2008/07/01 by Ohta, K., Yabe, K., Iwata, I. +4
#Astrophysics (astro-ph) #FOS: Physical sciences
paper · doi:10.48550/arxiv.0807.0138
Properties of Lyman Break Galaxies at z∼5 are presented and are compared with those at z∼ 2-3 LBGs to see evolution of LBGs from z∼5 to z ∼3-2. The LBGs at z∼5 are tend to have smaller stellar masses, but they may show large star formation rates and specific star formation rates.