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Fig. 8


Observed (black and white squares) and best-fit SEDs (solid lines) of a z = 5.786 galaxy. White squares show bands not used in the SED fitting because of possible impact of the Lyα line. The error bars of the observed wavelength indicate the surface of the normalized filter transmission curve. SED fits in blue and red are based on Bruzual & Charlot (2003) models with (red) and without (yellow) nebular emission, and a fit using BPASSv2.0 (Eldridge & Stanway 2016; Stanway et al. 2016) is shown in blue (Sect. 4.4). Color crosses show the synthesized flux in the filters. Without nebular emission, age and stellar mass are ~ 109 yr and ~ 1010.5M respectively, while accounting for nebular emission gives ~ 106 yr and ~ 109M.

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