Transit depth vs. revolution period for planets in the simulated yield of TESS over the whole sky (Sullivan et al. 2015, gray circles). Planet candidates with sizes ≤5R_⊕, transit depths ≥1 mmag, and periods ≥9.1 days located ≥20° away from the ecliptic poles (i.e., with <3 transits) are shown as orange dots. Those candidates are further distinguished based on their host star magnitude: stars with V ≤ 14 (orange red), V ≤ 12 (red), and V ≤ 10 (dark red). HD 106315c is represented by the blue dot.