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Record W4405963684 · doi:10.1093/mnras/stae2469

Multiwavelength study of OT 081: broadband modelling of a transitional blazar

2024· article· en· W4405963684 on OpenAlexfundno aff
Hidetarô Abe, S. Abe, V. A. Acciari, I. Agudo, T. Aniello, Stefano Ansoldi, L. A. Antonelli, A. Arbet Engels, Cornelia Arcaro, Manuel Artero, Katsuaki Asano, Dominik Baack, A. Babić, Andrés Baquero, U. Barres de Almeida, Ivana Batković, J. Baxter, E. Bernardini, M. Bernardos, J. Bernete, A. Berti, C. Bigongiari, A. Biland, O. Blanch, G. Bonnoli, Ž. Bošnjak, Irene Burelli, G. Busetto, A. Campoy-Ordaz, A. Carosi, R. Carosi, M. Carretero-Castrillo, A. J. Castro‐Tirado, Yating Chai, A. Cifuentes, S. Cikota, E. Colombo, Juan L. Contreras, J. Cortina, S. Covino, Giacomo D’Amico, V. D’Elia, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, M. Delfino, J. Delgado, C. Delgado Mendez, Davide Depaoli, F. Di Pierro, L. Di Venere, D. Dominis Prester, Alice Donini, D. Dorner, M. Doro, D. Elsäesser, Gabriel Emery, Juan Escudero, L. Fariña, Alicia Fattorini, L. Foffano, L. Font, Satoshi Fukami, Y Fukazawa, R. J. Garcı́a López, Sargis Gasparyan, M. Gaug, J. G. Giesbrecht Paiva, N. Giglietto, F. Giordano, Paweł Gliwny, R. Grau, Jarred Gershon Green, D. Hadasch, A. Hahn, Lea Heckmann, J. Herrera, Dario Hrupec, Moritz Hütten, Ryo Imazawa, Tomohiro Inada, Roman Iotov, Kazuma Ishio, Irene Jiménez Martínez, Jenni Jormanainen, D. Kerszberg, Gert Werner Kluge, Yukiho Kobayashi, H. Kubo, J. Kushida, M. Láinez Lezáun, A. Lamastra, F. Leone, E. Lindfors, Lena Linhoff, S. Lombardi, F. Longo, A. López-Oramas, S. Loporchio, A. Lorini, B. Machado de Oliveira Fraga, P. Majumdar, M. Makariev, G. Maneva, N. Mang, M. Manganaro, S. Mangano, K. Mannheim, M. Mariotti, M. Martı́nez, Alvaro Mas-Aguilar, D. Mazin, Stefano Menchiari, S. Mender, S. Mičanović, Davide Miceli, J. M. Miranda, Razmik Mirzoyan, E. Molina, H. A. Mondal, Daniel Morcuende, C. Nanci, V. Neustroev, C Nigro, K. Nishijima, T. Njoh Ekoume, K. Noda, S. Nozaki, Yoshiki Ohtani, Jorge Otero-Santos, S. Paiano, M Palatiello, D. Paneque, R. Paoletti, J. M. Paredes, Lovro Pavletić, M. Persic, Marine Pihet, G. Pirola, F. Podobnik, P. G. Prada Moroni, E. Prandini, G. Principe, C Priyadarshi, W. Rhode, M. Ribó, J. Rico, Chiara Righi, N. Sahakyan, Tatsuhiko Saito, K. Satalecka, Francesco Gabriele Saturni, Bernd Schleicher, K. Schmidt, Felix Schmuckermaier, J. Schubert, T. Schweizer, J. Sitarek, Alessia Spolon, A. Stamerra, Jelena Strišković, D. Strom, Y. Suda, T. Surić, Sofia Suutarinen, H. Tajima, Mari Takahashi, Ryuji Takeishi, F. Tavecchio, P. Temnikov, T. Terzić, M. Teshima, Luca Tosti, Stefano Truzzi, Santiago Ubach, Juliane van Scherpenberg, Sofia Ventura, V. Verguilov, Ilaria Viale, C. Vigorito, R. Walter, T. Yamamoto, F. Ait Benkhali, Y. Becherini, Baiyang Bi, M Böttcher, J. Bolmont, A. G. A. Brown, T. Bulik, S. Casanova, T Chand, S. Chandra, James O. Chibueze, O. Chibueze, K. Egberts, S Einecke, J.-P. Ernenwein, G. Fontaine, S. Gabici, P. Goswami, M. Holler, M. Jamrozy, Vikas Joshi, E. Kasai, K. Katarzyński, Rabeya Khatoon, B. Khélifi, W. Kluźniak, K. Kosack, Rodrigo Guedes Lang, S. Le Stum, A. Lemière, R. Marx, R. Moderski, M. O. Moghadam, M. de Naurois, J. Niemiec, P. O'Brien, M. Ostrowski, Giada Peron, S. Pita, G. Pühlhofer, A. Quirrenbach, B. Rudak, V. Sahakian, D. A. Sánchez, A. Santangelo, M. Sasaki, H. M. Schutte, M. Seglar-Arroyo, J. N. S. Shapopi, R. Steenkamp, C. Steppa, Hiroyuki Suzuki, Takaaki Tanaka, M. Tluczykont, C. Venter, Stefan Wagner, A. Wierzcholska, A. A. Zdziarski, Natalia Żywucka, J. Becerra González, S. Ciprini, T. M. Venters, F. D’Ammando, A. Esteban-Gutiérrez, V. Fallah Ramazanı, A. V. Filippenko, T. Hovatta, Helen Jermak, Svetlana G. Jorstad, S. Kiehlmann, A. Lähteenmäki, V. M. Larionov, Е. Г. Ларионова, Alan P. Marscher, D. A. Morozova, W. Max-Moerbeck, A. C. S. Readhead, R. Reeves, I. A. Steele, M. Tornikoski, F. Verrecchia, W. Zheng

