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Record W4389983603 · doi:10.3204/pubdb-2024-07344

First characterization of the emission behavior of Mrk 421 from radio to very high-energy gamma rays with simultaneous X-ray polarization measurements

2023· preprint· en· W4389983603 on OpenAlexfundno aff
S. Abe, J. Abhir, V. A. Acciari, I. Agudo, T. Aniello, Stefano Ansoldi, L. A. Antonelli, A. Arbet Engels, C. Arcaro, M. Artero, Katsuaki Asano, A. Babić, Andrés Baquero, U. Barres de Almeida, J. A. Barrio, Ivana Batković, J. Baxter, W. Bednarek, E. Bernardini, J. Bernete, A. Berti, Jürgen Besenrieder, 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, G. Ceribella, Yating Chai, A. Cifuentes, S. Cikota, E. Colombo, J. L. Contreras, J. Cortina, S. Covino, F. D’Ammando, Giacomo D’Amico, V. D'Elia, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, Raniere de Menezes, Antonino Del Popolo, J. Delgado, C. Delgado Mendez, F. Di Pierro, L. Di Venere, D. Dominis Prester, A. Donini, D. Dorner, M. Doro, D. Elsäesser, Gabriel Emery, Juan Escudero, L. Fariña, Alicia Fattorini, L. Foffano, L. Font, Stefan Fröse, S. Fukami, Y. Fukazawa, R. J. Garcı́a López, M. Garczarczyk, S. Gasparyan, M. Gaug, J. G. Giesbrecht Paiva, N. Giglietto, F. Giordano, Paweł Gliwny, N. Godinović, T. Gradetzke, R. Grau, D. Green, Jarred Gershon Green, Patrick Günther, D. Hadasch, A. Hahn, T. Hassan, Lea Heckmann, J. Herrera, D. Hrupec, Moritz Hütten, Ryo Imazawa, Tomohiro Inada, Kazuma Ishio, Irene Jiménez Martínez, Jenni Jormanainen, D. Kerszberg, Gert Werner Kluge, Y. Kobayashi, Pouya M. Kouch, H. Kubo, J. Kushida, M. Láinez Lezáun, A. Lamastra, F. Leone, E. Lindfors, Lena Linhoff, S. Lombardi, F. Longo, R. López-Coto, Marcos López, 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, María Martínez-Chicharro, Alvaro Mas-Aguilar, D. Mazin, S. Menchiari, S. Mender, D. Miceli, T. Miener, J. M. Miranda, Miguel Molero Gonzalez, E. Molina, H. A. Mondal, A. Moralejo, Daniel Morcuende, Takeshi Nakamori, C. Nanci, Lara Nava, V. Neustroev, Lukas Nickel, M. Nievas Rosillo, Cosimo Nigro, L. Nikolić, K. Nilsson, K. Nishijima, T. Njoh Ekoume, K. Noda, S. Nozaki, Y. Ohtani, A. Okumura, Jorge Otero-Santos, S. Paiano, M. Palatiello, D. Paneque, R. Paoletti, J. M. Paredes, D. Pavlović, M. Peresano, M. Persic, Marine Pihet, G. Pirola, F. Podobnik, P. G. Prada Moroni, E. Prandini, G. Principe, Chaitanya Priyadarshi, W. Rhode, M. Ribó, J. Rico, Chiara Righi, N. Sahakyan, T. Saito, K. Satalecka, Francesco Gabriele Saturni, Bernd Schleicher, K. Schmidt, Felix Schmuckermaier, J. L. Schubert, T. Schweizer, A. Sciaccaluga, J. Sitarek, Vitalii Sliusar, D. Sobczyńska, A. Stamerra, Jelena Strišković, D. Strom, M. Strzys, Y. Suda, Sofia Suutarinen, H. Tajima, Mitsunari Takahashi, R. Takeishi, F. Tavecchio, P. Temnikov, Kenta Terauchi, T. Terzić, M. Teshima, Luca Tosti, S. Truzzi, Antonio Tutone, Santiago Ubach, Juliane van Scherpenberg, M. Vázquez Acosta, Sofia Ventura, Ilaria Viale, C. Vigorito, V. Vitale, Ievgen Vovk, R. Walter, Martin Will, Carolin Wunderlich, T. Yamamoto, Ioannis Liodakis, S. G. Jorstad, Laura Di Gesu, I. Donnarumma, Dawoon E. Kim, Alan P. Marscher, R. Middei, M. Perri, Simonetta Puccetti, F. Verrecchia, C. Leto, E. Jiménez‐Bailón, D. Blinov, Ioakeim G. Bourbah, S. Kiehlmann, Evangelos Kontopodis, N. Mandarakas, Raphael Skalidis, Anna Vervelaki, F. J. Aceituno, Beatriz Agı́s-González, A. Sota, Mahito Sasada, Koji S. Kawabata, Makoto Uemura, Tsunefumi Mizuno, Hiroshi Akitaya, C. Casadio, I. Myserlis, A. Sievers, A. Lähteenmäki, I. Syrjärinne, M. Tornikoski, Q. Salomé, Mark Gurwell, Garrett K. Keating, Ramprasad Rao

