All Tables

Table 1: Summary of uncertainties attributed to the standard star spectra in the CWW network in the 2-200 $\mu$ m range.
Table 2: Summary of uncertainties attributed to the theoretical atmosphere spectra in the 2-200 $\mu$ m range at a resolution $\lambda$ / $\Delta$ $\lambda$ $\sim$ 100.
Table 3: Stellar parameters used to for the calculation of (1.) the M ARCS model atmosphere spectra (Cols. 2-5) and (2.) the Engelke function and blackbody (BB) (Cols. 6, 7) in Fig. 10. Effective temperature, T, is given in Kelvin, gravity, g, in cm/s², and angular diameter, $\theta_{\rm d}^{}$ , in mas.