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Table 2

Stellar parameters of our targets.

Star Teff (K) log 𝑔 [Fe/H] ξ (km s−1) [Fe/H] Vbroad (km s−1)
(HARPS-N) (HARPS-N) (HARPS-N) (GIANO-B) (GIANO-B) (GIANO-B)
g1 4530 ± 86 2.14 ± 0.10 0.01 ± 0.09 1.57 ± 0.20 −0.12 ± 0.05 4.6 ± 1.1
g2 4760 ± 111 2.69 ± 0.14 0.02 ± 0.10 1.10 ± 0.24 −0.04 ± 0.05 6.3 ± 1.6
g3 4937 ± 114 2.51 ± 0.35 0.04 ± 0.08 1.32 ± 0.26 −0.01 ± 0.06 6.3 ± 1.5
g4 4977 ± 117 2.82 ± 0.18 0.04 ± 0.08 1.21 ± 0.19 0.03 ± 0.04 4.7 ± 1.4
g5 5061 ± 56 2.99 ± 0.19 0.04 ± 0.07 1.07 ± 0.24 0.02 ± 0.05 5.8 ± 1.2
g6 5002±110 2.96 ± 0.20 0.03 ± 0.07 0.87 ± 0.20 0.09 ± 0.04 4.7 ± 1.2
g7 5058 ± 56 2.97 ± 0.20 0.03 ± 0.07 1.39 ± 0.31 0.02 ± 0.06 6.3 ± 1.0
g9 5062 ± 56 3.00 ± 0.19 0.00 ± 0.09 1.18 ± 0.24 −0.01 ± 0.05 5.6 ± 1.2
g10 5066 ± 56 3.01 ± 0.19 -0.03 ± 0.09 0.97 ± 0.29 −0.02 ± 0.05 5.6 ± 1.3

Notes. The table columns are as follows, from left to right: effective temperature (Teff), surface gravity (log (𝑔)), and [Fe/H] measured from the HARPS-N spectra in Alonso-Santiago et al. (2021), as well as the microturbulence velocity (ξ), [Fe/H], and broadening velocity (Vbroad) in this study using GIANO-B spectra.

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