All Tables

Table 1: Observing log. The total integration time, mutual observing time with HALCA, total flux density, the uniform weighted beam size, and the residual noise are given for each epoch and each source.
Table 2: Comparison of the polarization properties of 0836+710 on single-dish ( $P_{\rm Eff}$ and $\chi _{\rm Eff}$ ) and VLBI ( $P_{\rm VLBI}$ and $\chi _{\rm VLBI}$ ) scales. Using the fixed EVPA from Effelsberg, the measured EVPA from VLBI was corrected by $\Delta \chi = \chi _{\rm Eff} - \chi _{\rm VLBI}$ . The different value for the correction in the last epoch is due to the choice of a different reference antenna during the calibration.
Table 3: Effelsberg observing log. Shown are the mean flux density, $\langle S\rangle$ , the number of scans, N, the modulation index, m, and the reduced $\chi ^2_{\rm r}$ from a linear fit (see text for details).
Table 4: Summary of the ground VLBI maps.
Table 5: Summary of the flux densities of the VSOP maps (Note that reliable measurements of the jet's linear polarization were not possible).
Table 6: Linear polarization as observed by Effelsberg. $\langle \rangle$ indicate mean values.
Table 7: The VLBI results in comparison with the single-dish measurements from Effelsberg. The total linear polarization values of the VLBI images were calculated from the vector sum of the core and the jet polarization vectors.
Table 8: Linear polarization variability from two time intervals of VLBI data (October 4th) in comparison to the single-dish measurements from Effelsberg.