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Record W3036071585 · doi:10.1093/mnras/staa1702

An intermittent extreme BL Lac: MWL study of 1ES 2344+514 in an enhanced state

2020· article· en· W3036071585 on OpenAlexfundno aff
Stefano Ansoldi, L. A. Antonelli, A. Arbet Engels, A. Babić, B. Banerjee, U. Barres de Almeida, J. A. Barrio, J. Becerra González, W. Bednarek, Lorenzo Bellizzi, E. Bernardini, A. Berti, Jürgen Besenrieder, W. Bhattacharyya, C. Bigongiari, O. Blanch, G. Bonnoli, Ž. Bošnjak, G. Busetto, R. Carosi, G. Ceribella, M. Cerruti, Yating Chai, A. Chilingaryan, S. Cikota, S. M. Colak, U. Colin, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, V. D’Elia, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, M. Delfino, J. Delgado, Davide Depaoli, F. Di Pierro, L. Di Venere, E. Do Souto Espiñeira, D. Dominis Prester, Alice Donini, M. Doro, D. Elsäesser, V. Fallah Ramazanı, Alicia Fattorini, G. Ferrara, L. Foffano, M. V. Fonseca, L. Font, C. Fruck, Satoshi Fukami, R. J. Garcı́a López, M. Garczarczyk, Sargis Gasparyan, M. Gaug, N. Giglietto, F. Giordano, N. Godinović, Paweł Gliwny, D Green, D. Hadasch, A. Hahn, J. Herrera, John Hoang, Dario Hrupec, Moritz Hütten, Tomohiro Inada, Susumu Inoue, Kazuma Ishio, Y. Iwamura, L. Jouvin, Y. Kajiwara, D. Kerszberg, Yukiho Kobayashi, H. Kubo, J. Kushida, A. Lamastra, F. Leone, E. Lindfors, S. Lombardi, F. Longo, Marcos López, R. López-Coto, A. López-Oramas, S. Loporchio, B. Machado de Oliveira Fraga, C. Maggio, P. Majumdar, M. Makariev, M. Mallamaci, G. Maneva, M. Manganaro, L. Maraschi, M. Mariotti, M. Martı́nez, D. Mazin, S. Mender, S. Mičanović, Davide Miceli, Tjark Miener, M. Minev, J. M. Miranda, R. Mirzoyan, E. Molina, A. Moralejo, Daniel Morcuende, V. Moreno, E. Moretti, P. Munar-Adrover, V. Neustroev, Cosimo Nigro, K. Nilsson, D. Ninci, K. Nishijima, K. Noda, L. Nogués, 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. Peresano, M. Persic, P. G. Prada Moroni, E. Prandini, I. Puljak, M. Ribó, J. Rico, Chiara Righi, A. Rugliancich, L. Saha, N. Sahakyan, T. Saito, S. Sakurai, K. Satalecka, Bernd Schleicher, K. Schmidt, T. Schweizer, J. Sitarek, I. Šnidarić, D. Sobczyńska, Alessia Spolon, A. Stamerra, D. Strom, M. Strzys, Y. Suda, T. Surić, Mitsunari Takahashi, F. Tavecchio, P. Temnikov, T. Terzić, M. Teshima, N. Torres-Albà, Luca Tosti, Juliane van Scherpenberg, G. Vanzo, M. Vázquez Acosta, Sofia Ventura, V. Verguilov, C. Vigorito, V. Vitale, Ievgen Vovk, Martin Will, Darko Zarić, Matteo Balbo, Mattias Beck, Noah Biederbeck, A. Biland, Michael Blank, T. Bretz, Kai Bruegge, Michael Bulinski, Manuel Doerr, D. Dorner, D. Hildebrand, Roman Iotov, Marc Klinger, K. Mannheim, S. Mueller, Dominik Neise, A. Neronov, M. Nöthe, Aleksander Paravac, W. Rhode, Amit Shukla, Vitalii Sliusar, L. Tani, Fabian Theissen, R. Walter, MWL Collaborators J Acosta Pulido, A. V. Filippenko, T. Hovatta, S. Kiehlmann, V. M. Larionov, W. Max-Moerbeck, C. M. Raiteri, A. C. S. Readhead, Marko Šegon, M. Villata, WeiKang Zheng

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersAstrophysics DivisionAstrophysics Science DivisionInstituto Nazionale di Fisica NucleareGoddard Space Flight CenterNational Research CentreSmithsonian Astrophysical ObservatoryMinistry of Education, Culture, Sports, Science and TechnologyInstitut sur la Nutrition et les Aliments FonctionnelsMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroMinisterio de Economía y CompetitividadMax-Planck-GesellschaftJapan Society for the Promotion of ScienceConselho Nacional de Desenvolvimento Científico e TecnológicoInstituto de Astrofísica de CanariasEidgenössische Technische Hochschule ZürichHrvatska Zaklada za ZnanostEuropean Regional Development FundBundesministerium für Bildung und ForschungDeutsche ForschungsgemeinschaftSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungAdolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California BerkeleyComisión Nacional de Investigación Científica y TecnológicaNational Aeronautics and Space AdministrationAcademy of FinlandUniversity of ChicagoSmithsonian InstitutionNational Science Foundation
KeywordsPhysicsBL Lac objectAstrophysicsCrab NebulaFermi Gamma-ray Space TelescopeFlareBlazarSpectral energy distributionFlux (metallurgy)MAGIC (telescope)Light curveGamma rayGalaxy

Abstract

fetched live from OpenAlex

ABSTRACT Extreme high-frequency BL Lacs (EHBL) feature their synchrotron peak of the broad-band spectral energy distribution (SED) at νs ≥ 1017 Hz. The BL Lac object 1ES 2344+514 was included in the EHBL family because of its impressive shift of the synchrotron peak in 1996. During the following years, the source appeared to be in a low state without showing any extreme behaviours. In 2016 August, 1ES 2344+514 was detected with the ground-based γ-ray telescope FACT during a high γ-ray state, triggering multiwavelength (MWL) observations. We studied the MWL light curves of 1ES 2344+514 during the 2016 flaring state, using data from radio to very-high-energy (VHE) γ-rays taken with OVRO, KAIT, KVA, NOT, some telescopes of the GASP-WEBT collaboration at the Teide, Crimean, and St. Petersburg observatories, Swift-UVOT, Swift-XRT, Fermi-LAT, FACT, and MAGIC. With simultaneous observations of the flare, we built the broad-band SED and studied it in the framework of a leptonic and a hadronic model. The VHE γ-ray observations show a flux level of 55 per cent of the Crab Nebula flux above 300 GeV, similar to the historical maximum of 1995. The combination of MAGIC and Fermi-LAT spectra provides an unprecedented characterization of the inverse-Compton peak for this object during a flaring episode. The Γ index of the intrinsic spectrum in the VHE γ-ray band is 2.04 ± 0.12stat ± 0.15sys. We find the source in an extreme state with a shift of the position of the synchrotron peak to frequencies above or equal to 1018 Hz.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation 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 score0.164
Threshold uncertainty score0.783

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.015
GPT teacher head0.225
Teacher spread0.210 · 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 teacher head, 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".

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Citations27
Published2020
Admission routes1
Has abstractyes

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Same venueMonthly Notices of the Royal Astronomical SocietySame topicAstrophysics and Cosmic PhenomenaFrench-language works237,207