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Record W2886005926 · doi:10.1051/0004-6361/201833704

Extreme HBL behavior of Markarian 501 during 2012

2018· article· en· W2886005926 on OpenAlexafffund
M. L. Ahnen, Stefano Ansoldi, L. A. Antonelli, Cornelia Arcaro, A. Babić, B. Banerjee, P. Bangale, U. Barresde Almeida, J. A. Barrio, J. Becerra González, W. Bednarek, E. Bernardini, A. Berti, W. Bhattacharyya, O. Blanch, G. Bonnoli, R. Carosi, A. Carosi, A. Chatterjee, S. M. Colak, P. Colin, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, P. Cumani, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, M. Delfino, J. Delgado, F. Di ierro, M. Doert, A. Domínguez, D. Dominis Prester, M. Doro, D. Eisenacher lawion, M. Engelkemeier, V. Fallah Ramazanı, A. Fernández-Barral, D. Fidalgo, M. V. Fonseca, L. Font, C. Fruck, D. Galindo, R. J. Garcı́a López, M. Garczarczyk, M. Gaug, N. Godinović, D. Góra, D. Guberman, D. Hadasch, A. Hahn, T. Hassan, M. Hayashida, J. Herrera, J. Hose, Dario Hrupec, Kazuma Ishio, Y. Konno, H. Kubo, J. Kushida, D. Kuveždić, E. Lindfors, S. Lombardi, F. Longo, Marcos López, C. Maggio, P. Majumdar, M. Makariev, G. Maneva, M. Manganaro, L. Maraschi, M. Mariotti, M. Martı́nez, D. Mazin, U. Menzel, M. Minev, J. M. Miranda, R. Mirzoyan, A. Moralejo, V. Moreno, E. Moretti, T. Nagayoshi, V. Neustroev, A. Niedźwiecki, M. Nievas Rosillo, Cosimo Nigro, K. Nilsson, D. Ninci, K. Nishijima, K. Noda, L. Nogués, S. Paiano, J. Palacio, D. Paneque, R. Paoletti, J. M. Paredes, G. Pedaletti, M. Peresano, L. Perri, M. Persic, P. G. Prada Moroni, E. Prandini, I. Puljak, Javier A. García, I. Reichardt, M. Ribó, J. Rico, Chiara Righi, A. Rugliancich, T. Saito, K. Satalecka, S. Schroeder, T. Schweizer, S. N. Shore, J. Sitarek, I. Šnidarić, D. Sobczyńska, A. Stamerra, M. Strzys, T. Surić, L. O. Takalo, F. Tavecchio, P. Temnikov, T. Terzić, M. Teshima, N. Torres-Albà, A. Treves, S. Tsujimoto, G. Vanzo, M. Vázquez Acosta, Ievgen Vovk, J. E. Ward, Martin Will, Darko Zarić, Axel Arbet-Engels, Dominik Baack, Matteo Balbo, A. Biland, Michael Blank, T. Bretz, Kai Bruegge, Michael Bulinski, Anton Dmytriiev, D. Dorner, S. Einecke, D. Elsäesser, Tina Herbst, D. Hildebrand, L. Kortmann, Lena Linhoff, Max Mahlke, K. Mannheim, S. Mueller, Dominik Neise, A. Neronov, Maximilian Noethe, J. Oberkirch, Aleksander Paravac, W. Rhode, Bernd Schleicher, Florian Schulz, Amit Shukla, Vitalii Sliusar, R. Walter, A. Archer, W. Benbow, R. Bird, Robert Brose, J. H. Buckley, V. Bugaev, Jessie L. Christiansen, Wei Cui, M. K. Daniel, A. Falcone, Q. Feng, J. P. Finley, G. H. Gillanders, O. Gueta, D. Hanna, O. Hervet, J. Holder, G. Hughes, Moritz Hütten, T. B. Humensky, C. A. Johnson, P. Kaaret, P. Kar, N. Kelley-Hoskins, M. Kertzman, D. Kieda, M. Krause, F. Krennrich, S. Kumar, M. J. Lang, T. T. Y. Lin, G. Maier, S. McArthur, P. Moriarty, R. Mukherjee, S. O’Brien, R. A. Ong, A. N. Otte, N. Park, A. Petrashyk, A. Pichel, M. Pohl, J. Quinn, K. Ragan, P. T. Reynolds, G. T. Richards, E. Roache, Adrián Rovero, C. B. Rulten, I. Sadeh, M. Santander, G. H. Sembroski, K. Shahinyan, I. Sushch, J. Tyler, S. P. Wakely, A. J. Weinstein, R. M. Wells, P. Wilcox, A. Wilhel, D. A. Williams, T. J. Williamson, B. Zitzer, M. Perri, F. Verrecchia, C. Leto, M. Villata, C. M. Raiteri, S. G. Jorstad, V. M. Larionov, D. Blinov, T. S. Grishina, E. N. Kopatskaya, Е. Г. Ларионова, A. A. Nikiforova, D. A. Morozova, Yu. V. Troitskaya, I. S. Troitsky, O. M. Kurtanidze, M. G. Nikolashvili, S. O. Kurtanidze, G. N. Kimeridze, R. A. Chigladze, A. Strigachev, A. C. Sadun, J. W. Moody, W. P. Chen, H. C. Lin, J. A. Acosta‐Pulido, M. J. Arévalo, M. I. Carnerero, P. A. González-Morales, A. Manilla-Robles, Helen Jermak, I. A. Steele, C. G. Mundell, E. Benítez, D. Hiriart, Paul S. Smith, W. Max-Moerbeck, A. C. S. Readhead, J. L. Richards, T. Hovatta, A. Lähteenmäki, M. Tornikoski, J. Tammi, Markos Georganopoulos, Matthew G. Baring

