Table 1: Source flux value (20-60 keV), significance, average off-axis angle, and exposure time when IGR J16393-4643 is detected at the 4$\sigma $ level in the mosaic image of a spacecraft revolution. The median MJD of the visibility period is also given in reference to Fig. 4.
Visibility period Exp. Flux Sig. Angle
[Rev.] [MJD] [ks] [counts/s] $[\sigma]$ $[^{\circ}]$
37 52 672 204 0.55 $\pm$ 0.05 12.1 3.8
38 52 675 92 0.93 $\pm$ 0.07 13.7 3.6
47 52 703 153 0.83 $\pm$ 0.06 13.3 7.0
49 52 709 85 0.89 $\pm$ 0.08 11.1 6.2
50 52 712 104 1.05 $\pm$ 0.09 11.6 9.5
51 52 714 76 1.00 $\pm$ 0.14 7.0 11.3
52 52 718 93 0.53 $\pm$ 0.10 5.3 10.1
54 52 724 100 0.96 $\pm$ 0.10 10.0 9.7
55 52 726 96 1.39 $\pm$ 0.14 10.0 11.9
100 52 861 205 0.21 $\pm$ 0.05 4.0 6.9
118 52 915 146 0.75 $\pm$ 0.08 9.4 10.0
168 53 064 28 1.22 $\pm$ 0.22 5.7 11.5
173 53 078 27 1.22 $\pm$ 0.18 6.7 9.3
174 53 081 53 0.60 $\pm$ 0.14 4.5 9.3
233 53 259 72 0.74 $\pm$ 0.10 7.0 9.2


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