Authors

Herman L. Marshall, MIT Kavli Institute for Astrophysics and Space Research
Ioannis Liodakis, NASA Marshall Space Flight Center
Alan P. Marscher, Boston University
Niccolò Di Lalla, Kavli Institute for Particle Astrophysics and Cosmology
Svetlana G. Jorstad, Boston University
Dawoon E. Kim, Istituto Nazionale Di Astrofisica, Rome
Riccardo Middei, Agenzia Spaziale Italiana
Michela Negro, Louisiana State University
Nicola Omodei, Kavli Institute for Particle Astrophysics and Cosmology
Abel L. Peirson, Kavli Institute for Particle Astrophysics and Cosmology
Matteo Perri, Agenzia Spaziale Italiana
Simonetta Puccetti, Agenzia Spaziale Italiana
Marco Laurenti, Agenzia Spaziale Italiana
Iván Agudo, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Giacomo Bonnoli, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Andrei V. Berdyugin, Turun yliopisto
Elisabetta Cavazzuti, Agenzia Spaziale Italiana
Nicole Rodriguez Cavero, McDonnell Center for the Space Sciences
Immacolata Donnarumma, Agenzia Spaziale Italiana
Laura Di Gesu, Agenzia Spaziale Italiana
Jenni Jormanainen, Turun yliopisto
Henric Krawczynski, McDonnell Center for the Space Sciences
Elina Lindfors, Turun yliopisto
Greg Madjeski, Kavli Institute for Particle Astrophysics and Cosmology
Frédéric Marin, Observatoire Astronomique de Strasbourg
Francesco Massaro, Istituto Nazionale di Fisica Nucleare, Sezione di Torino
Luigi Pacciani, Istituto Nazionale Di Astrofisica, Rome
Juri Poutanen, Turun yliopisto
Fabrizio Tavecchio, Osservatorio Astronomico di Brera
Pouya M. Kouch, Turun yliopisto
Francisco José Aceituno, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Maria I. Bernardos, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Víctor Casanova, CSIC - Instituto de Astrofísica de Andalucía (IAA)

Document Type

Article

Publication Date

9-1-2024

Abstract

We present X-ray polarimetry observations from the Imaging X-ray Polarimetry Explorer (IXPE) of three low spectral peak and one intermediate spectral peak blazars, namely 3C 273, 3C 279, 3C 454.3, and S5 0716+714. For none of these objects was IXPE able to detect X-ray polarization at the 3σ level. However, we placed upper limits on the polarization degree at ∼10%-30%. The undetected polarizations favor models where the X-ray band is dominated by unpolarized photons upscattered by relativistic electrons in the jets of blazars, although hadronic models are not completely eliminated. We discuss the X-ray polarization upper limits in the context of our contemporaneous multiwavelength polarization campaigns.

Publication Source (Journal or Book title)

Astrophysical Journal

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