Table 2: Top: Stokes parameters of $5^\circ $ Galactic longitude bands. The intensity is the average over the longitude band and btaken in the range  $[-2^\circ,~2^\circ]$. Q and U are scaled from that intensity using the latitude profile fit. Bottom: Degree and orientation of polarization for these bands. Angles are counted counterclockwise, 0 being oriented towards the North Galactic Pole. Due to incomplete sky coverage some longitude bands are not quoted. Systematic error bars are derived from the dispersion of the results with different filtering parameters on the timelines (Sect. 6.4).
Gal. Long. Range $(^\circ)$ $I\;({\rm mK_{RJ}})$ (stat) (syst) $Q\;({\rm mK_{RJ}})$ (stat) (syst) $U\;({\rm mK_{RJ}})$ (stat) (syst)
$ 85 \;\; 90 $ $ 1.34 \pm 0.093 \pm 0.040 $ $ -0.008 \pm 0.009 \pm 0.000 $ $ 0.001 \pm 0.008 \pm 0.004 $
$ 90 \;\; 95 $ $ 1.47 \pm 0.088 \pm 0.053 $ $ -0.012 \pm 0.008 \pm 0.002 $ $ 0.010 \pm 0.007 \pm 0.002 $
$ 95 \;\; 100 $ $ 1.12 \pm 0.085 \pm 0.052 $ $ 0.001 \pm 0.008 \pm 0.000 $ $ -0.019 \pm 0.007 \pm 0.003 $
$ 100 \;\; 105 $ $ 0.79 \pm 0.081 \pm 0.062 $ $ 0.030 \pm 0.008 \pm 0.001 $ $ 0.037 \pm 0.006 \pm 0.005 $
$ 105 \;\; 110 $ $ 1.03 \pm 0.076 \pm 0.062 $ $ 0.030 \pm 0.007 \pm 0.003 $ $ 0.038 \pm 0.006 \pm 0.001 $
$ 110 \;\; 115 $ $ 1.21 \pm 0.071 \pm 0.031 $ $ 0.033 \pm 0.007 \pm 0.000 $ $ 0.042 \pm 0.007 \pm 0.002 $
$ 115 \;\; 120 $ $ 0.62 \pm 0.069 \pm 0.029 $ $ 0.009 \pm 0.008 \pm 0.009 $ $ 0.030 \pm 0.009 \pm 0.006 $
$ 180 \;\; 185 $ $ 0.52 \pm 0.068 \pm 0.048 $ $ 0.027 \pm 0.008 \pm 0.011 $ $ -0.007 \pm 0.008 \pm 0.000 $
$ 185 \;\; 190 $ $ 0.59 \pm 0.061 \pm 0.055 $ $ 0.028 \pm 0.006 \pm 0.008 $ $ 0.002 \pm 0.007 \pm 0.004 $
$ 190 \;\; 195 $ $ 0.82 \pm 0.041 \pm 0.055 $ $ 0.044 \pm 0.005 \pm 0.011 $ $ 0.010 \pm 0.006 \pm 0.001 $
$ 195 \;\; 197 $ $ 0.43 \pm 0.029 \pm 0.042 $ $ 0.011 \pm 0.008 \pm 0.005 $ $ 0.013 \pm 0.009 \pm 0.003 $

Gal. Long. Range $(^\circ)$ $p\;(\%)$ (stat) (syst) $\theta\;(^\circ)$ (stat) (syst)
$ 85 \;\; 90 $ $ 0.2^{+ 0.6}_{- 0.5} \pm 0.1 $ $ 86 \pm 34 \pm 15 $
$ 90 \;\; 95 $ $ 0.9^{+ 0.5}_{- 0.5} \pm 0.3 $ $ 70 \pm 16 \pm 6 $
$ 95 \;\; 100 $ $ 1.6^{+ 0.7}_{- 0.6} \pm 0.4 $ $ 136 \pm 15 \pm 0 $
$ 100 \;\; 105 $ $ 6.0^{+ 0.9}_{- 0.8} \pm 1.0 $ $ 25 \pm 4 \pm 2 $
$ 105 \;\; 110 $ $ 4.7^{+ 0.6}_{- 0.7} \pm 0.6 $ $ 26 \pm 4 \pm 1 $
$ 110 \;\; 115 $ $ 4.3^{+ 0.5}_{- 0.6} \pm 0.2 $ $ 26 \pm 4 \pm 0 $
$ 115 \;\; 120 $ $ 4.8^{+ 1.3}_{- 1.5} \pm 1.6 $ $ 36 \pm 8 \pm 9 $
$ 180 \;\; 185 $ $ 5.2^{+ 1.6}_{- 1.4} \pm 2.6 $ $ 172 \pm 9 \pm 3 $
$ 185 \;\; 190 $ $ 4.6^{+ 1.0}_{- 1.0} \pm 1.9 $ $ 2 \pm 8 \pm 4 $
$ 190 \;\; 195 $ $ 5.4^{+ 0.6}_{- 0.6} \pm 1.7 $ $ 6 \pm 4 \pm 1 $
$ 195 \;\; 197 $ $ 3.5^{+ 1.9}_{- 2.1} \pm 1.6 $ $ 25 \pm 17 \pm 8 $


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