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Polarization Studies in Different Blazar Types. I. Correlation Between Optical Brightness and Polarization Degree. / Shkodkina, E. A.; Savchenko, S. S.; Morozova, D. A.; Jorstad, S. G.; Borman, G. A.; Grishina, T. S.; Kopatskaya, E. N.; Larionova, E. G.; Vasilyev, A. A.; Troitskiy, I. S.; Troitskaya, Yu. V.; Novikova, P. A.; Shishkina, E. V.; Zhovtan, A. V.

в: Research in Astronomy and Astrophysics, Том 25, № 6, 065010, 29.05.2025.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Shkodkina, EA, Savchenko, SS, Morozova, DA, Jorstad, SG, Borman, GA, Grishina, TS, Kopatskaya, EN, Larionova, EG, Vasilyev, AA, Troitskiy, IS, Troitskaya, YV, Novikova, PA, Shishkina, EV & Zhovtan, AV 2025, 'Polarization Studies in Different Blazar Types. I. Correlation Between Optical Brightness and Polarization Degree', Research in Astronomy and Astrophysics, Том. 25, № 6, 065010. https://doi.org/10.1088/1674-4527/adcf82

APA

Shkodkina, E. A., Savchenko, S. S., Morozova, D. A., Jorstad, S. G., Borman, G. A., Grishina, T. S., Kopatskaya, E. N., Larionova, E. G., Vasilyev, A. A., Troitskiy, I. S., Troitskaya, Y. V., Novikova, P. A., Shishkina, E. V., & Zhovtan, A. V. (2025). Polarization Studies in Different Blazar Types. I. Correlation Between Optical Brightness and Polarization Degree. Research in Astronomy and Astrophysics, 25(6), [065010]. https://doi.org/10.1088/1674-4527/adcf82

Vancouver

Shkodkina EA, Savchenko SS, Morozova DA, Jorstad SG, Borman GA, Grishina TS и пр. Polarization Studies in Different Blazar Types. I. Correlation Between Optical Brightness and Polarization Degree. Research in Astronomy and Astrophysics. 2025 Май 29;25(6). 065010. https://doi.org/10.1088/1674-4527/adcf82

Author

Shkodkina, E. A. ; Savchenko, S. S. ; Morozova, D. A. ; Jorstad, S. G. ; Borman, G. A. ; Grishina, T. S. ; Kopatskaya, E. N. ; Larionova, E. G. ; Vasilyev, A. A. ; Troitskiy, I. S. ; Troitskaya, Yu. V. ; Novikova, P. A. ; Shishkina, E. V. ; Zhovtan, A. V. / Polarization Studies in Different Blazar Types. I. Correlation Between Optical Brightness and Polarization Degree. в: Research in Astronomy and Astrophysics. 2025 ; Том 25, № 6.

BibTeX

@article{7ec012098eac424bb28b967415989756,
title = "Polarization Studies in Different Blazar Types. I. Correlation Between Optical Brightness and Polarization Degree",
abstract = "We present an analysis of the cross-correlation between optical brightness and polarization degree in different types of blazars. The aim is to identify objects with simultaneous and consistent changes in characteristics and to determine if this behavior relates to the types of objects studied. The analysis includes 23 objects: 11 Flat Spectrum Radio Quasars (FSRQs), 11 BL Lacs, and 1 radio galaxy. Dense overlapping observation series in the R band were used, collected over more than 10 yr as part of a monitoring program for bright blazars at St. Petersburg State University. The cross-correlation analysis procedure is detailed, including a method for assessing significance based on Monte Carlo simulations of synthetic light curves modeled using a Damped Random Walk. Significant correlations were found for 5 FSRQs and 1 BL Lac. No significant correlation was detected for 10 BL Lacs and 6 FSRQs. One object did not yield a reliable estimate. Based on the current results, we cannot claim that the observed difference in the behavior of these emission characteristics for different classes of blazars is significant. It is possible that observed correlations may be explained by the contribution of simultaneous flare events to the changes in flux and polarization degree curves, which occur more frequently in FSRQs.",
keywords = "(galaxies:) BL Lacertae objects: general, galaxies: active, methods: data analysis, polarization",
author = "Shkodkina, {E. A.} and Savchenko, {S. S.} and Morozova, {D. A.} and Jorstad, {S. G.} and Borman, {G. A.} and Grishina, {T. S.} and Kopatskaya, {E. N.} and Larionova, {E. G.} and Vasilyev, {A. A.} and Troitskiy, {I. S.} and Troitskaya, {Yu. V.} and Novikova, {P. A.} and Shishkina, {E. V.} and Zhovtan, {A. V.}",
year = "2025",
month = may,
day = "29",
doi = "10.1088/1674-4527/adcf82",
language = "English",
volume = "25",
journal = "Research in Astronomy and Astrophysics",
issn = "1674-4527",
publisher = "IOP Publishing Ltd.",
number = "6",

