All Tables

Table 1: Limb darkening corrections $k = \theta _{\rm LD} / \theta _{\rm UD}$ derived from the linear limb darkening coefficients determined by Claret (2000). The k_R coefficients were used for the GI2T measurements, k_R/I forthe NPOI, k_H for the PTI, and k_K for VINCI/VLTI and FLUOR/IOTA
Table 2: Pulsation parameters (T₀ is the Julian date of the reference epoch, P is the period in days) and color excesses (from Fernie 1990) for the Cepheids discussed in this paper. (B-V)₀ is the mean dereddened (B-V) color as reported in the online database by Fernie et al. (1995).
Table 4: Surface brightness relations using $\it BVR{I}JHK$ based colors: $F_\lambda (C_\lambda - C_1) = a_\lambda (C_\lambda - C_1)+ b_\lambda$ . The 1 $\sigma$ errors in each coefficient are given in superscript, multiplied by 1000 to reduce the length of each line, i.e. -0.2944^2.4 stands for $-0.2944 \pm 0.0024$ . The standard deviation of the residuals $\sigma$ is listed for each SB relation, together with the reduced $\chi ^2$ of the fit and the total number of measurements $N_{\rm meas}$ taken into account (photometric data were unavailable for some stars).
Table 3: Interferometric and photometric data used in the present paper. The references for the interferometric measurements are: Nordgren et al. (2000, N00), Mourard et al. (1997, M97), Nordgren et al. (2002, N02), Lane et al. (2002, L02), and Kervella et al. (2004a, K04). JD is the Julian date of the measurement, $\lambda$ the interferometric measurement wavelength (in $\mu$ m), $\phi$ the phase, $\theta _{\rm UD}$ the uniform disk and $\theta _{\rm LD}$ the limb darkened angular diameters (in mas). The magnitudes are corrected for interstellar extinction (see Sect. 3.2).