arXiv (All)
open access
Basis function expansions of the two-point correlation function and reconstruction of the cosmological distance scale
The shape of the correlation function of galaxy pairs can be used as a cosmological distance indicator. Most estimators of this shape require that one bin the pair counts, and considerable effort is expended in finding the optimal bin size. Cosmological constraints are then derived, in a separate st
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Improved Cosmological Constraints from Morphology-Based Marked Correlation Functions#612510
- Improved Cosmological Constraints from Morphology-Based Marked Correlation Functions#611033
- Natural coordinates for constrained correlation functions: Partial autocorrelations and the geometry of positive power spectra#1050673
- Eliminating Dark Matter: Wave Geometry in the Time Field Model as an Alternative for Galactic Dynamics#721777
- Cosmological Correlators from Scattering Amplitudes: A Review#1013850
Record · ID 1051813
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive