Time Lag Between the Optical Continuum and Line Variabilities of NGC 4151
Using a long term spectroscopic observation of NGC 4151 (obtained with 6 m telescope of SAO Russia, between 1996 and 2006) we used Z-Transfomed Discrete Correlation Function (ZDCF) to find the time lag between the broad Hbeta and Halpha lines and the optical continuum variably.
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