Showing 1–20 of 60 results
/ Date/ Name
Feb 26, 1998BIMA and Keck Imaging of the Radio Ring PKS 1830-211Mar 6, 1998Keck Spectroscopy of Giant Arcs in Abell 2390May 22, 2019Stellar Properties of z ~ 8 Galaxies in the Reionization Lensing Cluster SurveyJul 19, 2022Panic! At the Disks: First Rest-frame Optical Observations of Galaxy Structure at $z > 3$ with JWST in the SMACS 0723 FieldSep 13, 2023The JWST Discovery of the Triply-imaged Type Ia "Supernova H0pe" and Observations of the Galaxy Cluster PLCK G165.7+67.0Oct 24, 2017The Reionization Lensing Cluster Survey (RELICS) and the Brightest High-z GalaxiesOct 21, 2025SKYSURF-11: A New Zodiacal Light Model Optimized for Optical WavelengthsJan 23, 2023PASSAGES: the wide-ranging, extreme intrinsic properties of Planck-selected, lensed dusty star-forming galaxiesOct 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 ClusterJan 12, 2023Strong gravitational lensing's 'external shear' is not shearMar 27, 2024JWST Spectroscopy of SN H0pe: Classification and Time Delays of a Triply-imaged Type Ia Supernova at z = 1.78Jul 28, 2022Seeing sharper and deeper: JWST's first glimpse of the photometric and spectroscopic properties of galaxies in the epoch of reionisationOct 13, 2023MAGNIF: A Tentative Lensed Rotating Disk at $z=8.34$ detected by JWST NIRCam WFSS with Dynamical Forward ModelingJan 3, 2018MUSE spectroscopy and deep observations of a unique compact JWST target, lensing cluster CLIOApr 11, 2024Identification of $>$40 gravitationally magnified stars in a galaxy at redshift of 0.725Mar 27, 2024SN H0pe: The First Measurement of $H_0$ from a Multiply-Imaged Type Ia Supernova, Discovered by JWSTJan 10, 2024TREASUREHUNT: Transients and Variability Discovered with HST in the JWST North Ecliptic Pole Time Domain FieldAug 5, 2025Globular Clusters in the Galaxy Cluster MACS0416 at z = 0.397