Illustration of our redshift assignment procedure, we show an example for each z slice. We first fit the SED leaving z as a free parameter (upper fit for each slice), based on the z-probability density from that fit we then assign a slice and fit for that z value (lower fit for each slice). We also provide thumbnail images covering 6 × 6 arcsec² around each object in broad band filter images from U through Spitzer channel 4. Errors on the photometry are included in the figure, but are in almost all cases too small to be visible.