Fig. 4
SED of the Class 0 source including the Herschel and NIKA detections and the MIPS 24 μm upper limit (non-detection) compared to the emission of several modified blackbodies with temperatures 15 and 17 K, β = 1.9, 1.7, and 1.5, and k70 = 118 and 505 cm2g−1 (see discussion in text). Error bars are smaller than the dots for the Herschel data.
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