Stellar luminosity vs temperature for all TOIs in this work. Intermediate- and low-mass stars are in blue and red, respectively. Intermediate-mass stars hosting planets with candidate status in Table B.1 are indicated with squares. The evolution along the MS is bracketed by the dashed lines, the bottom line being the ZAMS and the top line the end of the MS phase. Representative pre-MS tracks (dotted lines with the corresponding stellar masses indicated) and isochrones at 0, 1 and 3 Myr (green solid lines) are also indicated.