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Record W2191829672 · doi:10.3847/0004-637x/819/2/156

MULTIWAVELENGTH STUDY OF QUIESCENT STATES OF Mrk 421 WITH UNPRECEDENTED HARD X-RAY COVERAGE PROVIDED BY NuSTAR IN 2013

2016· article· en· W2191829672 on OpenAlexafffund
Mislav Baloković, D. Paneque, G. M. Madejski, A. Furniss, J. Chiang, M. Ajello, D. M. Alexander, D. Barret, R. D. Blandford, Steven E. Boggs, Finn E. Christensen, William W. Craig, Karl Förster, P. Giommi, Brian W. Grefenstette, Charles J. Hailey, Fiona A. Harrison, A. Hornstrup, T. Kitaguchi, Jason E. Koglin, Kristin K. Madsen, P. H. Mao, H. Miyasaka, Kaya Mori, M. Perri, M. J. Pivovaroff, Simonetta Puccetti, Vikram Rana, Daniel Stern, G. Tagliaferri, C. M. Urry, N. J. Westergaard, W. W. Zhang, Andreas Zoglauer, S. Archambault, A. Archer, A. Barnacka, W. Benbow, R. Bird, J. H. Buckley, V. Bugaev, M. Cerruti, X. Chen, L. Ciupik, M. P. Connolly, Wei Cui, H. J. Dickinson, J. Dumm, J. Eisch, A. Falcone, Q. Feng, J. P. Finley, Henrike Fleischhack, L. Fortson, S. Griffin, S. Griffiths, J. Grube, G. Gyuk, M. Huetten, N. Håkansson, J. Holder, T. B. Humensky, C. A. Johnson, P. Kaaret, M. Kertzman, Y. Khassen, D. Kieda, M. Krause, F. Krennrich, M. J. Lang, G. Maier, S. McArthur, K. Meagher, P. Moriarty, Thomas Nelson, D. Nieto, R. A. Ong, N. Park, M. Pohl, A. Popkow, E. Pueschel, P. T. Reynolds, G. T. Richards, E. Roache, M. Santander, G. H. Sembroski, K. Shahinyan, A. W. Smith, D. Staszak, I. Telezhinsky, N. Todd, J. V. Tucci, J. Tyler, S. Vincent, A. J. Weinstein, A. Wilhelm, D. A. Williams, B. Zitzer, M. L. Ahnen, Stefano Ansoldi, L. A. Antonelli, P. Antoranz, A. Babić, B. Banerjee, P. Bangale, U. Barres de Almeida, J. A. Barrio, J. Becerra González, W. Bednarek, E. Bernardini, B. Biasuzzi, A. Biland, O. Blanch, S. Bonnefoy, G. Bonnoli, F. Borracci, T. Bretz, E. Carmona, A. Carosi, A. Chatterjee, R. Clavero, P. Colin, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, E. de Oña Wilhelmi, C. Delgado Mendez, F. Di Pierro, D. Dominis Prester, D. Dorner, M. Doro, S. Einecke, D. Elsäesser, A. Fernández-Barral, D. Fidalgo, M. V. Fonseca, L. Font, K. Frantzen, C. Fruck, D. Galindo, R. J. Garcı́a López, M. Garczarczyk, D. Garrido Terrats, M. Gaug, D. Glawion, N. Godinović, Alfonso Muñoz, D. Guberman, A. Hahn, Y. Hanabata, M. Hayashida, J. Herrera, J. Hose, Dario Hrupec, G. Hughes, W. Idec, K. Kodani, Y. Konno, H. Kubo, J. Kushida, A. La Barbera, E. Lindfors, S. Lombardi, F. Longo, M. López, R. López-Coto, A. López-Oramas, E. Lorenz, P. Majumdar, M. Makariev, K. Mallot, G. Maneva, M. Manganaro, K. Mannheim, L. Maraschi, B. Marcote, M. Mariotti, M. Martínez, D. Mazin, U. Menzel, J. M. Miranda, R. Mirzoyan, A. Moralejo, E. Moretti, D. Nakajima, V. Neustroev, A. Niedźwiecki, M. Nievas Rosillo, K. Nilsson, K. Nishijima, K. Noda, R. Orito, A. Overkemping, S. Paiano, J. Palacio, M. Palatiello, R. Paoletti, J. M. Paredes, X. Paredes-Fortuny, M. Persic, Juri Poutanen, P. G. Prada Moroni, E. Prandini, I. Puljak, W. Rhode, M. Ribó, J. Rico, Javier A. García, T. Saito, K. Satalecka, V. Scapin, C. Schultz, T. Schweizer, S. N. Shore, A. Sillanpää, J. Sitarek, I. Šnidarić, D. Sobczyńska, A. Stamerra, T. Steinbring, M. Strzys, L. O. Takalo, H. Takami, F. Tavecchio, P. Temnikov, T. Terzić, D. Tescaro, M. Teshima, J. Thaele, D. F. Torres, T. Toyama, A. Treves, V. Verguilov, Ievgen Vovk, J. E. Ward, Martin Will, M. H. Wu, R. Zanin, J. S. Perkins, F. Verrecchia, C. Leto, M. Böttcher, M. Villata, C. M. Raiteri, J. A. Acosta‐Pulido, R. Bachev, A. Berdyugin, D. Blinov, M. I. Carnerero, Wen-Ping Chen, P. Chinchilla, G. Damljanović, Chakali Eswaraiah, T. S. Grishina, S. Ibryamov, B. Jordan, S. G. Jorstad, M. Joshi, E. N. Kopatskaya, O. M. Kurtanidze, S. O. Kurtanidze, Е. Г. Ларионова, L. V. Larionova, V. M. Larionov, G. Latev, H. C. Lin, Alan P. Marscher, A. A. Mokrushina, D. A. Morozova, M. G. Nikolashvili, E. Semkov, Paul S. Smith, A. Strigachev, Yu. V. Troitskaya, I. S. Troitsky, O. Vince, J. Barnes, Tolga Güver, J. W. Moody, A. C. Sadun, S. Sun, T. Hovatta, J. L. Richards, W. Max-Moerbeck, A. C. R. Readhead, A. Lähteenmäki, M. Tornikoski, J. Tammi, Venkatessh Ramakrishnan, R. Reinthal, E. Angelakis, L. Fuhrmann, I. Myserlis, V. Karamanavis, A. Sievers, H. Ungerechts, J. A. Zensus

