Showing 21–40 of 63 results
/ Date/ Name
Dec 18, 2023JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at $z=0.4$Nov 27, 2023The UV luminosity function at 0.6 < z < 1 from UVCANDELSOct 25, 2023JWST NIRCam Photometry: A Study of Globular Clusters Surrounding Bright Elliptical Galaxy VV 191a at z=0.0513Oct 11, 2023CEERS: 7.7 $μ$m PAH Star Formation Rate Calibration with JWST MIRISep 22, 2023PEARLS: JWST counterparts of micro-Jy radio sources in the Time Domain FieldAug 17, 2023The Lyman Continuum Escape Fraction of Star-forming Galaxies at $2.4\lesssim z\lesssim3.0$ from UVCANDELSJun 28, 2023Hidden giants in JWST's PEARLS: An ultra-massive z=4.26 sub-millimeter galaxy that is invisible to HSTApr 10, 2023The James Webb Space Telescope MissionNov 30, 2022The AstroSat UV Deep Field North: the far and near ultraviolet photometric catalogOct 25, 2022JWST reveals a possible $z \sim 11$ galaxy merger in triply-lensed MACS0647$-$JDOct 15, 2022JWST's PEARLS: A JWST/NIRCam view of ALMA sourcesOct 13, 2022SKYSURF-4: Panchromatic HST All-Sky Surface-Brightness Measurement Methods and ResultsSep 9, 2022JWST's PEARLS: Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First ResultsMay 12, 2022SKYSURF: Constraints on Zodiacal Light and Extragalactic Background Light through Panchromatic HST All-Sky Surface-Brightness Measurements: II. First Limits on Diffuse Light at 1.25, 1.4, and 1.6 micronsMay 12, 2022SKYSURF: Constraints on Zodiacal Light and Extragalactic Background Light through Panchromatic HST All-Sky Surface-Brightness Measurements: I. Survey Overview and MethodsSep 28, 2021The NuSTAR Extragalactic Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain FieldDec 18, 2020Interactive Cosmology Visualization Using the Hubble UltraDeep Field Data in the ClassroomNov 11, 2020SED Analysis of 13 Spectroscopically Confirmed Galaxies at z$\simeq$6 to Constrain UV-Slope, Model Dust Attenuation and Escape FractionsJul 27, 2020Limits to Rest-Frame Ultraviolet Emission From Far-Infrared-Luminous z~6 Quasar HostsApr 9, 2020The Lyman Continuum Escape Fraction of Galaxies and AGN in the GOODS Fields