Fig. 10.
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Centroid frequency, FWHM, and phase lags at the centroid frequency of the Lorentzian accounting for the dip in the real part of the cross spectrum of Swift J1727.8–1613 as a function of the QPO frequency. The lags are for the HE 28–200 keV with respect to the LE 2–10 keV data, and were obtained using the Gaussian phase-lag model.
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