Bibliographic record

VenuearXiv (Cornell University) · 2023
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersNuclear PhysicsInstitute for Cosmic Ray Research, University of TokyoAgencia Estatal de InvestigaciónConsejo Superior de Investigaciones CientíficasJapan Aerospace Exploration AgencyJapan Society for the Promotion of ScienceDeutsches Elektronen-SynchrotronNuclear Safety and Security CommissionMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesJunta de AndalucíaStockholms UniversitetJulius-Maximilians-Universität WürzburgHrvatska Zaklada za ZnanostHomi Bhabha National InstituteHigh Energy Accelerator Research OrganizationInstitut National de Physique Nucléaire et de Physique des ParticulesUniversité de GenèveBulgarian Academy of SciencesMinisterio de Ciencia e InnovaciónUniversitetet i OsloIstituto Nazionale di AstrofisicaU.S. Department of EnergyFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroOulun YliopistoSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungUniversity of CreteSmithsonian InstitutionVetenskapsrådetAarhus UniversitetChiba UniversityCentre National de la Recherche ScientifiqueMax-Planck-GesellschaftMinistry of Education, Culture, Sports, Science and TechnologyBundesministerium für Bildung und ForschungHáskóli ÍslandsConselho Nacional de Desenvolvimento Científico e TecnológicoSmithsonian Astrophysical ObservatoryTurun YliopistoGoddard Space Flight CenterAalto-YliopistoMarshall Space Flight CenterIstituto Nazionale di Fisica NucleareGeneralitat de CatalunyaUniversität InnsbruckSveučilište Josipa Jurja Strossmayera u OsijekuDeutsche ForschungsgemeinschaftInstituto de Astrofísica de AndalucíaCentres de Recerca de CatalunyaUniversità degli Studi di SienaInstituto de Astrofísica de CanariasCanadian Institute for Advanced ResearchAcademia SinicaCalifornia Institute of TechnologyW. M. Keck FoundationNational Aeronautics and Space AdministrationAgenzia Spaziale ItalianaTechnische Universität DortmundNational Science Foundation
KeywordsPhysicsBlazarAstrophysicsCrab NebulaFlarePolarization (electrochemistry)Gamma rayFermi Gamma-ray Space TelescopeBrewster's angleSpectral indexRedshiftRadio galaxyLight curveAstronomyPhotonGalaxyOpticsSpectral line

Abstract

fetched live from OpenAlex

Aims. We have performed the first broadband study of Mrk 421 from radio to TeV gamma rays with simultaneous measurements of theX-ray polarization from IXPE.Methods. The data were collected as part of an extensive multiwavelength campaign carried out between May and June 2022 using MAGIC,Fermi-LAT, NuSTAR, XMM-Newton, Swift, and several optical and radio telescopes to complement IXPE data.Results. During the IXPE exposures, the measured 0.2–1 TeV flux was close to the quiescent state and ranged from 25% to 50% of the CrabNebula without intra-night variability. Throughout the campaign, the very high-energy (VHE) and X-ray emission are positively correlated ata 4σ significance level. The IXPE measurements reveal an X-ray polarization degree that is a factor of 2–5 higher than in the optical/radiobands; that implies an energy-stratified jet in which the VHE photons are emitted co-spatially with the X-rays, in the vicinity of a shock front.The June 2022 observations exhibit a rotation of the X-ray polarization angle. Despite no simultaneous VHE coverage being available duringa large fraction of the swing, the Swift-XRT monitoring reveals an X-ray flux increase with a clear spectral hardening. This suggests that flaresin high synchrotron peaked blazars can be accompanied by a polarization angle rotation, as observed in some flat spectrum radio quasars.Finally, during the polarization angle rotation, NuSTAR data reveal two contiguous spectral hysteresis loops in opposite directions (clockwise andcounterclockwise), implying important changes in the particle acceleration efficiency on approximately hour timescales.

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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.001
Threshold uncertainty score0.005

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.001

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 head0.031
GPT teacher head0.163
Teacher spread0.131 · 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".

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Citations0
Published2023
Admission routes1
Has abstractyes

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