Optical Photometrical Observations and Variability for Quasar 4C 29.45
arXiv:astro-ph/0610227 · doi:10.1093/pasj/58.5.797
Abstract
We reported the result of long term optical variability of the blazar 4C 29.45 (QSO 1156+295, Ton 599), carried out optical photometric observations in Johnson V, Cousins RI passbands during April 1997 to March 2002 using the 1.56 meter telescope of the Shanghai Astronomical Observatory (SHAO) at Sheshan, China, compiled the post-1974 optical photometric data of the blazar by combining our new observations with the published optical data, and found maximum variations in different passbands: U = 4.41 mag, B = 5.55 mag, V = 4.53 mag, R = 5.80 mag, and I = 5.34 mag. The average color indices are: UB = 0.18 mag, BV = 0.560.21 mag, BR = 0.930.18 mag, BI = 1.510.24 mag, VR = 0.440.15 mag and VI = 1.030.23 mag. The post-1974 data give us an excellent opportunity to search for the existence of possible periodicity in the light curve. In search for periodicity in the R passband light curve, we performed Jurkevich test and power spectral (Fourier) analysis methods, and CLEANest algorithms to remove false signals. We found possible periods of 3.55 and 1.58 years. The possible mechanism for the periodic variability was discussed.
12 pages, 9 figures, 5 tables; PASJ in press
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- On the geometrical origin of periodicity in blazar-type sources
- A relativistic helical jet in the gamma-ray AGN 1156+295
- The binary black hole scenario for the BL Lacertae object AO 0235+16
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