Bayesian timing analysis of giant flare of SGR 180620 by RXTE PCA

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Table 1

Detected QPO frequencies not reported in the literature (Israel et al. 2005; Watts & Strohmayer 2006; Strohmayer & Watts 2006).

f_QPO [Hz]	Time intervals	Lorentzian	FWHM [Hz]
(68% credible region)	of QPOs^a	centroids [Hz]

16.88^b (16.87−16.90)	259.4−267.1	16.90 ± 0.004	0.12
21.36^b (21.35−21.38)	244.3−251.9	21.34 ± 0.003	0.35
36.84^b (36.83−36.88)	183.8−191.2	36.88 ± 0.004	0.24
59.04(58.58−59.28)	146.0−176.2	−	−
61.26(61.25−61.27)	251.9−395.6	−	−
116.27(116.24−116.28)	168.7−198.9	−	−

Notes.

^(a)

Giant Flare onset time is set to 0.

^(b)

Highly significant detection (for details, see text).

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