Showing 1–20 of 36 results
/ Date/ Name
Mar 18, 2025Data Release 1 of the Dark Energy Spectroscopic InstrumentNov 18, 2024DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering MeasurementsNov 18, 2024DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and QuasarsNov 18, 2024DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering StatisticsApr 3, 2024DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic OscillationsApr 3, 2024DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha ForestApr 3, 2024DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and QuasarsJun 9, 2023The Early Data Release of the Dark Energy Spectroscopic InstrumentJun 9, 2023Validation of the Scientific Program for the Dark Energy Spectroscopic InstrumentMay 22, 2022Overview of the Instrumentation for the Dark Energy Spectroscopic InstrumentFeb 25, 2020Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances and Weak LensingApr 24, 2019Spectral Variability of a Sample of Extreme Variability Quasars and Implications for the MgII Broad-line RegionMar 12, 2019Messengers from the Early Universe: Cosmic Neutrinos and Other Light RelicsJan 8, 2019The Buzzard Flock: Dark Energy Survey Synthetic Sky CatalogsOct 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 constant