Table A.1
Transit times, transit depth, and relative planet radius derived from individual CHEOPS and TESS measurements with pyaneti. For comparison, we show the derived transit times of Martioli et al. (2021) converted to BJD, with their published statistical MCMC errors. Our errors are precision values derived by parametric bootstraps, the errors in Martioli et al. are MCMC statistical errors describing the core 35% of the distribution.
| Transit | Tt (BJD) [This paper] | Rp ∕R⋆ [pyaneti] | Tt (BJD) [Martioli et al. (2021)] |
|---|---|---|---|
| CHEOPS #1 | 2459041.2828 ± 0.0006 | 0.0541 ± 0.0002 | — |
| CHEOPS #2 | 2459083.5970 ± 0.0004 | 0.0520 ± 0.0002 | — |
| CHEOPS #3 | 2459117.4515 ± 0.0008 | 0.0515 ± 0.0002 | — |
| TESS S1#1 | 2458330.3911 ± 0.0008 | 0.0546 ± 0.0004 | 2458330.39046 ± 0.00016 |
| TESS S1#2 | 2458347.3174 ± 0.0008 | 0.0565 ± 0.0005 | 2458347.31646 ± 0.00016 |
| TESS S27#1 | 2459041.2816 ± 0.0008 | 0.0517 ± 0.0003 | 2459041.28238 ± 0.00026 |
| TESS S27#2 | 2459049.7457 ± 0.0008 | 0.0582 ± 0.0003 | 2459049.74538 ± 0.00026 |
| TESS S27#3 | 2459058.20795 ± 0.0008 | 0.0548 ± 0.0004 | 2452058.20838 ± 0.00026 |
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