Fig. 8
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Spectrum reconstruction under large systematic noise. Panels a, c, and e show the reconstructed spectra of planet P1, planet P2, and planet P3 only through the SVD process. Panels b, d, and ſ show the spectra of planet P1, planet P2, and planet P3 reconstructed through subtracting the stellar leak from the demodulated signal before the SVD method. The OPD rms error was set to 7.5 nm for both the two cases.
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