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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] RpR [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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