Showing 21–40 of 607 results
/ Date/ Name
Sep 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 ForestMar 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 clustersSep 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 SDSSOct 26, 2021Euclid preparation: XVIII. Cosmic Dawn Survey. Spitzer observations of the Euclid deep fields and calibration fieldsMay 25, 2021Euclid preparation: XIII. Forecasts for galaxy morphology with the Euclid Survey using Deep Generative ModelsJan 3, 2016The Dark Energy Survey: more than dark energy - an overviewAug 4, 2017Dark Energy Survey Year 1 Results: Weak Lensing Shape CataloguesFeb 1, 2017Models of the strongly lensed quasar DES J0408-5354Jan 31, 2017Discovery of the Lensed Quasar System DES J0408-5354Aug 15, 2017OzDES multifibre spectroscopy for the Dark Energy Survey: Three year results and first data releaseDec 11, 2017Studying the Ultraviolet Spectrum of the First Spectroscopically Confirmed Supernova at redshift twoOct 16, 2017How Many Kilonovae Can Be Found in Past, Present, and Future Survey Datasets?Nov 2, 2017Baryon Content in a Sample of 91 Galaxy Clusters Selected by the South Pole Telescope at 0.2 < z < 1.25