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Table 4.

Physical stellar parameters of the targets obtained with the ROTFIT code.

Name Teff log g v sin i RV Prob
(K) (km s−1) (km s−1) %
2MASS J15383733-3422022 3111±70 4.75±0.13 < 8 4.1±2.7 99.8
Sz 70 3038±76 4.02±0.11 14.0±14.0 1.1±2.6 84.6
TYC 7335-550-1 4488±140 4.06±0.22 < 8 2.6±2.0 99.2
2MASS J15361110-3444473 2883±104 4.41±0.12 13.0±10.0 6.9±2.6 97.9
2MASS J15523574-3344288 2981±44 4.54±0.10 < 8 2.6±2.7 75.3
2MASS J15551027-3455045 2700±103 3.60±0.11 19.0±8.0 0.1±2.9 97.9
2MASS J16011870-3437332 3121±90 4.73±0.14 12.0±8.0 –0.5±2.3 98.7
UCAC4 269-083981 3846±47 4.53±0.11 < 8 0.6±2.7 99.6
Gaia DR2 6010590577947703936 3154±72 4.77±0.13 40.8±3.6 0.5±4.7 99.2
2MASS J15414827-3501458 3213±94 4.52±0.23 53.3±5.7 3.4±4.3 99.8
UCAC4 273-083363 3211±56 4.51±0.15 < 8 1.3±2.3 99.8
Gaia DR2 6014269268967059840 3019±108 4.75±0.14 44.0±12.0 1.7±4.6 98.3

Notes. ‘Prob’ column represents the probability of the target being a member of Lupus I according to BANYAN Σ, which is based on the RVs measured with ROTFIT and the kinematic properties reported by Gaia DR2.

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