Fig. 10.
Observed SEDs for HST+near-IR-dark galaxies, with their tentative best fitting templates (black for the broad-band SED and red for the far-IR SED, as in Fig. 6) and photometric redshifts found with LE PHARE. For all but one source, the fits are based only on the IRAC and ALMA data points, combined with the 3σ UV, optical, near- and far-IR 3σ upper limits.
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