Table 4.
Difference in mass and radius of the primary star (⋆) and the secondary (2) for a variety of different scenarios.
| ΔR⋆, l3 | ΔR2, l3 | ΔR⋆, ldy | ΔR2, ldy | ΔM⋆, αmlt | ΔM2, αmlt | Δταmlt | ΔM⋆, Y | ΔM2, Y | ΔτY | ||
|---|---|---|---|---|---|---|---|---|---|---|---|
| J2349-32 | −0.003 | 0.016 | −0.014 | −0.002 | −0.037 | −0.004 | 2.208 | 0.048 | 0.005 | −0.853 | |
| (−0.22%) | (7.8%) | (−1.46%) | (−0.98%) | (−3.73%) | (−2.30%) | (96%) | (4.84%) | (2.87%) | (−37%) | ||
| J2308-46 | −0.002 | 0.013 | −0.014 | −0.001 | −0.044 | −0.002 | 1.423 | 0.059 | 0.005 | −1.32 | |
| (−0.13%) | (3.60%) | (−0.91%) | (−0.28%) | (−3.59%) | (−0.46%) | (59%) | (4.82%) | (1.17%) | (−55%) | ||
| J0218-31 | −0.007 | 0.012 | −0.005 | −0.002 | −0.057 | −0.001 | 0.503 | 0.041 | 0.006 | −0.254 | |
| (−0.32%) | (3.32%) | (−0.23%) | (−0.55%) | (−3.68%) | (−0.23%) | (13%) | (2.65%) | (1.41%) | (−7%) | ||
| J1847+39 | −0.008 | 0.016 | −0.015 | −0.004 | −0.046 | −0.001 | 1.071 | 0.052 | 0.009 | −0.820 | |
| (−0.90%) | (5.57%) | (−1.50%) | (−1.39%) | (−4.36%) | (−0.33%) | (97%) | (4.93%) | (2.97%) | (−74%) | ||
| J1436-13* | −0.162 | 0.064 | −0.059 | −0.090 | −0.024 | −0.005 | −0.135 | 0.043 | 0.011 | −1.150 | |
| (−11.91%) | (15.68%) | (−4.34%) | (−22.05%) | (−2.03%) | (−1.02%) | (−6%) | (3.62%) | (−2.24%) | (−50%) | ||
 |
−0.39% | 5.07% | −1.02 % | −0.80 % | −3.84 % | −0.83 % | 63% | 4.31% | 2.11% | 43% | |
Notes. The measured values were subtracted from those in Table 3. For J2308−46 and J0218−31, we only considered the most probable solution in this work. We separately re-fitted with 10% third light (l3) and using the quadratic limb-darkening law over the Claret law (ldy) from which we re-measured only the radii of the stars in the systems. We also separately recalculate the masses of the stars in each system by changing mixing length parameter from 1.50 to 1.78 (αmlt) and a change in helium enhancement values from 0.00 to 0.02 (ΔY). We also show the mean of each column, 
, calculated with all values excluding those from J1436−13 (marked with an asterisk).
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