Showing 21–40 of 463 results
/ Date/ Name
Nov 6, 2018First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Effects of Chromatic Corrections to Supernova Photometry on Measurements of Cosmological ParametersNov 6, 2018Steve: A hierarchical Bayesian model for Supernova CosmologySep 3, 2019Trans-Neptunian objects found in the first four years of the Dark Energy SurveyDec 10, 2020A machine learning approach to galaxy properties: joint redshift-stellar mass probability distributions with Random ForestJul 25, 2020The Milky Way bar and bulge revealed by APOGEE DR16 and Gaia EDR3Mar 21, 2019Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clustersDec 3, 2018Chemical Abundance Analysis of Tucana III, the Second $r$-process Enhanced Ultra-Faint Dwarf GalaxyMay 25, 2020Is diffuse intracluster light a good tracer of the galaxy cluster matter distribution?Mar 23, 2020The impact of spectroscopic incompleteness in direct calibration of redshift distributions for weak lensing surveysJan 13, 2021Exploring the contamination of the DES-Y1 Cluster Sample with SPT-SZ selected clustersFeb 10, 2021No Evidence for Orbital Clustering in the Extreme Trans-Neptunian ObjectsSep 8, 2021A search of the full six years of the Dark Energy Survey for outer Solar System objectsFeb 20, 2021Synthetic Galaxy Clusters and Observations Based on Dark Energy Survey Year 3 DataOct 22, 2018Dark Energy Survey Year 1 Results: Methods for Cluster Cosmology and Application to the SDSSSep 14, 2015The Phoenix stream: a cold stream in the Southern hemisphereSep 14, 2015Discovery of a Stellar Overdensity in Eridanus-Phoenix in the Dark Energy SurveyJul 17, 2015Weak lensing by galaxy troughs in DES Science Verification dataAug 14, 2015Eight Ultra-faint Galaxy Candidates Discovered in Year Two of the Dark Energy SurveyJan 3, 2016The Dark Energy Survey: more than dark energy - an overviewJan 4, 2016Comparing Dark Energy Survey and HST-CLASH observations of the galaxy cluster RXC J2248.7-4431: implications for stellar mass versus dark matter