Same as Fig. 2. HD 150562 has no clear rotation variation, but obvious roAp variations around 133.7 d⁻¹, which were discovered by Martinez & Kurtz (1992). HD 151860 was discovered to be a multi-periodic roAp star by Kochukhov et al. (2013) with radial velocity variations in Lanthanide lines with a highest amplitude peak near 117 d⁻¹. The TESS photometry shows a highest amplitude pulsation peak at 73.4 d⁻¹ and a second peak at 117.8 d⁻¹, similar to the peak found in radial velocities. Photometry and radial velocities sample different depths in the atmospheres of roAp stars where different mode amplitudes are found, thus there is no inconsistency between the photometric results and the radial velocity study. Simultaneous radial velocity studies with TESS photometry would be synergistic in extracting more astrophysical understanding from these stars.