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Record W2149990597 · doi:10.1088/0004-637x/727/2/129

INSIGHTS INTO THE HIGH-ENERGY γ-RAY EMISSION OF MARKARIAN 501 FROM EXTENSIVE MULTIFREQUENCY OBSERVATIONS IN THE<i>FERMI</i>ERA

2011· article· en· W2149990597 on OpenAlexafffund
A. A. Abdo, M. Ackermann, M. Ajello, A. Allafort, L. Baldini, J. Ballet, G. Barbiellini, Matthew G. Baring, D. Bastieri, K. Bechtol, R. Bellazzini, B. Berenji, R. D. Blandford, E. D. Bloom, E. Bonamente, A. W. Borgland, A. Bouvier, T. J. Brandt, J. Bregeon, A. Brez, M. Brigida, P. Bruel, R. Buehler, S. Buson, G. A. Caliandro, R. A. Cameron, A. Cannon, P. A. Caraveo, S. Carrigan, J. M. Casandjian, E. Cavazzuti, C. Cecchi, Ö. Çelik, E. Charles, A. Chekhtman, C. C. Cheung, J. Chiang, S. Ciprini, R. Claus, J. Cohen-Tanugi, J. M. Conrad, S. Cutini, C. D. Dermer, E. do Couto e Silva, P. S. Drell, R. Dubois, D. Dumora, C. Favuzzi, S. Fegan, E. C. Ferrara, W. B. Focke, P. Fortin, M. Frailis, L. Fuhrmann, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, D. Gasparrini, N. Gehrels, S. Germani, N. Giglietto, F. Giordano, M. Giroletti, T. Glanzman, G. Godfrey, I. A. Grenier, L. Guillemot, S. Guiriec, M. Hayashida, E. Hays, D. Horan, R. E. Hughes, G. Jóhannesson, A. S. Johnson, W. N. Johnson, M. Kadler, T. Kamae, H. Katagiri, J. Kataoka, J. Knödlseder, M. Kuss, J. Landé, L. Latronico, S.-H. Lee, M. Lemoine‐Goumard, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, G. Madejski, A. Makeev, W. Max-Moerbeck, M. N. Mazziotta, J. E. McEnery, J. Méhault, P. F. Michelson, W. Mitthumsiri, Tsunefumi Mizuno, A. A. Moiseev, C. Monte, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, M. Naumann-Godó, S. Nishino, P. L. Nolan, J. P. Norris, E. Nuss, T. Ohsugi, A. Okumura, N. Omodei, J. F. Ormes, D. Paneque, J. Panetta, D. Parent, V. Pavlidou, T. J. Pearson, V. Pelassa, M. Pepé, M. Pesce-Rollins, F. Piron, T. A. Porter, S. Rainò, R. Rando, M. Razzano, A. C. S. Readhead, A. Reimer, O. Reimer, J. L. Richards, J. Ripken, S. Ritz, M. Roth, H. F-W. Sadrozinski, D. A. Sánchez, A. Sander, J. D. Scargle, C. Sgró, E. J. Siskind, P. D. Smith, G. Spandre, P. Spinelli, Ł. Stawarz, M. A. Stevenson, M. S. Strickman, K. V. Sokolovsky, D. J. Suson, H. Takahashi, T. Takahashi, Takaaki Tanaka, J. B. Thayer, J. G. Thayer, D. J. Thompson, L. Tibaldo, D. F. Torres, G. Tosti, A. Tramacere, Y. Uchiyama, T. Usher, J. Vandenbroucke, V. Vasileiou, N. Vilchez, V. Vitale, A. P. Waite, P. Wang, A. E. Wehrle, B. L. Winer, K. S. Wood, Z. Yang, T. Ylinen, J. A. Zensus, M. Ziegler, J. Aleksić, L. A. Antonelli, P. Antoranz, Michael Backes, J. A. Barrio, J. Becerra González, W. Bednarek, A. Berdyugin, K. Berger, E. Bernardini, A. Biland, O. Blanch, R. K. Böck, A. Boller, G. Bonnoli, P. Bordas, D. Borla Tridon, V. Bosch-Ramón, D. Bose, I. Braun, T. Bretz, Montaña Cámara, E. Carmona, A. Carosi, P. Colin, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, F. Dazzi, A. De Angelis, E. De Cea del Pozo, B. De Lotto, Mónica María, F. De Sabata, C. Delgado Mendez, A. Diago