Abstract
We present an optical-to-radio study of the BL Lac object S4 0954+658 observations during 1998–2023. The measurements were obtained with the SAO RAS Zeiss-1000 and AS-500/2 0.5-m telescopes in 2003–2023, with the RATAN-600 radio telescope at 1.25 (0.96, 1.1), 2.3, 4.7 (3.7, 3.9), 8.2 (7.7), 11.2, 22.3 (21.7) GHz in 1998–2023, with the IAA RAS RT-32 Zelenchukskaya and Badary telescopes at 5.05 and 8.63 GHz in 2020–2023, and with the RT-22 single-dish telescope of CrAO RAS at 36.8 GHz in 2009–2023. In this period the blazar was showing extremely high broadband activity with the variability amplitude of the flux densities up to 70–100\(\%\) both in the optical and radio domains. During the period of 2014–2023 the blazar displayed extremely high activity in the radio wavelengths, and we detected multiple radio flares of varying amplitude and duration. The large flares last on average from 0.3 to 1 year at 22–36.8 GHz and slightly longer at 5–11.2 GHz. The optical flares are shorter and last 7–50 days. The characteristic time scale \(\tau\) of variation at 5–22 GHz is about 100 days in the most active epoch of 2014–2023 and about 1000 days for the state with lower activity in 2009–2014. We found a general correlation between the optical, radio, and \(\gamma\)-ray flux variations, which suggesting that we observe the same photon population from different emission regions. We estimated the linear size of this region as 0.5–2 pc for different conditions. A broadband radio spectrum with two components of the S4 0954+658 jet was modeled using both electrons and protons as emitting particles. The results suggest that the synchrotron radio waves in this AGN may be produced by relativistic protons.
Notes
Institute of Applied Astronomy, Russian Academy of Sciences.
Crimean Astrophysical Observatory, Russian Academy of Sciences.
https://www.sao.ru/cats
https://www.sao.ru/blcat
https://www.bu.edu/blazars/VLBA_GLAST/0954.html
https://github.com/astronomerdamo/pydcf
https://github.com/samconnolly/DELightcurveSimula- tion/
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ACKNOWLEDGMENTS
The observations were carried out with the RATAN-600 scientific facility, the Zeiss-1000 and AS-500/2 optical reflectors of SAO RAS, and the RT-22 of CrAO RAS. Observations with the SAO RAS telescopes are supported by the Ministry of Science and Higher Education of the Russian Federation. The observations at 5.05 and 8.63 GHz were performed with the Badary and Zelenchukskaya RT-32 radio telescopes operated by the Shared Research Facility Center for the Quasar VLBI Network of IAA RAS (https://iaaras.ru/cu-center/).
VVV and SOI pay their tribute to N. S. Kardashev who had initiated the studies of blazars and made an important contribution to the issue debates. They would like to thank V. S. Bychkova for her involvement into blazar studies and valuable discussions on the topic of blazar variability. VAE and VLN are grateful to the staff of the Radio Astronomy Department of CrAO RAS for their participation in the observations.
This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration; the CATS database, available on the Special Astrophysical Observatory website; the SIMBAD database, operated at CDS, Strasbourg, France. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France. The development of the Fermi LAT Light Curve Repository has been funded in part through the Fermi Guest Investigator Program (NASA Research Announcements NNH19ZDA001N and NNH20ZDA001N). This study makes use of the VLBA data from the VLBA-BU Blazar Monitoring Program (BEAM-ME and VLBA-BU-BLAZAR; http://www.bu.edu/blazars/ BEAM-ME.html), funded by NASA through the Fermi Guest Investigator Program. The VLBA is an instrument of the National Radio Astronomy Observatory. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated by Associated Universities, Inc.
Funding
The reported study was funded by the Ministry of Science and Higher Education of the Russian Federation under contract 075-15-2022-1227. YYK was supported by the M2FINDERS project, which has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 Research and Innovation Programme (grant agreement No. 101018682). LY is supported by the National Natural Science Foundation of China (NSFC) grants No. 12205388.
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Vlasyuk, V.V., Sotnikova, Y.V., Volvach, A.E. et al. Optical and Radio Variability of the Blazar S4 0954+658. Astrophys. Bull. 78, 464–486 (2023). https://doi.org/10.1134/S1990341323600229
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DOI: https://doi.org/10.1134/S1990341323600229