani, J. Jormanainen, S. Jorstad, G. Keating, P. M. Kouch, M. Gurwell, A. Lähteenmäki, E. Lindfors, A. Marscher, D. Morcuende, I. Myserlis, K. Nilsson, C. A. Ortega Hunter, R. Rao, A. Sota, M. Tornikoski, H. Zhang
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28Institutions déclarées
10Pays d’affiliation déclarés
Résumé fourni par la source
BL Lacertae (BL Lac), the archetypal blazar of its subclass and one of the most studied blazars in the last decades, has undergone a series of major multi-wavelength outbursts since 2020, resulting in its highest recorded $γ$-ray flare to date between September and November 2022 together with those from August 2021 and October 2024. We characterised the $γ$-ray and multi-wavelength emission and spectral energy distribution (SED) of BL Lac, as well as their evolution during the major and extended $γ$-ray and multi-wavelength flare that occurred between September and November 2022. We evaluated the variability of the flare, focusing on the nights of October 20 and November 13, when clear intranight very-high-energy (VHE, $E>100$ GeV) $γ$-ray variability was observed. We modelled the $γ$-ray and broadband SEDs during periods of stable emission identified with a Bayesian block analysis and interpreted the flare's evolution in terms of the variability in the relativistic particles and the jet's physical parameters. The VHE emission shows an average flux of 0.23 Crab Units (C.U.) above 200 GeV and a variability amplitude of more than a factor ten. We observe intranight flux-doubling variations as fast as $\sim$8 minutes during the nights of October 20 and November 13, 2022 with maximum fluxes of 4.4 C.U. above 100 GeV and 2.8 C.U. above 200 GeV. The spectral analysis reveals a transition of the X-ray emission from the high- to the low-energy SED peak and a shift of the $γ$-ray peak towards higher energies. We interpret the broadband emission within a leptonic two-zone model in which intranight variability is explained as magnetic reconnection in a compact region closely oriented with the line of sight while variations in the relativistic electron distributions and the injection of freshly accelerated particles explain the weekly scale variations.
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Sujets associés
Astrophysics and Cosmic PhenomenaQuantum and Classical ElectrodynamicsInsects and Parasite Interactions