Showing 1–20 of 27 results
/ Date/ Name
Nov 13, 2025Large-Scale Structure in COSMOS-Web: Tracing Galaxy Evolution in the Cosmic Web up to $z \sim 7$ with the Largest JWST SurveySep 26, 2025Galaxy Zoo: Cosmic Dawn -- morphological classifications for over 41,000 galaxies in the Euclid Deep Field North from the Hawaii Two-0 Cosmic Dawn surveyJun 4, 2025COSMOS-Web: Estimating Physical Parameters of Galaxies Using Self-Organizing MapsFeb 28, 2025COSMOS Spectroscopic Redshift Compilation (First Data Release): 488k Redshifts Encompassing Two Decades of SpectroscopyOct 21, 2024UVCANDELS: Catalogs of photometric redshifts and galaxy physical propertiesMay 17, 2024UVCANDELS: The role of dust on the stellar mass-size relation of disk galaxies at 0.5 $\leq z \leq$ 3.0Nov 27, 2023The UV luminosity function at 0.6 < z < 1 from UVCANDELSNov 7, 2023The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5Oct 11, 2023CEERS: 7.7 $μ$m PAH Star Formation Rate Calibration with JWST MIRIAug 17, 2023The Lyman Continuum Escape Fraction of Star-forming Galaxies at $2.4\lesssim z\lesssim3.0$ from UVCANDELSNov 10, 2022CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWSTOct 16, 2022First Look at z > 1 Bars in the Rest-Frame Near-Infrared with JWST Early CEERS ImagingNov 1, 2018The clustering of typical Ly$α$ emitters from $z \sim 2.5 - 6$: host halo masses depend on Ly$α$ and UV luminositiesOct 16, 2017Demographics of Star-forming Galaxies since $z\sim2.5$. I. The $UVJ$ Diagram in CANDELSMay 2, 2017The clustering of H$β$+[OIII] and [OII] emitters since $z \sim 5$: dependencies with line luminosity and stellar massOct 10, 2016Galaxy Zoo: Quantitative Visual Morphological Classifications for 48,000 galaxies from CANDELSApr 8, 2016The Nature of H$β+$[O{\sc iii}] and [O{\sc ii}] emitters to $z \sim 5$ with HiZELS: stellar mass functions and the evolution of EWsFeb 27, 2015Evolution of the H$β$+[OIII] and [OII] luminosity functions and the [OII] star-formation history of the Universe up to $z$ ~ 5 from HiZELSDec 4, 2014The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-Frame Optical Spectroscopy for ~1500 H-Selected Galaxies at 1.37 < z < 3.8Feb 3, 2014Physical Properties of Emission-Line Galaxies at z ~ 2 from Near-Infrared Spectroscopy with Magellan FIRE