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Fig. 5.

image

SED fittings to the broadband UV to submillimeter data with MAGPHYS at z = 4.19 (left panel) and z = 3.1 (right panel). The thick orange line represents the AGN component, with contributions that are estimated at 18% and 1% to the total IR SED, respectively. The red solid circles are the photometric data and the black lines are the best-fitting model. The corresponding data to model ratios are shown in the middle panels. The blue line represents the (unattenuated) star formation component. The attenuated stellar emission and the reproduced dust emission are shown with the green line. The posterior probability distribution of best-fitting parameters are shown in the lower panels. The dashed lines are the median values and the dotted lines are the best-fitting values.

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