Fig. 1.

2D domain of orbital period and planet size, on a logarithmic scale. Red circles show the 603 detected planets in our survey of 42,557 bright Sun-like stars (Kp = 10–15 mag, GK spectral type). The color scale shows survey completeness measured by injection and recovery of synthetic planets into real photometry. Dark regions represent (P, R_P) with low completeness, C, where significant corrections for missed planets must be made to compute occurrence. The most common planets detected have orbital and (at middle left of graph). However, their detectability is favored by orbital tilt and detection completeness, C, that favors detection of such close-in, large planets.