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersInstitut National de Physique Nucléaire et de Physique des ParticulesAgencia Estatal de InvestigaciónJapan Society for the Promotion of ScienceJapan Aerospace Exploration AgencyDeutsche ForschungsgemeinschaftBundesministerium für Bildung, Wissenschaft und ForschungNational Astronomical Observatory of JapanIstituto Nazionale di AstrofisicaAcademy of FinlandMax-Planck-GesellschaftCentre National de la Recherche ScientifiqueU.S. Department of EnergyFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroNarodowym Centrum NaukiFondo Nacional de Desarrollo Científico y TecnológicoKnut och Alice Wallenbergs StiftelseHrvatska Zaklada za ZnanostHigh Energy Accelerator Research OrganizationUniversity of TokyoAustrian Science FundAgencia Nacional de Investigación y DesarrolloIstituto Nazionale di Fisica NucleareGeneralitat de CatalunyaMinistry of Education, Culture, Sports, Science and TechnologyBundesministerium für Bildung und ForschungHuman Growth FoundationUniversiteit van AmsterdamConselho Nacional de Desenvolvimento Científico e TecnológicoVetenskapsrådetInstitut sur la Nutrition et les Aliments FonctionnelsNational Natural Science Foundation of ChinaUniversity of NamibiaScience and Technology Facilities CouncilSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungCalifornia Institute of TechnologyInstituto Nazionale di Fisica NucleareMinisterio de Ciencia e InnovaciónEuropean CommissionNational Science FoundationInstitute for Cosmic Ray Research, University of TokyoStatens Naturvidenskabelige ForskningsradUniversity of ChicagoAalto-YliopistoAlexander von Humboldt-StiftungCentres de Recerca de CatalunyaH2020 European Research CouncilAgenzia Spaziale ItalianaNational Institutes of Natural SciencesAlbert Ellis InstituteMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesNational Commission on Research, Science and TechnologyKorea Astronomy and Space Science InstituteNational Aeronautics and Space Administration
KeywordsPhysicsBlazarBroadbandWavelengthAstrophysicsAstronomyOptics

Abstract

fetched live from OpenAlex

ABSTRACT OT 081 is a well-known, luminous blazar that is remarkably variable in many energy bands. We present the first broadband study of the source, which includes very high energy (VHE, $E\gt $ 100 GeV) $\gamma$-ray data taken by the MAGIC (Major Atmospheric Gamma-ray Imaging Cherenkov telescopes) and H.E.S.S. (High Energy Stereoscopic System) imaging Cherenkov telescopes. The discovery of VHE $\gamma$-ray emission happened during a high state of $\gamma$-ray activity in July 2016, observed by many instruments from radio to VHE $\gamma$-rays. We identify four states of activity of the source, one of which includes VHE $\gamma$-ray emission. Variability in the VHE domain is found on daily time-scales. The intrinsic VHE spectrum can be described by a power law with index $3.27\pm 0.44_{\rm stat}\pm 0.15_{\rm sys}$ (MAGIC) and $3.39\pm 0.58_{\rm stat}\pm 0.64_{\rm sys}$ (H.E.S.S.) in the energy range of 55–300 and 120–500 GeV, respectively. The broadband emission cannot be successfully reproduced by a simple one-zone synchrotron self-Compton model. Instead, an additional external Compton component is required. We test a lepto-hadronic model that reproduces the data set well and a proton-synchrotron-dominated model that requires an extreme proton luminosity. Emission models that are able to successfully represent the data place the emitting region well outside of the broad-line region to a location at which the radiative environment is dominated by the infrared thermal radiation field of the dusty torus. In the scenario described by this flaring activity, the source appears to be a flat spectrum radio quasar (FSRQ), in contrast with past categorizations. This suggests that the source can be considered to be a transitional blazar, intermediate between BL Lac and FSRQ objects.

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)0.001
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 score0.025
Threshold uncertainty score0.051

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0010.000
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0020.000

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 head0.208
Teacher spread0.196 · 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

Citations3
Published2024
Admission routes1
Has abstractyes

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