Hathi, Nimish PCohen, S. H.Ryan, R EFinkelstein, S LMcCarthy, P JWindhorst, Rogier AYan, HKoekemoer, AntonRutkowski, M JO’Connell, R. W.Straughn, AmberDopita, MichaelBalick, BruceBond, Howard, E.Kimble, Randy AWalker, Alistair RWhitmore, Bradley2015-12-130004-637Xhttp://hdl.handle.net/1885/70984We 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 arcmin2 in the GOODAuthor/s retain copyrightKeywords: galaxies: evolution; galaxies: fundamental parameters; galaxies: high-redshift; ultraviolet: galaxies201310.1088/0004-637X/765/2/882016-02-24