Showing 1–18 of 18 results
/ Date/ Name
Dec 11, 2025Connection Between Dwarf Galaxies and Globular Clusters: Insights from the Perseus Cluster Using Subaru Imaging and Keck SpectroscopyOct 28, 2025PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-domain Field IIIOct 9, 2025The Distribution of Quenched Galaxies in the Massive z = 0.87 Galaxy Cluster El GordoOct 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 ClusterJan 10, 2024TREASUREHUNT: Transients and Variability Discovered with HST in the JWST North Ecliptic Pole Time Domain FieldNov 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 UVCANDELSOct 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 MethodsMar 17, 2022The Dwarf Galaxy Population at $z\sim 0.7$: A Catalog of Emission Lines and Redshifts from Deep Keck ObservationsNov 11, 2020SED Analysis of 13 Spectroscopically Confirmed Galaxies at z$\simeq$6 to Constrain UV-Slope, Model Dust Attenuation and Escape FractionsApr 9, 2019The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition