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Fig. 1.

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Calibration of the antenna temperature of the HFI 857 GHz map in NHI units. Left panel: HFI 857 GHz map intensity observable within a dust-gas correlation region, characterised by low NHI values, a low contribution of intermediate- or high-velocity clouds (IVC and HVC) to the NHI values, and a low contamination from thermal SZ sources (see details in Sect. 3). Right panel: pixel-to-pixel correlation and linear regression between the HFI 857 GHz and HI4PI NHI maps in the sky region visible in the left panel.

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