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STELLAR POPULATIONS OF LYMAN BREAK GALAXIES AT<i>z</i>โ 1-3 IN THE<i>HST</i>/WFC3 EARLY RELEASE SCIENCE OBSERVATIONS
We analyze the spectral energy distributions (SEDs) of Lyman break galaxies (LBGs) at z=1-3 selected using the Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) UVIS channel filters. These HST/WFC3 observations cover about 50 sq. arcmin in the GOODS-South field as a part of the WFC3 Early Release Science โฆ