Multiwavelength variability of the blazar Ton 599

We present a study of the multiwavelength variability of the blazar Ton 599 based on the radio-to--ray data covering the period of 1997-2024. The data are represented by the 1-22 GHz measurements from the SAO RAS RATAN-600 radio telescope, the 5 and 8 GHz data from the IAA RAS RT-32 telescopes, and the 37 GHz data from the RT-22 telescope of CrAO RAS. The optical measurements in the R-band were collected with the SAO RAS 1-m Zeiss-1000 and 0.5-m AS-500/2, SPbSU 0.4-m LX-200, and CrAO RAS 0.7-m AZT-8 telescopes. We also used the archive data at 230 GHz from the Submillimeter Array (SMA) and the -ray data in the 0.1-100 GeV band from the Fermi-LAT point source catalogue 4FGL-DR2. The blazar exhibits extreme variability properties with a variability index varying from 0.47 to 0.98. A characteristic feature of the light curves is the presence of double and triple flares with different spectral properties. A significant correlation ($\geq 2\sigma$) between the radio, optical, and -ray bands is found with time delays from 0 to 365 days. The L-S periodograms show the significant peaks ($>3\sigma$) related to periods of 2.4-3.9 years, which coincides with global oscillations obtained earlier on the time scale of 1987-2010.

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Published
2024-12-27
DOI
https://doi.org/10.26119/vak2024.014
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
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0.00

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article

Multiwavelength variability of the blazar Ton 599

A. E. Volvach, A. V. Popkov, M. A. Kharinov, D. O. Kudryavtsev et al.
Astrophysics and Cosmic Phenomena
article

Multiwavelength variability of the blazar Ton 599

A. E. Volvach, A. V. Popkov, M. A. Kharinov, D. O. Kudryavtsev, М. Г. Мингалиев, Y. Y. Kovalev, R. Yu. Udovitskiy, Yu. V. Sotnikova, D. A. Morozova, A. G. Mikhailov, Т. В. Муфахаров, Т. А. Семенова, I. A. Rakhimov, М. Л. Хабибуллина, V. Stolyarov, T. Andreeva, V. V. Vlasyuk
article en

Abstract

We present a study of the multiwavelength variability of the blazar Ton 599 based on the radio-to--ray data covering the period of 1997-2024. The data are represented by the 1-22 GHz measurements from the SAO RAS RATAN-600 radio telescope, the 5 and 8 GHz data from the IAA RAS RT-32 telescopes, and the 37 GHz data from the RT-22 telescope of CrAO RAS. The optical measurements in the R-band were collected with the SAO RAS 1-m Zeiss-1000 and 0.5-m AS-500/2, SPbSU 0.4-m LX-200, and CrAO RAS 0.7-m AZT-8 telescopes. We also used the archive data at 230 GHz from the Submillimeter Array (SMA) and the -ray data in the 0.1-100 GeV band from the Fermi-LAT point source catalogue 4FGL-DR2. The blazar exhibits extreme variability properties with a variability index varying from 0.47 to 0.98. A characteristic feature of the light curves is the presence of double and triple flares with different spectral properties. A significant correlation ($\geq 2\sigma$) between the radio, optical, and -ray bands is found with time delays from 0 to 365 days. The L-S periodograms show the significant peaks ($>3\sigma$) related to periods of 2.4-3.9 years, which coincides with global oscillations obtained earlier on the time scale of 1987-2010.

P.N. Lebedev Physical Institute of the Russian Academy of Sciences (RU), Moscow Institute of Physics and Technology (RU), St Petersburg University (RU), Kazan Federal University (RU), University of Cambridge (GB), Special Astrophysical Observatory (RU), Astro Space Center (RU), Development Agency of Serbia (RS), Institute for Nuclear Research (RU), Institute of Applied Astronomy (RU), Max Planck Institute for Radio Astronomy (DE), Crimean Astrophysical Observatory (UA)
Ministry of Science and Higher Education of the Russian Federation
Openalex Percentile: Top 93%
Astrophysics and Cosmic Phenomena
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