Very-high-energy gamma-ray intranight variability from BL Lacertae during the extreme flaring state of 2022

Abe, K.; Abe, S.; Abhishek, Abhishek; Acero, F.; Aguasca-Cabot, A.; Agudo, I.; Alispach, C.; Ambrosino, D.; Ambrosino, F.; Antonelli, L. A.; Aramo, C.; Arbet-Engels, A.; Arcaro, C.; Arnesen, T. T. H.; Aubert, P.; Baktash, A.; Balbo, M.; Bamba, A.; Baquero Larriva, A.; Barres De Almeida, U.; Barrio, J. A.; Barrios Jiménez, L.; Batkovic, I.; Baxter, J.; Becerra González, J.; Bernete, J.; Berti, A.; Bissaldi, E.; Blanch, O.; Bonnoli, G.; Bordas, P.; Briscioli, A.; Brunelli, G.; Buces, J.; Bulgarelli, A.; Burelli, I.; Burmistrov, L.; Cardillo, M.; Caroff, S.; Carosi, A.; Carraro, R.; Cassol, F.; Cerasole, D.; Cerviño Cortínez, A.; Chai, Y.; Chon, G.; Chytka, L.; Cicciari, G. M.; Contreras, J. L.; Cortina, J.; Costantini, H.; Croisonnier, M.; Dalchenko, M.; D'Amico, G.; Da Vela, P.; Dazzi, F.; De Angelis, A.; De Bony De Lavergne, M.; Del Burgo, R.; Delgado, C.; Delgado Mengual, J.; Della Volpe, D.; De Lotto, B.; Del Peral, L.; De Menezes, R.; De Palma, G.; De Souza, V.; Díaz, C.; Di Bella, L.; Di Piano, A.; Di Pierro, F.; Di Tria, R.; Di Venere, L.; Dominis Prester, D.; Donini, A.; Dorner, D.; Eisenberger, L.; Elsässer, D.; Emery, G.; Feligioni, L.; Ferrarotto, F.; Fiasson, A.; Foffano, L.; Fukazawa, Y.; Gallozzi, S.; Garcia López, R.; Garcia Soto, S.; Gasbarra, C.; Gasparrini, D.; Giesbrecht Paiva, J.; Giglietto, N.; Giordano, F.; Godinovic, N.; Gradetzke, T.; Grau, R.; Green, J.; Grolleron, G.; Gunji, S.; Günther, P.; Hackfeld, J.; Hadasch, D.; Hashizume, M.; Hassan, T.; Hayashi, K.; Heckmann, L.; Heller, M.; Herrera Llorente, J.; Hiroshima, N.; Hoffmann, D.; Horns, D.; Houles, J.; Hrupec, D.; Imazawa, R.; Inada, T.; Inoue, S.; Ioka, K.; Iori, M.; Itokawa, T.; Iuliano, A.; Jahanvi, J.; Jimenez Martinez, I.; Jimenez Quiles, J.; Jorge Rodrigo, I.; Jurysek, J.; Kagaya, M.; Karas, V.; Katagiri, H.; Kerszberg, D.; Kiyomoto, T.; Kobayashi, Y.; Kohri, K.; Kornecki, P.; Kubo, H.; Kushida, J.; Lacave, B.; Lainez, M.; Lamastra, A.; Lemoigne, L.; Linhoff, M.; Lombardi, S.; Longo, F.; López-Coto, R.; López-Oramas, A.; Loporchio, S.; Lozano Bahilo, J.; Lucarelli, F.; Luciani, H.; Luque-Escamilla, P. L.; Makariev, M.; Mallamaci, M.; Mandat, D.; Mannheim, K.; Marini, F.; Mariotti, M.; Marquez, P.; Marsella, G.; Martí, J.; Martinez, O.; Martínez, G.; Martínez, M.; Massa, M.; Mazin, D.; Méndez-Gallego, J.; Menon, S.; Mestre Guillen, E.; Miceli, D.; Miener, T.; Miranda, J. M.; Molero Gonzalez, M.; Molina, E.; Montaruli, T.; Moralejo, A.; Morselli, A.; Moya, V.; Müller, A. L.; Muraishi, H.; Nagataki, S.; Nakamori, T.; Neronov, A.; Nieto Castaño, D.; Nievas Rosillo, M.; Nikolic, L.; Noda, K.; Novotny, V.; Nozaki, S.; Ohishi, M.; Ohtani, Y.; Okumura, A.; Orito, R.; Orsini, L.; Otero-Santos, J.; Ottanelli, P.; Palatiello, M.; Panebianco, G.; Paneque, D.; Paoletti, R.; Paredes, J. M.; Pech, M.; Pecimotika, M.; Peresano, M.; Perrotta, F.; Pfeifle, F.; Pihet, M.; Pirola, G.; Plard, C.; Podobnik, F.; Polo, M.; Pozo-Gonzaléz, C.; Prandini, E.; Rainò, S.; Rando, R.; Rhode, W.; Ribó, M.; Rodriguez Fernandez, G.; Rodríguez Frías, M. D.; Roy, A.; Ruina, A.; Ruiz-Velasco, E.; Saito, T.; Sakurai, S.; Sanchez, D. A.; Sano, H.; Santos Moura, E.; Šarić, T.; Sato, Y.; Saturni, F. G.; Savchenko, V.; Schiavone, F.; Schussler, F.; Schweizer, T.; Seglar Arroyo, M.; Silvestri, G.; Simongini, A.; Sitarek, J.; Sliusar, V.; Sofia, I.; Strišković, J.; Strzys, M.; Suda, Y.; Sunny, A.; Tajima, H.; Takahashi, M.; Takeishi, R.; Tanaka, S. J.; Tateishi, D.; Tavernier, T.; Temnikov, P.; Terada, Y.; Terauchi, K.; Terzic, T.; Teshima, M.; Tluczykont, M.; Tomura, T.; Torres, D. F.; Tramonti, F.; Travnicek, P.; Tripodo, G.; Tutone, A.; Vacula, M.; Vázquez Acosta, M.; Verna, G.; Viale, I.; Viana, A.; Vigliano, A.; Vigorito, C. F.; Visentin, E.; Vitale, V.; Voutsinas, G.; Vovk, I.; Vuillaume, T.; Walter, R.; Yamamoto, T.; Yamazaki, R.; Yao, Y.; Yoshida, T.; Yoshikoshi, T.; Zhang, W.; Zywucka, N.; Null, Null; Aceituno, F.; Acosta-Pulido, J. A.; Casanova, V.; Escudero Pedrosa, J.; Fallah Ramazani, V.; Jormanainen, J.; Jorstad, S.; Keating, G.; Kouch, P. M.; Gurwell, M.; Lähteenmäki, A.; Lindfors, E.; Marscher, A.; Morcuende, D.; Myserlis, I.; Nilsson, K.; Ortega Hunter, C. A.; Rao, R.; Sota, A.; Tornikoski, M.; Zhang, H.

