Fig. 1.

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LCOGT MuSCAT3 light curves of K2-399. The light curves from top to bottom are in the MuSCAT g, r, i, and zs bands. The small symbols show the unbinned data and the larger symbols show the same data in ten-minute bins. The transit model fits are overplotted. A V-shaped event was detected on-target with depths at mid-transit of 0.18, 0.48, 1.21, and 2.28 ppt in g, r, i, and zs bands, respectively, indicating that a fainter, much redder star is blended in the 5.1 arcsec follow-up photometric aperture and is hosting the eclipse.
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