Showing 1–18 of 18 results
/ Date/ Name
Apr 23, 2026Geometric Monomial (GEM): a family of rational 2N-differentiable activation functionsDec 10, 2024Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak LensingJul 9, 2021Dark Energy Survey Year 3 Results: A 2.7% measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835Dec 23, 2020Dark Energy Survey Year 3 Results: Deep Field Optical + Near-Infrared Images and CatalogueAug 25, 2020Combination of cluster number counts and two-point correlations: Validation on Mock Dark Energy SurveyNov 6, 2018Cosmological Constraints from Multiple Probes in the Dark Energy SurveyOct 4, 2018Dark Energy Survey Year 1 Results: tomographic cross-correlations between DES galaxies and CMB lensing from SPT+PlanckOct 4, 2018Dark Energy Survey Year 1 Results: Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point FunctionsJul 26, 2018Dark Energy Survey Year 1 Results: Measurement of the Galaxy Angular Power SpectrumDec 17, 2017Dark Energy Survey Year 1 Results: Measurement of the Baryon Acoustic Oscillation scale in the distribution of galaxies to redshift 1Oct 16, 2017The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova ModelsOct 16, 2017A gravitational-wave standard siren measurement of the Hubble constantAug 4, 2017Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic ShearAug 4, 2017Dark Energy Survey Year 1 Results: Galaxy-Galaxy LensingAug 4, 2017Dark Energy Survey Year 1 Results: Galaxy clustering for combined probesAug 4, 2017Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak LensingJun 28, 2017Dark Energy Survey Year 1 Results: Multi-Probe Methodology and Simulated Likelihood AnalysesJun 14, 2016A DECam Search for an Optical Counterpart to the LIGO Gravitational Wave Event GW151226