Fig. 10.
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σ as a function of the estimated redshift fractional uncertainties (
) from four different template-fitting codes, binned by the magnitude of the sample. The color of the scatter shows the i-magnitude of each bin as noted in the colorbar. We used the COSMOS galaxies with 18 < i < 23 in the wide depth and SPHEREx + 7DS survey combination. Most of the error bars in each point are obscured by the markers.
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