Fig. 6.
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LS, CLEAN, and Period04 power spectra of J130559 obtained from the TESS data for (a) sector 64 and (b) sector 65. The significant signals are distinctly marked. A zoomed-in plot corresponding to the orbital (Ω), negative superhump (SH−), and retrograde disc-precession (
) frequencies is also shown on the right. All observed frequencies in the power spectra lie above the 95% confidence level, which is represented by the dashed horizontal green line.
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