Table 3: Summary of the UVOT observations of the three sources. The magnitudes are not corrected for Galactic reddening (Schlegel et al. 1998).
Source Filter $T_{\rm exp}$ Magnitude

IGR J18249-3243 UVW2 4727 $17.53\pm0.02$

IGR J19443+2117 V 907 >20.3 (3 $\sigma$ ul)

B 907 >21.2 (3 $\sigma$ ul)

U 907 >20.8 (3 $\sigma$ ul)

UVW1 1826 >21.2 (3 $\sigma$ ul)

UVM2 2518 >21.5 (3 $\sigma$ ul)

UVW2 1417 >21.3 (3 $\sigma$ ul)

IGR J22292+6647 UVW1 11516 >21.83 (3 $\sigma$ ul)

UVM2 461 >20.41 (3 $\sigma$ ul)

UVW2 5179 >21.64 (3 $\sigma$ ul)

**Table 3:** Summary of the UVOT observations of the three sources. The magnitudes are not corrected for Galactic reddening (Schlegel et al. 1998).
Source	Filter	$T_{\rm exp}$	Magnitude
IGR J18249-3243	UVW2	4727	$17.53\pm0.02$
IGR J19443+2117	V	907	>20.3 (3 $\sigma$ ul)
	B	907	>21.2 (3 $\sigma$ ul)
	U	907	>20.8 (3 $\sigma$ ul)
	UVW1	1826	>21.2 (3 $\sigma$ ul)
	UVM2	2518	>21.5 (3 $\sigma$ ul)
	UVW2	1417	>21.3 (3 $\sigma$ ul)
IGR J22292+6647	UVW1	11516	>21.83 (3 $\sigma$ ul)
	UVM2	461	>20.41 (3 $\sigma$ ul)
	UVW2	5179	>21.64 (3 $\sigma$ ul)

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