Table 1
Observation details.
| ObsID(a) | TM(b) | Time | Exposure(c) | Pointing | Target |
|---|---|---|---|---|---|
| UT | (ks) | RA, Dec | |||
| 700016 | 3,4 | 2019–09–15 09:28:20 – 2019–09–16 21:30:00 | 25 002 | 83.83637,–69.31139 | SN1987A |
| 700161 | 1–7 | 2019–10–18 16:54:34 – 2019–10–19 15:07:54 | 71 544 | 83.83638,–69.31139 | SN 1987A FL |
| 700156 | 5–7 | 2019–10–10 01:58:14 – 2019–10-10 15:18:14 | 19 349 | 81.25917,–69.64417 | N 132D |
| 700179 | 1–7 | 2019–11–22 15:44:11 – 2019–11–23 08:24:11 | 59 549 | 81.25917,–69.64417 | N 132D |
| 700184I | 1–7 | 2019–11–23 21:04:51 – 2019–11–24 08:11:31 | 34702 | 80.68758,–69.37765 | N 132D off-axis |
| 700185(d) | 1–7 | 2019–11-25 08:03:01 – 2019–11–25 19:09:41 | 20594 | 81.90048,–69.89292 | N 132D off-axis |
| 700183(d) | 1–7 | 2019–11–25 19:13:51 – 2019–11–26 06:20:31 | 33805 | 81.9935,–69.43154 | N 132D off-axis |
| 700182 | 1–7 | 2019–11–27 06:11:41 – 2019–11–27 17:18:21 | 31 483 | 80.51012,–69.85367 | N 132D off-axis |
| 700205 | 1–7 | 2019–12–07 13:00:00 – 2019–12–07 21:14:00 | 18839 | 84.44442,–69.17140 | PSR J0537–6910 |
| 700206 | 1–7 | 2019–12–07 21:20:00 – 2019–12–08 02:50:00 | 15 344 | 85.04515,–69.33173 | PSR J0540–6919 |
| 700207 | 1–7 | 2019–12–08 02:56:00 – 2019–12–08 13:00:00 | 22255 | 84.74217,–69.25035 | PSR J0540 and J0537 |
| 700001 | 1–7 | 2019–11–07 17:13:18 – 2019–11–08 09:53:18 | 54610 | 16.00833,–72.03194 | 1E 0102.2–7219 |
| 700002 | 1–7 | 2019–11–08 09:57:18 – 2019–11–09 02:37:18 | 58714 | 15.03687,–71.88838 | 1E 0102.2–7219 off-axis |
| 700003 | 1–7 | 2019–11–09 02:41:38 – 2019–11–09 19:21:38 | 59931 | 16.99466,–72.17060 | 1E 0102.2–7219 off-axis |
| 700004 | 1–7 | 2019–11–09 19:25:38 – 2019–11–10 10:42:18 | 55 594 | 16.28235,–71.85088 | 1E 0102.2–7219 off-axis |
| 700005 | 1–7 | 2019–11–10 10:45:48 – 2019–11–11 02:02:28 | 55 672 | 16.41901,–71.76044 | 1E 0102.2–7219 off-axis |
| 710000(e) | 1–7 | 2020–06–18 20:00:00 – 2020–06–19 06:00:00 | 37056 | 16.00833,–72.03194 | 1E 0102.2–7219 |
Notes. (a)eROSITA observation ID. (b) Active telescope modules. (c)Maximum exposure from vignetting-corrected exposure map normalised to one TM, i.e. total exposure divided by 7. In this way, the resulting count rates in the source detection lists are for the total of seven TMs even when not all TMs were active. (d)During part of these observations, the electronic chopper was set to 2, which was not handled correctly by the pipeline processing. We corrected this in the event files (see Appendix A). (e)Calibration observation near the end of the first eROSITA all-sky survey (eRASS1).
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