Table 1: Programme eclipsing binaries. Data from the Hipparcos Catalogue. $H_{\rm P}, B_{\rm T}, V_{\rm T}$ are out-of-eclipse median values.

Name		   Spct.   $H_{\rm P}$   $B_{\rm T}$   $V_{\rm T}$   $\alpha_{J2000}$   $\delta_{J2000}$ parallax         dist $\mu_\alpha$ $\mu_\delta$           
            (h m s)   ($^{\circ}$ ' '') (mas)           (pc) (mas yr-1)   (mas yr-1)    

V781 Tau		 HIP 27562 G0   8.71   9.41   8.74   05 50 13.12   +26 57 43.4   $ 12.31\pm1.35$    $\rm 81^{91}_{73}$   $-0.084 \pm 0.004$   $-0.091 \pm 0.004$

UV Leo		 HIP 52066 G0   9.20   9.78   9.00   10 38 20.77   +14 16 03.7   $10.85 \pm 1.16$    $\rm 91^{103}_{83}$   $-0.007 \pm 0.004$    $0.010 \pm 0.004$

GK Dra		 HIP 82056 G0   8.92   9.19   8.81   16 45 41.19   +68 15 30.9 $3.37 \pm 0.69$    $\rm 297^{373}_{246}$   $-0.013 \pm 0.002$    $0.014 \pm 0.002 $


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