}

RIS

TY - JOUR

T1 - Polarization Studies in Different Blazar Types. I. Correlation Between Optical Brightness and Polarization Degree

AU - Shkodkina, E. A.

AU - Savchenko, S. S.

AU - Morozova, D. A.

AU - Jorstad, S. G.

AU - Borman, G. A.

AU - Grishina, T. S.

AU - Kopatskaya, E. N.

AU - Larionova, E. G.

AU - Vasilyev, A. A.

AU - Troitskiy, I. S.

AU - Troitskaya, Yu. V.

AU - Novikova, P. A.

AU - Shishkina, E. V.

AU - Zhovtan, A. V.

PY - 2025/5/29

Y1 - 2025/5/29

N2 - We present an analysis of the cross-correlation between optical brightness and polarization degree in different types of blazars. The aim is to identify objects with simultaneous and consistent changes in characteristics and to determine if this behavior relates to the types of objects studied. The analysis includes 23 objects: 11 Flat Spectrum Radio Quasars (FSRQs), 11 BL Lacs, and 1 radio galaxy. Dense overlapping observation series in the R band were used, collected over more than 10 yr as part of a monitoring program for bright blazars at St. Petersburg State University. The cross-correlation analysis procedure is detailed, including a method for assessing significance based on Monte Carlo simulations of synthetic light curves modeled using a Damped Random Walk. Significant correlations were found for 5 FSRQs and 1 BL Lac. No significant correlation was detected for 10 BL Lacs and 6 FSRQs. One object did not yield a reliable estimate. Based on the current results, we cannot claim that the observed difference in the behavior of these emission characteristics for different classes of blazars is significant. It is possible that observed correlations may be explained by the contribution of simultaneous flare events to the changes in flux and polarization degree curves, which occur more frequently in FSRQs.

AB - We present an analysis of the cross-correlation between optical brightness and polarization degree in different types of blazars. The aim is to identify objects with simultaneous and consistent changes in characteristics and to determine if this behavior relates to the types of objects studied. The analysis includes 23 objects: 11 Flat Spectrum Radio Quasars (FSRQs), 11 BL Lacs, and 1 radio galaxy. Dense overlapping observation series in the R band were used, collected over more than 10 yr as part of a monitoring program for bright blazars at St. Petersburg State University. The cross-correlation analysis procedure is detailed, including a method for assessing significance based on Monte Carlo simulations of synthetic light curves modeled using a Damped Random Walk. Significant correlations were found for 5 FSRQs and 1 BL Lac. No significant correlation was detected for 10 BL Lacs and 6 FSRQs. One object did not yield a reliable estimate. Based on the current results, we cannot claim that the observed difference in the behavior of these emission characteristics for different classes of blazars is significant. It is possible that observed correlations may be explained by the contribution of simultaneous flare events to the changes in flux and polarization degree curves, which occur more frequently in FSRQs.

KW - (galaxies:) BL Lacertae objects: general

KW - galaxies: active

KW - methods: data analysis

KW - polarization

UR - https://www.mendeley.com/catalogue/75018cf5-0b61-3e00-a1ed-0737f36f5ee0/

U2 - 10.1088/1674-4527/adcf82

DO - 10.1088/1674-4527/adcf82

M3 - Article

VL - 25

JO - Research in Astronomy and Astrophysics

JF - Research in Astronomy and Astrophysics

SN - 1674-4527

IS - 6

M1 - 065010

ER -

ID: 136075767