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Table 1

Stellar sample, atmospheric parameters, and characteristics of the observed spectra.


Name Classification ref.1 Teff (K) log g2 (cm s−2) [Fe/H] ξt (km s−1) S/T3 S/Nred R 103 Program ID
2MASS J09124370+0216236 rs (AP15) 6130 4.51 (0.04) −2.41 1.1 U 42 31 078.D-0217(A)
BPS CS 31062-012 rs (AP15) 6200 4.44 (0.02) −2.60 1.2 U 114 65 105.20LJ. 002
BPS CS 22881-036 rs (AP15) 6140 4.38 (0.03) −1.87 1.2 U 114 52, 42 165.N-0276(A), 078.B-0238(A)
BPS BS 16080-175 rs (AP15) 6210 4.11 (0.03) −1.46 1.4 K 146 48 U013Hr
BD −01 2582 rs (MS25) 5220 2.82 (0.03) −2.16 1.4 U 266 57 68.D-0546(A)
HD 196944 s (AP15), rs (KV21) 5390 2.13 (0.04) −2.21 2.0 H 224 115 60.A-9036(A)
2MASS J11140709+1828320 s, rs (SC13) 6160 4.53 (0.08) −2.84 1.1 U 68 32 087.D-0123(A)
2MASS J11432342+2020582 s, rs (SC13) 6390 4.53 (0.18) −3.06 1.2 U 58 32 087.D-0123(A)
HE 1029-0546 s (HH15) 6440 4.05 (0.09) −3.22 1.5 U 46 57 077.D-0035(A)
HE 0450-4902 s (HH15) 6570 4.44 (0.05) −2.56 1.4 U 32 35 077.D-0035(A)

Notes. 1 – Classification from the literature: AP15 – Abate et al. (2015), HH15 – Hansen et al. (2015), MS25 – Mashonkina & Smogorzhevskii (2025), KV21 – Karinkuzhi et al. (2021), SC13 – Spite et al. (2013). 2 – The log g uncertainties are indicated in parentheses. For each sample star, the uncertainties in Teff, [Fe/H], and ξt of 80 K, 0.2 dex, and 0.1 km s−1, respectively, were adopted. 3 – Spectrograph/Telescope: U – UVES/UT2, K – HIRES/Keck I, H – HARPS/La Silla 3.6 m.

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