A ionized reflecting skin above the accretion disk of GX 349+2

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Table 2:

Percentage of photon pile-up at different energies.
Energy	Pile-up (%)	Pile-up (%)
(keV)	RAWX [29:45]	RAWX [29:36] and RAWX[39:45]
5	$1.3 \pm 0.1$	$0.2 \pm 0.2$
6	$2.0 \pm 0.1$	$0.6 \pm 0.2$
7	$3.2 \pm 0.2$	$1.6 \pm 0.2$
8	$5.1 \pm 0.3$	$1.9 \pm 0.4$
9	$7.4 \pm 0.4$	$4.8 \pm 0.5$
10	$9.8 \pm 0.6$	$6.5 \pm 0.8$

Note. The associated errors are reported at 1 $\sigma$ . In the first column we report the energies, in the second and third column the estimated percentage of photon pile-up, extracting the events from the whole source region and excluding the brightest columns at RAWX =37 and RAWX =38, respectively.

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