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Fig. A.1
Spectral energy distributions of the CORNISH Hii regions with Hi-GAL counterparts of at least three bands. In addition to Hi-GAL, the MSX 21 μm, WISE 22 μm, ATLASGAL 870 μm, and BGPS 1.1 mm flux densities have also been used. The number in each box identifies the source according to the numbering in Table A.1.
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