Showing 1–20 of 22 results
/ Date/ Name
Jun 18, 2020Blind Observers of the SkyJun 14, 2021ShapeFit: extracting the power spectrum shape information in galaxy surveys beyond BAO and RSDJun 22, 2021Model-independent versus model-dependent interpretation of the SDSS-III BOSS power spectrum: Bridging the divideJan 20, 2022PT challenge: Validation of ShapeFit on large-volume, high-resolution mocksDec 8, 2022A tale of two (or more) $h$'sJan 11, 2019KiDS+GAMA: Constraints on Horndeski gravity from combined large-scale structure probesApr 25, 2022Model-agnostic interpretation of 10 billion years of cosmic evolution traced by BOSS and eBOSS dataSep 3, 2020HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedbackAug 14, 2025Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parametersJan 23, 2026Illuminating the Physics of Cosmic Origin and Evolution: A UK Space Frontiers 2035 White PaperApr 2, 2025The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physicsNov 18, 2024DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and QuasarsSep 28, 2022BAO+BBN revisited -- Growing the Hubble tension with a 0.7km/s/Mpc constraintDec 14, 2018KiDS+VIKING-450: Cosmic shear tomography with optical+infrared dataNov 18, 2024DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering MeasurementsApr 10, 2024Comparing Compressed and Full-modeling Analyses with FOLPS: Implications for DESI 2024 and beyondJun 9, 2023Validation of the Scientific Program for the Dark Energy Spectroscopic InstrumentMay 22, 2022Overview of the Instrumentation for the Dark Energy Spectroscopic InstrumentNov 18, 2024DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering StatisticsApr 3, 2024DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations