Fig. 2.
Fraction of detected, simulated and injected transiting objects as a function of their orbital period. Aliases of the 100 min orbital period of CHEOPS are visible as drops in detection efficiency near integer multiples of 100 min. The upper limit of the shaded region represents the fraction of objects detected for the brightest white dwarf in the sample, and the lower limit marks the detection fraction for the faintest white dwarf.
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