Showing 1–20 of 21 results
/ Date/ Name
May 13, 2024JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noonMar 27, 2024JWST Photometric Time-Delay and Magnification Measurements for the Triply-Imaged Type Ia "Supernova H0pe" at z = 1.78Sep 22, 2023PEARLS: JWST counterparts of micro-Jy radio sources in the Time Domain FieldSep 28, 2021The NuSTAR Extragalactic Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain FieldMar 14, 2019An Ultra Deep Field survey with WFIRSTMar 1, 2017The Lyman Continuum escape fraction of faint galaxies at z~3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBCJun 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 GalaxiesNov 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 GalaxiesOct 4, 1999NICMOS Imaging of the Dusty Microjansky Radio Source VLA J123642+621331 at z = 4.424Feb 8, 1998Morphological number-count and redshift distributions to I < 26 from the Hubble Deep Field: Implications for the evolution of Ellipticals, Spirals and Irregulars