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Table A.1

Chi-square fit results of BT-Settl model for stellar photospheric spectra in VOSA.

2MASS Name SpTy M*/M Distance [pc] Av [mag] Teff [Κ] log(g)* Lbol/L ΔLbol/L
J11071668−7735532 NC1 M7.74 0.05(1) 194.6 0 2400 4 2.020e-2 9.704e-4
J15582981−2310077 J1558 M4.5 0.14 141.1 1 3600 4 4.181e-2 7.151e-4
J11071860−7732516 NC9 M5.5 0.08 197.5 4.8 2800 5 6.512e-2 6.261e-3
J04390163+2336029 J0439 M6 0.12 126.8 0 3100 4 7.212e-2 7.466e-4
J11074245−7733593 HKCha M5.25 0.09 191.0 2.4 3100 2.5 1.214e-l 3.271e-4
J11085090−7625135 Sz28 M5.25 0.08 192.2 0.8 3000 4.5 6.593e-2 1.281e-3
J11082650−7715550 IC147 M5.75 0.07 195.8 2.5 3700 3 2.886e-2 1.694e-3
J12073346−3932539 TWA27 M9 0.02(2) 64.4 0 2500 3 3.025e-3 6.101e-5
J16053215−1933159 J1605 M4.5 0.13(3) 152.3 1.6 3400 4.5 4.626e-2 9.038e-4

Notes. Distances are collected from Gaia DR3 (Gaia Collaboration et al. 2021), and stellar properties, including Av, are obtained from Manara et al. (2023), which provides collected data from Manara et al. (2017); Herczeg & Hillenbrand (2014, 2008). Values with superscripts are obtained from (1) Luhman (2007), (2) Manjavacas et al. (2024), and (3) Testi et al. (2022). *The values are uncertain because they are fit based on SED shapes instead of using a detailed spectroscopic model.

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