Photometric Monitoring of Blazar 3C 66A with the Yunnan University Astronomical Observatory 1 m Telescope

• Published in: Research in astronomy and astrophysics Vol. 23; no. 4; pp. 45014 - 45029
• Main Authors: Zeng, Wei, Wen, Tao, Gong, Zhen-Lu, Chen, Shi, Wu, Fan, Zhang, Hao-Yang, Dai, Ben-Zhong
• Format: Journal Article
• Language: English
• Published: Beijing National Astromonical Observatories, CAS and IOP Publishing 01.04.2023; IOP Publishing
• Subjects: (galaxies:) BL Lacertae objects: individual (3C 66A); Correlation; galaxies: active; galaxies: photometry; Monitoring; Observatories; Photometry; Variability; China; Yunnan China
• ISSN: 1674-4527; 2397-6209
• DOI: 10.1088/1674-4527/acc29a

Abstract 3C 66A is one of our first batches of photometric monitoring objects with the 1 m optical telescope at Yunnan University Astronomical Observatory. In the present work, the observational campaign was performed from 2021 November 1 to 2022 February 27 in the Johnson–Morgan system V and R bands. The average magnitudes in each band were V ¯ = 15.52 ± 0.18 mag and R ¯ = 15.07 ± 0.17 mag. The overall variability amplitudes were Δ V = 0.ͫ74, Amp = 70.27% and Δ R = 0.ͫ72, Amp = 68.56%, respectively. Most of the intraday variabilities (IDVs) occurred in 2021 December and 2022 February. The minimal rise/decay timescale was about 6 minutes (5.82 ± 2.74 minutes and 6.18 ± 2.81 minutes on 2022 February 11, 6.99 ± 3.70 minutes and 6.17 ± 2.91 minutes on 2022 February 12). Durations of these rapid variabilities were from 11.99 to 179.67 minutes. The discrete correlation function analyses between V and R bands showed significantly correlated variability. Color index analysis of IDVs showed that the spectrums do not change with variabilities.