Observed photometry of object GOODS-S 31759 with the best fit solutions at the two possible spectroscopic redshifts of z = 1.393 (black curve) and z = 6.34 (red curve and blue curve) corresponding respectively to the identification of the emission line visible in the spectrum as the [OII] doublet or the Lyα line. The two SEDs for the high-redshift solution correspond to models with and without nebular contribution (blue and red, respectively).
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