Fig. 13

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NHI of WNM, CNM, and LNM over the column density interval 0.03 · 1020 ≤ NHI cm−2 ≤ 9.5 · 1020 according to Kalberla & Haud (2018) versus Tdust in bins of 0.5 K for central sight lines with H I 21-cm absorption detections (left) and non-detections (right). The error bars represent the scatter as the median absolute deviation (MAD), corresponding to 0.68σ for normally distributed data.
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