Showing 1–20 of 63 results
/ Date/ Name
Mar 12, 2026JWST's PEARLS: A clumpy ring galaxy at $z = 4.0148$Dec 4, 2025Little red dot variability over a century reveals black hole envelope via a giant Einstein crossNov 18, 2025VENUS: A Strongly Lensed Clumpy Galaxy at $z\sim11-12$ behind the Galaxy Cluster MACS J0257.1-2325Nov 4, 2025The SPHEREx Satellite MissionOct 30, 2025The $N_H$ Distribution of Hard X-ray Selected AGN in the NEP FieldOct 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 GordoJun 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 EstimatesMay 27, 2024EPOCHS Paper X: Environmental effects on Galaxy Formation and Protocluster Galaxy candidates at $4.5<z<10$ from JWST observationsMay 17, 2024UVCANDELS: The role of dust on the stellar mass-size relation of disk galaxies at 0.5 $\leq z \leq$ 3.0May 13, 2024JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noonApr 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 ClusterMar 27, 2024JWST Photometric Time-Delay and Magnification Measurements for the Triply-Imaged Type Ia "Supernova H0pe" at z = 1.78Feb 21, 2024PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field IIJan 24, 2024LyC Leakers in the AstroSat UV Deep Field: Extreme UV emitters at the Cosmic NoonJan 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 Fields