**Table 9:** Summary of the statistical comparison of the 2XMM fluxes from the EPIC cameras.
Energy band	pn-M1	${N_{\rm pn-M1}}$	pn-M2	${N_{\rm pn-M2}}$	M2-M1	${N_{\rm M2-M1}}$
[keV]	[%]		[%]		[%]
(1)	(2)	(3)	(4)	(5)	(6)	(7)
0.2-0.5	$4.9 \pm 1.2$	785	$8.4 \pm 0.9$	771	$-0.9 \pm 0.6$	987
0.5-1.0	$-2.4 \pm 0.3$	1906	$-2.7 \pm 0.2$	1957	$1.0 \pm 0.3$	2384
1.0-2.0	$-7.6 \pm 0.3$	2394	$-8.6 \pm 0.3$	2461	$0.6 \pm 0.2$	2932
2.0-4.5	$-6.1 \pm 0.3$	1311	$-5.4 \pm 0.3$	1342	$-0.8 \pm 0.2$	1552
4.5-12.0	$-12.4\pm0.7$	387	$-9.5\pm0.6$	408	$-3.2\pm0.4$	441

(1): energy band definition in keV; (2) and (3): difference (in %) in the measured flux in pn and M1 and number of sources used in the comparison; (4) and (5): same as Cols. (2) and (3) but for pn and M2; (6) and (7): same as Cols. (2) and (3) but for M2 and M1.

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