Showing 1–20 of 22 results
/ Date/ Name
Oct 28, 2025PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-domain Field IIIJun 7, 2025GNHeII J1236+6215: A He II $λ$1640 emitting and potentially LyC leaking galaxy at $z$ = 2.9803 unveiled through JWST & Keck observationsOct 21, 2024UVCANDELS: Catalogs of photometric redshifts and galaxy physical propertiesOct 2, 2024The Tale of Two Telescopes: How Hubble Uniquely Complements the James Webb Space Telescope: GalaxiesJul 17, 2024SKYSURF VI: The Impact of Thermal Variations of HST on Background Light EstimatesApr 11, 2024Birds of a Feather: Resolving Stellar Mass Assembly With JWST/NIRCam in a Pair of Kindred $z \sim 2$ Dusty Star-forming Galaxies Lensed by the PLCK G165.7+67.0 ClusterFeb 21, 2024PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field IIJan 10, 2024TREASUREHUNT: Transients and Variability Discovered with HST in the JWST North Ecliptic Pole Time Domain FieldJan 5, 2024Lyman Continuum Emission from AGN at 2.3$\lesssim$z$\lesssim$3.7 in the UVCANDELS FieldsDec 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=0.0513Aug 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 HSTNov 30, 2022The AstroSat UV Deep Field North: the far and near ultraviolet photometric catalogOct 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 ResultsNov 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 Hosts