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Record W4293074991 · doi:10.3847/1538-4357/ac6dd9

Multiwavelength Observations of the Blazar VER J0521+211 during an Elevated TeV Gamma-Ray State

2022· article· en· W4293074991 on OpenAlexafffund
C. B. Adams, P. Batista, W. Benbow, A. Brill, Robert Brose, J. Buckley, M. Capasso, Jessie L. Christiansen, M. Errando, Q. Feng, J. P. Finley, G. M. Foote, L. Fortson, A. Furniss, George Gallagher, A. Gent, C. Giuri, W. Hanlon, D. Hanna, T. Hassan, O. Hervet, J. Holder, B. Hona, G. Hughes, T. B. Humensky, W. Jin, P. Kaaret, M. Kertzman, D. Kieda, T. K. Kleiner, F. Krennrich, S. Kumar, M. J. Lang, M. Lundy, G. Maier, J. Millis, P. Moriarty, R. Mukherjee, M. Nievas Rosillo, S. O’Brien, R. A. Ong, A. N. Otte, S. Patel, Sonal Ramesh Patel, K. Pfrang, M. Pohl, R. R. Prado, E. Pueschel, J. Quinn, K. Ragan, P. T. Reynolds, D. Ribeiro, E. Roache, J. Ryan, I. Sadeh, M. Santander, G. H. Sembroski, R. Shang, B. Stevenson, J. V. Tucci, V. V. Vassiliev, S. P. Wakely, A. J. Weinstein, R. M. Wells, D. A. Williams, T. J. Williamson, V. A. Acciari, T. Aniello, Stefano Ansoldi, L. A. Antonelli, A. Arbet Engels, C. Arcaro, Manuel Artero, Katsuaki Asano, Dominik Baack, A. Babić, Andrés Baquero, U. Barres de Almeida, J. A. Barrio, Ivana Batković, J. Becerra González, W. Bednarek, E. Bernardini, M. Bernardos, A. Berti, J. Besenrieder, W. Bhattacharyya, C. Bigongiari, A. Biland, O. Blanch, H. Bökenkamp, G. Bonnoli, Ž. Bošnjak, Irene Burelli, G. Busetto, R. Carosi, G. Ceribella, M. Cerruti, Yating Chai, A. Chilingarian, S. Cikota, 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, Antonino Del Popolo, M. Delfino, J. Delgado, C. Delgado Mendez, Davide Depaoli, F. Di Pierro, L. Di Venere, E. Do Souto Espiñeira, D. Dominis Prester, Alice Donini, D. Dorner, M. Doro, D. Elsäesser, V. Fallah Ramazanı, L. Fariña, Alicia Fattorini, L. Font, C. Fruck, Satoshi Fukami, Y. Fukazawa, M. Garczarczyk, Sargis Gasparyan, M. Gaug, N. Giglietto, F. Giordano, Paweł Gliwny, N. Godinović, Jarred Gershon Green, D. Green, D. Hadasch, A. Hahn, Lea Heckmann, J. Herrera, Dario Hrupec, Moritz Hütten, Tomohiro Inada, R. Iotov, Kazuma Ishio, Y. Iwamura, Irene Jiménez Martínez, J. Jormanainen, L. Jouvin, D. Kerszberg, Yukiho Kobayashi, H. Kubo, J. Kushida, A. Lamastra, F. Leone, E. Lindfors, Lena Linhoff, S. Lombardi, F. Longo, R. López-Coto, Marcos López, A. López-Oramas, S. Loporchio, A. Lorini, B. Machado de Oliveira Fraga, C. Maggio, P. Majumdar, M. Makariev, G. Maneva, M. Manganaro, K. Mannheim, M. Mariotti, M. Martı́nez, Alvaro Mas-Aguilar, D. Mazin, S. Menchiari, S. Mender, S. Mičanović, Davide Miceli, Tjark Miener, J. M. Miranda, E. Molina, H. A. Mondal, A. Moralejo, Daniel Morcuende, V. Moreno, Takeshi Nakamori, C. Nanci, Lara Nava, V. Neustroev, Cosimo Nigro, K. Nilsson, K. Nishijima, K. Noda, S. Nozaki, Yoshiki Ohtani, Tomohiko Oka, Jorge Otero-Santos, S. Paiano, M. Palatiello, D. Paneque, R. Paoletti, J. M. Paredes, Lovro Pavletić, Pablo Peñil, M. Persic, M. Pihet, P. G. Prada Moroni, E. Prandini, Chaitanya Priyadarshi, Ivica Puljak, W. Rhode, M. Ribó, J. Rico, Chiara Righi, A. Rugliancich, N. Sahakyan, T. Saito, S. Sakurai, K. Satalecka, Francesco Gabriele Saturni, Bernd Schleicher, K. Schmidt, Felix Schmuckermaier, J. L. Schubert, T. Schweizer, J. Sitarek, I. Šnidarić, D. Sobczyńska, Alessia Spolon, A. Stamerra, Jelena Strišković, D. Strom, M. Strzys, Y. Suda, T. Surić, Mitsunari Takahashi, Ryuji Takeishi, F. Tavecchio, P. Temnikov, T. Terzić, M. Teshima, L. Tosti, S. Truzzi, Antonio Tutone, Santiago Ubach, Juliane van Scherpenberg, G. Vanzo, M. Vázquez Acosta, Sofia Ventura, V. Verguilov, Ilaria Viale, C. Vigorito, V. Vitale, Ievgen Vovk, Martin Will, Carolin Wunderlich, Tokonatsu Yamamoto, Darko Zarić

