Showing 1–20 of 21 results
/ Date/ Name
Oct 10, 2025Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 3. Inference and ForecastsMar 18, 2025Data Release 1 of the Dark Energy Spectroscopic InstrumentDec 10, 2024Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak LensingNov 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 InstrumentMay 22, 2022Overview of the Instrumentation 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 ResultsNov 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 FunctionsDec 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 Lensing