Observations of Low and Intermediate Spectral Peak Blazars with the Imaging X-Ray Polarimetry Explorer

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 3 σ 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.

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Publication Details

Journal
The Astrophysical Journal
Published
2024-08-26
DOI
https://doi.org/10.3847/1538-4357/ad5671
Citations
14
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
9.23

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article

Observations of Low and Intermediate Spectral Peak Blazars with the Imaging X-Ray Polarimetry Explorer

Niccolò Di Lalla, Fabian Kislat, Stylianos Romanopoulos, Hiroshi Akitaya et al.
14 citations
The Astrophysical Journal
Astrophysics and Cosmic Phenomena
9.23
article

Observations of Low and Intermediate Spectral Peak Blazars with the Imaging X-Ray Polarimetry Explorer

Niccolò Di Lalla, Fabian Kislat, Stylianos Romanopoulos, Hiroshi Akitaya, F. Massaro, Alessandro Marchini, Jeffery J. Kolodziejczak, Juri Poutanen, R. Bonino, A. Brez, G. V. Panopoulou, Laura Di Gesu, Simonetta Puccetti, Joana A. Kramer, Michal Dovčiak, Y. Evangelista, S. Ciprini, Greg Madjeski, Dawoon E. Kim, A. A. Vasilyev, Silvia Zane, J. Masiero, M. Pilia, Allyn F. Tennant, Jeremy Heyl, Evangelos Kontopodis, Andrea Possenti, Ioakeim G. Bourbah, Victor Doroshenko, C. Husillos, Jacco Vink, A. Sota, Herman L. Marshall, A. Kraus, Ioannis Liodakis, А. В. Жовтан, A. Berdyugin, Pouya M. Kouch, E. Costa, Garrett K. Keating, F. Tavecchio, E. Angelakis, G. Matt, Sincheol Kang, Javier A. García, Pierre-Olivier Petrucci, Hiroshi Nagai, Svetlana G. Jorstad, R. Kneißl, Alessandro Di Marco, P. Soffitta, Alberto Manfreda, W. H. Baumgartner, Alessandra De Rosa, D. Blinov, Takeshi Sakanoi, Kinwah Wu, M. Perri, Martin C. Weisskopf, M. Bernardos, Beatriz Agı́s-González, Е. Г. Ларионова, E. Del Monte, Antonio Hales, С. С. Савченко, G. Spandre, Samaporn Tinyanont, O. J. Roberts, I. Myserlis, Fei Xie, Masato Kagitani, Raphael Skalidis, George G. Pavlov, Roger W. Romani, I. Agudo, M. Laurenti, Francesco Tombesi, Ramprasad Rao, M. Pesce-Rollins, Seiji Kameno, Frédéric Marin, Patrick Slane, D. A. Morozova, Toru Tamagawa, Yuzuru Tawara, Fiamma Capitanio, Steven R. Ehlert, Stephen L. O’Dell, Stephen D. Bongiorno, S. Maldera, C. Sgrò, V. Karas, Hyeon‐Woo Jeong, John Rankin, Alessandro Papitto, F. J. Aceituno, A. Trois, Vadim Kravtsov, Makoto Uemura, Sergey S. Tsygankov, Hugo Messias, E. N. Kopatskaya, Maya García‐Comas, Riccardo Ferrazzoli, W. Iwakiri, Sang-Sung Lee, Fabio Muleri, N. Mandarakas, G. Bonnoli, Brian D. Ramsey, E. Lindfors, V. Casanova, Tsunefumi Mizuno, Ikuyuki Mitsuishi, Roberto Taverna, Teruaki Enoto, Dimitri Mawet, R. Bellazzini, Г. А. Борман, E. Cavazzuti, Sergio Fabiani, Douglas A. Swartz, H. Krawczynski, Shuichi Gunji, Michela Negro, Whee Yeon Cheong, Mahito Sasada, C. Casadio, Jenni Jormanainen, Ryo Imazawa, Y. Fukazawa, Andrea Marinucci, R. Middei, Mark Gurwell, L. Pacciani, Alan P. Marscher, Abel L. Peirson, Matteo Bachetti, C. Oppedisano, Nicole Rodriguez Cavero, Simone Castellano, P. Kaaret, L. Baldini, Ajay Ratheesh, N. Bucciantini, Koji S. Kawabata, Fabio La Monaca, L. Latronico, Nicholas E. Thomas, I. Donnarumma, L. A. Antonelli, S. Bianchi, Anna Vervelaki, Sebastian Kielhmann, Efthalia Trainou, Sang-Hyun Kim, Juan Escudero, Roberto Turolla, Matthew Dattolo, N. Omodei, Tatsuya Nakaoka, C.‐Y. Ng, Kiyoshi Hayashida, Takao Kitaguchi, Chen-Ting Chen
article en
14 citations

Abstract

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 3 σ 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.

