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 st...
Ausführliche Beschreibung
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| Autor*in: |
Savchenko, S. S. [verfasserIn] Morozova, D. A. [verfasserIn] Jorstad, S. G. [verfasserIn] Blinov, D. A. [verfasserIn] Borman, G. A. [verfasserIn] Vasilyev, A. A. [verfasserIn] Grishina, T. S. [verfasserIn] Zhovtan, A. V. [verfasserIn] Kopatskaya, E. N. [verfasserIn] Larionova, E. G. [verfasserIn] Troitskiy, I. S. [verfasserIn] Troitskaya, Yu. V. [verfasserIn] Shishkina, E. V. [verfasserIn] Shkodkina, E. A. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2024 |
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| Anmerkung: |
© Pleiades Publishing, Ltd. 2024 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysical bulletin - Pleiades Publishing, 2007, 79(2024), 2 vom: Juni, Seite 186-202 |
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| Übergeordnetes Werk: |
volume:79 ; year:2024 ; number:2 ; month:06 ; pages:186-202 |
| Links: |
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| DOI / URN: |
10.1134/S1990341323600394 |
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| Katalog-ID: |
SPR056803559 |
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| 100 | 1 | |a Savchenko, S. S. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a The Method of Searching for Rotations of the Polarization Position Angle of Quasars |
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| 520 | |a 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. | ||
| 700 | 1 | |a Morozova, D. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Jorstad, S. G. |e verfasserin |4 aut | |
| 700 | 1 | |a Blinov, D. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Borman, G. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Vasilyev, A. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Grishina, T. S. |e verfasserin |4 aut | |
| 700 | 1 | |a Zhovtan, A. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Kopatskaya, E. N. |e verfasserin |4 aut | |
| 700 | 1 | |a Larionova, E. G. |e verfasserin |4 aut | |
| 700 | 1 | |a Troitskiy, I. S. |e verfasserin |4 aut | |
| 700 | 1 | |a Troitskaya, Yu. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Shishkina, E. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Shkodkina, E. A. |e verfasserin |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Astrophysical bulletin |d Pleiades Publishing, 2007 |g 79(2024), 2 vom: Juni, Seite 186-202 |w (DE-627)546895565 |w (DE-600)2390996-1 |x 1990-3421 |7 nnns |
| 773 | 1 | 8 | |g volume:79 |g year:2024 |g number:2 |g month:06 |g pages:186-202 |
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10.1134/S1990341323600394 doi (DE-627)SPR056803559 (SPR)S1990341323600394-e DE-627 ger DE-627 rakwb eng 520 VZ Savchenko, S. S. verfasserin aut The Method of Searching for Rotations of the Polarization Position Angle of Quasars 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2024 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. Morozova, D. A. verfasserin aut Jorstad, S. G. verfasserin aut Blinov, D. A. verfasserin aut Borman, G. A. verfasserin aut Vasilyev, A. A. verfasserin aut Grishina, T. S. verfasserin aut Zhovtan, A. V. verfasserin aut Kopatskaya, E. N. verfasserin aut Larionova, E. G. verfasserin aut Troitskiy, I. S. verfasserin aut Troitskaya, Yu. V. verfasserin aut Shishkina, E. V. verfasserin aut Shkodkina, E. A. verfasserin aut Enthalten in Astrophysical bulletin Pleiades Publishing, 2007 79(2024), 2 vom: Juni, Seite 186-202 (DE-627)546895565 (DE-600)2390996-1 1990-3421 nnns volume:79 year:2024 number:2 month:06 pages:186-202 https://dx.doi.org/10.1134/S1990341323600394 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 79 2024 2 06 186-202 |
| spelling |
10.1134/S1990341323600394 doi (DE-627)SPR056803559 (SPR)S1990341323600394-e DE-627 ger DE-627 rakwb eng 520 VZ Savchenko, S. S. verfasserin aut The Method of Searching for Rotations of the Polarization Position Angle of Quasars 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2024 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. Morozova, D. A. verfasserin aut Jorstad, S. G. verfasserin aut Blinov, D. A. verfasserin aut Borman, G. A. verfasserin aut Vasilyev, A. A. verfasserin aut Grishina, T. S. verfasserin aut Zhovtan, A. V. verfasserin aut Kopatskaya, E. N. verfasserin aut Larionova, E. G. verfasserin aut Troitskiy, I. S. verfasserin aut Troitskaya, Yu. V. verfasserin aut Shishkina, E. V. verfasserin aut Shkodkina, E. A. verfasserin aut Enthalten in Astrophysical bulletin Pleiades Publishing, 2007 79(2024), 2 vom: Juni, Seite 186-202 (DE-627)546895565 (DE-600)2390996-1 1990-3421 nnns volume:79 year:2024 number:2 month:06 pages:186-202 https://dx.doi.org/10.1134/S1990341323600394 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 79 2024 2 06 186-202 |
