Authors

Manel Errando, McDonnell Center for the Space Sciences
Ioannis Liodakis, Turun yliopisto
Alan P. Marscher, Boston University
Herman L. Marshall, MIT Kavli Institute for Astrophysics and Space Research
Riccardo Middei, Agenzia Spaziale Italiana
Michela Negro, Louisiana State University
Abel Lawrence Peirson, Kavli Institute for Particle Astrophysics and Cosmology
Matteo Perri, Agenzia Spaziale Italiana
Simonetta Puccetti, Agenzia Spaziale Italiana
Pazit L. Rabinowitz, McDonnell Center for the Space Sciences
Iván Agudo, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Svetlana G. Jorstad, Boston University
Sergey S. Savchenko, Saint Petersburg State University
Dmitry Blinov, Foundation for Research and Technology-Hellas
Ioakeim G. Bourbah, University of Crete
Sebastian Kiehlmann, Foundation for Research and Technology-Hellas
Evangelos Kontopodis, University of Crete
Nikos Mandarakas, Foundation for Research and Technology-Hellas
Stylianos Romanopoulos, Foundation for Research and Technology-Hellas
Raphael Skalidis, Foundation for Research and Technology-Hellas
Anna Vervelaki, University of Crete
Francisco José Aceituno, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Maria I. Bernardos, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Giacomo Bonnoli, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Víctor Casanova, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Beatriz Agís-González, CSIC - Instituto de Astrofísica de Andalucía (IAA)
César Husillos, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Alessandro Marchini, Università degli Studi di Siena
Alfredo Sota, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Pouya M. Kouch, Turun yliopisto
Elina Lindfors, Turun yliopisto
Carolina Casadio, Foundation for Research and Technology-Hellas
Juan Escudero, CSIC - Instituto de Astrofísica de Andalucía (IAA)

Document Type

Article

Publication Date

3-1-2024

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.

Publication Source (Journal or Book title)

Astrophysical Journal

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