Showing 1–20 of 21 results
/ Date/ Name
Feb 23, 2026Little Red Dots: One Photometric Tag Concealing Diverse Spectroscopic Flavors of Massive Star Formation and Black Hole ActivityOct 9, 2025The CEERS Photometric and Physical Parameter CatalogJun 26, 2025Optical Strong Line Ratios Cannot Distinguish Between Stellar Populations and Accreting Black Holes at High Ionization Parameters and Low MetallicitiesMay 7, 2025CAPERS-LRD-z9: A Gas Enshrouded Little Red Dot Hosting a Broad-line AGN at z=9.288Jan 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 < 3.6Nov 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>2May 23, 2023Extremely red galaxies at $z=5-9$ with MIRI and NIRSpec: dusty galaxies or obscured AGNs?Feb 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 ImagingSep 21, 2018X-UDS: The Chandra Legacy Survey of the UKIDSS Ultra Deep Survey FieldJul 12, 2018Searching for Environmental Effects on Galaxy Kinematics in Groups and Clusters at z~1 from the ORELSE SurveyOct 16, 2017Demographics of Star-forming Galaxies since $z\sim2.5$. I. The $UVJ$ Diagram in CANDELSMay 15, 2017UVI colour gradients of 0.4<z<1.4 star-forming main sequence galaxies in CANDELS: dust extinction and star formation profilesJul 28, 2014No More Active Galactic Nuclei in Clumpy Disks Than in Smooth Galaxies at z~2 in CANDELS / 3D-HST