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Table 1.

Log of all observations used in this paper.

OBSID Target TSTART TSTOP Exp. (a) Flux (b) EHR
(UTC) (UTC) (ks) (10−12 cgs) (keV)
0823990201 IGR J18483−0311 2019-04-07 03:40:03 2019-04-07 13:33:11 23.3 47.9 3.0
0823990301 IGR J11215−5952 2018-12-30 12:46:57 2018-12-30 20:50:37 17.1 < 0.006 (c)
0823990401 IGR J16418−4532 2019-02-21 06:06:15 2019-02-21 12:37:19 16.3 41.9 3.5
0823990501 AX J1949.8+2534 2018-10-25 17:40:29 2018-10-26 01:47:21 22.3 0.8 3.72
0823990601 IGR J16479−4514 2018-08-28 06:19:06 2018-08-28 14:01:46 9.3 13.3 4
0823990801 IGR J18462−0223 2018-10-21 17:00:27 2018-10-2 15.3 0.2 3.5
0823990901 IGR J16328−4726 2018-09-18 15:26:40 2018-09-18 22:02:40 14.3 2.2 4
0823991001 SAX J1818.6−1703 2019-03-13 17:04:48 2019-03-13 23:24:12 18.9 3.0 4
0844100101 IGR J18410−0535 2019-10-18 17:52:09 2019-10-18 23:21:30 17.0 < 0.02 (c)
0844100701 IGR J18450−0435 2019-09-27 08:37:04 2019-09-27 16:49:43 24.0 2.7 3.5

Notes. We reported for completeness the total available exposure time for each observation after the application of the good time intervals, the estimated flux of time averaged spectra, as well as the energy EHR used to separate the soft and high-energy bands in the computation of the HR (see Sect. 2.1 for details).

(a)

EPIC-pn exposure after filtering.

(b)

Absorbed flux in the 1–10 keV energy band.

(c)

We set an upper limit at 90% confidence level on the unabsorbed flux, as the target is not detected in this observation. See Sect. 2.3 for details on the computation.

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