Showing 1–18 of 18 results
/ Date/ Name
Feb 26, 2026Extreme Emission Line Galaxies in CEERS Are Powered by Star Formation, not AGNDec 22, 2025Ionizing Photon Production Efficiencies and Chemical Abundances at Cosmic Dawn Revealed by Ultra-Deep Rest-Frame Optical Spectroscopy of JADES-GS-z14-0Dec 14, 2025THRILS -- The High-(Redshift+Ionization) Line Search: Program Description & Redshift CatalogNov 24, 2025Beyond the Monsters: A More Complete Census of Black Hole Activity at Cosmic DawnJun 26, 2025Optical Strong Line Ratios Cannot Distinguish Between Stellar Populations and Accreting Black Holes at High Ionization Parameters and Low MetallicitiesApr 16, 2025CAPERS Observations of Two UV-Bright Galaxies at z>10. More Evidence for Bursting Star Formation in the Early UniverseFeb 5, 2025Emission-Line Diagnostics at z>4: [OIII]λ4363/HγJan 7, 2025The Cosmic Evolution Early Release Science Survey (CEERS)Oct 9, 2024Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their HostsSep 10, 2024Broad-Line AGN at 3.5<z<6: The Black Hole Mass Function and a Connection with Little Red DotsApr 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 < 3.6Dec 12, 2023A Census from JWST of Extreme Emission Line Galaxies Spanning the Epoch of Reionization in CEERSNov 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>2May 23, 2023Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?Nov 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 Imaging