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Fig. F.1


Comparison between GREAT spectra of the O i line (gray filled) with those observed with Herschel/PACS (red hatched). The blue spectrum results from the convolution of the GREAT spectrum with a Gaussian of 86.6 km s-1 width (FWHM). All spectra are normalized to unity at the continuum level. From top to bottom: W31C (G10.62), G34.26, and W49N.

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