Fig. 2
Left panel: the large systematic noise is clearly visible on the raw light curve of EPIC 201465501, a 14.95 magnitude star in Campaign 1. Right panel: same light curve after being position-decorrelated. The improvement of the precision is evident, the RMS improved from 1358 ppm for the RAWLC to 417 ppm for the DECLC, allowing to clearly see the transits.
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