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Table C.1.

Comparison to parameters determined in Carini et al. (2020) of the ten stars in common between the studies.

this work Carini et al. (2020)

ID Teff log g v sin i Flag ID Teff log g v sin i
[K] [dex] [km s−1] [K] [dex] [km s−1]
670 A4 17000±1000 2.9±0.1 100
643 A5 21400±3000 3.5±0.2 250
313 SB1 A10 20500±1000 3.7±0.1 200
289 A17 21700±1000 3.6±0.1 100
420 A21 21000±1000 3.6±0.2 150
522 A23 21600±2000 3.6±0.2 100
573 A24 21700±1500 3.9±0.3 150
134 A34 20500±1500 3.8±0.2 150
228 A40 17500±500 3.1±0.1 100
519 SB1 A48 22000±1500 3.1±0.3 150

Notes. Here, we use the parameters given in table 4 of Carini et al. (2020) which are based on their analysis considering stellar rotation. The two SB1s detected in Paper II are indicated in the column Flag.

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