Early-type galaxies are not the simple Population II systems they have long been assumed to be. While upwards of 80% of the stellar mass of early-type galaxies likely formed at high redshift, small frostings of intermediate-age stellar populations (a few to 20% percent by mass of 1-2 Gyr old stars) are present in nearly every field and group early-type galaxy and in at least some cluster early-types. These frostings of young stars have little effect on the determination of photometric redshifts, thanks to the age-metallicity degeneracy of broad-band colors, but even mild bursts of star formation at modest redshifts (a few tenths) may make identification of the progenitors of todays early-type galaxies difficult at cosmological distances.
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