Showing 1–20 of 21 results
/ Date/ Name
Oct 18, 2018RELICS: High-Resolution Constraints on the Inner Mass Distribution of the z=0.83 Merging Cluster RXJ0152.7-1357 from strong lensingApr 10, 2012A highly magnified candidate for a young galaxy seen when the Universe was 500 Myrs oldApr 16, 2012CLASH: Mass Distribution in and around MACS J1206.2-0847 from a Full Cluster Lensing AnalysisDec 5, 2019RELICS: A Very Large ($θ_{E}\sim40"$) Cluster Lens -- RXC J0032.1+1808May 22, 2019Stellar Properties of z ~ 8 Galaxies in the Reionization Lensing Cluster SurveySep 19, 2019RELICS: Spectroscopy of gravitationally-lensed $z\simeq 2$ reionization-era analogs and implications for CIII] detections at $z>6$Aug 7, 2013The Contribution of Halos with Different Mass Ratios to the Overall Growth of Cluster-Sized HalosOct 24, 2017The Reionization Lensing Cluster Survey (RELICS) and the Brightest High-z GalaxiesOct 25, 2017RELICS: Strong Lens Models for Five Galaxy Clusters From the Reionization Lensing Cluster SurveyMar 1, 2018RELICS: Strong-lensing analysis of the massive clusters MACS J0308.9+2645 and PLCK G171.9-40.7Oct 31, 2018RELICS: Strong Lensing Analysis of MACS J0417.5-1154 and Predictions for Observing the Magnified High-Redshift Universe with JWSTMar 5, 2019RELICS: Reionization Lensing Cluster SurveyMay 24, 2018RELICS: A Strong Lens Model for SPT-CLJ0615-5746, a z=0.972 ClusterMay 18, 2011CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey - The Hubble Space Telescope Observations, Imaging Data Products and MosaicsApr 4, 2013CLASH: Complete Lensing Analysis of the Largest Cosmic Lens MACS J0717.5+3745 and Surrounding StructuresOct 11, 2016The Astropy ProblemJan 8, 2012CLASH: Precise New Constraints on the Mass Profile of Abell 2261Jun 16, 2011Cluster Lensing And Supernova survey with Hubble (CLASH): An OverviewAug 31, 2020RELICS: Properties of z>5.5 Galaxies Inferred from Spitzer and Hubble Imaging Including A Candidate z~6.8 Strong [OIII] EmitterJan 9, 2018A Candidate $z\sim10$ Galaxy Strongly Lensed into a Spatially Resolved Arc