CCD PHOTOMETRIC MONITORING OF THE BL LACERTAE OBJECT S5 0716+714 FROM 2001 TO 2006
CCD PHOTOMETRIC MONITORING OF THE BL LACERTAE OBJECT S5 0716+714 FROM 2001 TO 2006
复制标题
DOI：
10.1088/0004-6256/136/5/1846
复制
发表时间：
2008-09
期刊：
影响因子：
--
通讯作者：
X. Zhang;Y. Zheng;H. Zhang;Y. Liu;Y. Wen;W. Wang
中科院分区：
文献类型：
--
作者：
X. Zhang;Y. Zheng;H. Zhang;Y. Liu;Y. Wen;W. Wang
本文给出了2001年2月至2006年4月用云南天文台1m望远镜和上海天文台1.56m望远镜观测的BLLac天体S50716+714(z>；0.3)的B、V、R和I的光学光度学特性。我们的结果显示出显著的快速变化，并呈现出短时间变化，28分钟内ΔI=0.60MAG，23分钟内ΔR=1.58MAG，10分钟内ΔV=1.06MAG，33分钟内ΔB=1.36MAG。我们发现V−R颜色指数与292min的震级有很强的相关性。我们对S50716+714的CCD测光表明，它们与Raiteri等人和钱等人有很好的相似性。给出了1994-2001年的光学变率、震级和光强曲线。
We present the optical photometries (B, V, R, and I) of the BL Lac object S5 0716+714 (z > 0.3), which were observed with the 1 m telescope at Yunnan Astronomical Observatory and the 1.56 m telescope at Shanghai Astronomical Observatory from 2001 February to 2006 April. Our results show a significant rapid variation and exhibit a short time variability of ΔI = 0.60 mag in 28 minutes, ΔR = 1.58 mag in 23 minutes, ΔV = 1.06 mag in 10 minutes, and ΔB = 1.36 mag in 33 minutes. We find a strong correlation between the V − R color index and the magnitude in 292 minutes. Our CCD photometry of the S5 0716+714 showed they are in good similitude with Raiteri et al., and Qian et al. presented the optical variability magnitude and light curves from 1994 to 2001.