Turning JWST/MIRI backgrounds into a survey of diffuse molecular hydrogen

Open Access

Fig. B.1

Integrated properties of the observational sample. Left panel: Distribution of the line-of-sight–averaged dust temperature, T_dust. Right panel: Distribution of the logarithm of the total hydrogen column density projected perpendicular to the Galactic plane, $N_{H}^{⊥}$ $Mathematical equation: $N_{\rm{H}}^ \bot $$ . Lines of sight classified as non-diffuse $T_{dust} > 25 K$ $Mathematical equation: ${T_{{\rm{dust}}}} > 25{\rm{K}}$$ are highlighted in color.

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