doi:10.1051/0004-6361/202557924

Context. BL Lacertae (BL Lac), the archetypal blazar of its subclass and one of the most studied blazars of recent decades, has undergone a series of major multi-wavelength outbursts since 2020, resulting in its highest recorded gamma-ray flare to date between September and November 2022, together with those from August 2021 and October 2024.Aims. We characterised the gamma-ray and multi-wavelength emission and spectral energy distribution (SED) of BL Lac, as well as their evolution during the major and extended gamma-ray and multi-wavelength flare that occurred between September and November 2022.Methods. We evaluated the variability of the flare, focusing on the nights of October 20 and November 13, 2022 when clear intranight veryhigh-energy (VHE, E > 100 GeV) gamma-ray variability was observed. We modelled the gamma-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.Results. During this flare, 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 of ten. We observe intranight flux-doubling variations as fast as similar to 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 in the gamma-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 orientated with the line of sight, while variations in the relativistic electron distributions and the injection of freshly accelerated particles explain the weekly scale variations.

Abe, K., Abe, S., Abhishek, A., Acero, F., Aguasca-Cabot, A., Agudo, I., et al. (2026). Very-high-energy gamma-ray intranight variability from BL Lacertae during the extreme flaring state of 2022. ASTRONOMY & ASTROPHYSICS, 710 [10.1051/0004-6361/202557924].