QPO frequency in Swift J1727.8-1613 shows a two-branch correlation with disk luminosity, negative below about 3 Hz and positive above.
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Temporal evolution of quasi-periodic oscillations in an accreting black hole Swift J1727.8-1613: coevolution of the disk-corona during the state transition
QPO frequency in Swift J1727.8-1613 shows a two-branch correlation with disk luminosity, negative below about 3 Hz and positive above.