Fig. 1.

Comparison between photometric and spectroscopic redshifts for galaxies spectroscopically confirmed at z ∼ 3 − 7. Long-dashed and dashed lines display the locus of zphot = zspec ± 0.05(1 + z) and ±0.15(1 + z) respectively, and the solid black line is the one-to-one relation. Colors encode the observed magnitudes in the F125W filter, showing that the vast majority of galaxies with poor photometric redshifts have m(F125W) ≥ 28.
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