Disentangling the Faraday rotation sky | Astronomy & Astrophysics (A&A)

Open Access

Fig. 7

Inference results for the logarithmic ϱ_EM/DM (panel a) and $L_{{DM}^{2} / EM}$ ${{\rm{L}}_{{\rm{D}}{{\rm{M}}^2}/{\rm{EM}}}}$ (Fig. b)) skies. Both quantities highlight different aspects of the ionized ISM (see Eqs. (11) and (12) for their definitions and Sect. 2.3.1 for the accompanying discussion). The $L_{{DM}^{2} / EM}$ ${{\rm{L}}_{{\rm{D}}{{\rm{M}}^2}/{\rm{EM}}}}$ sky map is directly modeled in our work, while the ϱ_EM/DM map was calculated in a post-processing step.

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