Synchrotron emission from the blazar PG 1553+113. An analysis of its flux and polarization variability
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Volume Title
A1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä
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Date
2017
Department
INAF - Osservatorio Astrofisico di Torino
Osservatorio Astronomico di Roma
Scuola Normale Superiore di Pisa
St. Petersburg State University
Instituto de Astrofísica de Canarias
RAS - Pulkovo Astronomical Observatory
Bulgarian Academy of Sciences
Crimean Astrophysical Observatory
EPT Observatories
TNG Fundación Galileo Galilei
National Central University
Astronomical Observatory Belgrade
Academy of Sciences of the Republic of Uzbekistan
INAF - Osservatorio Astrofisico di Catania
INAF - Istituto di Radioastronomia
Georgian National Academy of Sciences
Department of Radio Science and Engineering
University of Crete
Brigham Young University
Münster University of Applied Sciences
Osservatorio Astronomico Sirio
University of Colorado Denver
Metsähovi Radio Observatory
Department of Electronics and Nanoengineering
Osservatorio Astronomico di Roma
Scuola Normale Superiore di Pisa
St. Petersburg State University
Instituto de Astrofísica de Canarias
RAS - Pulkovo Astronomical Observatory
Bulgarian Academy of Sciences
Crimean Astrophysical Observatory
EPT Observatories
TNG Fundación Galileo Galilei
National Central University
Astronomical Observatory Belgrade
Academy of Sciences of the Republic of Uzbekistan
INAF - Osservatorio Astrofisico di Catania
INAF - Istituto di Radioastronomia
Georgian National Academy of Sciences
Department of Radio Science and Engineering
University of Crete
Brigham Young University
Münster University of Applied Sciences
Osservatorio Astronomico Sirio
University of Colorado Denver
Metsähovi Radio Observatory
Department of Electronics and Nanoengineering
Major/Subject
Mcode
Degree programme
Language
en
Pages
13
3762-3774
3762-3774
Series
Monthly Notices of the Royal Astronomical Society, Volume 466, issue 3
Abstract
In 2015 July 29-September 1, the satellite XMM-Newton pointed at the BL Lac object PG 1553+133 six times, collecting data for 218 h. During one of these epochs, simultaneous observations by the Swift satellite were requested to compare the results of the X-ray and optical-UV instruments. Optical, near-infrared and radio monitoring was carried out by the Whole Earth Blazar Telescope (WEBT) collaboration for the whole observing season. We here present the results of the analysis of all these data, together with an investigation of the source photometric and polarimetric behaviour over the last 3 yr. The 2015 EPIC spectra show slight curvature and the corresponding light curves display fast X-ray variability with a time-scale of the order of 1 h. In contrast to previous results, during the brightest X-ray states detected in 2015 the simple log-parabolic model that best fits the XMM-Newton data also reproduces reasonably well the whole synchrotron bump, suggesting a peak in the near- UV band. We found evidence ofa wide rotation of the polarization angle in 2014, when the polarization degree was variable, but the flux remained almost constant. This is difficult to interpret with deterministic jet emission models, while it can be easily reproduced by assuming some turbulence of the magnetic field.Description
Keywords
BL Lacertae objects: general, BL Lacertae objects: individual: PG 1553+113, Galaxies: active
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Citation
Raiteri , C M , Nicastro , F , Stamerra , A , Villata , M , Larionov , V M , Blinov , D , Acosta-Pulido , J A , Arévalo , M J , Arkharov , A , Bachev , R , Borman , G A , Carnerero , M I , Carosati , D , Cecconi , M , Chen , W P , Damljanovic , G , Di Paola , A , Ehgamberdiev , S A , Frasca , A , Giroletti , M , González-Morales , P A , Griñon-Marín , A B , Grishina , T S , Huang , P-C , Ibryamov , S , Klimanov , S A , Kopatskaya , E N , Kurtanidze , O M , Kurtanidze , S O , Lähteenmäki , A , Larionova , E G , Larionova , L V , Lázaro , C , Leto , G , Liodakis , I , Martínez-Lombilla , C , Mihov , B , Mirzaqulov , D O , Mokrushina , A A , Moody , J W , Morozova , D A , Nazarov , S V , Nikolashvili , M G , Ohlert , J M , Panopoulou , G V , Pastor Yabar , A , Pinna , F , Protasio , C , Rizzi , N , Sadun , A C , Savchenko , S S , Semkov , E , Sigua , L A , Slavcheva-Mihova , L , Strigachev , A , Tornikoski , M , Troitskaya , Y V , Troitsky , I S , Vasilyev , A A , Vera Rodriguez , R , Vince , O & Zanmar Sanchez , R 2017 , ' Synchrotron emission from the blazar PG 1553+113. An analysis of its flux and polarization variability ' , Monthly Notices of the Royal Astronomical Society , vol. 466 , no. 3 , pp. 3762-3774 . https://doi.org/10.1093/mnras/stw3333