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10.1134/S1990341323600394 doi (DE-627)SPR056803559 (SPR)S1990341323600394-e DE-627 ger DE-627 rakwb eng 520 VZ Savchenko, S. S. verfasserin aut The Method of Searching for Rotations of the Polarization Position Angle of Quasars 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2024 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. Morozova, D. A. verfasserin aut Jorstad, S. G. verfasserin aut Blinov, D. A. verfasserin aut Borman, G. A. verfasserin aut Vasilyev, A. A. verfasserin aut Grishina, T. S. verfasserin aut Zhovtan, A. V. verfasserin aut Kopatskaya, E. N. verfasserin aut Larionova, E. G. verfasserin aut Troitskiy, I. S. verfasserin aut Troitskaya, Yu. V. verfasserin aut Shishkina, E. V. verfasserin aut Shkodkina, E. A. verfasserin aut Enthalten in Astrophysical bulletin Pleiades Publishing, 2007 79(2024), 2 vom: Juni, Seite 186-202 (DE-627)546895565 (DE-600)2390996-1 1990-3421 nnns volume:79 year:2024 number:2 month:06 pages:186-202 https://dx.doi.org/10.1134/S1990341323600394 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 79 2024 2 06 186-202 |
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10.1134/S1990341323600394 doi (DE-627)SPR056803559 (SPR)S1990341323600394-e DE-627 ger DE-627 rakwb eng 520 VZ Savchenko, S. S. verfasserin aut The Method of Searching for Rotations of the Polarization Position Angle of Quasars 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2024 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. Morozova, D. A. verfasserin aut Jorstad, S. G. verfasserin aut Blinov, D. A. verfasserin aut Borman, G. A. verfasserin aut Vasilyev, A. A. verfasserin aut Grishina, T. S. verfasserin aut Zhovtan, A. V. verfasserin aut Kopatskaya, E. N. verfasserin aut Larionova, E. G. verfasserin aut Troitskiy, I. S. verfasserin aut Troitskaya, Yu. V. verfasserin aut Shishkina, E. V. verfasserin aut Shkodkina, E. A. verfasserin aut Enthalten in Astrophysical bulletin Pleiades Publishing, 2007 79(2024), 2 vom: Juni, Seite 186-202 (DE-627)546895565 (DE-600)2390996-1 1990-3421 nnns volume:79 year:2024 number:2 month:06 pages:186-202 https://dx.doi.org/10.1134/S1990341323600394 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 79 2024 2 06 186-202 |
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10.1134/S1990341323600394 doi (DE-627)SPR056803559 (SPR)S1990341323600394-e DE-627 ger DE-627 rakwb eng 520 VZ Savchenko, S. S. verfasserin aut The Method of Searching for Rotations of the Polarization Position Angle of Quasars 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2024 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. Morozova, D. A. verfasserin aut Jorstad, S. G. verfasserin aut Blinov, D. A. verfasserin aut Borman, G. A. verfasserin aut Vasilyev, A. A. verfasserin aut Grishina, T. S. verfasserin aut Zhovtan, A. V. verfasserin aut Kopatskaya, E. N. verfasserin aut Larionova, E. G. verfasserin aut Troitskiy, I. S. verfasserin aut Troitskaya, Yu. V. verfasserin aut Shishkina, E. V. verfasserin aut Shkodkina, E. A. verfasserin aut Enthalten in Astrophysical bulletin Pleiades Publishing, 2007 79(2024), 2 vom: Juni, Seite 186-202 (DE-627)546895565 (DE-600)2390996-1 1990-3421 nnns volume:79 year:2024 number:2 month:06 pages:186-202 https://dx.doi.org/10.1134/S1990341323600394 X:SPRINGER Resolving-System lizenzpflichtig Volltext SYSFLAG_0 GBV_SPRINGER SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 79 2024 2 06 186-202 |
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Savchenko, S. S. @@aut@@ Morozova, D. A. @@aut@@ Jorstad, S. G. @@aut@@ Blinov, D. A. @@aut@@ Borman, G. A. @@aut@@ Vasilyev, A. A. @@aut@@ Grishina, T. S. @@aut@@ Zhovtan, A. V. @@aut@@ Kopatskaya, E. N. @@aut@@ Larionova, E. G. @@aut@@ Troitskiy, I. S. @@aut@@ Troitskaya, Yu. V. @@aut@@ Shishkina, E. V. @@aut@@ Shkodkina, E. A. @@aut@@ |
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Savchenko, S. S. |
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Savchenko, S. S. ddc 520 The Method of Searching for Rotations of the Polarization Position Angle of Quasars |
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The Method of Searching for Rotations of the Polarization Position Angle of Quasars |
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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. |
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the method of searching for rotations of the polarization position angle of quasars |
| title_auth |
The Method of Searching for Rotations of the Polarization Position Angle of Quasars |
| abstract |
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. © Pleiades Publishing, Ltd. 2024 |
| abstractGer |
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. © Pleiades Publishing, Ltd. 2024 |
| abstract_unstemmed |
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. © Pleiades Publishing, Ltd. 2024 |
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The Method of Searching for Rotations of the Polarization Position Angle of Quasars |
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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. |
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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. |
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| score |
7.4008274 |