Detection of periodic transit timing variations in the warm sub-Saturn planet HD 332231 b

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Table F.1

Best-fitting parameters from the RM effect modelling for HD 332231 b.

Parameter	HARPS-N	CARMENES	CARMENES+slope
λ_b(deg)	$- 4_{- 19}^{+ 20}$ $Mathematical equation: $-4_{-19}^{+20}$$	$1 . 2_{- 8.0}^{+ 8.2}$ $Mathematical equation: $1.2_{-8.0}^{+8.2}$$	$0_{- 20}^{+ 21}$ $Mathematical equation: $0_{-20}^{+21}$$
v sin i_*(km s⁻¹)	$6 . 2_{- 0.4}^{+ 0.5}$ $Mathematical equation: $6.2_{-0.4}^{+0.5}$$	10.0 ± 0.6	6.3 ± 0.7
T_{mid, b}(BJD_TDB-2459000)	$66 . 5114_{- 0.0018}^{+ 0.0018}$ $Mathematical equation: $66.5114_{-0.0018}^{+0.0018}$$	$141 . 3498_{- 0.0042}^{+ 0.0041}$ $Mathematical equation: $141.3498_{-0.0042}^{+0.0041}$$	$141 . 3316_{- 0.0077}^{+ 0.0070}$ $Mathematical equation: $141.3316_{-0.0077}^{+0.0070}$$

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