Fig. 3
Photometric errors of the individual K2 asteroid measurements in the M35 field as a function of the apparent brightness of the asteroids (light blue dots). The red line plots the Kepler preflight estimate of the photometric precision (Van Cleeve & Caldwell 2016)2, the purple line shows the scaled Combined Differential Photometric Precision data (Christiansen et al. 2013), the black line represents the photometry of a faint RR Lyrae star in Leo IV for comparison (Molnár et al. 2015), and the dashed line shows the linear interpolation between the last two.
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