All Tables

Table 1: Top: Stokes parameters of significantly polarized Galactic clouds (above double line) and of Taurus complex (below double line). Bottom: Coordinates of the maximum of intensity, measured area, degree and orientation of polarization of these clouds. Systematic error bars are derived from the dispersion of the results with different filtering parameters on the timelines (see Sect. 6.4). Last line correspond to a 95% CL upper limit. Angles are counted counterclockwise, 0 being oriented towards the North Galactic Pole. A brightness of $1~{\rm mK_{RJ}}$ is equivalent to $4.36~{\rm MJy~sr}^{-1}$ using IRAS convention (constant $\nu I_{\nu }$ ) for Archeops 353 GHz bandpass filter. Absolute calibration error of 6% is not included.
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).