Table A.1.
Metallicity-adjusted fractional radius residuals for the sample of ten very-low-mass stars, and for 13 very-low-mass stars from the literature, with respect to the Exeter/Lyon models (Baraffe et al. 1998, 2003, 2015), and the Dartmouth models (Dotter et al. 2008) if M2 > 0.15 M⊙.
| Low-mass star | ΔR/R [Baraffe] | σ+ | σ− | ΔR/R [Dartmouth] | σ+ | σ− |
|---|---|---|---|---|---|---|
| This work | ||||||
| EBLM J0339+03Ab | −0.056 | 0.055 | 0.057 | −0.045 | 0.056 | 0.054 |
| EBLM J0954–23Ab | −0.139 | 0.170 | 0.241 | – | – | – |
| EBLM J1013+01Ab | 0.064 | 0.020 | 0.019 | 0.076 | 0.023 | 0.022 |
| EBLM J1431–11Ab | 0.001 | 0.042 | 0.031 | – | – | – |
| EBLM J1403–32Ab | −0.010 | 0.025 | 0.025 | 0.008 | 0.026 | 0.028 |
| EBLM J1038–37Ab | 0.037 | 0.044 | 0.046 | 0.054 | 0.047 | 0.047 |
| EBLM J2017+02Ab | −0.035 | 0.077 | 0.066 | – | – | – |
| EBLM J0543–56Ab | 0.019 | 0.046 | 0.031 | 0.038 | 0.045 | 0.036 |
| EBLM J1115–36Ab | −0.040 | 0.037 | 0.030 | −0.022 | 0.038 | 0.029 |
| EBLM J0555–57Ab | −0.218 | 0.148 | 0.100 | – | – | – |
| Literature objects | ||||||
| EBLM J1219–39 | 0.039 | 0.055 | 0.059 | – | – | – |
| OGLE-TR-122Ab | 0.044 | 0.167 | 0.204 | – | – | – |
| C4780b | −0.133 | 0.202 | 0.254 | – | – | – |
| KOI-686Ab | −0.013 | 0.053 | 0.053 | – | – | – |
| HATS-550-016Ab | 0.041 | 0.047 | 0.047 | – | – | – |
| HATS-551-021Ab | 0.007 | 0.074 | 0.077 | – | – | – |
| KIC1571511Ab | 0.036 | 0.027 | 0.027 | – | – | – |
| HATS-551-019Ab | −0.038 | 0.071 | 0.079 | −0.033 | 0.075 | 0.078 |
| HATS-553-001Ab | 0.012 | 0.073 | 0.078 | 0.031 | 0.072 | 0.077 |
| Kepler-16B | 0.030 | 0.006 | 0.006 | 0.031 | 0.006 | 0.006 |
| KOI-126C | 0.003 | 0.012 | 0.012 | 0.005 | 0.013 | 0.013 |
| KOI-126B | −0.002 | 0.012 | 0.012 | −0.002 | 0.013 | 0.013 |
| EBLM J0113+31Ab | 0.041 | 0.061 | 0.068 | 0.039 | 0.064 | 0.068 |
Notes. References for the literature objects are provided in Table 3.
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