Showing 1–20 of 200 results
/ Date/ Name
Oct 27, 2025Dark Energy Survey Year 6 Results: Redshift Calibration of the Weak Lensing Source GalaxiesDec 22, 2025Weak Lensing Mass Calibration of the ACT DR5 Galaxy Clusters with the DES Year 3 Weak Lensing DataJul 12, 2021Dark Energy Survey Year 3 Results: Galaxy Sample for BAO MeasurementJul 7, 2025The final WaZP galaxy cluster catalog of the Dark Energy Survey and comparison with SZE dataMar 21, 2022Dark Energy Survey Year 3 results: imprints of cosmic voids and superclusters in the Planck CMB lensing mapAug 20, 2020The WaZP galaxy cluster sample of the Dark Energy Survey Year 1Oct 19, 2021Dark Energy Survey Year 3 results: Cosmology with peaks using an emulator approachDec 30, 2025photoD with Rubin's Data Preview 1: first stellar photometric distances and deficit of faint blue stars. Stellar distances with Rubin's DP1Sep 20, 2021Dark Energy Survey Year 3 results: Marginalisation over redshift distribution uncertainties using ranking of discrete realisationsJan 10, 2025OpenUniverse2024: A shared, simulated view of the sky for the next generation of cosmological surveysSep 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 variationsOct 20, 2023Dark Energy Survey Year 3 Results: Mis-centering calibration and X-ray-richness scaling relations in redMaPPer clustersFeb 16, 2022Robust sampling for weak lensing and clustering analyses with the Dark Energy SurveySep 8, 2021A search of the full six years of the Dark Energy Survey for outer Solar System objectsJun 7, 2024Modelling the impact of host galaxy dust on type Ia supernova distance measurementsMar 4, 2024Dark Energy Survey Year 3 results: likelihood-free, simulation-based $w$CDM inference with neural compression of weak-lensing map statisticsFeb 13, 2024The SRG/eROSITA All-Sky Survey: Dark Energy Survey Year 3 Weak Gravitational Lensing by eRASS1 selected Galaxy ClustersJun 7, 2024The Dark Energy Survey Supernova Program: Slow supernovae show cosmological time dilation out to $z \sim 1$Jan 17, 2025High-Significance Detection of Correlation Between the Unresolved Gamma-Ray Background and the Large Scale Cosmic Structure