All Tables

Table 1: Best fit parameters obtained by modelling the angular power spectra of the northern and southern cuts at 1420 MHz according to Eq. (1).
Table 2: As in Table 1 but at 408 MHz.
Table 3: Frequency spectral index of the Galactic synchrotron fluctuations between 408 MHz and 1420 MHz derived from the APS.
Table 4: Characteristics of the synchrotron APS best fit parameters derived in the local analysis of the 408 MHz map. k₁₀₀¹ refers to the patches covering about the brightest half of the sky, which includes the Galactic plane and the NPS. k₁₀₀² correspond to the other half with weak high latitude emission.
Table 5: As in Table 4, but at 1420 MHz.
Table 6: Characteristics of the source term derived in the local analysis at 1420 MHz for $\vert b_{\rm gal}\vert {\protect\ga} 45^{\circ}$ ( $c^{\rm src}_{1}$ ) and $\vert b_{\rm gal}\vert {\protect\la} 45^{\circ}$ ( $c^{\rm src}_{2}$ ).