Authors

Chien Ting J. Chen, Huntsville Program Office
Ioannis Liodakis, NASA Marshall Space Flight Center
Riccardo Middei, Agenzia Spaziale Italiana
Dawoon E. Kim, Istituto Nazionale Di Astrofisica, Rome
Laura Di Gesu, Agenzia Spaziale Italiana
Alessandro Di Marco, Istituto Nazionale Di Astrofisica, Rome
Steven R. Ehlert, NASA Marshall Space Flight Center
Manel Errando, McDonnell Center for the Space Sciences
Michela Negro, Louisiana State University
Svetlana G. Jorstad, Boston University
Alan P. Marscher, Boston University
Kinwah Wu, UCL Mullard Space Science Laboratory
Iván Agudo, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Juri Poutanen, Turun yliopisto
Tsunefumi Mizuno, Hiroshima University
Pouya M. Kouch, Turun yliopisto
Elina Lindfors, Turun yliopisto
George A. Borman, Crimean Astrophysical Observatory
Tatiana S. Grishina, Saint Petersburg State University
Evgenia N. Kopatskaya, Saint Petersburg State University
Elena G. Larionova, Saint Petersburg State University
Daria A. Morozova, Saint Petersburg State University
Sergey S. Savchenko, Saint Petersburg State University
Ivan S. Troitsky, Saint Petersburg State University
Yulia V. Troitskaya, Saint Petersburg State University
Andrey A. Vasilyev, Saint Petersburg State University
Alexey V. Zhovtan, Crimean Astrophysical Observatory
Francisco José Aceituno, 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)
Juan Escudero, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Beatriz Agís-González, Foundation for Research and Technology-Hellas
César Husillos, CSIC - Instituto Geológico y Minero de España (IGME)

Document Type

Article

Publication Date

10-1-2024

Abstract

We present multiwavelength polarization measurements of the luminous blazar Mrk 501 over a 14 month period. The 2-8 keV X-ray polarization was measured with the Imaging X-ray Polarimetry Explorer (IXPE) with six 100 ks observations spanning from 2022 March to 2023 April. Each IXPE observation was accompanied by simultaneous X-ray data from NuSTAR, Swift/XRT, and/or XMM-Newton. Complementary optical-infrared polarization measurements were also available in the B, V, R, I, and J bands, as were radio polarization measurements from 4.85 GHz to 225.5 GHz. Among the first five IXPE observations, we did not find significant variability in the X-ray polarization degree and angle with IXPE. However, the most recent sixth observation found an elevated polarization degree at >3 above the average of the other five observations. The optical and radio measurements show no apparent correlations with the X-ray polarization properties. Throughout the six IXPE observations, the X-ray polarization degree remained higher than, or similar to, the R-band optical polarization degree, which remained higher than the radio value. This is consistent with the energy-stratified shock scenario proposed to explain the first two IXPE observations, in which the polarized X-ray, optical, and radio emission arises from different regions.

Publication Source (Journal or Book title)

Astrophysical Journal

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