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.
Parameter, x $x_{\rm min}$ $x_{\rm max}$ $\langle x \rangle$ $\sigma_{x}$ $\%~(x \in \langle x \rangle \pm \sigma_{x})$

$\alpha$ -3.50 -0.70 -2.70 0.60 54

${\rm log}(k_{100}^{1}/{\rm mK}^2)$ 2.90 5.90 3.80 0.81 70

${\rm log}(k_{100}^{2}/{\rm mK}^2)$ 1.00 2.90 2.40 0.36 69

**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.
Parameter, x	$x_{\rm min}$	$x_{\rm max}$	$\langle x \rangle$	$\sigma_{x}$	$\%~(x \in \langle x \rangle \pm \sigma_{x})$
$\alpha$	-3.50	-0.70	-2.70	0.60	54
${\rm log}(k_{100}^{1}/{\rm mK}^2)$	2.90	5.90	3.80	0.81	70
${\rm log}(k_{100}^{2}/{\rm mK}^2)$	1.00	2.90	2.40	0.36	69

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