Fig. 5
a) Close-up of LABOCA emission at core L (similar contour levels as in Fig. 2). Red cross represents the position of the IRAC 2 Spitzer emission at the position of core L. b) Spectral energy distribution of core L (black thick line) and the proto-BD candidates J041757-B, L328-IRS, and IC348-SMM2E (brown thin lines; Palau et al. 2012, 2014; Lee et al. 2013). Arrows represent upper limits.
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