The relation between galaxy structure and spectral type : implications for the buildup of the quiescent galaxy population at 0.5 < z < 2.0

We present the relation between galaxy structure and spectral type, using a K-selected galaxy sample at 0.5 1.5 and significantly smaller than all other galaxy types at the same redshift. This result suggests that the suppression of star formation may be associated with significant structural evolution at z > 1.5. At z < 1, galaxy types with intermediate sSFRs (10(-11.5)-10(-10.5) yr(-1)) do not have post-starburst SED shapes. These galaxies have similar sizes as older quiescent galaxies, implying that they can passively evolve onto the quiescent sequence, without increasing the average size of the quiescent galaxy population