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Table A.2

Transits of planet WASP-47b from ground-based telescopes included in our global analysis.

source (+ band) UT date (of T0) N cadence (s) σphot (ppm) T0 (BJDTDB) σ(T0) (days) σ(T0) (s)
REM (g′) 2021-09-25 137 60 3002 2459482.61821 0.00197 171
REM (r′) 2021-09-25 139 60 2119 2459482.62461 0.00106 91
REM (i′) 2021-09-25 139 60 2672 2459482.62212 0.00145 125
ETD (R) 2020-08-30 145 60 1315 2459091.66670 0.00064 56
ETD (R) 2021-07-12 144 60 1581 2459407.76213 0.00082 71
ETD (R) 2021-08-06 141 60 1658 2459432.71923 0.00081 70
ETD (R) 2021-08-31 155 60 1617 2459457.67291 0.00077 67
ETD (R) 2021-09-25 147 60 1540 2459482.62786 0.00073 63
ETD (clear) 2021-09-25 142 60 1723 2459482.62868 0.00084 72
ETD (R) 2021-10-20 129 60 1730 2459507.58050 0.00085 74

Notes. The columns give the instrument name and pass band, the UT date closest to the transit center T0, the number of photometric data points, the average cadence of the light curve in seconds, the scatter of the residuals from our best-fit model in parts per million, the transit time T0 in the BJDTDB standard and its associated error, and the latter converted into seconds. The fitting procedure is described in detail in Section 3.1.

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