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Table 3:

Calibrators used for the VINCI observations of Betelgeuse.
Name Sp.Type $d_{\rm UD}$ (mas) Night
$\varepsilon$ Peg K2Ib $7.70 \pm 0.24$ 2001 Oct. 12 (4)
$\beta$ Cet G9II-III $5.18 \pm 0.05$ 2001 Oct. 12 (6)
      2002 Dec. 06 (2)
$\varepsilon$ Lep K4III $5.90 \pm 0.06$ 2001 Oct. 12 (3)
      2002 Dec. 06 (1)
      2003 Jan. 09 (1)
Sirius A1V $5.60 \pm 0.15$ 2001 Oct. 12 (4)
      2002 Dec. 06 (1)
      2003 Jan. 07 (1)
      2003 Jan. 18 (6)
$\delta$ CMa F8Iab $3.29 \pm 0.46 $ 2001 Oct. 12 (2)
      2003 Jan. 07 (1)
$\pi $ Eri M1III $4.8 \pm 0.5 $ 2002 Dec. 06 (1)
$\tau$ Pup K1III $4.38 \pm 0.07$ 2002 Dec. 06 (1)
      2003 Jan. 09 (1)
Procyon F5IV-V $5.37 \pm 0.11 $ 2002 Dec. 06 (1)
      2003 Jan. 07 (1)
1 Pup K5III $3.8 \pm 0.4 $ 2002 Dec. 06 (1)
$\chi$ Phe K5III $2.69 \pm 0.03 $ 2002 Dec. 06 (1)
$\iota$ Cet K1.5III $3.28 \pm 0.04$ 2003 Jan. 07 (1)
31 Ori K5III $3.55 \pm 0.06$ 2003 Jan. 07 (1)
$\theta $ CMa K4III $4.13 \pm 0.4$ 2003 Jan. 07 (1)
$\beta$ Cnc K4III $4.88 \pm 0.03$ 2003 Jan. 07 (1)
      2003 Jan. 09 (2)
$\zeta$ Hya G9II-III $3.1 \pm 0.2$ 2003 Jan. 07 (1)
      2003 Jan. 09 (1)
$\alpha$ Hya K3II-III $9.44 \pm 0.9$ 2003 Jan. 07 (1)
      2003 Jan. 09 (6)
      2003 Jan. 13 (6)
$\iota$ Hya K2.5III $3.41 \pm 0.05$ 2003 Jan. 07 (2)
      2003 Jan. 09 (4)
      2003 Jan. 13 (4)
$\mu $ Hya K2.5III $4.69 \pm 0.5$ 2003 Jan. 09 (3)
      2003 Jan. 13 (9)
      2003 Jan. 15 (2)
$\gamma^1$ Leo K1IIIb $7.70 \pm 0.70$ 2003 Jan. 09 (3)
$\beta$ Ori B8Iab $2.43 \pm 0.05$ 2003 Jan. 13 (16)
      2003 Jan. 14 (22)
      2003 Jan. 15 (15)
V337 Car K3IIa $5.09 \pm 0.06$ 2003 Jan. 14 (6)
N Vel K5III $6.92 \pm 0.08$ 2003 Jan. 07 (1)
Note: Uniform-disk diameters ( $d_{\rm UD}$) are taken from Richichi & Percheron (2005). The number of the observations of the individual calibrators on each night is indicated in parenthesis.

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