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Fig. H.1


The CO and H2O rotational diagrams for NGC 1333-IRAS4B and Serpens SMM1. Both the full spectroscopy line and the selected lines observed in the line scan mode are shown. Two component fit is done to the CO diagram with the break at 1700 K (i.e. transitions J ≥ 24 correspond to the warm component) and a single component fit to the H2O diagram. Errors associated with the fit are shown in the brackets.

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