Long-term Variability Properties of Mkn501

Optical photometric observations at the I and R wavebands were carried out towards Mkn501 using the 1.56 meter optical telescope of Shanghai Astronomical Observatory at Sheshan. Combining our new observations with the published historical data, we have obtained the light curves of Mkn501 at the optical, infrared and radio wavebands with a time coverage of nearly 80 years. The relationship between the light variability and the color index is discussed, it is found that a strong correlation exists between the color indices (B − V) and (B − R), with the correlation coefficient reaching r = 0.73. The correlations of multi-band light variabilities are analyzed by the DCF method, it is found that certain positive correlations of B-band light variability with the 4.8 GHz and infrared light variabilities exist. And the spectral analysis on the B-band light curve with the CLEANest method indicates that the light curve of Mkn501 contains probably two periodical components of (10.06 ± 0.04) yr and (21.60 ± 0.17) yr.