Table 4
Observed quantities and predictions for each of the six stars with the five different surface corrections.
Name | Corr. | Teff/K | log g | [Fe/H] s | L/L⊙ | R/R⊙ | χ 2 |
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o | 5248 ± 130 | 3.826 ± 0.013 | 0.250 ± 0.230 | 3.246 ± 0.445 | 2.175 ± 0.070 | |||
c | 5409 ± 51 | 3.835 ± 0.001 | 0.073 ± 0.032 | 3.983 ± 0.173 | 2.275 ± 0.008 | 229.5 | 10.9 | |
b | 5434 ± 47 | 3.834 ± 0.001 | 0.061 ± 0.028 | 4.065 ± 0.158 | 2.277 ± 0.006 | 204.5 | 10.2 | |
A | s | 5255 ± 45 | 3.831 ± 0.001 | 0.170 ± 0.026 | 3.495 ± 0.141 | 2.258 ± 0.006 | 325.6 | 16.3 |
p | 5545 ± 37 | 3.837 ± 0.001 | −0.005 ± 0.021 | 4.443 ± 0.126 | 2.287 ± 0.004 | 237.9 | 11.9 | |
k | 5532 ± 10 | 3.848 ± 0.000 | −0.086 ± 0.007 | 4.706 ± 0.035 | 2.364 ± 0.003 | 4467.4 | 212.7 | |
o | 5540 ± 60 | 3.761 ± 0.010 | −0.090 ± 0.060 | 4.935 ± 0.404 | 2.413 ± 0.075 | |||
c | 5708 ± 21 | 3.757 ± 0.001 | −0.207 ± 0.016 | 5.764 ± 0.103 | 2.458 ± 0.006 | 308.6 | 14.0 | |
b | 5746 ± 26 | 3.757 ± 0.001 | −0.223 ± 0.017 | 5.865 ± 0.112 | 2.447 ± 0.006 | 258.3 | 12.3 | |
B | s | 5690 ± 28 | 3.758 ± 0.002 | −0.201 ± 0.020 | 5.713 ± 0.130 | 2.462 ± 0.010 | 401.1 | 19.1 |
p | 5846 ± 25 | 3.756 ± 0.001 | −0.272 ± 0.015 | 6.250 ± 0.101 | 2.440 ± 0.005 | 297.2 | 14.2 | |
k | 5811 ± 9 | 3.769 ± 0.001 | −0.268 ± 0.006 | 6.636 ± 0.044 | 2.544 ± 0.004 | 2510.7 | 114.1 | |
o | 4978 ± 167 | 3.758 ± 0.013 | 0.240 ± 0.160 | 2.870 ± 0.511 | 2.268 ± 0.074 | |||
c | 5098 ± 12 | 3.773 ± 0.001 | 0.084 ± 0.008 | 3.231 ± 0.029 | 2.307 ± 0.005 | 19.7 | 1.2 | |
b | 5100 ± 14 | 3.773 ± 0.001 | 0.084 ± 0.009 | 3.236 ± 0.040 | 2.307 ± 0.006 | 19.2 | 1.2 | |
C | s | 5075 ± 13 | 3.776 ± 0.001 | 0.079 ± 0.009 | 3.223 ± 0.033 | 2.325 ± 0.005 | 36.8 | 2.3 |
p | 5247 ± 27 | 3.770 ± 0.001 | 0.027 ± 0.014 | 3.535 ± 0.058 | 2.278 ± 0.008 | 53.8 | 3.4 | |
k | 5114 ± 10 | 3.767 ± 0.001 | 0.125 ± 0.006 | 3.174 ± 0.021 | 2.272 ± 0.004 | 457.1 | 26.9 | |
o | 5264 ± 60 | 3.704 ± 0.011 | −0.150 ± 0.060 | 5.426 ± 0.486 | 2.802 ± 0.098 | |||
c | 5433 ± 17 | 3.688 ± 0.001 | −0.333 ± 0.019 | 5.667 ± 0.095 | 2.690 ± 0.007 | 224.7 | 8.6 | |
b | 5407 ± 19 | 3.688 ± 0.001 | −0.324 ± 0.017 | 5.582 ± 0.104 | 2.696 ± 0.008 | 199.5 | 8.0 | |
D | s | 5461 ± 15 | 3.690 ± 0.001 | −0.370 ± 0.014 | 5.875 ± 0.077 | 2.711 ± 0.006 | 443.8 | 17.8 |
p | 5445 ± 21 | 3.688 ± 0.001 | −0.366 ± 0.012 | 5.708 ± 0.094 | 2.688 ± 0.007 | 284.9 | 11.4 | |
k | 5470 ± 13 | 3.695 ± 0.000 | −0.384 ± 0.007 | 6.080 ± 0.063 | 2.749 ± 0.003 | 1718.1 | 66.1 | |
o | 5115 ± 60 | 3.670 ± 0.008 | 0.410 ± 0.060 | 4.646 ± 0.385 | 2.747 ± 0.082 | |||
c | 5056 ± 40 | 3.689 ± 0.001 | 0.124 ± 0.014 | 4.927 ± 0.157 | 2.896 ± 0.007 | 223.0 | 8.9 | |
b | 4989 ± 62 | 3.686 ± 0.001 | 0.168 ± 0.014 | 4.595 ± 0.227 | 2.873 ± 0.005 | 153.8 | 6.4 | |
E | s | 4995 ± 29 | 3.686 ± 0.001 | 0.169 ± 0.011 | 4.622 ± 0.109 | 2.874 ± 0.006 | 160.8 | 6.7 |
p | 5038 ± 44 | 3.683 ± 0.002 | 0.150 ± 0.008 | 4.692 ± 0.143 | 2.846 ± 0.009 | 339.9 | 14.2 | |
k | 4845 ± 9 | 3.700 ± 0.000 | 0.174 ± 0.005 | 4.434 ± 0.035 | 2.993 ± 0.002 | 6195.3 | 247.8 | |
o | 5120 ± 55 | 3.580 ± 0.009 | −0.400 ± 0.080 | 4.898 ± 0.464 | 2.814 ± 0.111 | |||
c | 5183 ± 21 | 3.575 ± 0.002 | −0.424 ± 0.022 | 4.920 ± 0.081 | 2.754 ± 0.011 | 64.8 | 3.2 | |
b | 5182 ± 19 | 3.574 ± 0.001 | −0.412 ± 0.018 | 4.896 ± 0.085 | 2.749 ± 0.011 | 54.9 | 2.9 | |
F | s | 5169 ± 19 | 3.578 ± 0.002 | −0.438 ± 0.015 | 4.943 ± 0.112 | 2.776 ± 0.014 | 131.4 | 6.9 |
p | 5267 ± 15 | 3.578 ± 0.002 | −0.487 ± 0.012 | 5.300 ± 0.067 | 2.768 ± 0.012 | 188.1 | 9.9 | |
k | 5561 ± 8 | 3.600 ± 0.000 | −0.488 ± 0.005 | 7.468 ± 0.049 | 2.948 ± 0.003 | 2378.0 | 118.9 |
Notes. The labelling is as in Table 3, with an extra row “o” that gives the observed quantities. The effective temperature Teff and surface metallicity [Fe/H] s are as listed by Deheuvels et al. (2014). The other observables – surface gravity log g, luminosity L and radius R – are derived from the scaling relations. The last two columns give the total χ2 (Eq. (6)) and χ2 per degree of freedom.
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