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• W2158686925 abstract "We report B, V, and R band CCD photometry of the Seyfert galaxy NGC 4151 obtained with the 1.0-m telescope at Weihai Observatory of Shandong University and the 1.56-m telescope at Shanghai Astronomical Observatory from 2005 December to 2013 February. Combining all available data from literature, we have constructed a historical light curve from 1910 to 2013 to study the periodicity of the source using three different methods (the Jurkevich method, the Lomb-Scargle periodogram method and the Discrete Correlation Function method). We find possible periods of P_1=4pm0.1, P_2=7.5pm0.3 and P_3=15.9pm0.3 yr." @default.
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• W2158686925 date "2014-07-23" @default.
• W2158686925 modified "2023-10-16" @default.
• W2158686925 title "Optical monitoring of the Seyfert galaxy NGC 4151 and possible periodicities in its historical light curve" @default.
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• W2158686925 doi "https://doi.org/10.1088/1674-4527/14/8/003" @default.
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