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Table C.1

Slope (S) and associated uncertainty (σS) that was adjusted to the residuals between CCF and s-BART RVs, when using the large sample of stars described in Section 2.3

Star Night S [m s−1 h−1] σS [m s−1 h−1]
HD106315 2021-04-29 −53.69 0.32
HAT-P-26 2021-04-09 −27.04 0.55
WASP-20 2021-11-03 −11.63 0.98
WASP-178 2021-07-09 −11.33 1.36
WASP-54 2021-04-06 −10.7 0.85
HD40307 2018-12-26 −9.07 0.06
WASP-31 2022-01-26 −8.19 0.75
Kelt-14 2021-01-18 −7.83 0.17
HD40307 2018-12-27 −7.28 0.06
TOI-132 2021-08-13 −6.96 0.21
HAT-P-26 2021-03-23 −6.88 0.15
WASP-12 2021-12-30 −5.71 0.56
HD40307 2018-12-24 −5.53 0.05
HD40307 2018-12-25 −5.49 0.06
TOI-824 2022-06-28 −5.44 0.25
WASP-156 2021-10-11 −5.14 0.21
HD40307 2018-12-23 −4.89 0.02
WASP-34 2021-02-25 −4.32 0.16
WASP-126 2021-10-23 −4.21 0.56
TOI-132 2022-09-18 −3.75 0.16
WASP-62 2022-01-16 −3.74 0.36
WASP-12 2021-11-25 −3.72 0.34
Kelt-14 2021-02-11 −3.59 0.16
WASP-62 2021-12-25 −3.42 0.37
WASP-126 2019-11-19 −3.06 0.2
WASP-34 2021-04-18 −2.82 0.12
HD3167 2019-10-08 −2.19 0.19
WASP-54 2021-05-13 −1.03 0.15
HD209458 2019-09-10 −1.02 0.06
55CncA 2020-02-04 −0.75 0.02
HD209458 2019-07-19 −0.74 0.05
HD3167 2022-11-02 −0.6 0.08
ϵ Indi 2022-09-09 −0.4 0.01
ϵ Indi 2022-09-08 −0.38 0.01
ϵ Indi 2022-09-10 −0.36 0.01
ϵ Indi 2022-09-07 −0.34 0.01
ϵ Indi 2022-09-06 −0.34 0.01
ϵ Indi 2022-09-05 −0.32 0.01

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