All Tables

Table 1: Observing log of IRS 3. The wavelength dependent ${\it TF}$ has been estimated for each night on the basis of regularly conducted calibrator measurements, typically about once per hour (Sect. 2). The number of calibrators used per night is given, and the applied parameters are given in Table 2.
Table 2: Parameters of the calibrators used for estimating the transfer function.
Table 3: Measured mean visibility moduli below and above the silicate absorption, centered at 9.8 $\mu$ m.
Table 4: Temperatures from the N-band MIDI data based on size and relative flux estimates of the two-Gaussian model and $\tau = 0.5$ of the outer dust.
Table 5: Best parameters of the RT models, shown in Figs. 18-22. The dust shell was confined to end at a radius of $10^4~R_{\rm i}$ .