Table 3
Log of the CHEOPS observations of HD 108236.
| id | Planets | File Key | OBSID | Start date | Duration | Exp. time | Efficiency |
|---|---|---|---|---|---|---|---|
| # | [UTC] | [h] | [s] | [%] | |||
| 1(a) | c, e, (g) | CH_PR300046_TG000101_V0200 | 1015572 | 2020-03-10T18:09:15.91 | 18.33 | 42.0 | 61.1 |
| 2 | b | CH_PR100031_TG015701_V0200 | 1084970 | 2020-04-19T08:48:11.23 | 17.04 | 49.0 | 59.6 |
| 3(a) | d | CH_PR100031_TG015401_V0200 | 1088211 | 2020-04-28T07:06:11.05 | 18.63 | 49.0 | 54.8 |
| 4 | c | CH_PR100031_TG015601_V0200 | 1088443 | 2020-04-29T16:02:11.28 | 11.24 | 49.0 | 53.7 |
| 5(a) | b,f | CH_PR100031_TG015702_V0200 | 1087957 | 2020-04-30T17:06:11.04 | 16.40 | 49.0 | 54.5 |
| 6 | c | CH_PR100031_TG015602_V0200 | 1096738 | 2020-05-05T21:36:10.33 | 10.57 | 49.0 | 57.1 |
| 7 | c | CH_PR100031_TG022401_V0200 | 1107339 | 2020-05-12T02:10:11.27 | 07.08 | 49.0 | 57.5 |
| 8 | b | CH_PR100031_TG023001_V0200 | 1111865 | 2020-05-19T23:34:51.37 | 08.91 | 49.0 | 56.6 |
| 9 | d, (g) | CH_PR100031_TG024301_V0200 | 1117140 | 2020-05-26T09:18:11.28 | 26.37 | 49.0 | 51.0 |
| 10 | b | CH_PR100031_TG023002_V0200 | 1117572 | 2020-05-27T14:31:10.32 | 08.35 | 49.0 | 47.6 |
| 11 | e | CH_PR100031_TG022701_V0200 | 1117376 | 2020-05-28T05:21:10.39 | 13.14 | 49.0 | 50.4 |
| 12 | b | CH_PR100031_TG023003_V0200 | 1124008 | 2020-05-31T09:24:11.59 | 08.89 | 49.0 | 52.8 |
| 13 | c | CH_PR100031_TG022901_V0200 | 1124302 | 2020-06-05T22:42:30.53 | 10.38 | 49.0 | 51.6 |
| 14 | f | CH_PR110045_TG002601_V0200 | 1458282 | 2021-04-20T06:58:13.84 | 10.95 | 49.0 | 62.2 |
| 15 | (g) | CH_PR110045_TG002701_V0200 | 1456848 | 2021-04-29T18:51:51.55 | 17.98 | 49.0 | 53.9 |
Notes. The second column shows the planetary transits observed during each CHEOPS visit. The last column shows the observation efficiency of each visit, considering the gaps produced by Earth occultations or SAA crossings. We report the unique identifiers of each CHEOPS visit: OBSID and File Key. (a)Observations presented in Bonfanti et al. (2021).
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