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Fig. A.13

image

Left panel: overview of spectrum positions for HIFI and upGREAT maps. Right panel: zoom into the central map region. The sparse sampling of the HIFI map with 11-arcsecond spacing between OTF scans arises because half the OTF scan is spent observing the internal cold load andthere are gaps in coverage in the scan direction. HIFI observed in a ABBA format, so that we see two ON spectra taken in succession, followed by two load observations. HIFI and upGREAT beam size are overplotted for comparison at 11.4 and 14.1 arcseconds, respectively.

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