Image Details
Caption: Figure 13.
Comparison between our estimates (using the da Cunha et al. 2008 models) and estimates using three typical galaxy templates of (a) infrared luminosity; (b)–(d) distribution of continuum flux density at 345, 230, and 100 GHz (ALMA bands 7, 6, 3; PdBI/NOEMA bands 4, 3, 1), respectively.
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