Fig. 6.
Example of observed SEDs of ALPINE continuum non-target sources with an identification and a photo-z in the available catalogues. The observed SEDs have been fitted with LE PHARE by fixing the redshift at the catalogue value: the best fit template to all the data is shown in black, while the template best reproducing the IR data (i.e. from 8 to 1000 μm rest frame, used to derive LIR) is shown in red.
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