All Tables

Table 1: Continuum and 3- $\sigma$ noise level in the antenna temperature scale on the CO(1-0) and CO(2-1) spectral bands.
Table 2: Collisional line width $\gamma$ $\rm [cm^{-1}~atm^{-1}]$ (at 300 K) and temperature dependence factor n for NH₃, PH₃ and CO with H₂ and He and for Saturn and Uranus (a blank space means that no data is available).
Table 3: Saturn and Uranus physical characteristics (Conrath & Gautier 2000; de Graauw et al. 1997; Baines et al. 1995; Conrath et al. 1987; Lindal 1992).