PKS 2155-304 is a well studied BL Lac object in the southern sky. The historical optical data during different periods have been collected and compiled. Light curves spanning 35 yr have been constructed. The R-band light curve has been analyzed by means of three methods: the epoch folding method, the Jurkevich method and the discrete correlation function method. It is derived that there is an evident periodic component of 317 d (i.e. 0.87 yr) superposed on a long-term trend with largeamplitude variation in the light curve. The variability of this source is accompanied by a slight color variation, and the brightness and color index are correlated with each other. On a long-term time scale, PKS 2155-304 exhibits a tendency of bluer-when brighter, which means the spectrum becomes flatter when the source brightens. © 2014 National Astronomical Observatories of Chinese Academy of Sciences and IOP Publishing Ltd.
CITATION STYLE
Zhang, B. K., Zhao, X. Y., Wang, C. X., & Dai, B. Z. (2014). Optical quasi-periodic oscillation and color behavior of blazer PKS 2155-304. Research in Astronomy and Astrophysics, 14(8), 933–941. https://doi.org/10.1088/1674-4527/14/8/004
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