Simferopol, Simferopol, Russian Federation
Russian Federation
Russian Federation
Russian Federation
Russian Federation
Russian Federation
VAK Russia 1.3.1
UDC 524
UDC 520.8
UDC 524.7
CSCSTI 41.27
CSCSTI 41.17
Russian Classification of Professions by Education 03.05.01
Russian Classification of Professions by Education 03.06.01
Russian Library and Bibliographic Classification 223
Russian Trade and Bibliographic Classification 61
BISAC SCI004000 Astronomy
BISAC SCI005000 Physics / Astrophysics
The TESS satellite provides unique data from nearly continuous observations with high temporal resolution. Each sky sector is observed for 27 days. For the blazar S5 1803+784, there are three observing seasons during which the object remains in the TESS field of view for extended periods, approximately 10 months in total. By supplementing these data with multi-band photometric observations from the Zwicky Transient Facility (ZTF) and the AZT-8 telescope at the Crimean Astrophysical Observatory of the Russian Academy of Sciences, we obtain a unique opportunity to study the relation between the shortest characteristic variability timescales and the parameters of long-term variability. Based on this analysis, we conclude that short-term variability is caused by the emergence and evolution of jet regions, whose motion deviates from the general trajectory, and, therefore, they have different Doppler factors. We performed light curve modeling under this assumption and obtained good qualitative agreement with the observations.
active galaxies: blazars; optical variability
1. Butuzova M.S., Guseva V.A., Gorbachev M.A., et al., 2025, Journal of High Energy Astrophysics, 45, p. 19 DOI: https://doi.org/10.1016/j.jheap.2024.11.008; EDN: https://elibrary.ru/BUYQDF
2. Butuzova M.S., 2021, Astroparticle Physics, 129, id. 102577 DOI: https://doi.org/10.1016/j.astropartphys.2021.102577
3. Gorbachev M.A. and Butuzova M.S., 2025, Astronomical and Astrophysical Transactions, in press
4. Gorbachev M.A., Butuzova M.S., Nazarov S.V., et al., 2024, Astroparticle Physics, 160, id. 102965 DOI: https://doi.org/10.1016/j.astropartphys.2024.102965
5. Gorbachev M.A., Butuzova M.S., Sergeev S.G., et al., 2022, Astrophysical Journal, 928, 1, p. 86 DOI: https://doi.org/10.3847/1538-4357/ac4fc3
6. Marscher A.P. and Gear W.K., 1985, Astrophysical Journal, 298, p. 114 DOI: https://doi.org/10.1086/163592
7. Marscher A.P., 2014, Astrophysical Journal, 780, 1, p. 87 DOI: https://doi.org/10.1088/0004-637X/780/1/87
8. Raiteri C.M., Villata M., Carosati D., et al., 2021a, Monthly Notices of the Royal Astronomical Society, 501, 1, p. 1100
9. Raiteri C.M., Villata M., Larionov V.M., et al., 2021b, Monthly Notices of the Royal Astronomical Society, 504, 4, p. 5629
10. Simonetti J.H., Cordes J.M., Heeschen D.S., 1985, Astrophysical Journal, 296, p. 46 DOI: https://doi.org/10.1086/163418
11. Weaver Z.R., Williamson K.E., Jorstad S.G., et al., 2020, Astrophysical Journal, 900, 2, p. 137




