Showing 1–20 of 81 results
/ Date/ Name
Apr 20, 2010Lifting the Veil of Dust from NGC 0959: The Importance of a Pixel-Based 2D Extinction CorrectionMar 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 LBCJan 31, 2005High Resolution Studies of Radio Sources in the Hubble Deep and Flanking FieldsJan 31, 2012A Panchromatic Catalog of Early-Type Galaxies at Intermediate Redshift in the Hubble Space Telescope Wide Field Camera 3 Early Release Science FieldJun 12, 2008"GiGa": the Billion Galaxy HI Survey -- Tracing Galaxy Assembly from Reionization to the PresentJun 23, 2008Is the Optically Unidentified Radio Source, FIRST J121839.7+295325, a Dark Lens?Jun 11, 2012Newborn spheroids at high redshift: when and how did the dominant, old stars in today's massive galaxies form?Nov 17, 2022JWST/NIRCam Probes Young Star Clusters in the Reionization Era Sunrise ArcOct 28, 2015Do the Most Massive Black Holes at $z=2$ Grow via Major Mergers?Jul 24, 2025JWST spectroscopic confirmation of the Cosmic Gems arc at z=9.625 -- Insights into the small scale structure of a post-burst systemOct 11, 2024Extending the cosmic distance ladder two orders of magnitude with strongly lensed Cepheids, carbon AGB, and RGB starsJun 15, 2018Deep Extragalactic VIsible Legacy Survey (DEVILS): Motivation, Design and Target CatalogueApr 28, 2010UV-dropout Galaxies in the GOODS-South Field from WFC3 Early Release Science ObservationsNov 30, 2018LSST Observing Strategy White Paper: LSST Observations of WFIRST Deep FieldsJul 30, 2014The role of major mergers in the size growth of intermediate-mass spheroidsJul 3, 2001The LBDS Hercules sample of mJy radio sources at 1.4 GHz - II. Redshift distribution, radio luminosity function, and the high-redshift cut-offJul 31, 2002Old elliptical galaxies at z=1.5 and the Kormendy relationApr 24, 2002An HST Survey of the mid-UV Morphology of Nearby GalaxiesDec 18, 1996Detection of a Small Scale Cosmic Background Anisotropy at 3.6 cm