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Record W4392035942 · doi:10.3847/1538-4357/ad1ce4

Detection of X-Ray Polarization from the Blazar 1ES 1959+650 with the Imaging X-Ray Polarimetry Explorer

2024· article· en· W4392035942 on OpenAlexaff
M. Errando, Ioannis Liodakis, Alan P. Marscher, Herman L. Marshall, R. Middei, Michela Negro, Abel L. Peirson, M. Perri, Simonetta Puccetti, P. Rabinowitz, I. Agudo, Svetlana G. Jorstad, С. С. Савченко, D. Blinov, Ioakeim G. Bourbah, S. Kiehlmann, Evangelos Kontopodis, N. Mandarakas, Stylianos Romanopoulos, Raphael Skalidis, Anna Vervelaki, F. J. Aceituno, M. Bernardos, G. Bonnoli, V. Casanova, Beatriz Agı́s-González, C. Husillos, Alessandro Marchini, A. Sota, Pouya M. Kouch, E. Lindfors, C. Casadio, Juan Escudero, I. Myserlis, Ryo Imazawa, Mahito Sasada, Y. Fukazawa, Koji S. Kawabata, Makoto Uemura, Tsunefumi Mizuno, Tatsuya Nakaoka, Hiroshi Akitaya, Mark Gurwell, Garrett K. Keating, Ramprasad Rao, Adam Ingram, F. Massaro, L. A. Antonelli, R. Bonino, E. Cavazzuti, Chien‐Ting Chen, Nicolò Cibrario, S. Ciprini, Alessandra De Rosa, Laura Di Gesu, F. Di Pierro, I. Donnarumma, Steven R. Ehlert, Francesco Fenu, Ephraim Gau, V. Karas, Dawoon E. Kim, H. Krawczynski, M. Laurenti, Lindsey Lisalda, R. López-Coto, G. Madejski, Frédéric Marin, Andrea Marinucci, Ikuyuki Mitsuishi, Fabio Muleri, L. Pacciani, A. Paggi, Pierre-Olivier Petrucci, Nicole Rodriguez Cavero, Roger W. Romani, F. Tavecchio, Stefano Tugliani, Kinwah Wu, Matteo Bachetti, L. Baldini, W. H. Baumgartner, R. Bellazzini, S. Bianchi, Stephen D. Bongiorno, A. Brez, N. Bucciantini, Fiamma Capitanio, Simone Castellano, E. Costa, E. Del Monte, Niccolò Di Lalla, 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, P. Kaaret, Fabian Kislat, Takao Kitaguchi, Jeffery J. Kolodziejczak, Fabio La Monaca, L. Latronico, S. Maldera, Alberto Manfreda, G. Matt, C.‐Y. Ng, Stephen L. O’Dell, N. Omodei, C. Oppedisano, Alessandro Papitto, George G. Pavlov, M. Pesce-Rollins, M. Pilia, Andrea Possenti, Juri Poutanen, Brian D. Ramsey, John Rankin, Ajay Ratheesh, O. J. Roberts, C. Sgró, Patrick Slane, P. Soffitta, G. Spandre, Douglas A. Swartz, Toru Tamagawa, Roberto Taverna, Yuzuru Tawara, Allyn F. Tennant, Nicholas E. Thomas, Francesco Tombesi, A. Trois, Sergey S. Tsygankov, Jacco Vink, Martin C. Weisskopf, Fei Xie, Silvia Zane

Bibliographic record

VenueThe Astrophysical Journal · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsUniversity of British Columbia
FundersIstituto Nazionale di Fisica NucleareMinisterio de Ciencia e InnovaciónAgencia Estatal de InvestigaciónGoddard Space Flight CenterUniversity of CreteNational Science FoundationAgenzia Spaziale ItalianaNuclear Safety and Security CommissionCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationOak Ridge Associated UniversitiesInstituto de Astrofísica de AndalucíaMarshall Space Flight CenterIstituto Nazionale di Astrofisica
KeywordsPhysicsBlazarPolarimetryX-rayPolarization (electrochemistry)AstronomyAstrophysicsX-ray astronomyX-ray telescopeQuasarGamma rayOpticsScatteringGalaxyTelescope

Abstract

fetched live from OpenAlex

Abstract Observations of linear polarization in the 2–8 keV energy range with the Imaging X-ray Polarimetry Explorer (IXPE) explore the magnetic field geometry and dynamics of the regions generating nonthermal radiation in relativistic jets of blazars. These jets, particularly in blazars whose spectral energy distribution peaks at X-ray energies, emit X-rays via synchrotron radiation from high-energy particles within the jet. IXPE observations of the X-ray-selected BL Lac–type blazar 1ES 1959+650 on 2022 May 3–4 showed a significant linear polarization degree of Πx = 8.0% ± 2.3% at an electric-vector position angle ψ x = 123° ± 8°. However, on 2022 June 9–12, only an upper limit of Πx ≤ 5.1% could be derived (at the 99% confidence level). The degree of optical polarization at that time, ΠO ∼ 5%, is comparable to the X-ray measurement. We investigate possible scenarios for these findings, including temporal and geometrical depolarization effects. Unlike some other X-ray-selected BL Lac objects, there is no significant chromatic dependence of the measured polarization in 1ES 1959+650, and its low X-ray polarization may be attributed to turbulence in the jet flow with dynamical timescales shorter than 1 day.

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 score0.003
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 science0.0000.000
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 head0.005
GPT teacher head0.200
Teacher spread0.195 · 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

Citations31
Published2024
Admission routes1
Has abstractyes

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