Robust fit of the Kepler light curves. Q0 is from 953.53825 to 963.24461, Q1 from 964.51154 to 997.98296, and Q2 from 1002.76455 to 1091.46678. The solid line is the best fit of the first solution. The residuals, shown at the top, are ± 2.36 mmag. The gaps are artificially bridged by straight connecting lines.
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