Here we provide some additional figures as supporting material to Knudstrup et al. (2024). Phase-folded light curves: The best-fitting models are shown as the white line in the top panel and the residuals are given in the bottom panel. HD 118203 b: TESS 2 min. cadence data shown as gray points with error bars. Black markers are binned data in ~10 min. intervals. HD 149193 b: TESS light curves 20 sec., 2 min., and 30 min. cadence data are shown in light gray, gray, and black, respectively. K2-261 b: K2 light curve in black, TESS 20 sec. and 2 min. in light gray and gray, respectively. A light curve for each passband is shown. K2-287 b: K2 30 min cadence shown in orange with CHEOPS 1 min. and ground-based 2 min. observations in light gray and gray, respectively. A light curve for each passband is also shown with a matching color. KELT-3 b: TESS 2 min. cadence data shown in gray. KELT-4Ab: TESS 2 min. cadence data shown in gray. LTT 1445Ab: Black TESS 2 min. and gray TESS 20 sec. TOI-451Ab: Unbinned 2 min. cadence data are shown in gray and in black the binned (~6 min.) data are shown. TOI-813 b: TESS 20 sec., 2 min., and 30 min. cadence data are shown in light gray, gray, and black, respectively. TOI-892 b: TESS 2 min. and 30 min. cadence data are shown in gray and black, respectively. TOI-1130 c: TESS 20 sec. and 30 min. cadence data shown in gray and black, respectively. WASP-50 b: TESS 20 sec. and 2 min. cadence data shown in gray and black, respectively. WASP-59 b: TESS 2 min. cadence data shown in gray and ground-based 2 min. KeplerCam photometry in orange. WASP-136 b: TESS 20 sec. and 2 min. cadence data shown in gray and black, respectively. WASP-172 b: TESS 20 sec. and 30 min. cadence data shown in gray and black, respectively. WASP-173Ab: TESS 20 sec. and 2 min. cadence data shown in gray and black, respectively. WASP-186 b: TESS 20 sec., 2 min., and 30 min. cadence data are shown in light gray, gray, and black, respectively. XO-7 b: TESS 20 sec., 2 min., and 30 min. cadence data are shown in light gray, gray, and black, respectively. WASP-148 b: The MuSCAT-2 photometry obtained simultaneous with our spectroscopic transit observations. The observations in the different griz filters are shown as blue, orange, green, and red markers, respectively. WASP-26 b: Unbinned 20 sec. cadence data from TESS are shown in gray and in black the binned (~6 min.) data are shown. Peak of the stacked CCFs: Similar to Fig. A.8. we show the peaks of the stacked CCFs for KELT-4 and XO-7 created by assuming the best-fitting value of b from the RV-RM fit. KELT-4A: The gray contours show a peak around (v sin i⋆,λ)=(6.0 km/s,90 deg). The red contours are the same as created from the posterior shown to the right in Fig. A.9. XO-7: The gray contours show a peak around (v sin i⋆,λ)=(4 km/s,-60 deg). The red contours are the same as created from the posterior shown to the right in Fig. A.28. References: Knudstrup, E., Albrecht, S. H., Winn, J. N., et al., 2024, arXiv:2408.09793