THE EVOLUTION OF THE ULTRAVIOLET LUMINOSITY FUNCTION FROM z similar to 0.75 TO z similar to 2.5 USING HST ERS WFC3/UVIS OBSERVATIONS
PA Oesch, RJ Bouwens, CM Carollo, GD Illingworth, D Magee, M Trenti, M Stiavelli, M Franx, I Labbe, PG van Dokkum
The Astrophysical Journal | IOP PUBLISHING LTD | Published : 2010
Awarded by NASA
We thank the GOODS and the GOODS-MUSIC teams for providing their data to the community. P.O. acknowledges support from the Swiss National Foundation (SNF). This work has been supported by NASA grant NAG5-7697 and NASA grant HST-GO-11563.