Impact and measurability of linear relativistic effects in galaxy surveys
Robin Y. Wen, Henry S. Grasshorn Gebhardt, Olivier Doré
astro-ph.CO
Submitted: 2026-07-07
Comments: 25+12 pages, 26 figures, 7 tables
Code: https://github.com/SPHEREx/Public-products
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering Statistics
- Euclid. I. Overview of the Euclid mission
- The SPHEREx Satellite Mission
- Acoustic Signatures in the Primary Microwave Background Bispectrum
- Primordial Non-Gaussianities from Inflation Models
- The Effective Field Theory of Multifield Inflation
- Testing Inflation with Large Scale Structure: Connecting Hopes with Reality
- Non-Gaussian features of primordial fluctuations in single field inflationary models
- Single field consistency relation for the 3-point function
- The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
- Constraints on local primordial non-Gaussianity from large scale structure
- The effect of primordial non-Gaussianity on halo bias
- Linear Redshift Distortions: A Review
- New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects
- The linear power spectrum of observed source number counts
- What galaxy surveys really measure
- Large-scale clustering of galaxies in general relativity
- Wide-angle and relativistic effects in Fourier-space clustering statistics
- Large Scale Limit of the Observed Galaxy Power Spectrum
- Ultra large-scale cosmology in next-generation experiments with single tracers
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