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Fig. 4
Two additional transits with different levels of completeness for USco16m25. We observed the system on the night of 18 May and 11 June 2015 in the SDSSi filter with IAC80/CAMELOT. The red line corresponds to the best-fit model to the global set of data (light curves, photometric transits, and radial velocities).
This figure is made of several images, please see below:
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