Bibliographic record

VenueAstronomy and Astrophysics · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsMcGill University
FundersJapan Aerospace Exploration AgencyOffice of ScienceInstituto de Astrofísica de CanariasIstituto Nazionale di Fisica NucleareMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesCentre National de la Recherche ScientifiqueFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungUniversity of CreteSmithsonian InstitutionU.S. Department of EnergyVetenskapsrådetMax-Planck-GesellschaftNatural Sciences and Engineering Research Council of CanadaIstituto Nazionale di AstrofisicaNational Science FoundationLiverpool John Moores UniversityJapan Society for the Promotion of ScienceConselho Nacional de Desenvolvimento Científico e TecnológicoNational Research CentreBulgarian National Science FundHigh Energy Accelerator Research OrganizationInstitut National de Physique Nucléaire et de Physique des ParticulesScience and Technology Facilities CouncilAalto-YliopistoHrvatska Zaklada za ZnanostEuropean Regional Development FundBundesministerium für Bildung und ForschungDeutsche ForschungsgemeinschaftRussian Science FoundationMinistry of Education, Culture, Sports, Science and TechnologyNational Aeronautics and Space AdministrationAgenzia Spaziale Italiana
KeywordsPhysicsCrab NebulaAstrophysicsCherenkov radiationFlux (metallurgy)FlareFermi Gamma-ray Space TelescopeBL Lac objectBlazarExtragalactic background lightHigh energyMAGIC (telescope)AstronomyGamma rayOptics

Abstract

fetched live from OpenAlex

Aims. We aim to characterize the multiwavelength emission from Markarian 501 (Mrk 501), quantify the energy-dependent variability, study the potential multiband correlations, and describe the temporal evolution of the broadband emission within leptonic theoretical scenarios. Methods. We organized a multiwavelength campaign to take place between March and July of 2012. Excellent temporal coverage was obtained with more than 25 instruments, including the MAGIC, FACT and VERITAS Cherenkov telescopes, the instruments on board the Swift and Fermi spacecraft, and the telescopes operated by the GASP-WEBT collaboration. Results. Mrk 501 showed a very high energy (VHE) gamma-ray flux above 0.2 TeV of ∼0.5 times the Crab Nebula flux (CU) for most of the campaign. The highest activity occurred on 2012 June 9, when the VHE flux was ∼3 CU, and the peak of the high-energy spectral component was found to be at ∼2 TeV. Both the X-ray and VHE gamma-ray spectral slopes were measured to be extremely hard, with spectral indices < 2 during most of the observing campaign, regardless of the X-ray and VHE flux. This study reports the hardest Mrk 501 VHE spectra measured to date. The fractional variability was found to increase with energy, with the highest variability occurring at VHE. Using the complete data set, we found correlation between the X-ray and VHE bands; however, if the June 9 flare is excluded, the correlation disappears (significance < 3 σ ) despite the existence of substantial variability in the X-ray and VHE bands throughout the campaign. Conclusions. The unprecedentedly hard X-ray and VHE spectra measured imply that their low- and high-energy components peaked above 5 keV and 0.5 TeV, respectively, during a large fraction of the observing campaign, and hence that Mrk 501 behaved like an extreme high-frequency-peaked blazar (EHBL) throughout the 2012 observing season. This suggests that being an EHBL may not be a permanent characteristic of a blazar, but rather a state which may change over time. The data set acquired shows that the broadband spectral energy distribution (SED) of Mrk 501, and its transient evolution, is very complex, requiring, within the framework of synchrotron self-Compton (SSC) models, various emission regions for a satisfactory description. Nevertheless the one-zone SSC scenario can successfully describe the segments of the SED where most energy is emitted, with a significant correlation between the electron energy density and the VHE gamma-ray activity, suggesting that most of the variability may be explained by the injection of high-energy electrons. The one-zone SSC scenario used reproduces the behavior seen between the measured X-ray and VHE gamma-ray fluxes, and predicts that the correlation becomes stronger with increasing energy of the X-rays.

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 categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Other design · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.867
Threshold uncertainty score1.000

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 science0.0000.000
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 head0.010
GPT teacher head0.204
Teacher spread0.194 · 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.

Study designOther design
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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Citations82
Published2018
Admission routes2
Has abstractyes

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