at $z_\mathrm{spec}\!<$1.5 in AEGIS from the DEEP2 survey [@Davis03] with $\sigma_{z}$/(1+$z$)=0.017. Both fields have very few catastrophic failures, with only 3% $>$5$\sigma$ outliers. Spectroscopic redshifts also exist for 125 Lyman Break Galaxies (LBGs) at $z\!\sim$3 within the AEGIS field from @Steidel03, for which we find $\sigma_{z}$/(1+$z$)=0.045, with 10% $>$5$\sigma$ outliers. However, we note that LBGs are very faint in the rest-frame optical (observer’s near-IR) and their spectra have relatively weak Balmer/4000Å breaks. There is excellent agreement between the NMBS photometric redshifts and the Gemini/GNIRS redshifts from @Kriek06, with a biweight scatter in ($z_{\mathrm{phot}}-z_{\mathrm{spec}}$)/(1+$\!z_{\mathrm{spec}}$) of only 0.010, albeit this is only for four galaxies [see @vanDokkum09a]. The photometric redshift accuracies range from $\sigma_{z}$/(1+$z$)$\sim\!0.01$ for galaxies with stronger Balmer/4000Å breaks to $\sigma_{z}$/(1+$z$)$\sim\!0.05$ for galaxies with less defined breaks. The lack of spectroscopic redshifts above $z\sim\!1$ highlights the necessity for both follow-up spectroscopy at high redshift, as well as the innovation of new techniques to accurately diagnose the reliability of the photometric redshifts [see @Quadri09].

From the best-fit EAZY template, we compute the rest-frame $U$-$V$ colors following the method used by @Wolf03 in the COMBO-17 survey. We measure the rest frame $U$-$V$ color from the best-fit template, using the filter definitions of @Maiz06. 