All Tables

Table 1: $E_{f, {\rm Smooth}}^{{\rm FD}}$ estimated according to Eq. (4).
Table 2: Correlation between Galaxy, ZLE and Differential ZLE at 857 GHz, for $\mbox{$r_{{\rm dsc}}$ }= 1^\circ$ , $\mbox{$\beta$ }= 85^\circ$ , $\mbox{$\delta\ell$ }= 2^\circ$ .
Table 3: Expected effect at 857 GHz of an isotropic, random pointing error on the E_f sensitivity as a function of $\mbox{$\sigma_{{\rm p}}$ }$ . Calculations are for a cut of 1 MJy/sr on the Galaxy and $1^\circ$ and $2^\circ$ patches.
Table 4: Effect of a random relative calibration error $\mbox{$E_{{\rm r},2^\circ}$ }= 1\%$ on the E_f determination at different PLANCK frequencies. Column 2 is the minimum rms error for the optimal surface brightness cut reported in Col. 3. Columns 4 and 5 give the range for which the rms error is less than twice the value in Col. 2.