Long-period magnetic activity in the K dwarf GJ1137 and a new super-Earth on a 9-day orbit - A cautionary tale for Jovian-analogue detection from Doppler surveys

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Table A.5

RV semi-amplitude posteriors of GJ 1137 c in units of m s⁻¹ from the grid-search in Fig. 5.

Planetary config.	Stellar-activity kernel
Planetary config.	MEP	ESP2	ESP3	ESP4
K_bC_c	${1.73}_{- 0.23}^{+ 0.24}$ $Mathematical equation: $1.73^{+0.24}_{-0.23}$$	1.67 ± 0.23	${1.68}_{- 0.25}^{+ 0.24}$ $Mathematical equation: $1.68^{+0.24}_{-0.25}$$	${1.70}_{- 0.25}^{+ 0.24}$ $Mathematical equation: $1.70^{+0.24}_{-0.25}$$
K_bK_c	${1.71}_{- 0.24}^{+ 0.23}$ $Mathematical equation: $1.71^{+0.23}_{-0.24}$$	${1.65}_{- 0.26}^{+ 0.23}$ $Mathematical equation: $1.65^{+0.23}_{-0.26}$$	${1.65}_{- 0.30}^{+ 0.25}$ $Mathematical equation: $1.65^{+0.25}_{-0.30}$$	${1.35}_{- 0.71}^{+ 0.47}$ $Mathematical equation: $1.35^{+0.47}_{-0.71}$$

Notes. Reported uncertainties reflect the 16^th and the 84^th percentiles.

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