All Tables

Table 1: Weighted scaling factors for the individual bands for different measurements of our program stars.
Table 2: Fundamental stellar parameters for our sample stars as determined by Decin (2000). The effective temperature $T_{{\rm eff}}$ is given in K, the logarithm of the gravity in cgs units, the microturbulent velocity $\xi _{\rm t}$ in km s^-1, the angular diameter in mas, the parallax $\pi$ in mas, the distance D in parsec, the radius R in $R_{\odot }$ , the gravity-induced mass $M_{\rm g}$ in $M_{\odot }$ and the luminosity L in $L_{\odot }$ . PP denotes a plane-parallel geometry, SPH a spherical geometry.
Table 3: Scaling factors between the IRAS-PSC & LRS products and the MARCS model spectra.
Table 4: Line lists used for the synthetic spectra.
Table 5: Estimated uncertainties of the different instrumental artifacts present in band 3 for the 10 AOT 01 speed 4 spectra of our sample of standard stars.