Open Access
Table B.1
Details of the TESS observations used.
| System | Sector | Camera | CCD | from – to (UT) | Nobs | PNR (ppth) | Ntr |
|---|---|---|---|---|---|---|---|
| HATS-18 | 10 | 1 | 1 | 2019 Mar 26 – 2019 Apr 22 | 16135 | 12.3 | 25 |
| 36 | 1 | 2 | 2021 Mar 07 – 2021 Apr 01 | 16928 | 9.73 | 26 | |
| 63 | 1 | 2 | 2023 Mar 10 – 2023 Apr 06 | 17486 | 9.45 | 27 | |
| total: | 78 | ||||||
| HIP 65A | 1 | 2 | 2 | 2018 Jul 25 – 2018 Aug 22 | 18279 | 1.33 | 25 |
| 2 | 2 | 1 | 2018 Aug 23 – 2018 Sep 20 | 18300 | 1.25 | 26 | |
| 28 | 2 | 2 | 2020 Jul 31 – 2020 Aug 25 | 17284 | 1.40 | 24 | |
| 29 | 2 | 1 | 2020 Aug 26 – 2020 Sep 21 | 17929 | 1.49 | 26 | |
| 68 | 2 | 2 | 2023 Jul 29 – 2023 Aug 25 | 17586 | 1.48 | 21 | |
| 69 | 2 | 1 | 2023 Aug 25 – 2023 Sep 20 | 16550 | 1.43 | 24 | |
| total: | 146 | ||||||
| TrES-3 | 25 | 2 | 4 | 2020 May 14 – 2020 Jun 08 | 17246 | 3.59 | 18 |
| 26 | 2 | 3 | 2020 Jun 09 – 2020 Jul 04 | 16941 | 3.37 | 18 | |
| 40 | 2 | 3 | 2021 Jun 25 – 2021 Jul 23 | 19611 | 3.54 | 22 | |
| 52 | 2 | 4 | 2022 May 19 – 2022 Jun 12 | 16749 | 3.25 | 18 | |
| 53 | 2 | 3 | 2022 Jun 13 – 2022 Jul 08 | 17306 | 3.31 | 18 | |
| total: | 94 | ||||||
| WASP-19 | 9 | 2 | 2 | 2019 Mar 01 – 2019 Mar 25 | 16878 | 4.16 | 29 |
| 36 | 2 | 1 | 2021 Mar 07 – 2021 Apr 01 | 17343 | 3.94 | 29 | |
| 62 | 2 | 2 | 2023 Feb 12 – 2023 Mar 10 | 18025 | 4.02 | 28 | |
| 63 | 2 | 1 | 2023 Mar 10 – 2023 Apr 06 | 18358 | 3.62 | 33 | |
| total: | 119 | ||||||
| WASP-43 | 9 | 1 | 1 | 2019 Mar 01 – 2019 Mar 25 | 16878 | 2.57 | 28 |
| 35 | 1 | 2 | 2021 Feb 09 – 2021 Mar 06 | 13992 | 2.45 | 24 | |
| 62 | 1 | 3 | 2023 Feb 12 – 2023 Mar 10 | 18024 | 2.52 | 31 | |
| total: | 83 | ||||||
| WASP-173A | 2 | 1 | 1 | 2018 Aug 23 – 2018 Sep 20 | 18300 | 1.66 | 18 |
| 29 | 1 | 1 | 2020 Aug 26 – 2020 Sep 21 | 16653 | 1.78 | 15 | |
| 69 | 1 | 1 | 2023 Aug 25 – 2023 Sep 20 | 16696 | 1.68 | 16 | |
| total: | 49 |
Notes. Nobs is the number of useful data points. PNR is the photometric noise rate (Fulton et al. 2011) in parts per thousand (ppth) of the normalised flux per minute of observation. Ntr is the number of complete transit light curves used in this study.
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