Table 1: XMM-Newton observation log. The EPIC modes are Full Frame (FF) and Timing (TI). In the March 17, 2003 observation IGR J17544-2619 was outside the OM field of view. The effective wavelengths of the UVW1, UVW2 and UVM2 filters are 2945 Å, 2180 Å, and 2340 Å, respectively.
Obs. Start time End time Exposure (ks) EPIC mode OM

(UTC) (UTC) pn MOS pn MOS1 MOS2 Exp (ks) Filter

1 2003 Mar. 17 20:53 Mar. 18 00:33 10.2 11.9 FF FF FF ... ...

2 2003 Sep. 11 17:54 Sep. 11 22:09 9.3 11.0 FF FF FF 2.2, 3.2 B, UVW1

3 2003 Sep. 17 17:13 Sep. 17 19:59 2.5 8.3 TI TI FF 1.8, 1.6 UVM2, UVW2

**Table 1:** XMM-Newton observation log. The EPIC modes are Full Frame (FF) and Timing (TI). In the March 17, 2003 observation IGR J17544-2619 was outside the OM field of view. The effective wavelengths of the *UVW*1, *UVW*2 and *UVM*2 filters are 2945 Å, 2180 Å, and 2340 Å, respectively.
Obs.	Start time	End time	Exposure (ks)	EPIC mode	OM
	(UTC)	(UTC)	pn	MOS	pn	MOS1	MOS2	Exp (ks)	Filter
1	2003 Mar. 17 20:53	Mar. 18 00:33	10.2	11.9	FF	FF	FF	...	...
2	2003 Sep. 11 17:54	Sep. 11 22:09	9.3	11.0	FF	FF	FF	2.2, 3.2	B, UVW1
3	2003 Sep. 17 17:13	Sep. 17 19:59	2.5	8.3	TI	TI	FF	1.8, 1.6	UVM2, UVW2

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