Photometric vs. spectroscopic redshift comparison of objects selected as LAEs and LBGs. The red line indicates the one-to-one relation, and the dashed black lines indicate the typical error bounds of |z_spec − z_phot|< 0.15(1 + z_spec) and |z_spec − z_phot|< 0.05(1 + z_spec). Almost all of the photometric redshifts agree with their spectroscopic equivalents within the outer of these two bounds. Those that do not tend to be fainter objects, with magnitudes of 28 and above.