The Astrophysical JournalVol. 972(1)
University of Siena (IT), University of Pisa (IT), Boston University (US), Yamagata University (JP), Hiroshima University (JP), Tokyo Institute of Technology (JP), University of Rome Tor Vergata (IT), Roma Tre University (IT), Louisiana State University (US), California Institute of Technology (US), Marshall Space Flight Center (US), Centre National de la Recherche Scientifique (FR), Goddard Space Flight Center (US), Pennsylvania State University (US), Universities Space Research Association (US), University of Padua (IT), University of British Columbia (CA), University of Crete (GR), Guangxi University (CN), University of Turku (FI), Chiba University (JP), Istituto Nazionale di Fisica Nucleare (IT), University of New Hampshire (US), St Petersburg University (RU), Turku Centre for Computer Science (FI), University of California, Santa Cruz (US), The Graduate University for Advanced Studies, SOKENDAI (JP), National and Kapodistrian University of Athens (GR), Tohoku University (JP), Washington University in St. Louis (US), National Radio Astronomy Observatory (US), Atacama Large Millimeter Submillimeter Array (CL), Special Astrophysical Observatory (RU), Arcetri Astrophysical Observatory (IT), Astronomical Observatory of Rome (IT), Czech Academy of Sciences, Astronomical Institute (CZ), Agenzia Spaziale Italiana (IT), Korea Astronomy and Space Science Institute (KR), Pulkovo Observatory (RU), Observatoire astronomique de Strasbourg (FR), Brera Astronomical Observatory (IT), Kavli Institute for Particle Astrophysics and Cosmology (US), Istituto Nazionale di Fisica Nucleare, Sezione di Torino (IT), Institute for Space Astrophysics and Planetology (IT), Pioneer (Japan) (JP), RIKEN (JP), Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata (IT), Center for Astrophysics Harvard & Smithsonian (US), European Southern Observatory (CL), Istituto Nazionale di Fisica Nucleare, Sezione di Firenze (IT), Instituto de Radioastronomía Milimétrica (ES), Osservatorio Astronomico di Cagliari (IT), Max Planck Institute for Radio Astronomy (DE), Instituto de Astrofísica de Andalucía (ES), National Astronomical Observatory of Japan (JP), Istituto Nazionale di Fisica Nucleare, Sezione di Pisa (IT), Crimean Astrophysical Observatory (UA), University of Florence (IT), University College London (GB), University of Turin (IT), Nagoya University (JP), Massachusetts Institute of Technology (US), University of Maryland, College Park (US), Université de Strasbourg (FR), University of Tübingen (DE), Chiba Institute of Technology (JP), Sapienza University of Rome (IT), University of Amsterdam (NL), Korea University of Science and Technology (KR), University of Hong Kong (HK), Foundation for Research and Technology Hellas (GR), Université Grenoble Alpes (FR), Stanford University (US), The University of Osaka (JP)
National Science Foundation, Smithsonian Institution, National Aeronautics and Space Administration, Yale University, California Institute of Technology, Aarhus Universitet, Space Telescope Science Institute, National Radio Astronomy Observatory, European Commission, Ministry of Education, Culture, Sports, Science and Technology, Academia Sinica, Nuclear Safety and Security Commission, Korea Institute of Science and Technology, Korea Institute of Science and Technology Information, Korea Astronomy and Space Science Institute, Agenzia Spaziale Italiana, Max-Planck-Gesellschaft, University of Crete, Centre National de la Recherche Scientifique, Ministerio de Ciencia e Innovación, Istituto Nazionale di Astrofisica, Universitetet i Oslo, Háskóli Íslands, Turun Yliopisto, National Astronomical Observatory of Japan, Stockholms Universitet, Junta de Andalucía, Istituto Nazionale di Fisica Nucleare, Instituto de Astrofísica de Andalucía, Korea Research Environment Open Network, Marshall Space Flight Center, Goddard Space Flight Center, Smithsonian Astrophysical Observatory, Leibniz-Gemeinschaft, Japan Society for the Promotion of Science, Consejo Superior de Investigaciones Científicas, National Institutes of Natural Sciences
Openalex Percentile: Top 1%
Astrophysics and Cosmic Phenomena
9.23
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