Radii, masses, and transit-timing variations of the three-planet system orbiting the naked-eye star TOI-396

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Table 4

Same as Table 3, but this time the Keplerian signals with K = K_in have period P = P_rot,⋆.

K_in	ρ_p	M_p	K_out	Detection	$\frac{Δ K}{K}$ ${{\Delta K} \over K}$	ΔK
(m s⁻¹)	(g cm⁻³)	(M_⊕)	(m s⁻¹)	level		(σ)
1.0	2.0	3.1	0.29 ± 0.28	~1σ	−71%	−2.5
K_d = 1.79	3.6	5.6	0.80 ± 0.39	~2σ	−55%	−2.5
3.0	6.1	9.4	1.90 ± 0.40	~5σ	−37%	−2.8
10.0	20.2	31.4	9.02 ± 0.36	~25σ	−10%	−2.7

Notes. Column $\frac{Δ K}{K}$ ${{\Delta K} \over K}$ gives the relative difference (in percentage) between the obtained RV semi-amplitude (K_out) and the expected one (K_in), while the last column ΔK ≡ K_out − K_in lists the semi-amplitude difference in terms of the 1σ uncertainty of K_out.

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