Bibliographic record

VenueThe Astrophysical Journal · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsMcGill University
FundersInstitute for Cosmic Ray Research, University of TokyoInstituto de Astrofísica de CanariasMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesAcademy of FinlandOffice of ScienceUniversity of TokyoFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroMax-Planck-GesellschaftJapan Society for the Promotion of ScienceConselho Nacional de Desenvolvimento Científico e TecnológicoMinisterio de Ciencia e InnovaciónHrvatska Zaklada za ZnanostGeneralitat de CatalunyaNational Research CentreEuropean Regional Development FundBundesministerium für Bildung und ForschungMinistry of Education, Culture, Sports, Science and TechnologyNational Energy Research Scientific Computing CenterSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungSmithsonian InstitutionU.S. Department of EnergySoochow UniversityCentres de Recerca de CatalunyaDeutsche ForschungsgemeinschaftNatural Sciences and Engineering Research Council of CanadaNational Science Foundation
KeywordsPhysicsBlazarGamma rayAstrophysicsAstronomy

Abstract

fetched live from OpenAlex

Abstract We report on a long-lasting, elevated gamma-ray flux state from VER J0521+211 observed by VERITAS, MAGIC, and Fermi-LAT in 2013 and 2014. The peak integral flux above 200 GeV measured with the nightly binned light curve is (8.8 ± 0.4) × 10−7 photons m−2 s−1, or ∼37% of the Crab Nebula flux. Multiwavelength observations from X-ray, UV, and optical instruments are also presented. A moderate correlation between the X-ray and TeV gamma-ray fluxes was observed, and the X-ray spectrum appeared harder when the flux was higher. Using the gamma-ray spectrum and four models of the extragalactic background light (EBL), a conservative 95% confidence upper limit on the redshift of the source was found to be z ≤ 0.31. Unlike the gamma-ray and X-ray bands, the optical flux did not increase significantly during the studied period compared to the archival low-state flux. The spectral variability from optical to X-ray bands suggests that the synchrotron peak of the spectral energy distribution (SED) may become broader during flaring states, which can be adequately described with a one-zone synchrotron self-Compton model varying the high-energy end of the underlying particle spectrum. The synchrotron peak frequency of the SED and the radio morphology of the jet from the MOJAVE program are consistent with the source being an intermediate-frequency-peaked BL Lac object.

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)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.004
Threshold uncertainty score0.008

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
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 head0.013
GPT teacher head0.214
Teacher spread0.201 · 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 designObservational
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

Citations8
Published2022
Admission routes2
Has abstractyes

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