\begin{table}%t3
\caption{\label{cal_vinci}Calibrators used for the VINCI observations of Betelgeuse. }
\small%%\centerline

{
\begin{tabular}{r l l l}
\hline\hline
Name & Sp.Type & $d_{\rm UD}$ (mas) & Night \\
\hline
\object{$\varepsilon$ Peg} & K2Ib & $7.70 \pm 0.24$     & 2001 Oct. 12 (4)\\
\object{$\beta$ Cet}       & G9II-III & $5.18 \pm 0.05$ & 2001 Oct. 12 (6)\\
                  &          &                 & 2002 Dec. 06 (2)\\
\object{$\varepsilon$ Lep} & K4III & $5.90 \pm    0.06$ & 2001 Oct. 12 (3)\\
                  &       &                    & 2002 Dec. 06 (1)\\
                  &       &                    & 2003 Jan. 09 (1)\\
\object{Sirius}            & A1V   & $5.60 \pm 0.15$    & 2001 Oct. 12 (4)\\
                  &       &                    & 2002 Dec. 06 (1)\\
                  &       &                    & 2003 Jan. 07 (1)\\
                  &       &                    & 2003 Jan. 18 (6)\\
\object{$\delta$ CMa}      & F8Iab & $3.29 \pm  0.46 $  & 2001 Oct. 12 (2)\\
                   &       &                    & 2003 Jan. 07 (1)\\
\object{$\pi$ Eri}         & M1III & $4.8  \pm   0.5 $  & 2002 Dec. 06 (1)\\
\object{$\tau$ Pup}        & K1III & $4.38 \pm   0.07$  & 2002 Dec. 06 (1)\\
                   &       &                    & 2003 Jan. 09 (1)\\
\object{Procyon}           & F5IV-V & $5.37 \pm 0.11 $  & 2002 Dec. 06 (1)\\
                  &       &                    & 2003 Jan. 07 (1)\\
\object{1 Pup}             & K5III & $3.8  \pm   0.4 $  & 2002 Dec. 06 (1)\\
\object{$\chi$ Phe}        & K5III & $2.69 \pm   0.03 $ & 2002 Dec. 06 (1)\\
\object{$\iota$ Cet}       & K1.5III & $3.28 \pm  0.04$ & 2003 Jan. 07 (1)\\
\object{31 Ori}            & K5III & $3.55 \pm 0.06$    & 2003 Jan. 07 (1)\\
\object{$\theta$ CMa}      & K4III & $4.13 \pm   0.4$   & 2003 Jan. 07 (1)\\
\object{$\beta$ Cnc}       & K4III & $4.88 \pm   0.03$  & 2003 Jan. 07 (1)\\
                  &       &                    & 2003 Jan. 09 (2)\\
\object{$\zeta$ Hya}       & G9II-III & $3.1 \pm   0.2$ & 2003 Jan. 07 (1)\\
                  &       &                    & 2003 Jan. 09 (1)\\
\object{$\alpha$ Hya}      & K3II-III & $9.44 \pm   0.9$& 2003 Jan. 07 (1)\\
                  &       &                    & 2003 Jan. 09 (6)\\
                  &       &                    & 2003 Jan. 13 (6)\\
\object{$\iota$ Hya}       & K2.5III & $3.41 \pm   0.05$& 2003 Jan. 07 (2)\\
                  &       &                    & 2003 Jan. 09 (4)\\
                  &       &                    & 2003 Jan. 13 (4)\\
\object{$\mu$ Hya}         & K2.5III & $4.69 \pm   0.5$ & 2003 Jan. 09 (3)\\
                  &       &                    & 2003 Jan. 13 (9)\\
                  &       &                    & 2003 Jan. 15 (2)\\
\object{$\gamma^1$ Leo}    & K1IIIb & $7.70 \pm 0.70$   & 2003 Jan. 09 (3)\\
\object{$\beta$ Ori}       & B8Iab  & $2.43 \pm   0.05$ & 2003 Jan. 13 (16)\\
                  &       &                    & 2003 Jan. 14 (22)\\
                  &       &                    & 2003 Jan. 15 (15)\\
\object{V337 Car}          & K3IIa & $5.09 \pm   0.06$  & 2003 Jan. 14 (6)\\
\object{N Vel}             & K5III & $6.92 \pm 0.08$    & 2003 Jan. 07 (1)\\
\hline
\end{tabular}}
\smallskip
Note: Uniform-disk diameters ($d_{\rm UD}$) are 
taken from Richichi \& 
Percheron (\cite{richichi05}).  
The number of the observations of the 
individual calibrators on each night 
is indicated in parenthesis.  
\end{table}