Table 3: Calibrators used in the VLTI observations.
Star $\phi$ , $\Delta\phi$ Sp. T. Ref. # Obs.

(mas) (K) /Scans

12-Jan.-2002

$\alpha$ Cet $11.69\pm0.69$ M1.5III 1 3 / 1310

$\sigma$ Pup $6.66\pm0.10$ K5III 2 2 / 884

1 Pup $3.80\pm0.40$ K5III 2 3 / 741

$\zeta$ Hya $3.10\pm0.20$ G9II-III 2 2 / 450

$\alpha$ Hya $9.31\pm0.16$ K3II-III 1,3 4 / 649

$\alpha$ Ant $3.60\pm0.30$ K4III 2 2 / 501

$\delta$ Crt $3.10\pm0.20$ K0III 2 2 / 541

$\epsilon$ Crv $4.99\pm0.23$ K2III 1 3 / 1303

2-Oct.-2003

HR 7092 $2.81\pm0.03$ M0III 4 4 / 941

$\eta$ Cet $3.35\pm0.04$ K1.5III 4 4 / 1816

$\alpha$ Cet $11.69\pm0.69$ M1.5IIIa 1 4 / 1914

$\eta$ Eri $2.50\pm0.12$ K1III 2 3 / 1181

31 Ori $3.56\pm0.06$ K5III 4 6 / 2124

References:
1) CHARM Catalogue (Richichi & Percheron 2002);
2) VLTI/VINCI Calibrators Catalogue (Percheron et al. 2003);
3) VLTI measurement (ESO Press Release 06/2001);
4) Bordé et al. (2002).

**Table 3:** Calibrators used in the VLTI observations.
Star	$\phi$ , $\Delta\phi$	Sp. T.	Ref.	# Obs.
	(mas)		(K)	/Scans
12-Jan.-2002
$\alpha$ Cet	$11.69\pm0.69$	M1.5III	1	3 / 1310
$\sigma$ Pup	$6.66\pm0.10$	K5III	2	2 / 884
1 Pup	$3.80\pm0.40$	K5III	2	3 / 741
$\zeta$ Hya	$3.10\pm0.20$	G9II-III	2	2 / 450
$\alpha$ Hya	$9.31\pm0.16$	K3II-III	1,3	4 / 649
$\alpha$ Ant	$3.60\pm0.30$	K4III	2	2 / 501
$\delta$ Crt	$3.10\pm0.20$	K0III	2	2 / 541
$\epsilon$ Crv	$4.99\pm0.23$	K2III	1	3 / 1303
2-Oct.-2003
HR 7092	$2.81\pm0.03$	M0III	4	4 / 941
$\eta$ Cet	$3.35\pm0.04$	K1.5III	4	4 / 1816
$\alpha$ Cet	$11.69\pm0.69$	M1.5IIIa	1	4 / 1914
$\eta$ Eri	$2.50\pm0.12$	K1III	2	3 / 1181
31 Ori	$3.56\pm0.06$	K5III	4	6 / 2124

Source LaTeX | All tables | In the text

	1 Introduction
	2 Lunar occultation observations and data analysis
	3 Interferometric observations and data analysis
	4 Results and discussion
	5 Conclusions
	References