Fig. D.2
Masses MF derived from fitting Fν for the isothermal models of both isolated and embedded starless cores and protostellar envelopes. Compared to the results for isolated models, all derived masses of embedded models are underestimated by approximately a factor of 1.3, owing to background over-subtraction (Sect. 5.2). See Fig. D.1 for SEDs and Fig. 6 for more details.
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