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Fig. 7

image

Phase coverage (in percent) as a function of orbital period reached after one season of observations with CHEOPS. From top to bottom panel: HD 149382 (7 × 2 orbits), CW83 1419-09 (4 × 3 orbits), TYC 982-614-1 (6 × 3 orbits), and TYC 499-2297-1 (6 × 2 orbits). In all cases, the blue lines represent the full range of 5000 periods we explored, and the orange lines show the binning at each ~1.7 h. The orbital periods for which the phase coverages are ~80% are marked with dotted vertical red lines.

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