Showing 1–20 of 24 results
/ Date/ Name
Sep 9, 2022Using peculiar velocity surveys to constrain the growth rate of structure with the wide-angle effectJun 1, 2023Faster cosmological analysis with power spectrum without simulationsJan 9, 2022The Sloan Digital Sky Survey Peculiar Velocity CatalogueJul 16, 2025Can a multi-tracer approach improve the constraints on the turnover scale at low redshift?May 8, 2024Evolving R2 to R2+: Optimal, Delayed Line-of-sight Vector-based Path PlanningAug 11, 2024Rapid Vector-based Any-angle Path Planning with Non-convex ObstaclesJun 28, 2022R2: Heuristic Bug-Based Any-angle Path-Planning using Lazy SearchesApr 10, 2024Full Modeling and Parameter Compression Methods in configuration space for DESI 2024 and beyondApr 14, 2025Enhancing DESI DR1 Full-Shape analyses using HOD-informed priorsJul 31, 2025Effective Theories of Redshift-Space Galaxy Peculiar VelocitiesNov 18, 2024DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and QuasarsDec 2, 2025The DESI DR1 peculiar velocity survey: growth rate measurements from the galaxy power spectrumNov 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 beyondDec 2, 2025The DESI DR1 Peculiar Velocity Survey: growth rate measurements from galaxy and momentum correlation functionsNov 18, 2024DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering StatisticsApr 10, 2024An analysis of parameter compression and full-modeling techniques with Velocileptors for DESI 2024 and beyondApr 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 Quasars