Field-level inference of growth rate from DESI BGS galaxy and ZTF supernova simulations
astro-ph.CO
Submitted: 2026-09-28
Updated: 2026-09-28
Code: https://github.com/corentinravoux/flip2https:
Terminology
Sources
- Dark Energy and the Accelerating Universe
- The Road to Precision Cosmology
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements
- Quintessence: A Review
- Modified theories of Gravity: Why, How and What?
- Generalized Brans-Dicke theories
- f(R) Theories Of Gravity
- Horndeski theory and beyond: a review
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Testing General Relativity in Cosmology
- Cosmological Probes of Structure Growth and Tests of Gravity
- An estimation of the Local growth rate from Cosmicflows-3 peculiar velocities
- The Redshift-Space Momentum Power Spectrum I: Optimal Estimation From Peculiar Velocity Surveys
- The Redshift-Space Momentum Power Spectrum III: measuring the growth rate from the SDSSv survey using auto- and cross- power spectrum of the galaxy density and momentum fields
- The 6dF Galaxy Survey: Peculiar Velocity Field and Cosmography
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data
- Growth-rate measurement with type-Ia supernovae using ZTF survey simulations
- Reconstructing dark matter distribution with peculiar velocities: Bayesian forward modelling with corrections for inhomogeneous Malmquist bias
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