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Record W4309905423 · doi:10.1038/s41586-022-05338-0

Polarized blazar X-rays imply particle acceleration in shocks

2022· article· en· W4309905423 on OpenAlexaff
Ioannis Liodakis, Alan P. Marscher, I. Agudo, A. Berdyugin, M. Bernardos, G. Bonnoli, Г. А. Борман, C. Casadio, V. Casanova, E. Cavazzuti, Nicole Rodriguez Cavero, Laura Di Gesu, Niccolò Di Lalla, I. Donnarumma, Steven R. Ehlert, M. Errando, Juan Escudero, Maya Garcı́a-Comas, Beatriz Agı́s-González, C. Husillos, Jenni Jormanainen, Svetlana G. Jorstad, Masato Kagitani, E. N. Kopatskaya, Vadim Kravtsov, H. Krawczynski, E. Lindfors, Е. Г. Ларионова, G. Madejski, Frédéric Marin, Alessandro Marchini, Herman L. Marshall, D. A. Morozova, F. Massaro, J. Masiero, Dimitri Mawet, R. Middei, Maxwell A. Millar‐Blanchaer, I. Myserlis, Michela Negro, K. Nilsson, Stephen L. O’Dell, N. Omodei, L. Pacciani, A. Paggi, G. V. Panopoulou, Abel L. Peirson, M. Perri, Pierre-Olivier Petrucci, Juri Poutanen, Simonetta Puccetti, Roger W. Romani, Takeshi Sakanoi, С. С. Савченко, A. Sota, F. Tavecchio, Samaporn Tinyanont, A. A. Vasilyev, Z. R. Weaver, 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, Simone Castellano, S. Ciprini, E. Costa, Alessandra De Rosa, E. Del Monte, Alessandro Di Marco, Victor Doroshenko, Michal Dovčiak, Teruaki Enoto, Y. Evangelista, Sergio Fabiani, Riccardo Ferrazzoli, Javier A. García, Shuichi Gunji, Kiyoshi Hayashida, Jeremy Heyl, W. Iwakiri, V. Karas, Takao Kitaguchi, Jeffery J. Kolodziejczak, Fabio La Monaca, L. Latronico, S. Maldera, Alberto Manfreda, Andrea Marinucci, G. Matt, Ikuyuki Mitsuishi, Tsunefumi Mizuno, Fabio Muleri, Stephen C. Y. Ng, C. Oppedisano, Alessandro Papitto, George G. Pavlov, M. Pesce-Rollins, M. Pilia, Andrea Possenti, Brian D. Ramsey, John Rankin, Ajay Ratheesh, C. Sgró, Patrick Slane, P. Soffitta, G. Spandre, Toru Tamagawa, Roberto Taverna, Yuzuru Tawara, Allyn F. Tennant, Nicolas E. Thomas, Francesco Tombesi, A. Trois, Sergey S. Tsygankov, R. Turolla, Jacco Vink, Martin C. Weisskopf, Kinwah Wu, Fei Xie, Silvia Zane

Bibliographic record

VenueNature · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of British Columbia
FundersConsejo Superior de Investigaciones CientíficasJapan Society for the Promotion of ScienceGoddard Space Flight CenterInstituto de Astrofísica de AndalucíaIstituto Nazionale di Fisica NucleareMarshall Space Flight CenterNuclear Safety and Security CommissionHáskóli ÍslandsIstituto Nazionale di AstrofisicaMinisterio de Ciencia e InnovaciónStockholms UniversitetAarhus UniversitetTurun YliopistoCentre National de la Recherche ScientifiqueNational Science FoundationAgenzia Spaziale ItalianaUniversitetet i OsloYale UniversityUniversity of CreteJet Propulsion LaboratoryCentre National d’Etudes SpatialesMax-Planck-GesellschaftSpace Telescope Science InstituteNordForskNational Aeronautics and Space AdministrationCalifornia Institute of Technology
KeywordsPhysicsBlazarParticle accelerationAstrophysicsPolarization (electrochemistry)Active galactic nucleusAstrophysical jetPlasmaLinear polarizationShock waveOpticsGamma rayGalaxyLaserNuclear physics

Abstract

fetched live from OpenAlex

Abstract Most of the light from blazars, active galactic nuclei with jets of magnetized plasma that point nearly along the line of sight, is produced by high-energy particles, up to around 1 TeV. Although the jets are known to be ultimately powered by a supermassive black hole, how the particles are accelerated to such high energies has been an unanswered question. The process must be related to the magnetic field, which can be probed by observations of the polarization of light from the jets. Measurements of the radio to optical polarization—the only range available until now—probe extended regions of the jet containing particles that left the acceleration site days to years earlier1–3, and hence do not directly explore the acceleration mechanism, as could X-ray measurements. Here we report the detection of X-ray polarization from the blazar Markarian 501 (Mrk 501). We measure an X-ray linear polarization degree ΠX of around 10%, which is a factor of around 2 higher than the value at optical wavelengths, with a polarization angle parallel to the radio jet. This points to a shock front as the source of particle acceleration and also implies that the plasma becomes increasingly turbulent with distance from the shock.

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 score0.003
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 studies0.0000.001
Scholarly communication0.0010.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.001

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 head0.006
GPT teacher head0.230
Teacher spread0.224 · 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

Citations134
Published2022
Admission routes1
Has abstractyes

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