Showing 1–20 of 23 results
/ Date/ Name
May 7, 2025Euclid preparation. The impact of redshift interlopers on the two-point correlation function analysisMar 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 29, 2023Cosmological constraints from the tomography of DES-Y3 galaxies with CMB lensing from ACT DR4Jun 9, 2023The Early Data Release of the Dark Energy Spectroscopic InstrumentJun 9, 2023Validation of the Scientific Program for the Dark Energy Spectroscopic InstrumentJul 9, 2021Dark Energy Survey Year 3 Results: A 2.7% measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835Mar 26, 2021Galaxy Clustering in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Real-Space ResultsSep 27, 2020Machine Learning for Searching the Dark Energy Survey for Trans-Neptunian ObjectsJun 12, 2020Constraints on the Physical Properties of GW190814 through Simulations based on DECam Follow-up Observations by the 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 18, 2017Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO