Table 3: Limb darkened angular diameters and linear radii for the five program stars.
Star Baseline Band ( $\lambda_{\rm eff}$) $\rho^{{a}}$ $\theta_{\rm LD} \pm \sigma_{\rm stat} \pm \sigma_{\rm syst}$ [mas] $R \pm \sigma_{\rm tot} [R_{\odot}]$ $\chi^2_{\rm red}$

$\tau $ Cet		 B3-M0 K (2.179 $\mu $m) 1.025 2.078 $\pm$ 0.014 $\pm$ 0.028 0.816 $\pm$ 0.013 0.57

$\epsilon $ Eri		 UT1-UT3 + B3-M0 K (2.179 $\mu $m) 1.027 2.148 $\pm$ 0.010 $\pm$ 0.027 0.743 $\pm$ 0.010 0.17

$\beta $ Leo		 B3-M0 K (2.177 $\mu $m) 1.014 1.449 $\pm$ 0.014 $\pm$ 0.023 1.728 $\pm$ 0.037 1.32

$\beta $ Pic		 UT1-UT3 K (2.177 $\mu $m) 1.014 0.849 $\pm$ 0.060 $\pm$ 0.100 1.759 $\pm$ 0.241 1.19

$\alpha $ PsA		 UT1-UT3 + B3-M0 K (2.177 $\mu $m) 1.014 2.222 $\pm$ 0.021 $\pm$ 0.015 1.835 $\pm$ 0.022 0.41
  E0-G1 K (2.177 $\mu $m) 1.014 2.321 $\pm$ 0.042 $\pm$ 0.046 1.917 $\pm$ 0.054 0.44
  E0-G1 H (1.632 $\mu $m) 1.016 2.235 $\pm$ 0.056 $\pm$ 0.046 1.846 $\pm$ 0.061 0.15
  All baselines K (2.177 $\mu $m) 1.014 2.228 $\pm$ 0.011 $\pm$ 0.020 1.840 $\pm$ 0.023 0.62
a
The linear limb-darkening coefficients were taken from Claret tables (Claret 2000)
to compute the conversion factor $\rho$.


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