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Table 7.

Physical stellar parameters of the targets.

Name SpT AV L R M Age log g
(mag) (L) (R) (M) (Myr)
2MASS J15383733-3422022 M5 0 0.012±0.006 0.39±0.01 0.09±0.05 10.7±5 4.20±0.5
Sz 70 M5 0.5 0.25±0.11 1.87±0.05 0.17±0.05 0.5±0.3 3.28±0.2
TYC 7335-550-1 K4.5 0.7 0.94±0.56 1.60±0.05 1.1±0.1 3.50±1 4.04±0.2
2MASS J15361110-3444473 M5.5 1.75 0.006±0.003 0.32±0.01 0.05±0.05 9.77±5 4.13±0.3
2MASS J15523574-3344288 M5.5 0.5 0.02±0.01 0.55±0.01 0.11±0.03 6.3±3 4.04±0.4
2MASS J15551027-3455045 M7.5 0.75 0.0072±0.0034 0.39±0.02 0.03±0.02 1.7±1.5 3.71±0.3
2MASS J16011870-3437332 M5 0 0.013±0.006 0.41±0.01 0.09±0.04 9.55±5 4.16±0.5
UCAC4 269-083981 M0 0.5 0.30±0.14 1.23±0.02 0.6±0.3 4.2±1 4.03±0.5
Gaia DR2 6010590577947703936 M4.5 0 0.017±0.007 0.45±0.01 0.11±0.05 8.8±4 4.16±0.3
2MASS J15414827-3501458 M4 0 0.12±0.06 1.13±0.03 0.2±0.08 1.82±1 3.64±0.4
UCAC4 273-083363 M3.5 0 0.069±0.032 0.83±0.01 0.2±0.04 3.63±1.5 3.88±0.3
Gaia DR2 6014269268967059840 M6 0 0.01±0.005 0.41±0.02 0.05±0.03 6.46±2 3.93±0.5

Notes. The methods used for calculating SpT, AV, L, and R are described in the text. M, log g, and the age of the stars are evaluated according to Baraffe et al. (2015) isochrones, except for TYC 7335-550-1, for which we have used the MIST isochrones. The SpT for TYC 7335-550-1 and UCAC4 269-083981 (in italics) are obtained using the temperatures derived by the ROTFIT code (Table 4) and the SpT–Teff calibration of Pecaut & Mamajek (2013). The errors associated with SpT and AV are 0.5 subclasses and 0.4 mag, respectively. The errors associated with mass and age are internal to the tracks and isochrones.

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