Ortega, M. Doert, A. Domínguez, D. Dominis Prester, D. Dorner, M. Doro, D. Elsäesser, D. Ferenc, M. V. Fonseca, L. Font, R. J. Garcı́a López, M. Garczarczyk, M. Gaug, G. Giavitto, N. Godinovi, D. Hadasch, A. Herrero, D. Hildebrand, D. Höhne-Mönch, J. Hose, Dario Hrupec, T. Jogler, S. Klepser, T. Krähenbühl, D. Kranich, J. Krause, A. La Barbera, E. Leonardo, E. Lindfors, S. Lombardi, Marcos López, E. Lorenz, P. Majumdar, E. Makariev, G. Maneva, N. Mankuzhiyil, K. Mannheim, L. Maraschi, M. Mariotti, M. Martı́nez, D. Mazin, M. Meucci, J. M. Miranda, R. Mirzoyan, H. Miyamoto, J. Moldón, A. Moralejo, D. Nieto, K. Nilsson, R. Orito, R. Paoletti, J. M. Paredes, S. Partini, M. Pasanen, F. Pauß, R. Pegna, M. A. Pérez‐Torres, M. Persic, J. Peruzzo, J. Pochon, P. G. Prada Moroni, F. Prada, E. Prandini, N. Puchades, I. Puljak, Thomas Reichardt, R. Reinthal, W. Rhode, M. Ribó, J. Rico, M. Rissi, S. Rügamer, A. Saggion, Koji Saito, T. Y. Saito, M. Salvati, M. Sánchez‐Conde, K. Satalecka, V. Scalzotto, V. Scapin, C. Schultz, T. Schweizer, M. Shayduk, S. N. Shore, A. Sierpowska-Bartosik, A. Sillanpää, J. Sitarek, D. Sobczyńska, F. Spanier, S. Spiro, A. Stamerra, B. Steinke, J. Storz, N. Strah, J. C. Struebig, T. Surić, L. O. Takalo, F. Tavecchio, P. Temnikov, T. Terzić, D. Tescaro, M. Teshima, H. Vankov, Robert Wagner, Q. Weitzel, V. Zabalza, F. Zandanel, R. Zanin, V. A. Acciari, T. Arlen, T. Aune, W. Benbow, D. Boltuch, S. M. Bradbury, J. H. Buckley, V. Bugaev, A. Cesarini, L. Ciupik, Wei Cui, R. Dickherber, M. Errando, A. Falcone, J. P. Finley, G. Finnegan, L. Fortson, A. Furniss, N. Galante, D. Gall, G. H. Gillanders, S. Godambe, J. Grube, R. Guénette, G. Gyuk, D. Hanna, J. Holder, Dezhi Huang, C. M. Hui, T. B. Humensky, P. Kaaret, N. Karlsson, M. Kertzman, D. Kieda, A. Konopelko, H. Krawczynski, F. Krennrich, M. J. Lang, G. Maier, S. McArthur, A. McCann, M. McCutcheon, P. Moriarty, R. Mukherjee, R. A. Ong, A. N. Otte, D. Pandel, J. S. Perkins, A. Pichel, M. Pohl, J. Quinn, K. Ragan, L. C. Reyes, P. T. Reynolds, E. Roache, H. J. Rose, A. C. Rovero, M. Schroedter, G. H. Sembroski, G. D. Şentürk, D. Steele, S. P. Swordy, G. Tešić, M. Theiling, S. Thibadeau, A. Varlotta, S. Vincent, S. P. Wakely, J. E. Ward, T. C. Weekes, A. J. Weinstein, T. Weisgarber, D. A. Williams, M. Wood, B. Zitzer, M. Villata, C. M. Raiteri, H. D. Aller, M. F. Aller, A. A. Arkharov, D. Blinov, P. Calcidese, W. P. Chen, Н. В. Ефимова, G. N. Kimeridze, T. S. Konstantinova, E. N. Kopatskaya, E. Koptelova, O. M. Kurtanidze, S. O. Kurtanidze, A. Lähteenmäki, V. M. Larionov, Е. Г. Ларионова, L. V. Larionova, R. Ligustri, D. A. Morozova, M. G. Nikolashvili, L. A. Sigua, I. S. Troitsky, E. Angelakis, M. Capalbi, A. Carramiñana, L. Carrasco, P. Cassaro, E. De la Fuente, Mark Gurwell, Yu. A. Kovalev, Yu. A. Kovalev, T. P. Krichbaum, H. A. Krimm, P. Leto, M. L. Lister, G. Maccaferri, J. W. Moody, Y. Mori, I. Nestoras, A. Orlati, C. Pagani, C. Pace, R.L. Pearson, M. Perri, B. G. Piner, A. B. Pushkarev, E. Ros, A. C. Sadun, T. Sakamoto, M. Tornikoski, Yoichi Yatsu, A. C. Zook

