The coherent magnetic field of the Milky Way halo, the Local Bubble, and the Fan region

Open Access

Table 1

The result of the global fit.

	χ²	χ²/ndf	ndf	$χ_{var}^{2}$ $\chi _{{\rm{var}}}^2$	$χ_{var}^{2} / ndf$ $\chi _{{\rm{var}}}^2/{\rm{ndf}}$
RM	544	1.92	283	145	0.51
Q	385	1.11	348	238	0.68
U	482	1.38	348	251	0.72

Total	1411	1.36	1037	634	0.61

Notes. First three columns show the performance of the best-fit model: the overall χ² and χ² per degree of freedom, as well as their breakup between RM and polarisation Q and U maps. The last two columns show the same quantities when the standard deviation within the bins (calculated after removal of outliers) is taken as an error estimate.

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