Showing 1–20 of 80 results
/ Date/ Name
Mar 16, 2022The Compact Structures of Massive $z\sim0.7$ Post-Starburst Galaxies in the SQuIGG$\vec{L}$E SampleFeb 8, 2024UNCOVER NIRSpec/PRISM Spectroscopy Unveils Evidence of Early Core Formation in a Massive, Centrally Dusty Quiescent Galaxy at $z_{spec}=3.97$Nov 5, 2024Little Red Dots at an Inflection Point: Ubiquitous "V-Shaped" Turnover Consistently Occurs at the Balmer LimitMar 3, 2025A confirmed deficit of hot and cold dust emission in the most luminous Little Red DotsAug 21, 2023The Large Magellanic Cloud's $\sim30$ Kiloparsec Bow Shock and its Impact on the Circumgalactic MediumAug 29, 2025SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxiesDec 9, 2022DESI Survey Validation Spectra Reveal an Increasing Fraction of Recently Quenched Galaxies at $z\sim1$Oct 9, 2020SQuIGG$\vec{L}$E Survey: Massive z$\sim$0.6 Post-Starburst Galaxies Exhibit Flat Age GradientsJan 6, 2023The UNCOVER Survey: A first-look HST+JWST catalog of 60,000 galaxies near Abell 2744 and beyondDec 8, 2022The JWST UNCOVER Treasury survey: Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of ReionizationNov 29, 2021SQuIGGLE: Studying Quenching in Intermediate-z Galaxies -- Gas, AnguLar Momentum, and EvolutionSep 17, 2024UNCOVER: Significant Reddening in Cosmic Noon Quiescent GalaxiesJul 6, 2020The Role of Active Galactic Nuclei in the Quenching of Massive Galaxies in the SQuiGGLE SurveyJul 6, 2022Recovering the star formation histories of recently-quenched galaxies: the impact of model and prior choicesAug 5, 2023UNCOVER: The growth of the first massive black holes from JWST/NIRSpec -- spectroscopic redshift confirmation of an X-ray luminous AGN at z=10.1Dec 22, 2023Two Distinct Classes of Quiescent Galaxies at Cosmic Noon Revealed by JWST PRIMER and UNCOVERAug 19, 2024The All-Sky Impact of the LMC on the Milky Way Circumgalactic MediumJul 25, 2025MINERVA: A NIRCam Medium Band and MIRI Imaging Survey to Unlock the Hidden Gems of the Distant UniverseMay 2, 2024RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpecApr 8, 2025UNCOVER/MegaScience: No Evidence of Environmental Quenching in a z$\sim$2.6 Proto-cluster