Open Access
Table B.2.
Same as Table B.1 but for 2023, when the soft-intermediate state lasted the longest.
| Date | HJD | Exposure time | Orbital phase ϕ | sstar for He II | FX | Instrument |
|---|---|---|---|---|---|---|
| [UT] | [ks] | [photons s−1 cm−2] | ||||
| 2023-04-28 00:25:23.923 | 2460062.52 | 3.6 | 0.915 | 1.4166 | 2.6443 | OES |
| 2023-04-28 01:39:40.176 | 2460062.57 | 3.6 | 0.925 | CCD700 | ||
| 2023-05-05 00:13:28.618 | 2460069.51 | 3.6 | 0.164 | 0.9450 | 2.3452 | OES |
| 2023-05-05 01:00:18.778 | 2460069.54 | 3.6 | 0.170 | CCD700 | ||
| 2023-05-25 00:42:36.144 | 2460089.53 | 3.6 | 0.740 | 0.6029 | 3.0157 | OES |
| 2023-05-25 01:45:36.317 | 2460089.58 | 1.8 | 0.747 | CCD700 | ||
| 2023-06-18 23:16:06.787 | 2460114.47 | 3.6 | 0.193 | CCD700 | ||
| 2023-06-19 00:20:54.960 | 2460114.52 | 3.6 | 0.201 | 0.8110 | 3.0874 | OES |
| 2023-06-29 20:33:27.302 | 2460125.36 | 3.6 | 0.137 | CCD700 | ||
| 2023-06-29 21:39:06.451 | 2460125.40 | 3.6 | 0.145 | 0.8851 | 2.6557 | OES |
| 2023-07-03 21:50:18.557 | 2460129.41 | 3.6 | 0.861 | CCD700 | ||
| 2023-07-03 22:54:26.726 | 2460129.45 | 3.6 | 0.869 | 0.5505 | 2.4501 | OES |
| 2023-07-04 01:23:38.976 | 2460129.56 | 2.6 | 0.888 | CCD700 | ||
| 2023-07-06 20:59:13.085 | 2460132.38 | 4.2 | 0.391 | CCD700 | ||
| 2023-07-06 22:13:53.184 | 2460132.43 | 4.2 | 0.400 | 0.7407 | 2.3463 | OES |
| 2023-07-15 20:25:37.805 | 2460141.35 | 3.6 | 0.993 | 0.7209 | 2.1947 | OES |
| 2023-07-15 21:42:25.862 | 2460141.41 | 3.6 | 0.003 | CCD700 | ||
| 2023-09-08 18:37:35.472 | 2460196.28 | 3.6 | 0.801 | 1.2337 | 1.0473 | OES |
| 2023-09-08 19:52:22.310 | 2460196.33 | 3.6 | 0.811 | CCD700 | ||
| 2023-09-10 19:12:33.869 | 2460198.30 | 3.6 | 0.163 | CCD700 | ||
| 2023-09-10 20:57:30.614 | 2460198.38 | 3.6 | 0.176 | 0.9174 | 1.1046 | OES |
| 2023-09-15 23:13:17.270 | 2460203.47 | 3.6 | 0.086 | CCD700 | ||
| 2023-09-16 00:31:47.107 | 2460203.52 | 3.6 | 0.095 | 0.7002 | 0.9783 | OES |
Notes. The orbital phases are calculated from the ephemeris defined at the inferior conjunction of the companion star from (Gies et al. 2003): 2451730.449(8)+5.599829(16)×E. The X-ray flux FX is taken from MAXI/GSC data.
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