Highest radial orders of pulsation modes with (k, m)=(0, 1) that can theoretically be resolved with a light curve spanning two consecutive TESS sectors (left) or nine TESS sector (right), as a function of the stellar buoyancy travel time Π₀ and rotation frequency ν_rot. It is assumed that the (k, m)=(0, 1) modes do not overlap with any other pulsations, and the effects of aliasing are ignored. The location of HD 112429 is marked by a red square in both panels.