Bibliographic record

VenueThe Astrophysical Journal · 2016
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsMcGill University
FundersJapan Society for the Promotion of ScienceJet Propulsion LaboratoryInstituto de Astrofísica de CanariasIstituto Nazionale di Fisica NucleareNatural Sciences and Engineering Research Council of CanadaIstituto Nazionale di AstrofisicaCentre National de la Recherche ScientifiqueBilim AkademisiSmithsonian InstitutionU.S. Department of EnergyVetenskapsrådetMax-Planck-GesellschaftNational Research FoundationHigh Energy Accelerator Research OrganizationInstitut National de Physique Nucléaire et de Physique des ParticulesScience and Technology Facilities CouncilHrvatska Zaklada za ZnanostEuropean Regional Development FundBundesministerium für Bildung und ForschungRussian Foundation for Basic ResearchNASA HeadquartersOffice of ScienceAcademy of FinlandDeutsche ForschungsgemeinschaftCentre National d’Etudes SpatialesSLAC National Accelerator LaboratoryMinistry of Education, Culture, Sports, Science and TechnologyCalifornia Institute of TechnologyShota Rustaveli National Science FoundationNational Aeronautics and Space AdministrationJapan Aerospace Exploration AgencyTürkiye Bilimsel ve Teknolojik Araştırma KurumuSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungAgenzia Spaziale ItalianaNational Science Foundation
KeywordsPhysicsAstrophysicsX-rayAstronomyOptics

Abstract

fetched live from OpenAlex

ABSTRACT We present coordinated multiwavelength observations of the bright, nearby BL Lacertae object Mrk 421 taken in 2013 January–March, involving GASP-WEBT, Swift , NuSTAR , Fermi -LAT, MAGIC, VERITAS, and other collaborations and instruments, providing data from radio to very high energy (VHE) γ -ray bands. NuSTAR yielded previously unattainable sensitivity in the 3–79 keV range, revealing that the spectrum softens when the source is dimmer until the X-ray spectral shape saturates into a steep power law, with no evidence for an exponential cutoff or additional hard components up to ∼80 keV. For the first time, we observed both the synchrotron and the inverse-Compton peaks of the spectral energy distribution (SED) simultaneously shifted to frequencies below the typical quiescent state by an order of magnitude. The fractional variability as a function of photon energy shows a double-bump structure that relates to the two bumps of the broadband SED. In each bump, the variability increases with energy, which, in the framework of the synchrotron self-Compton model, implies that the electrons with higher energies are more variable. The measured multi band variability, the significant X-ray-to-VHE correlation down to some of the lowest fluxes ever observed in both bands, the lack of correlation between optical/UV and X-ray flux, the low degree of polarization and its significant (random) variations, the short estimated electron cooling time, and the significantly longer variability timescale observed in the NuSTAR light curves point toward in situ electron acceleration and suggest that there are multiple compact regions contributing to the broadband emission of Mrk 421 during low-activity states.

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: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.568
Threshold uncertainty score0.527

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)0.0000.000

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 head0.006
GPT teacher head0.209
Teacher spread0.204 · 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 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

Citations140
Published2016
Admission routes2
Has abstractyes

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