Showing 1–20 of 105 results
/ Date/ Name
May 15, 2020ALMA Characterises the Dust Temperature of z ~ 5.5 Star-Forming GalaxiesFeb 25, 2019SILVERRUSH. VIII. Spectroscopic Identifications of Early Large Scale Structures with Protoclusters Over 200 Mpc at z~6-7: Strong Associations of Dusty Star-Forming GalaxiesOct 9, 2019The Redshift Evolution of Rest-UV Spectroscopic Properties to z~5May 28, 2018The art of modeling CO, [CI], and [CII] in cosmological galaxy formation modelsSep 23, 2019Quiescent galaxies 1.5 billion years after the Big Bang and their progenitorsAug 24, 2023Uncovering a Massive z~7.7 Galaxy Hosting a Heavily Obscured Radio-Loud QSO Candidate in COSMOS-WebApr 14, 2023A Near-Infrared Faint, Far-Infrared-Luminous Dusty Galaxy at z~5 in COSMOS-WebMay 20, 2016Revisiting the Lyman Continuum Escape Crisis: Predictions for z > 6 from Local GalaxiesJul 10, 2017Dust Properties of [CII] Detected z $\sim$ 5.5 Galaxies: New HST/WFC3 Near-IR ObservationsAug 25, 2017Are high redshift Galaxies hot? - Temperature of z > 5 Galaxies and Implications on their Dust PropertiesJan 21, 2024Efficient PSF Modeling with ShOpt.jl: A PSF Benchmarking Study with JWST NIRCam ImagingNov 10, 2017SILVERRUSH. V. Census of Lya, [OIII]5007, Ha, and [CII]158um Line Emission with ~1000 LAEs at z=4.9-7.0 Revealed with Subaru/HSCJul 22, 2024BUFFALO Wild Wings: A High Precision Free-Form Lens Model of MACSJ0416 with Constraints on Dark Matter from Substructure and Highly Magnified ArcsNov 15, 2022COSMOS-Web: An Overview of the JWST Cosmic Origins SurveyApr 9, 2025Joint Survey Processing. III. Compact Oddballs in the COSMOS Field -- Little Red Dots and TransientsSep 2, 2025The ALPINE-CRISTAL-JWST Survey: Revealing Less Massive Black Holes in High-Redshift GalaxiesJan 20, 2025Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12Nov 19, 2025The SPHEREx Image and Spectrophotometry Processing PipelineSep 9, 2025A comprehensive separation of dark matter and baryonic mass components in galaxy clusters I: Mass constraints from Abell S1063Dec 8, 2025Spatially Resolved Physical Properties of Young Star Clusters and Star-forming Clumps in the Brightest z>6 Galaxy, the Strongly Lensed Cosmic Spear at z=6.2