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Optical Photometric Observations of 7-Ray Loud Blazars
引用本文:O. M. Kurtanidze,M. G. Nikolashvili,A. C. Gupta. Optical Photometric Observations of 7-Ray Loud Blazars[J]. 中国天文和天体物理学报, 2004, 0(2)
作者姓名:O. M. Kurtanidze  M. G. Nikolashvili  A. C. Gupta
作者单位:Abstumani Observatory,383762 Abstumani,Republic of Georgia,Abstumani Observatory,383762 Abstumani,Republic of Georgia,Harish-Chandra Research Institute,Chhatnag Road,Jhunsi,Allahabad - 211019,India,Landessternwarte Heidelberg-Koenigshtuhl,D-69117,Heidelberg,Germany Astrophysikalisches Institute Potsdam,An der Sternwarte 16,D-14482,Germany
基金项目:Supported by the National Natural Science Foundation of China
摘    要:We report results of our optical photometric observations of ten gamma-ray loud blazers, namely: 0219+428 (3C66A), PKS 0420-014 (OA 129), S5 0716+714, 0754+100 (OI 090.4), 0827+243 (OJ248), 1652+398 (Mrk 501), 2200+420 (BL Lacertae), 2230+114 (CTA 102), 2251+158 (3C 454.3) and 2344+514. The observations were carried out in September-October, 2000 using the 70 cm optical telescope at Abstumani Observatory, Georgia. We found intra-day variations in 0420-014, S5 0716+714, BL Lacertae and CTA 102. A variation of 0.3 magnitude over a time scale of about 3 hours was observed in the R passband in BL Lacertae on JD 2451827. We did not detect any variation in 3C 66A, Mrk 501, or 3C 454.3 during our observations. Nor did we detect any clear evidence of variation in 1ES 2344+514 during our two weeks' observing run of the TeV gamma-ray source.


Optical Photometric Observations of 7-Ray Loud Blazars
Jun-Hui Fan,O. M. Kurtanidze,M. G. Nikolashvili,A. C. Gupta,Jiang-Shui Zhang and Yu-Hai YuanCenter for Astrophysics,Guangzhou University,Guangzhou , fjh@gzhu.edu.cnAbstumani Observatory, Abstumani,Republic of GeorgiaLandessternwarte Heidelberg-Koenigshtuhl,D-,Heidelberg,GermanyAstrophysikalisches Institute Potsdam,An der Sternwarte ,D-,GermanyHarish-Chandra Research Institute,Chhatnag Road,Jhunsi,Allahabad - ,India, agupta@mri.ernet.in. Optical Photometric Observations of 7-Ray Loud Blazars[J]. Chinese Journal of Astronomy and Astrophysics, 2004, 0(2)
Authors:Jun-Hui Fan  O. M. Kurtanidze  M. G. Nikolashvili  A. C. Gupta  Jiang-Shui Zhang  Yu-Hai YuanCenter for Astrophysics  Guangzhou University  Guangzhou    fjh@gzhu.edu.cnAbstumani Observatory   Abstumani  Republic of GeorgiaLandessternwarte Heidelberg-Koenigshtuhl  D-  Heidelberg  GermanyAstrophysikalisches Institute Potsdam  An der Sternwarte   D-  GermanyHarish-Chandra Research Institute  Chhatnag Road  Jhunsi  Allahabad -   India   agupta@mri.ernet.in
Affiliation:Jun-Hui Fan,O. M. Kurtanidze,M. G. Nikolashvili,A. C. Gupta,Jiang-Shui Zhang and Yu-Hai YuanCenter for Astrophysics,Guangzhou University,Guangzhou 510400, fjh@gzhu.edu.cnAbstumani Observatory,383762 Abstumani,Republic of GeorgiaLandessternwarte Heidelberg-Koenigshtuhl,D-69117,Heidelberg,GermanyAstrophysikalisches Institute Potsdam,An der Sternwarte 16,D-14482,GermanyHarish-Chandra Research Institute,Chhatnag Road,Jhunsi,Allahabad - 211019,India, agupta@mri.ernet.in
Abstract:We report results of our optical photometric observations of ten gamma-ray loud blazers, namely: 0219+428 (3C66A), PKS 0420-014 (OA 129), S5 0716+714, 0754+100 (OI 090.4), 0827+243 (OJ248), 1652+398 (Mrk 501), 2200+420 (BL Lacertae), 2230+114 (CTA 102), 2251+158 (3C 454.3) and 2344+514. The observations were carried out in September-October, 2000 using the 70 cm optical telescope at Abstumani Observatory, Georgia. We found intra-day variations in 0420-014, S5 0716+714, BL Lacertae and CTA 102. A variation of 0.3 magnitude over a time scale of about 3 hours was observed in the R passband in BL Lacertae on JD 2451827. We did not detect any variation in 3C 66A, Mrk 501, or 3C 454.3 during our observations. Nor did we detect any clear evidence of variation in 1ES 2344+514 during our two weeks' observing run of the TeV gamma-ray source.
Keywords:galaxies: active - Blazars: individual: PKS 0219+428 (3C 66A)   PKS 0420-014 (OA129)   S5 0716+714   0754+100 (OI090.4)   0827+243 (OJ248)   1652+398 (Mrk 501)   2200+420 (BL Lacertae)   2230+114 (CTA102)   2251+158 (3C 454.3)   and 1ES 2344+514 - galax
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