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Record W4405715583 · doi:10.3204/pubdb-2025-05635

Time-dependent modelling of short-term variability in the TeV-blazar VER J0521+211 during the major flare in 2020

2024· preprint· en· W4405715583 on OpenAlexfundno aff
MAGIC Collaboration, S. Abe, J. Abhir, A. Abhishek, V. A. Acciari, Arnau Aguasca-Cabot, I. Agudo, T. Aniello, S. Ansoldi, L. A. Antonelli, A. Arbet Engels, C. Arcaro, M. Artero, K. Asano, Dominik Baack, A. Babić, U. Barres de Almeida, J. A. Barrio, I. Batković, A. Bautista, 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, E. Bronzini, I. Burelli, A. Campoy-Ordaz, A. Carosi, R. Carosi, M. Carretero-Castrillo, A. J. Castro‐Tirado, Davide Cerasole, G. Ceribella, Y. Chai, A. Cifuentes, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, Giacomo D’Amico, V. D'Elia, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, Raniere de Menezes, M. Delfino, J. Delgado, C. Delgado Mendez, F. Di Pierro, R. Di Tria, L. Di Venere, A. Donini, D. Dorner, M. Doro, Laura Eisenberger, D. Elsäesser, Juan Escudero, L. Fariña, A. Fattorini, L. Foffano, L. Font, Stefan Fröse, S. Fukami, Y. Fukazawa, R. J. García López, M. Garczarczyk, S. Gasparyan, M. Gaug, J. G. Giesbrecht Paiva, N. Giglietto, F. Giordano, Paweł Gliwny, T. Gradetzke, R. Grau, D Green, J. G. Green, Patrick Günther, D. Hadasch, A. Hahn, T. Hassan, Lea Heckmann, J. Herrera Llorente, D. Hrupec, R. Imazawa, K. Ishio, Irene Jiménez Martínez, J. Jormanainen, S. Kankkunen, T. Kayanoki, D. Kerszberg, Gert Werner Kluge, Y. Kobayashi, Pouya M. Kouch, H. Kubo, J. Kushida, Miguel J. A. Láinez, A. Lamastra, F. Leone, E. Lindfors, S. Lombardi, F. Longo, R. López-Coto, S. Loporchio, A. Lorini, E. Lyard, B. Machado de Oliveira Fraga, P. Majumdar, M. Makariev, G. Maneva, M. Manganaro, S. Mangano, K. Mannheim, M. Mariotti, M. Martínez-Chicharro, Alvaro Mas-Aguilar, D. Mazin, S. Menchiari, S. Mender, D. Miceli, T. Miener, J. M. Miranda, R. Mirzoyan, Miguel Molero Gonzalez, E. Molina, H. A. Mondal, A. Moralejo, Daniel Morcuende, T. Nakamori, C. Nanci, V. Neustroev, L. Nickel, 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, D. Paneque, R. Paoletti, J. M. Paredes, M. Peresano, M. Persic, M. Pihet, G. Pirola, F. Podobnik, P. G. Prada Moroni, E. Prandini, G. Principe, W. Rhode, M. Ribó, J. Rico, Chiara Righi, N. Sahakyan, T. Saito, F. G. Saturni, K. Schmidt, F. Schmuckermaier, J. L. Schubert, T. Schweizer, A. Sciaccaluga, Gabriella Silvestri, J. Sitarek, V. Sliusar, D. Sobczyńska, A. Spolon, A. Stamerra, J. Strišković, D. Strom, M. Strzys, Y. Suda, Hiroyasu Tajima, M. Takahashi, R. Takeishi, P. Temnikov, K. Terauchi, T. Terzić, M. Teshima, S. Truzzi, Antonio Tutone, S. Ubach, Juliane van Scherpenberg, M. Vazquez Acosta, S. Ventura, G. Verna, I. Viale, C. F. Vigorito, V. Vitale, I. Vovk, R. Walter, F. Wersig, Martin Will, C. Wunderlich, T. Yamamoto, MWL collaborators, R. Bachev, V. Fallah Ramazani, A. V. Filippenko, T. Hovatta, S. G. Jorstad, S. Kiehlmann, A. Lähteenmäki, Ioannis Liodakis, Alan P. Marscher, W. Max-Moerbeck, Anastasiia Omeliukh, T. Pursimo, A. C. S. Readhead, Xavier Rodrigues, M. Tornikoski, F. Wierda, W. Zheng

Bibliographic record

VenueDesy publication database (The Deutsches Elektronen-Synchrotron) · 2024
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersInstitute for Cosmic Ray Research, University of TokyoMarshall Space Flight CenterUniversidad de ChileUniversitetet i OsloBulgarian Academy of SciencesUniversity of TokyoChiba UniversityMax-Planck-GesellschaftJapan Society for the Promotion of ScienceConselho Nacional de Desenvolvimento Científico e TecnológicoDeutscher Akademischer AustauschdienstBulgarian National Science FundTurun YliopistoHrvatska Zaklada za ZnanostAarhus UniversitetAalto-YliopistoAgencia Estatal de InvestigaciónOulun YliopistoSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungMinistry of Education, Culture, Sports, Science and TechnologyMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesEuropean Southern ObservatoryCentres de Recerca de CatalunyaDeutsche ForschungsgemeinschaftCalifornia Institute of TechnologyEuropean CommissionGeneralitat de CatalunyaEuropean Regional Development FundBundesministerium für Bildung und ForschungFoundation for Research and Technology-HellasAlfred Kordelinin SäätiöInstituto de Astrofísica de CanariasCanadian Institute for Advanced ResearchFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroNuclear Safety and Security CommissionMinisterio de Ciencia, Innovación y UniversidadesNational Aeronautics and Space AdministrationNational Science Foundation
KeywordsFlareBlazarTerm (time)AstrophysicsPhysicsAstronomyGamma ray

Abstract

fetched live from OpenAlex

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.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.002
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.071
Threshold uncertainty score0.141

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0020.001
Open science0.0010.000
Research integrity0.0020.001
Insufficient payload (model declined to judge)0.0010.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.017
GPT teacher head0.238
Teacher spread0.221 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations0
Published2024
Admission routes1
Has abstractyes

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