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Record W4412158672 · doi:10.1093/mnras/staf1122

IXPE observations of the blazar Mrk 501 in 2022: a multiwavelength view

2025· article· en· W4412158672 on OpenAlexafffund
Lindsey Lisalda, Ephraim Gau, H. Krawczynski, F. Tavecchio, Ioannis Liodakis, Andrea Gokus, Nicole Rodriguez Cavero, Michael A. Nowak, M. Negro, R. Middei, M. Perri, Simonetta Puccetti, S. G. Jorstad, I. Agudo, A P Marscher, Beatriz Agı́s-González, A. V. Berdyugin, M. Bernardos, D. Blinov, G. Bonnoli, Г. А. Борман, Ioakeim G. Bourbah, C. Casadio, V. Casanova, A. J. Castro‐Tirado, Emilio J. Fernández-García, Maya Garcı́a-Comas, T. S. Grishina, Pasi Hakala, T. Hovatta, Y. D. Hu, C. Husillos, Juan Escudero, Jenni Jormanainen, F. J. Aceituno, Masato Kagitani, S. Kiehlmann, Evangelos Kontopodis, E. N. Kopatskaya, Pouya M. Kouch, Vadim Kravtsov, A. Lähteenmäki, Е. Г. Ларионова, E. Lindfors, N. Mandarakas, Alessandro Marchini, J. Masiero, Dimitri Mawet, W. Max-Moerbeck, D. A. Morozova, I. Myserlis, K. Nilsson, G. V. Panopoulou, T. J. Pearson, A. C. S. Readhead, R. Reeves, Stylianos Romanopoulos, Takeshi Sakanoi, Q. Salomé, С. С. Савченко, Raphael Skalidis, A. Sota, I. Syrjärinne, Samaporn Tinyanont, M. Tornikoski, Yu. V. Troitskaya, I. S. Troitskiy, A. A. Vasilyev, Anna Vervelaki, А. В. Жовтан, L. A. Antonelli, Matteo Bachetti, L. Baldini, W. H. Baumgartner, R. Bellazzini, S. Bianchi, Stephen D. Bongiorno, R. Bonino, A Brez, N. Bucciantini, Fiamma Capitanio, S Castellano, E. Cavazzuti, C Chen, S. Ciprini, E. Costa, Alessandra De Rosa, E. Del Monte, Laura Di Gesu, N Di Lalla, Alessandro Di Marco, I. Donnarumma, Victor Doroshenko, Michal Dovčiak, Steven R. Ehlert, Teruaki Enoto, Y. Evangelista, Sergio Fabiani, Riccardo Ferrazzoli, Javier A. Garcia, Shuichi Gunji, Mark Gurwell, Kentaro Hayashida, J Heyl, W. Iwakiri, P. Kaaret, V. Karas, Garrett K. Keating, Fabian Kislat, T Kitaguchi, J J Kolodziejczak, Fabio La Monaca, L. Latronico, S. Maldera, A. Manfreda, Frédéric Marin, Andrea Marinucci, Herman L. Marshall, F. Massaro, G. Matt, Ikuyuki Mitsuishi, Tsunefumi Mizuno, Fabio Muleri, C. S. Ng, Stephen L O'Dell, N. Omodei, C. Oppedisano, Alessandro Papitto, George G. Pavlov, Abel L. Peirson, M. Pesce-Rollins, Pierre-Olivier Petrucci, M. Pilia, A Possenti, Juri Poutanen, B. D. Ramsey, John Rankin, Ramprasad Rao, Ajay Ratheesh, O. J. Roberts, Roger W. Romani, C. Sgró, Patrick Slane, P Soffitta, G. Spandre, Douglas A. Swartz, T. Tamagawa, Roberto Taverna, Yuzuru Tawara, Allyn F. Tennant, Nicholas E. Thomas, F Tombesi, A Trois, Sergey S. Tsygankov, Roberto Turolla, J Vink, M. C. Weisskopf, Kinwah Wu, Fei Xie, Silvia Zane

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of British Columbia
FundersH2020 European Research CouncilEuropean CommissionMinisterio de Ciencia e InnovaciónInstituto Nazionale di Fisica NucleareNational Aeronautics and Space AdministrationCollege of Natural Resources and Sciences, Humboldt State UniversityGoddard Space Flight CenterAgencia Nacional de Investigación y DesarrolloIstituto Nazionale di Fisica NucleareMarshall Space Flight CenterIstituto Nazionale di AstrofisicaAcademy of FinlandAcademia SinicaAgencia Estatal de InvestigaciónOak Ridge Associated UniversitiesNuclear Safety and Security CommissionInstitut national des sciences de l'UniversFondo Nacional de Desarrollo Científico y TecnológicoInstitut sur la Nutrition et les Aliments FonctionnelsInstituto de Astrofísica de AndalucíaMichelson Prize and GrantsSmithsonian InstitutionWashington University in St. LouisAgenzia Spaziale ItalianaNational Science FoundationCentre national d'études spatiales
KeywordsPhysicsBlazarAstrophysicsAstronomyQuasarGalaxyGamma ray

Abstract

fetched live from OpenAlex

ABSTRACT The blazar Markarian 501 (Mrk 501) was observed on three occasions over a 4-month period between 2022 March and July with the Imaging X-ray Polarimetry Explorer (IXPE). In this paper, we report for the first time on the third IXPE observation, performed between 2022 July 9 and 12, during which IXPE detected a linear polarization degree of $\Pi _X=6\pm 2$ per cent at a polarization angle, measured east of north, of $\Psi _X=143^\circ \pm 11^\circ$ within the 2 – 8 keV X-ray band. The X-ray polarization angle and degree during this observation are consistent with those obtained during the first two observations. The chromaticity of the polarization across radio, optical, and X-ray bands is likewise consistent with the result from the simultaneous campaigns during the first two observations. Furthermore, we present two types of models to explain the observed spectral energy distributions (SEDs) and energy-resolved polarization: a synchrotron self-Compton model with an anisotropic magnetic field probability distribution in the emitting volume, as well as an energy-stratified shock model. Our results support both the shock scenario as well as support that small levels of magnetic field anisotropy can explain the observed polarization.

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 score0.011
Threshold uncertainty score0.021

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 studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0010.001
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 head0.009
GPT teacher head0.210
Teacher spread0.201 · 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

Citations2
Published2025
Admission routes2
Has abstractyes

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