Showing 1–20 of 20 results
/ Date/ Name
Jun 4, 2025COSMOS-Web: Estimating Physical Parameters of Galaxies Using Self-Organizing MapsMay 6, 2025SHELLQs-JWST Unveils the Host Galaxies of 12 Quasars at z>6Oct 11, 2023CEERS: 7.7 $μ$m PAH Star Formation Rate Calibration with JWST MIRIJul 26, 2023CEERS MIRI Imaging: Data Reduction and Quality AssessmentJun 24, 2020The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to $z\sim5$Jul 15, 2019Astro2020 APC White Paper: Elevating the Role of Software as a Product of the Research EnterpriseMar 28, 2019Observational constraints on the merger history of galaxies since $z\approx6$: Probabilistic galaxy pair counts in the CANDELS fieldsMar 14, 2019Observing Galaxy Evolution in the Context of Large-Scale StructureMar 11, 2019UV Diagnostics of Galaxies from the Peak of Star-Formation to the Epoch of ReionizationMar 11, 2019Unveiling the Phase Transition of the Universe During the Reionization Epoch with Lyman-alphaApr 27, 2018The ionisation parameter of star-forming galaxies evolves with the specific star formation rateOct 16, 2017Demographics of Star-forming Galaxies since $z\sim2.5$. I. The $UVJ$ Diagram in CANDELSSep 7, 2017Review: Far-Infrared Instrumentation and Technology Development for the Next DecadeDec 16, 2014ALMA Imaging of HCN, CS and dust in Arp 220 and NGC 6240Jul 28, 2014No More Active Galactic Nuclei in Clumpy Disks Than in Smooth Galaxies at z~2 in CANDELS / 3D-HSTDec 3, 2013Optical-faint, Far-infrared-bright Herschel Sources in the CANDELS Fields: Ultra-Luminous Infrared Galaxies at z>1 and the Effect of Source BlendingJun 20, 2013CANDELS: The correlation between galaxy morphology and star formation activity at z~2Sep 21, 2012GOODS-Herschel: Impact of Active Galactic Nuclei and Star Formation Activity on Infrared Spectral Energy Distributions at High RedshiftSep 12, 2012Evidence for a wide range of UV obscuration in z ~ 2 dusty galaxies from the GOODS-Herschel surveyMar 24, 2010Major Galaxy Mergers and the Growth of Supermassive Black Holes in Quasars