(a) Top panel: Full TESS light curve of J0935. Bottom panel: Zoomed-in segment of the TESS light curve over ∼0.25 d, corresponding to the shaded region highlighted in the top panel, shown for clarity. (b) LS, CLEAN, and Period04 power spectra obtained from the combined TESS data. The significant signals are distinctly marked. A zoomed-in plot corresponding to the orbital (Ω), positive superhump (SH+), and prograde disc-precession (${\mathrm{\Omega }}_{\text{pr}}^{\text{+}}$) frequencies is also shown on the right. All observed frequencies in the power spectrum lie above the 95% confidence level, which is represented by the dashed horizontal green line.