All Tables

Table 1: Narrow band filter characteristics and interferometric coupler splitting ratios as measured in laboratory calibrations.
Table 2: Reference sources.
Table 4: Photometric data.
Table 5: Model fit of the 1997 K band data and 2000 L' band data of R Leo and comparison with the results obtained by Mennesson et al. (2002).
Table 6: Model fit of the 2001 K band data and 2000 L' band data of R Leo.
Table 7: Model fit parameters of the October 2000 narrow band data and November 2000 L' band data and of the November 2001 narrow band data of Mira.
Table 8: Model fit parameters of the May 2002 narrow band data of T Cep.
Table 9: Model fit parameters of the October 2000 narrow band and November 2000 L' band data and of the November 2001 data of U Ori. It was not possible to estimate useful error bars for several of the parameters with the 2000 dataset.
Table 10: Model fit parameters of the November 2001 and May 2002 narrow band data of $\chi$ Cyg.
Table 11: Model fit parameters of the October 2000 wide K' band data of R Tri with FLUOR and PTI.
Table 12: Comparison of model $T_\star$ with the excitation temperature of the "cool'' CO component observed spectroscopically at a similar phase by Hinkle et al. (1984, 1997). Typical error estimates are 100 K for T_* and 200 K for excitation temperature $T_{{\rm exc}}$ .
Table 13: Comparison between the radius of the layer reported in this paper and the average radius of the SiO maser ring of Cotton et al. (2004) for R Leo, Mira and U Ori.
Table 14: Linear radii derived from angular radii determined in this study. Parallaxes are from Hipparcos except for U Ori which was derived from a period-luminosity relation (Whitelock et al. (2000b)). $T_{{\rm PE}}$ is the pseudo-effective temperature defined in this paper and determined from the observed luminosity $L_\star$ and our diameter measurements R_*.
Table 3: Log of observations.