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@ARTICLE{Abe:643441,
      author       = {Abe, S. and Abhir, J. and Abhishek, A. and Acciari, V. A.
                      and Aguasca-Cabot, 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 de Almeida, U. Barres and Barrio, J. A. and
                      Batković, I. and Bautista, A. 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 Bronzini, E. and Burelli, I. and Campoy-Ordaz, A. and
                      Carosi, A. and Carosi, R. and Carretero-Castrillo, M. and
                      Castro-Tirado, A. J. and Cerasole, D. and Ceribella, G. and
                      Chai, Y. and Cifuentes, A. and Colombo, E. and Contreras, J.
                      L. and Cortina, J. and Covino, S. and D’Amico, G. and
                      D’Elia, V. and Vela, P. Da and Dazzi, F. and Angelis, A.
                      De and Lotto, B. De and de Menezes, R. and Delfino, M. and
                      Delgado, J. and Mendez, C. Delgado and Pierro, F. Di and
                      Tria, R. Di and Venere, L. Di and Prester, D. Dominis and
                      Donini, A. and Dorner, D. and Doro, M. and Eisenberger, L.
                      and Elsaesser, D. and Escudero, J. and Fariña, L. and
                      Fattorini, A. and Foffano, L. and Font, L. and Fröse, S.
                      and Fukami, S. and Fukazawa, Y. and López, R. J. García
                      and Garczarczyk, M. and Gasparyan, S. and Gaug, M. and
                      Giesbrecht Paiva, J. G. and Giglietto, N. and Giordano, F.
                      and Gliwny, P. and Gradetzke, T. and Grau, R. and Green, D.
                      and Green, J. G. and Günther, P. and Hadasch, D. and Hahn,
                      A. and Hassan, T. and Heckmann, L. and Llorente, J. Herrera
                      and Hrupec, D. and Imazawa, R. and Ishio, K. and Martínez,
                      I. Jiménez and Jormanainen, J. and Kankkunen, S. and
                      Kayanoki, T. and Kerszberg, D. and Kluge, G. W. and
                      Kobayashi, Y. and Kouch, P. M. and Kubo, H. and Kushida, J.
                      and Láinez, M. and Lamastra, A. and Leone, F. and Lindfors,
                      E. 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
                      Manganaro, M. and Mangano, S. and Mannheim, K. and Mariotti,
                      M. and Martínez, M. and Martínez-Chicharro, M. and
                      Mas-Aguilar, A. and Mazin, D. and Menchiari, S. and Mender,
                      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
                      Nakamori, T. and Nanci, C. and Neustroev, V. and Nickel, L.
                      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 Paneque, D. and
                      Paoletti, R. and Paredes, J. M. and Peresano, M. and Persic,
                      M. and Pihet, M. and Pirola, G. and Podobnik, F. and Prada
                      Moroni, P. G. and Prandini, E. and Principe, G. and Rhode,
                      W. and Ribó, M. and Rico, J. and Righi, C. and Sahakyan, N.
                      and Saito, T. and Saturni, F. G. and Schmidt, K. and
                      Schmuckermaier, F. and Schubert, J. L. and Schweizer, T. and
                      Sciaccaluga, A. and Silvestri, G. 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 Tajima, H. and Takahashi, M. and Takeishi, R.
                      and Temnikov, P. and Terauchi, K. and Terzić, T. and
                      Teshima, M. and Truzzi, S. and Tutone, A. and Ubach, S. and
                      van Scherpenberg, J. and Acosta, M. Vazquez and Ventura, S.
                      and Verna, G. and Viale, I. and Vigorito, C. F. and Vitale,
                      V. and Vovk, I. and Walter, R. and Wersig, F. and Will, M.
                      and Wunderlich, C. and Yamamoto, T. and Bachev, R. and
                      Fallah Ramazani, V. and Filippenko, A. V. and Hovatta, T.
                      and Jorstad, S. G. and Kiehlmann, S. and Lähteenmäki, A.
                      and Liodakis, I. and Marscher, A. P. and Max-Moerbeck, W.
                      and Omeliukh, A. and Pursimo, T. and Readhead, A. C. S. and
                      Rodrigues, X. and Tornikoski, M. and Wierda, F. and Zheng,
                      W.},
      collaboration = {{MAGIC Collaboration}},
      title        = {{T}ime-dependent modelling of short-term variability in the
                      {T}e{V}-blazar {VER} {J}0521+211 during the major flare in
                      2020},
      reportid     = {PUBDB-2026-00202, arXiv:2412.15836},
      year         = {2025},
      note         = {$A\&A$ 694, A308 (2025). Accepted for publication in
                      $A\&A$},
      abstract     = {The BL Lacertae object VER J0521+211 underwent a notable
                      flaring episode in February 2020. A short-term monitoring
                      campaign, led by the MAGIC (Major Atmospheric Gamma Imaging
                      Cherenkov) collaboration, covering a wide energy range from
                      radio to very high-energy (VHE, 100 GeV < E < 100 TeV) gamma
                      rays was organised to study its evolution. These
                      observations resulted in a consistent detection of the
                      source over six consecutive nights in the VHE gamma-ray
                      domain. Combining these nightly observations with an
                      extensive set of multi-wavelength data made modelling of the
                      blazar’s spectral energy distribution (SED) possible
                      during the flare. This modelling was performed with a focus
                      on two plausible emission mechanisms: (i) a leptonic
                      two-zone synchrotron-self-Compton scenario, and (ii) a
                      lepto-hadronic one-zone scenario. Both models effectively
                      replicated the observed SED from radio to the VHE gamma-ray
                      band. Furthermore, by introducing a set of evolving
                      parameters, both models were successful in reproducing the
                      evolution of the fluxes measured in different bands
                      throughout the observing campaign. Notably, the
                      lepto-hadronic model predicts enhanced photon and neutrino
                      fluxes at ultra-high energies (E > 100 TeV). While the
                      photon component, generated via decay of neutral pions, is
                      not directly observable as it is subject to intense pair
                      production (and therefore extinction) through interactions
                      with the cosmic microwave background photons, neutrino
                      detectors (e.g. IceCube) can probe the predicted neutrino
                      component. Finally, the analysis of the gamma-ray spectra,
                      observed by MAGIC and the Fermi-LAT telescopes, yielded a
                      conservative $95\%$ confidence upper limit of z ≤ 0.244
                      for the redshift of this blazar.Key words: galaxies: active
                      / BL Lacertae objects: individual: VER J0521+211 / gamma
                      rays: galaxies⋆⋆ Eustace Specialist in Astronomy.},
      cin          = {$Z_GA$},
      ddc          = {520},
      cid          = {$I:(DE-H253)Z_GA-20210408$},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613) /
                      DFG project G:(GEPRIS)390783311 - EXC 2094: ORIGINS: Vom
                      Ursprung des Universums bis zu den ersten Bausteinen des
                      Lebens (390783311)},
      pid          = {G:(DE-HGF)POF4-613 / G:(GEPRIS)390783311},
      experiment   = {EXP:(DE-H253)MAGIC-20170101},
      typ          = {PUB:(DE-HGF)25},
      eprint       = {2412.15836},
      howpublished = {arXiv:2412.15836},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2412.15836;\%\%$},
      url          = {https://bib-pubdb1.desy.de/record/643441},
}