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The Method of Searching for Rotations of the Polarization Position Angle of Quasars. / Savchenko, S. S.; Morozova, D. A.; Jorstad, S. G.; Blinov, D. A.; Borman, G. A.; Vasilyev, A. A.; Grishina, T. S.; Zhovtan, A. V.; Kopatskaya, E. N.; Larionova, E. G.; Troitskiy, I. S.; Troitskaya, Yu. V.; Shishkina, E. V.; Shkodkina, E. A.

в: Astrophysical Bulletin, Том 79, № 2, 01.06.2024, стр. 186-202.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

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@article{7f252eafad6449549446bcf558aa6735,
title = "The Method of Searching for Rotations of the Polarization Position Angle of Quasars",
abstract = "Observations of quasars show that the polarization position angle of the emission coming from them varies greatly over time, including periods called rotations during which the angle changes in an orderly manner. The study proposes a method for identifying such events and assessing their statistical significance. The operation of the method is demonstrated using the example of long-term polarimetric observations of the blazars CTA 102, 3C 454.3, and OT 081. During the analysis of light curves, 51 rotations of the polarization position angle were found and it was shown that for CTA 102 and 3C 454.3 the rotations are predominantly oriented in one direction.",
keywords = "Methods: data analysis—techniques: polarimetric—quasars: general",
author = "Savchenko, {S. S.} and Morozova, {D. A.} and Jorstad, {S. G.} and Blinov, {D. A.} and Borman, {G. A.} and Vasilyev, {A. A.} and Grishina, {T. S.} and Zhovtan, {A. V.} and Kopatskaya, {E. N.} and Larionova, {E. G.} and Troitskiy, {I. S.} and Troitskaya, {Yu. V.} and Shishkina, {E. V.} and Shkodkina, {E. A.}",
year = "2024",
month = jun,
day = "1",
doi = "10.1134/s1990341323600394",
language = "русский",
volume = "79",
pages = "186--202",
journal = "Astrophysical Bulletin",
issn = "1990-3413",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "2",

}

RIS

TY - JOUR

T1 - The Method of Searching for Rotations of the Polarization Position Angle of Quasars

AU - Savchenko, S. S.

AU - Morozova, D. A.

AU - Jorstad, S. G.

AU - Blinov, D. A.

AU - Borman, G. A.

AU - Vasilyev, A. A.

AU - Grishina, T. S.

AU - Zhovtan, A. V.

AU - Kopatskaya, E. N.

AU - Larionova, E. G.

AU - Troitskiy, I. S.

AU - Troitskaya, Yu. V.

AU - Shishkina, E. V.

AU - Shkodkina, E. A.

PY - 2024/6/1

Y1 - 2024/6/1

N2 - Observations of quasars show that the polarization position angle of the emission coming from them varies greatly over time, including periods called rotations during which the angle changes in an orderly manner. The study proposes a method for identifying such events and assessing their statistical significance. The operation of the method is demonstrated using the example of long-term polarimetric observations of the blazars CTA 102, 3C 454.3, and OT 081. During the analysis of light curves, 51 rotations of the polarization position angle were found and it was shown that for CTA 102 and 3C 454.3 the rotations are predominantly oriented in one direction.

AB - Observations of quasars show that the polarization position angle of the emission coming from them varies greatly over time, including periods called rotations during which the angle changes in an orderly manner. The study proposes a method for identifying such events and assessing their statistical significance. The operation of the method is demonstrated using the example of long-term polarimetric observations of the blazars CTA 102, 3C 454.3, and OT 081. During the analysis of light curves, 51 rotations of the polarization position angle were found and it was shown that for CTA 102 and 3C 454.3 the rotations are predominantly oriented in one direction.

KW - Methods: data analysis—techniques: polarimetric—quasars: general

UR - https://www.mendeley.com/catalogue/b9654e9a-176e-3467-b5f2-9ff2d344fe4f/

U2 - 10.1134/s1990341323600394

DO - 10.1134/s1990341323600394

M3 - статья

VL - 79

SP - 186

EP - 202

JO - Astrophysical Bulletin

JF - Astrophysical Bulletin

SN - 1990-3413

IS - 2

ER -

ID: 122268427