Swift J1727.8-1613 shows a dip at 3 to 15 Hz in the real part of its high-energy cross spectrum, with hard X-ray photons lagging soft photons by between pi/2 and pi.
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Timing analysis of the black-hole candidate Swift J1727.8-1613: detection of a dip-like feature in the high-energy cross spectrum
Swift J1727.8-1613 shows a dip at 3 to 15 Hz in the real part of its high-energy cross spectrum, with hard X-ray photons lagging soft photons by between pi/2 and pi.