Showing 1–19 of 19 results
/ Date/ Name
Dec 3, 2025The DESI Single Fiber Lens Search. I. Four Thousand Spectroscopically Selected Galaxy-Galaxy Gravitational Lens CandidatesSep 19, 2025A New Way to Discover Strong Gravitational Lenses: Pair-wise Spectroscopic Search from DESI DR1Sep 18, 2025DESI DR1 Ly$α$ forest: 3D full-shape analysis and cosmological constraintsMar 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 QuasarsFeb 28, 2024Impact of Systematic Redshift Errors on the Cross-correlation of the Lyman-$α$ Forest with Quasars at Small Scales Using DESI Early DataDec 30, 2023Synthetic spectra for Lyman-$α$ forest analysis in the Dark Energy Spectroscopic InstrumentAug 21, 20233D Correlations in the Lyman-$α$ Forest from Early DESI DataJun 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 17, 2017Dark Energy Survey Year 1 Results: Measurement of the Baryon Acoustic Oscillation scale in the distribution of galaxies to redshift 1Aug 4, 2017Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak LensingMar 29, 2012The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function