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Fig. 1


Percentage of the recovered flux in the ALMA observations of 12CO J = 3−2 when compared to JCMT observations. The points show the percentage of recovered flux across channels (left vertical axis), with error bars including uncertainties in the calibration of both instruments. The filled, grey histogram corresponds to the total recovered flux profile of NGC 6302 in the 12CO J = 3−2 ALMA maps convolved with the HPBW of JCMT at 345 GHz and at the position observed by Peretto et al. (right vertical axis). The emission around VLSR = −62 km s-1, which is not present in the 13CO J = 3−2 map, is actually contamination from NS (see Fig. A.1).

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