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Evolution of optical spectral index and variability properties of S5 0716+714

We analyze the spectral variability and spectral evolution in the optical en- ergy region by using multiband (BVRI) optical observations of S5 0716+714 spanning 1994 to 2005. The spectrum hardens when the source becomes brighter, which is con- sistent with general BL Lac objects. The spectral evolut...

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Bibliographic Details
Published in:Research in astronomy and astrophysics 2010-02, Vol.10 (2), p.125-134, Article 125
Main Authors: Hao, Jian-Ming, Wang, Bai-Juan, Jiang, Ze-Jun, Dai, Ben-Zhong
Format: Article
Language:English
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Summary:We analyze the spectral variability and spectral evolution in the optical en- ergy region by using multiband (BVRI) optical observations of S5 0716+714 spanning 1994 to 2005. The spectrum hardens when the source becomes brighter, which is con- sistent with general BL Lac objects. The spectral evolution parameter implies that the spectral variability is small in optical bands over 10 years. A simple model represent- ing the variability of a synchrotron component can explain the spectral changes. In addition, we employ the z-transformed discrete correlation function (ZDCF) to ana- lyze the optical multiband flux correlation. The long-term light curve behavior reveals that the variability time scales are 3.5 yr in the B-band, 3.3 yr in the V-band, 3.4 yr in the R-band and 3.5 yr in the/-band. The time lags between any two optical bands were not found when considering statistical errors.
ISSN:1674-4527
2397-6209
DOI:10.1088/1674-4527/10/2/003