Mitigating prior-volume effects in galaxy clustering by adopting Mpc over Mpc/h units
astro-ph.CO
Submitted: 2026-10-06
Updated: 2026-10-08
Comments: 24 pages, 13 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements
- Euclid Definition Study Report
- Euclid. I. Overview of the Euclid mission
- The Effective Field Theory of Cosmological Large Scale Structures
- Redshift Space Distortions in the Effective Field Theory of Large Scale Structures
- Biased Tracers in Redshift Space in the EFT of Large-Scale Structure
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the configuration-space clustering wedges
- Boosting galaxy clustering analyses with non-perturbative modelling of redshift-space distortions
- Cosmology with 6 parameters in the Stage-IV era: efficient marginalisation over nuisance parameters
- Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors
- DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
- HOD-informed prior for EFT-based full-shape analyses of LSS
- Debiasing inference in large-scale structure with non-flat volume measures
- A fast test to assess the impact of marginalization in Monte Carlo analyses, and its application to cosmology
- Bayesian and frequentist investigation of prior effects in EFTofLSS analyses of full-shape BOSS and eBOSS data
- Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy
- Frequentist Cosmological Constraints from Full-Shape Clustering Measurements in DESI DR1
- Arguments against using $h^{-1}{\rm Mpc}$ units in observational cosmology
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