Showing 1–20 of 27 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 InstrumentDec 23, 2020Dark Energy Survey Year 3 Results: Deep Field Optical + Near-Infrared Images and CatalogueNov 6, 2018Cosmological Constraints from Multiple Probes in the Dark Energy SurveyOct 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: Cosmological Constraints from Galaxy Clustering and Weak LensingApr 26, 2016Supplement: Localization and broadband follow-up of the gravitational-wave transient GW150914