Table 1: The INTEGRAL Data set. We selected all public and core programme revolutions when IGR J17252-3616 was within the ISGRI PCFOV of $29\hbox {$^\circ $ }\times 29 \hbox {$^\circ $ }$ . The observing time fraction was calculated as the ratio between the net exposure time on the source and the elapsed time during the visibility periods.
Visibility periods Start End Revolutions Observing time fraction

[MJD] [MJD]

1 52671 52752 37-63 0.23

2 52859 52925 100-121 0.51

3 53050 53116 164-185 0.20

4 53236 53294 226-244 0.16

**Table 1:** The *INTEGRAL* Data set. We selected all public and core programme revolutions when IGR J17252-3616 was within the ISGRI PCFOV of $29\hbox {$^\circ $ }\times 29 \hbox {$^\circ $ }$ . The observing time fraction was calculated as the ratio between the net exposure time on the source and the elapsed time during the visibility periods.
Visibility periods	Start	End	Revolutions	Observing time fraction
	[MJD]	[MJD]
1	52671	52752	37-63	0.23
2	52859	52925	100-121	0.51
3	53050	53116	164-185	0.20
4	53236	53294	226-244	0.16

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