Showing 21–40 of 134 results
/ Date/ Name
Nov 22, 2009The WiggleZ Dark Energy Survey: Survey Design and First Data ReleaseFeb 13, 1998The Slope of the Cluster Elliptical Red Sequence: A Probe of Cluster EvolutionJan 28, 2009Subaru Weak Lensing Measurements of Four Strong Lensing Clusters: Are Lensing Clusters Over-Concentrated?Feb 26, 2010Two Lensed z~3 Lyman Break Galaxies Discovered in the SDSS Giant Arcs SurveyDec 16, 2023JWST Early Release Science Program TEMPLATES: Targeting Extremely Magnified Panchromatic Lensed Arcs and their Extended Star formationFeb 27, 2014The Mass-Independence of Specific Star Formation Rates in Galactic DisksMay 2, 2014Resolved Star Formation on Sub-galactic Scales in a Merger at z=1.7Oct 31, 2018The importance of secondary halos for strong lensing in massive galaxy clusters across redshiftOct 30, 2019Strong Lensing Model of SPT-CLJ0356-5337, a Major Merger Candidate at Redshift 1.0359Mar 1, 2019Lens Model and Source Reconstruction Reveal the Morphology and Star Formation Distribution in the Cool Spiral LIRG SGAS J143845.1$+$145407Mar 31, 2020Three-Dimensional Kinematic Reconstruction of the Optically-Emitting, High-Velocity, Oxygen-Rich Ejecta of Supernova Remnant N132DSep 27, 2021A 30 kpc Spatially Extended Clumpy and Asymmetric Galactic Outflow at z $\sim$ 1.7Sep 25, 2020A Comparison of Rest-frame Ultraviolet and Optical Emission-Line Diagnostics in the Lensed Galaxy SDSS J1723+3411 at Redshift z=1.3293Nov 4, 1998The David Dunlap Observatory IVC Distance Project: First ResultsFeb 15, 2002The Optical Afterglow of GRB 011211Jun 29, 2000Spectroscopic Gravitational Lens Candidates in the CNOC2 Field Galaxy Redshift SurveyMar 18, 2013The IMACS Cluster Building Survey: V. Further Evidence for Starburst Recycling from Quantitative Galaxy MorphologiesJul 8, 2025Intergalactic Medium Tomography with the Sunburst ArcOct 13, 2025The Sunburst Arc with JWST. IV. The importance of interaction, turbulence, and feedback for Lyman-continuum escapeMay 14, 2010A bright, spatially extended lensed galaxy at z = 1.7 behind the cluster RCS2 032727-132623