All Tables

Table 1: Maximal cross-polarization discrimination angle $\phi _{{\rm XPD}}$ , $\Delta W_{{\rm max}}$ and the residual angle $\Delta _{\phi }$ for the 30 GHz and the 100 GHz feeds on positions 1, 4 and 27, for different orientations $\psi _{{\rm FP}}$ of the feeds being $\phi _{{\rm XPD}}$ determined by the 1st Method described in Sect. 2.2 and $\Delta W_{{\rm Max}}$ evaluated using Eq. (4).
Table 2: Same as Table 1, with $\phi _{{\rm XPD}}$ being determined by the 2nd Method, as described in Sect. 2.2.
Table 3: Same as Table 1, with $\phi _{{\rm XPD}}$ being determined by the 3rd Method, as described in Sect. 2.2.
Table 4: Misalignment angle between the y-axis of both the feed and the far-field coordinate systems, for each position of the feed in the focal plane. Feed positions are shown in Fig. A.3.
Table 5: Normalized Stokes parameters q_B and u_B for different limits of integration $\theta _0$ ; at FWHM, $3^{\circ }$ and $20^{\circ }$ . These parameters represent the optical spurious polarization introduced by PLANCK telescope optics for the studied focal plane configuration (in bold) and other study cases (see text).
Table A.1: Early PLANCK Telescope configuration used for the present study (current telescope dimensions are slightly different).