A comprehensive study on radial velocity signals using ESPRESSO: Pushing precision to the 10 cm/s level

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Table 1

Literature parameters for the stars discussed in the paper.

Parameter	HD 10700		HD 20794		HD 102365		HD 304636
	G8.5V	[1]	G8V	[4]	G5	[9]	M0	[14]/[15]
Spectral type	K0	[2]	K0	[2]	G8	[2]	M1	[2]/[16]
T_eff [K]	5339±19	[2]	5388±14	[2]	5652±18	[2]	3820±92	[2]
					5618±14	[10]	3770±40	[16]
[Fe/H]	−0.51±0.01	[2]	−0.385±0.011	[2]	−0.3±0.01	[2]	−0.16±0.05	[2]
					−0.31±0.02	[11]	−0.16±0.09	[15]
log g [cm s⁻²]	4.45±0.06	[2]	4.379±0.036	[2]	4.4±0.05	[2]	4.72±0.02	[16]
ξ_t[km/s]	0.67±0.04	[2]	0.568±0.040	[2]	0.98±0.03	[2]	−	−
					0.7	[9]
v.sin(i) [km/s]	~1	[3]	<3	[4]	<2	[2]	2.32±0.65	[2]
$\log (R_{H K}^{'})$ $\[\log \left(R_{H K}^{\prime}\right)\]$	−4.96±0.003	[4]	−4.976±0.003	[4]	−4.99	[9]	−4.94±0.01	[2]
	−4.90±0.01	[2]	−5.00±0.01	[2]	−4.88±0.01	[2]	−4.94±0.01	[2]
P_rot [d]	34	[5]	33.19±3.61	[4]	40	[12]	31±5	[2]
P_rot [d]	46±4	[6]	33.19±3.61	[4]	40	[12]	31±5	[2]
π [mas]	273.8097±0.1701	[7]	165.5242±0.0784	[7]	107.3024±0.0873	[7]	95.6982±0.0145	[7]
d [pc]	3.65	[7]	6.04	[7]	9.32	[7]	10.45	[7]
							0.55±0.05	[17]
M_star[M_⊙]	0.783±0.012	[8]	0.70	[4]	${0.88}_{- 0.03}^{+ 0.02}$ $\[0.88_{-0.03}^{+0.02}\]$	[13]	0.53±0.05	[15]
							0.48±0.03	[16]
R_star[R_⊙]	0.793±0.004	[8]	−	−	−	−	${0.5066}_{- 0.0172}^{+ 0.0169}$ $\[0.5066_{-0.0172}^{+0.0169}\]$	[16]
L_star[L_⊙]	0.488±0.010	[8]	0.656±0.003	[4]	−	−	0.046±0.0015	[16]

Notes. [1] Gray et al. (2006), [2] Hojjatpanah et al. (2019), [3] Gray & Baliunas (1994), [4] Pepe et al. (2011), [5] Baliunas et al. (1996), [6] Korolik et al. (2023), [7] Gaia Collaboration (2023), [8] Teixeira et al. (2009), [9] Tinney et al. (2011), [10] Meunier et al. (2022), [11] Soubiran et al. (2022), [12] Noyes et al. (1984b), [13] Aguilera-Gómez et al. (2018), [14] Koen et al. (2010), [15] Maldonado et al. (2019b), [16] DiTomasso et al. (2025), [17] Neves et al. (2013).

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