Table 3: The excess variances of the 300 s binned light curves.
Obs. period $\sigma^2_{\rm rms}$

( $\times 10^{-3}$ )

[0.2-0.8] keV [0.8-2.4] keV [2.4-10] keV [0.2-10] keV

4-11(1) $0.33\pm0.15$ $0.39\pm0.30$ $2.53\pm2.00$ $0.35\pm0.15$

4-11(2) $0.76\pm 0.19$ $1.23\pm0.40$ $3.59\pm1.91$ $0.78\pm0.17$

14-11 $21.14\pm 2.24$ $40.96\pm4.33$ $86.95\pm 10.04$ $32.76\pm3.46$

1-12 $0.77\pm0.08$ $1.73\pm0.16$ $4.02\pm0.43$ $1.07\pm0.10$

**Table 3:** The excess variances of the 300 s binned light curves.
Obs. period	$\sigma^2_{\rm rms}$
	( $\times 10^{-3}$ )
	[0.2-0.8] keV	[0.8-2.4] keV	[2.4-10] keV	[0.2-10] keV
4-11(1)	$0.33\pm0.15$	$0.39\pm0.30$	$2.53\pm2.00$	$0.35\pm0.15$
4-11(2)	$0.76\pm 0.19$	$1.23\pm0.40$	$3.59\pm1.91$	$0.78\pm0.17$
14-11	$21.14\pm 2.24$	$40.96\pm4.33$	$86.95\pm 10.04$	$32.76\pm3.46$
1-12	$0.77\pm0.08$	$1.73\pm0.16$	$4.02\pm0.43$	$1.07\pm0.10$

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