Fig. 26
Top: detected period against detection efficiency for all hot Jupiter populations around M dwarfs (divided by red lines). One can see two gaps at 1.6 and 4.0 days, resulting from our alias detection removal (blue arrows). Bottom: histogram of stellar radius against detection efficiency. We combined the results from the M dwarf VHJ simulation and the VHJ simulations for hotter dwarf stars (divided by red line).
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