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Table B.3

Radial velocity measurements, full width at half maximum (FWHM), contrast, and skewness extracted from the cross-correlation functions of the TOI-282’s ESPRESSO spectra.


BJDTDB − 2 450 000 RV (km s−1) eRV (km s−1) RVdetrended (km s−1) eRVdetrended (km s−1) FWHM (km s−1) Contrast (A) (%) Skewness (γ) Texp (s) S/N
ESPRESSO 1st set
8771.715834 −0.0061 0.0022 −0.0019 0.0026 12.7080 54.1188 −0.0206 1115 88.2
8776.730177 0.0011 0.0022 0.0044 0.0026 12.6990 53.9773 −0.0198 1115 88.5
8788.726805 −0.0010 0.0023 0.0007 0.0027 12.7019 54.0500 −0.0182 1115 82.5
8804.620886 −0.0079 0.0017 −0.0046 0.0022 12.7019 53.9437 −0.0198 1115 114.7
... ... ... ... ... ... ... ...

ESPRESSO 2nd set
9492.867880 0.0011 0.0018 0.0026 0.0019 12.7134 54.1612 −0.0175 935 105.5
9493.733784 −0.0035 0.0024 −0.0002 0.0024 12.6995 54.1398 −0.0170 935 79.3
9496.727138 0.0022 0.0020 0.0003 0.0021 12.6939 53.9965 −0.0160 935 95.1
9497.753690 −0.0014 0.0030 −0.0011 0.0030 12.7090 54.1882 −0.0220 935 63.1
... ... ... ... ... ... ... ...

Notes. Barycentric Julian dates are given in barycentric dynamical time (BJDTDB; Eastman et al. 2010). We split the data into ESPRESSO 1st and ESPRESSO 2nd sets, and treat the two sets independently to account for a potential RV offset that may have resulted from the instrument refurbishment performed between 2019 and 2020. The last two columns provide the exposure time and S/N per pixel at 550 nm. The detrended dataset RVdetrended was derived following the procedure outlined in Sect. 4.1. The errors associated with the detrended measurements account for the jitter. The entire RV data set is available in a machine-readable table at the Strasbourg astronomical Data Center (CDS)

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