Nobunari Kashikawa ( National Astronomical Observatory of Japan ) appeared in Kashikawa et al., AJ, 125, 53, 2003 Rest-frame Luminosity Functions Based on The K’-Selected Galaxy Sample on The Subaru Deep Field
Feb 02, 2016
Nobunari KashikawaNational Astronomical Observatory of Japan
appeared in Kashikawa et al., AJ, 125, 53, 2003Rest-frame Luminosity Functions Based on The K-Selected Galaxy Sample on The Subaru Deep Field
Star Formation Rate Densityrest UV-LF SFRDbroadly consistent with previous results @z1.5 due to the shallower faint- end slope of our UV-LFIf the slope of the rest UV-LF @ z=3 is really as steep as =-1.6, our K-selected sample contributes only 42% of the total UV luminosity density @ z=358%faint blue galaxies @z>3but uncertainty is large
N(z) on SDF
consistent with previous obs. on K