Showing 1–17 of 17 results
/ Date/ Name
Apr 17, 2023An Updated Dust-to-Star Geometry: Dust Attenuation Does Not Depend on Inclination in $1.3\leq z\leq 2.6$ Star-Forming Galaxies from MOSDEFSep 26, 2024Stacking and Analyzing $z\approx 2$ MOSDEF Galaxies by Spectral Types: Implications for Dust Geometry and Galaxy EvolutionMay 15, 2025Measuring Emission Lines with JWST-MegaScience Medium-Bands: A New Window into Dust and Star Formation at Cosmic NoonApr 19, 2024Medium Bands, Mega Science: a JWST/NIRCam Medium-Band Imaging Survey of Abell 2744Mar 7, 2023Constraints on Fluctuating Star Formation Rates for Intermediate-mass Galaxies with H$α$ and UV LuminositiesFeb 11, 2026Evidence for Shallow Nebular Attenuation Curves and Patchy Dust Geometry at z~2 with Pa-beta/H-alpha Measurements from JWST-MegaScience Medium Band PhotometryFeb 27, 2026Everything Every Band All at Once I: A Global Morphology Catalog in Abell 2744 based on UNCOVER/MegaScienceApr 18, 2024The JWST-SUSPENSE Ultradeep Spectroscopic Program: Survey Overview and Star-Formation Histories of Quiescent Galaxies at 1 < z < 3Jan 22, 2026UNCOVER/MegaScience Finds Uniform and Highly Bursty Star Formation at 3 < z < 9, consistent with the High-Redshift UV Luminosity FunctionSep 15, 2025Clues to inside-out quenching in quiescent galaxies at $1.2\lesssim z\lesssim2.2$: age, Fe-, and Mg-abundance gradients from JWST-SUSPENSEJul 25, 2025MINERVA: A NIRCam Medium Band and MIRI Imaging Survey to Unlock the Hidden Gems of the Distant UniverseJan 28, 2026Bottom-heavy initial mass functions reveal hidden mass in early galaxiesJul 2, 2024Carbon and Iron Deficiencies in Quiescent Galaxies at z=1-3 from JWST-SUSPENSE: Implications for the Formation Histories of Massive GalaxiesDec 27, 2021Moments of Gaussian Periods and Modified Fermat CurvesJun 4, 2025Fast Rotators at Cosmic Noon: Stellar Kinematics for 15 Quiescent Galaxies from JWST-SUSPENSEDec 8, 2023The Heavy Metal Survey: The Evolution of Stellar Metallicities, Abundance Ratios, and Ages of Massive Quiescent Galaxies Since z~2Nov 27, 2023The Heavy Metal Survey: Star Formation Constraints and Dynamical Masses of 21 Massive Quiescent Galaxies at $z=1.3-2.3$