Kepler light-curve analysis of the blazar W2R 1926+42
Kepler light-curve analysis of the blazar W2R 1926+42
We study the long term Kepler light curve of the blazar W2R 1926+42 ($\sim$ 1.6 years) which indicates a variety of variability properties during different intervals of observation. The normalized excess variance, $F_{\rm var}$ ranges from 1.8 % in the quiescent phase and 43.3 % in the outburst phase. We …