Showing 1–20 of 44 results
/ Date/ Name
Mar 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 StatisticsOct 12, 2024The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number countsApr 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 13, 2024The SRG-eROSITA All-Sky Survey : Constraints on f(R) Gravity from Cluster AbundanceFeb 13, 2024The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphereFeb 13, 2024The SRG/eROSITA All-Sky Survey: Dark Energy Survey Year 3 Weak Gravitational Lensing by eRASS1 selected Galaxy ClustersFeb 13, 2024The SRG/eROSITA All-Sky Survey: The first catalog of galaxy clusters and groups in the Western Galactic HemisphereJan 30, 2024The SRG/eROSITA all-sky survey: First X-ray catalogues and data release of the western Galactic hemisphereAug 7, 2023Beyond the 3rd moment: A practical study of using lensing convergence CDFs for cosmology with DES Y3Jun 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 0.835