Fig. B.1
SED fitting results obtained using BAGPIPES for ILTJ160227.18+544759.8, ILTJ160930.42+544435.9, ILTJ16209.13+544818.7, and ILTJ161447.04+550401.8 (in order from top to bottom). Left: reduced χ2 as a function of redshift. The redshifts corresponding to the [OIII], [OII], and Lyα emission lines are indicated, and both resulting reduced χ2 values using normal error (pink) and 10% extra flux error (grey) are shown. Right: posterior median model obtained from BAGPIPES (yellow) with z = 1.47 and over-plotted photometric fluxes as a function of wavelength (blue).
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