Showing 1–20 of 34 results
/ Date/ Name
Feb 23, 2026Little Red Dots: One Photometric Tag Concealing Diverse Spectroscopic Flavors of Massive Star Formation and Black Hole ActivityNov 18, 2025VENUS: A Strongly Lensed Clumpy Galaxy at $z\sim11-12$ behind the Galaxy Cluster MACS J0257.1-2325Oct 9, 2025The CEERS Photometric and Physical Parameter CatalogJan 7, 2025The Cosmic Evolution Early Release Science Survey (CEERS)Apr 4, 2024The Rise of Faint, Red AGN at $z>4$: A Sample of Little Red Dots in the JWST Extragalactic Legacy FieldsDec 15, 2023The Next Generation Deep Extragalactic Exploratory Public Near-Infrared Slitless Survey Epoch 1 (NGDEEP-NISS1): Extra-Galactic Star-formation and Active Galactic Nuclei at 0.5 < z < 3.6Nov 7, 2023The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5Jul 18, 2023CEERS Key Paper VIII: Emission Line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z>2Apr 10, 2023The James Webb Space Telescope MissionFeb 10, 2023The Next Generation Deep Extragalactic Exploratory Public (NGDEEP) SurveyNov 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 ImagingMay 11, 2020The Semi-forbidden CIII]$λ$1909Å~ Emission in the Rest-Ultraviolet Spectra of Green Pea GalaxiesMar 14, 2019Observing Galaxy Evolution in the Context of Large-Scale StructureNov 8, 2018Galaxy inclination and the IRX-beta relation: Effects on UV star-formation rate measurements at intermediate to high redshiftsOct 16, 2017Demographics of Star-forming Galaxies since $z\sim2.5$. I. The $UVJ$ Diagram in CANDELSOct 10, 2016Galaxy Zoo: Quantitative Visual Morphological Classifications for 48,000 galaxies from CANDELSSep 16, 2014The HST/ACS Coma Cluster Survey. X. Nuclear star clusters in low-mass early-type galaxies: scaling relationsSep 3, 2014Galaxy Zoo: CANDELS Barred Disks and Bar FractionsJul 28, 2014No More Active Galactic Nuclei in Clumpy Disks Than in Smooth Galaxies at z~2 in CANDELS / 3D-HST