Fig. 9
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Photometric data for the eight spectroscopically confirmed quasars at z > 7 and the Owl-z best-fit solutions for quasars and MLT dwarfs. The original photometric data points are represented by blue squares. The best-fit quasar model is in dashed grey, the best-fit model for an MLT dwarf is in dashed brown, and the filter transmission curves are shown in solid light purple. Model photometry for best-fit solutions is represented by green triangles for quasars and red stars for MLT dwarfs.
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