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).
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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