Table 5: Statistical parameters characterising the 86 GHz polarization variability of 0716+714 and the secondary calibrators, but 1928+738, during 2003 November 10-16.

Source		 N $\langle P\rangle $ $\sigma_{P}$ $\chi_{r,P}^{2}$ $\langle \chi\rangle$ $\sigma_{\chi}$ $\chi_{r,\chi}^{2}$
    [Jy] [Jy]   [$^{\circ }$] [$^{\circ }$]  

0212+735		 5 0.122 0.024 0.3 -33.1 6.0 0.2
0633+734 5 0.092 0.021 0.1 69.3 8.5 0.3
0716+714a 10 0.648 0.103 1.8 30.9 4.3 1.7
0716+714b 6 0.639 0.095 2.4 31.0 3.3 2.2
0836+710 6 0.085 0.020 0.2 -76.3 8.5 0.1
1642+690 5 0.064 0.023 0.1 54.6 17.6 0.3
1803+784 5 0.111 0.022 0.1 76.4 4.5 1.2
a0716+714 results for $\la $12 h.
b0716+714 results for <24 h are also presented to allow direct comparison with the secondary calibrators.
Note 1: $\langle P\rangle $ and $\langle \chi\rangle$ in this Table, which are based on P and $\chi $ fittings over <24 h time bins, are less accurate than those from Table 4, which where fitted over the whole time span of the observations.
Note 2: The weak linearly polarized flux density of 1928+738 (see Table 4) does not allow us to analyse its variability.

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