Bibliographic record

VenueThe Astrophysical Journal · 2011
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsMcGill University
FundersJapan Aerospace Exploration AgencyInstitut National de Physique Nucléaire et de Physique des ParticulesScience and Technology Facilities CouncilSmithsonian Astrophysical ObservatoryInstituto de Astrofísica de CanariasNatural Sciences and Engineering Research Council of CanadaIstituto Nazionale di AstrofisicaGeorgian National Science FoundationCentre National de la Recherche ScientifiqueSmithsonian InstitutionU.S. Department of EnergyVetenskapsrådetMax-Planck-GesellschaftHigh Energy Accelerator Research OrganizationMinisterio de Ciencia e InnovaciónBundesministerium für Bildung und ForschungRussian Foundation for Basic ResearchAcademia SinicaIstituto Nazionale di Fisica NucleareDeutsche ForschungsgemeinschaftSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungAgenzia Spaziale ItalianaHelmholtz-GemeinschaftAssociated UniversitiesMinistry of Education, Culture, Sports, Science and TechnologyNational Aeronautics and Space AdministrationScience Foundation IrelandNational Science Foundation
KeywordsPhysicsAstrophysicsBlazarFermi Gamma-ray Space TelescopeSpectral indexSpectral energy distributionSynchrotronFlux (metallurgy)LuminosityAstronomyGamma rayPhotonActive galactic nucleusGalaxySpectral lineOptics

Abstract

fetched live from OpenAlex

We report on the γ-ray activity of the blazar Mrk 501 during the first 480 days of Fermi operation. We find that the average Large Area Telescope (LAT) γ-ray spectrum of Mrk 501 can be well described by a single power-law function with a photon index of 1.78 ± 0.03. While we observe relatively mild flux variations with the Fermi -LAT (within less than a factor of two), we detect remarkable spectral variability where the hardest observed spectral index within the LAT energy range is 1.52 ± 0.14, and the softest one is 2.51 ± 0.20. These unexpected spectral changes do not correlate with the measured flux variations above 0.3 GeV. In this paper, we also present the first results from the 4.5 month long multifrequency campaign (2009 March 15—August 1) on Mrk 501, which included the Very Long Baseline Array (VLBA), Swift , RXTE , MAGIC, and VERITAS, the F-GAMMA, GASP-WEBT, and other collaborations and instruments which provided excellent temporal and energy coverage of the source throughout the entire campaign. The extensive radio to TeV data set from this campaign provides us with the most detailed spectral energy distribution yet collected for this source during its relatively low activity. The average spectral energy distribution of Mrk 501 is well described by the standard one-zone synchrotron self-Compton (SSC) model. In the framework of this model, we find that the dominant emission region is characterized by a size ≲0.1 pc (comparable within a factor of few to the size of the partially resolved VLBA core at 15–43 GHz), and that the total jet power (≃10 44 erg s −1 ) constitutes only a small fraction (∼10 −3 ) of the Eddington luminosity. The energy distribution of the freshly accelerated radiating electrons required to fit the time-averaged data has a broken power-law form in the energy range 0.3 GeV–10 TeV, with spectral indices 2.2 and 2.7 below and above the break energy of 20 GeV. We argue that such a form is consistent with a scenario in which the bulk of the energy dissipation within the dominant emission zone of Mrk 501 is due to relativistic, proton-mediated shocks. We find that the ultrarelativistic electrons and mildly relativistic protons within the blazar zone, if comparable in number, are in approximate energy equipartition, with their energy dominating the jet magnetic field energy by about two orders of magnitude.

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 score0.005
Threshold uncertainty score0.010

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
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 head0.018
GPT teacher head0.211
Teacher spread0.193 · 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

Citations237
Published2011
Admission routes2
Has abstractyes

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Same venueThe Astrophysical JournalSame topicAstrophysics and Cosmic PhenomenaFrench-language works237,207