Image Details
Caption: Figure 11.
ASXDF1100.231.1 SED at observed optical/near-/mid-IR wavelengths. Top: Best-fit SEDs, without emission lines, toward ASXDF1100.231.1 for z = 3.5, 4.5 and 5.5, as obtained with Le Phare. Black points correspond to the observed flux densities, while arrows indicate 2σ upper limits. Bottom: Best-fit SEDs, this time including emission lines.
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