Fig. 15.

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Examples of photometry at z = 6 showing how different assumptions affect the emergent SEDs. For the same galaxy we show different MBH, fEdd and lines of sight. The galaxy photometry is calculated along the same line of sight as that of the AGN. The SFR is in units of M⊙ yr−1 and masses in units of M⊙ inside the logarithm. The NIRCAM response for the filters analyzed in this paper is shown in gray.
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