Showing 1–20 of 626 results
/ Date/ Name
Aug 7, 2023Beyond the 3rd moment: A practical study of using lensing convergence CDFs for cosmology with DES Y3Sep 1, 2023Dark Energy Survey Year 6 Results: Intra-Cluster Light from Redshift 0.2 to 0.5Jul 12, 2022A galaxy-driven model of type Ia supernova luminosity variationsDec 10, 2010Measurement of Reciprocity Failure in Near Infrared DetectorsAug 3, 2012PreCam, a Precursor Observational Campaign for Calibration of the Dark Energy SurveyOct 20, 2023Dark Energy Survey Year 3 Results: Mis-centering calibration and X-ray-richness scaling relations in redMaPPer clustersDec 11, 2023The High Energy Light Isotope eXperiment program of direct cosmic-ray studiesDec 1, 2023A Large Sample of Extremely Metal-poor Galaxies at $z<1$ Identified from the DESI Early DataFeb 16, 2022Robust sampling for weak lensing and clustering analyses with the Dark Energy SurveyMay 16, 2014Mass and galaxy distributions of four massive galaxy clusters from Dark Energy Survey Science Verification dataJul 14, 2014Combining Dark Energy Survey Science Verification Data with Near Infrared Data from the ESO VISTA Hemisphere SurveyOct 25, 2018Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol DataNov 27, 2019The Mystery of Photometric Twins DES17X1boj and DES16E2bjyNov 6, 2019Dark Energy Survey Year 1 Results: the lensing imprint of cosmic voids on the Cosmic Microwave BackgroundJan 29, 2020Increasing the census of L and T dwarfs in wide binary and multiple systems using Dark Energy Survey DR1 and Gaia DR2 dataJul 24, 2018Is every strong lens model unhappy in its own way? Uniform modelling of a sample of 13 quadruply+ imaged quasarsJan 17, 2020Optical follow-up of gravitational wave triggers with DECam during the first two LIGO/VIRGO observing runsSep 27, 2020Machine Learning for Searching the Dark Energy Survey for Trans-Neptunian ObjectsOct 23, 2018Dynamical Analysis of Three Distant Trans-Neptunian Objects with Similar OrbitsNov 6, 2018First Cosmological Results using Type Ia Supernovae from the Dark Energy Survey: Measurement of the Hubble Constant