Alan P. Marscher, Alberto Floris, Alessandro Maselli, Alexander Kraus, Alexey V. Zhovtan, Alfredo Sota, Alkmini Koukoutsi, Anastasia Glykopoulou, Andrea Gokus, Andrey A. Vasilyev, Aristeidis Polychronakis, A. Trindade Falc\~ao, Beatriz Ag\'is-Gonz\'alez, Dana Kirchner, Daria A. Morozova, Dawoon E. Kim, Dimitrios A. Langis, Dimitrios Rompogiannakis, D. \L. Kr\'ol, Dmitry Blinov, Ekaterina V. Shishkina, Elena G. Larionova, Elina Lindfors, Emanuele Nardini, Emmanouil Angelakis, Evgenia N. Kopatskaya, Florian Eppel, Florian R\"osch, Francisco Jos\'e Aceituno, Gabriel Emery, Garrett Keating, George A. Borman, Georgios F. Paraschos, Hiroshi Akitaya, Ioannis Liodakis, Ioannis Myserlis, Iv\'an Agudo, Ivan S. Troitskiy, John A. Kypriotakis, Jonas He{\ss}d\"orfer, Jorge Otero-Santos, Juan Escudero Pedrosa, Julia Eich, Kari Nilsson, Koji S. Kawabata, Laura Di Gesu, Lena Debbrecht, Lucio A. Antonelli, Mahito Sasada, Makoto Uemura, Mark Gurwell, Matteo Perri, Matthias Kadler, Orestis Zoumpoulakis, Panagiotis Fotis, Petra Benke, Pouya M. Kouch, Ramprasad Rao, Riccardo Middei, Ryo Imazawa, Sara Capecchiacci, Sergey S. Savchenko, Simonetta Puccetti, Stavros Vogiatzis, Stefano Ciprini, Steven H\"ammerich, Sumie Tochihara, Svetlana G. Jorstad, Takahiro Akai, Tapio Pursimo, Tatiana S. Grishina, Tatsuya Nakaoka, Tommaso Aniello, Tsunefumi Mizuno, Vasiliki Tsioupli, V\'ictor Casanova, Vilppu Piirola, Vladimir A. Hagen-Thorn, Wladislaw Schulga, Yasushi Fukazawa, Yulia V. Troitskaya
X-ray and optical emissions from the blazar PG 1553+113 arise from closely related but not identical regions in its jet.
The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same
current state with the deterministic merge algorithm.
Claims
C1strongest claim
the data support a picture in which the X-ray and optical emissions arise from closely related but not strictly co-spatial regions within a dynamically evolving, magnetically structured jet.
C2weakest assumption
The assumption that the observed polarization variability and EVPA rotation directly trace magnetic field configurations in the jet plasma rather than propagation effects or unrelated components.
C3one line summary
New IXPE X-ray polarimetry and optical monitoring of PG 1553+113 reveal variable polarization and a large EVPA swing, supporting jet models with related but non-co-spatial X-ray and optical emission regions.
References
226 extracted · 226 resolved · 88 Pith anchors
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2025 · doi:10.1051/0004-6361/202555392
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