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Table 2.

Positions, magnitudes and atmospheric parameters of the stellar sample, including references to literature work (in parenthesis when the spectrum is different from that analysed here).

Star RA Dec G Teff log g vturb Ref.
[hh:mm:ss] [hh:mm:ss] [mag] [K] [km s−1]
HR sample

AS00039 00:58:45.60 − 33:42:21.8 16.932 4372 0.76 2.0 (1)
AF20549 01:00:47.84 − 33:41:03.2 17.940 4758 1.37 1.8 2,3
JS14296 00:59:38.76 − 33:46:14.6 18.783 4929 1.79 1.7 3
JS66402 01:00:00.41 − 33:29:15.5 18.774 4985 1.81 1.7 3
MT00749 01:00:05.02 − 33:61:16.6 17.973 4797 1.41 1.8 3,4
MT00750 (a) 01:00:01.15 − 33:59:21.4 18.271 4876 1.56 1.8 3,4
PJ00206 01:01:26.76 − 33:02:59.8 16.687 4359 0.65 2.0 5,(6)
PJ03059 01:01:22.25 − 33:46:21.9 17.538 4618 1.14 1.9 5
PJ03111 00:57:10.22 − 33:28:35.8 17.460 4650 1.13 1.9 5,(6)
PJ07402 00:57:34.85 − 33:39:45.7 17.758 4608 1.22 1.8 5,(6)
UHAL004 01:01:49.43 − 33:54:10.4 16.521 4202 0.49 2.0

LR sample

DR20080 00:57:44.16 − 33:61:14.3 17.839 4682 1.29 1.8
ES03170 01:01:47.48 − 33:47:27.6 18.385 4962 1.65 1.8 6

Notes. Typical random errors on the stellar parameters are: ΔTeff = 86 K; Δlog g = 0.14; and Δvturb = 0.1 km s−1.

(a)

No available spectra of the CH G-band.

References. (1)Skúladóttir et al. (2021); (2)Frebel et al. (2010a); (3)]Simon et al. (2015); (4)Tafelmeyer et al. (2010); (5)Jablonka et al. (2015); (6)Starkenburg et al. (2013).

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