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Table 2
Ground-based transit follow-up observations of TOI-1685.
| Instrument | Country | Date | Filter | Exposure | Duration(a) | Nobs | rms(b) |
|---|---|---|---|---|---|---|---|
| (s) | (min) | (ppt) | |||||
| LCOGT | USA | 26 August 2020 | I | 50 | 173 | 123 | 1.29 |
| 07 November 2020 | ip | 25 | 266 | 270 | 1.47 | ||
| 11 November 2020 | ip | 50 | 279 | 199 | 1.01 | ||
| PESTO | Canada | 08 March 2020 | i′ | 15 | 187 | 724 | 2.63 |
| MuSCAT2 | Spain | 19 January 2021 | zs | 15 | 179 | 328 | 1.24 |
| i′ | 15 | 179 | 238 | 1.18 | |||
| 29 January 2021 | zs | 15 | 331 | 333 | 1.70 | ||
| i′ | 15 | 331 | 333 | 1.71 | |||
| LCOGT(c) | Spain, USA | 22–31 December 2020 | V | 100 | 39.83 (d) | 20 | 13.7 |
Notes. (a) Time span of the observation. (b) Root mean square in parts-per-thousand. (c)Data used only inSect. 4.2 for determining the stellar rotational period. The duration of the long-term monitoring is in days insteadof minutes.
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