Showing 41–60 of 63 results
/ Date/ Name
Mar 14, 2019An Ultra Deep Field survey with WFIRSTMar 11, 2019Electromagnetic probes of primordial black holes as dark matterMar 11, 2019Populations behind the source-subtracted cosmic infrared background anisotropiesJun 5, 2018A Two-Dimensional Spectroscopic Study of Emission Line Galaxies in the Faint Infrared Grism Survey (FIGS) I: Detection Method and CatalogAug 8, 2017The Effect of Atmospheric Cooling on the Vertical Velocity Dispersion and Density Distribution of Brown DwarfsMar 1, 2017The Lyman Continuum escape fraction of faint galaxies at z~3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBCFeb 4, 2016Hubble Space Telescope Wide Field Camera 3 Observations of Escaping Lyman Continuum Radiation from Galaxies and Weak AGN at Redshifts $z$$\,\simeq\,$2.3-4.1Jun 26, 2012Stellar Populations of Lyman Break Galaxies at z=1-3 in the HST/WFC3 Early Release Science ObservationsJun 11, 2012Newborn spheroids at high redshift: when and how did the dominant, old stars in today's massive galaxies form?Jan 31, 2012A Panchromatic Catalog of Early-Type Galaxies at Intermediate Redshift in the Hubble Space Telescope Wide Field Camera 3 Early Release Science FieldJul 8, 2010The Size Evolution of Passive Galaxies: Observations from the Wide Field Camera 3 Early Release Science ProgramMay 17, 2010Hubble Space Telescope WFC3 Early Release Science: Emission-Line Galaxies from Infrared Grism ObservationsApr 28, 2010UV-dropout Galaxies in the GOODS-South Field from WFC3 Early Release Science ObservationsJun 23, 2008Is the Optically Unidentified Radio Source, FIRST J121839.7+295325, a Dark Lens?Jun 12, 2008"GiGa": the Billion Galaxy HI Survey -- Tracing Galaxy Assembly from Reionization to the PresentDec 4, 2007Galaxy Mergers at z>1 in the HUDF: Evidence for a Peak in the Major Merger Rate of Massive GalaxiesJun 7, 2006The James Webb Space TelescopeNov 14, 2005Clues to AGN Growth from Optically Variable Objects in the Hubble Ultra Deep FieldJul 31, 2002Old elliptical galaxies at z=1.5 and the Kormendy relationApr 24, 2002An HST Survey of the mid-UV Morphology of Nearby Galaxies