Showing 21–40 of 254 results
/ Date/ Name
May 16, 2007Evolution of the Frequency of Luminous (\geq L_V*) Close Galaxy Pairs at z < 1.2 in the COSMOS FieldJun 24, 2020The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to $z\sim5$Mar 11, 2019Unveiling the Phase Transition of the Universe During the Reionization Epoch with Lyman-alphaMar 11, 2019UV Diagnostics of Galaxies from the Peak of Star-Formation to the Epoch of ReionizationMar 28, 2019Observational constraints on the merger history of galaxies since $z\approx6$: Probabilistic galaxy pair counts in the CANDELS fieldsJul 26, 2023CEERS MIRI Imaging: Data Reduction and Quality AssessmentOct 11, 2023CEERS: 7.7 $μ$m PAH Star Formation Rate Calibration with JWST MIRIOct 16, 2017Demographics of Star-forming Galaxies since $z\sim2.5$. I. The $UVJ$ Diagram in CANDELSSep 21, 2012GOODS-Herschel: Impact of Active Galactic Nuclei and Star Formation Activity on Infrared Spectral Energy Distributions at High RedshiftJul 28, 2014No More Active Galactic Nuclei in Clumpy Disks Than in Smooth Galaxies at z~2 in CANDELS / 3D-HSTJun 20, 2013CANDELS: The correlation between galaxy morphology and star formation activity at z~2Sep 12, 2012Evidence for a wide range of UV obscuration in z ~ 2 dusty galaxies from the GOODS-Herschel surveyDec 16, 2014ALMA Imaging of HCN, CS and dust in Arp 220 and NGC 6240Dec 3, 2013Optical-faint, Far-infrared-bright Herschel Sources in the CANDELS Fields: Ultra-Luminous Infrared Galaxies at z>1 and the Effect of Source BlendingSep 7, 2017Review: Far-Infrared Instrumentation and Technology Development for the Next DecadeApr 27, 2018The ionisation parameter of star-forming galaxies evolves with the specific star formation rateJun 4, 2025COSMOS-Web: Estimating Physical Parameters of Galaxies Using Self-Organizing MapsMar 24, 2010Major Galaxy Mergers and the Growth of Supermassive Black Holes in QuasarsMar 14, 2019Observing Galaxy Evolution in the Context of Large-Scale StructureMay 6, 2025SHELLQs-JWST Unveils the Host Galaxies of 12 Quasars at z>6