Showing 21–40 of 224 results
/ Date/ Name
Jun 15, 2023GN-z11: The environment of an AGN at $z=$10.603Jul 12, 2022The Science Performance of JWST as Characterized in CommissioningJun 11, 2018Evidence of Environmental Quenching at Redshift z ~ 2Feb 25, 2019Extremely Low Molecular Gas Content in a Compact, Quiescent Galaxy at z=1.522Jul 9, 2020The Universe at z>10: Predictions for JWST from the UniverseMachine DR1Mar 4, 2021Early Science with the Large Millimeter Telescope: Constraining the Gas Fraction of a Compact Quiescent Galaxy at z=1.883Jan 4, 2022Significant Molecular Gas Deficiencies in Star-forming Cluster Galaxies at $z\sim1.4$Sep 7, 2022First Sample of H$α$+[O III] $λ$5007 Line Emitters at $z > 6$ Through JWST/NIRCam Slitless Spectroscopy: Physical Properties and Line Luminosity FunctionsAug 6, 2019Evidence for Inside-Out Galaxy Growth and Quenching of a z~2 Compact Galaxy from High-Resolution Molecular Gas ImagingJan 6, 2023The UNCOVER Survey: A first-look HST+JWST catalog of 60,000 galaxies near Abell 2744 and beyondOct 7, 2022Molecular Gas Reservoirs in Massive Quiescent Galaxies at $\mathrm{z\sim0.7}$ Linked to Late Time Star FormationJun 20, 2023NANCY: Next-generation All-sky Near-infrared Community surveYJun 4, 2023The Cosmos in its Infancy: JADES Galaxy Candidates at z > 8 in GOODS-S and GOODS-NApr 10, 2023JWST and ALMA imaging of dust-obscured, massive substructures in a typical $z \sim 3$ star-forming disk galaxyMay 2, 2023JWST UNCOVER: Discovery of $z>9$ Galaxy Candidates Behind the Lensing Cluster Abell 2744Oct 27, 2023JADES: Using NIRCam Photometry to Investigate the Dependence of Stellar Mass Inferences on the IMF in the Early UniverseOct 17, 2011What turns galaxies off? The different morphologies of star-forming and quiescent galaxies since z~2 from CANDELSFeb 8, 2024UNCOVER NIRSpec/PRISM Spectroscopy Unveils Evidence of Early Core Formation in a Massive, Centrally Dusty Quiescent Galaxy at $z_{spec}=3.97$Jun 20, 2023JADES: The incidence rate and properties of galactic outflows in low-mass galaxies across 3 < z < 9Jun 5, 2024The SMILES Mid-Infrared Survey