arXiv (All)
open access
Cosmology-dependent covariance in galaxy cluster number counts: consequences for parameter inference
Galaxy clusters provide constraints on cosmology through their abundance as a function of mass and redshift. Parameter inference from cluster counts requires modelling the covariance entering the likelihood, including contributions from Poisson shot noise and super-sample covariance (SSC) induced by
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
- (Re)Assessing Galaxy Clusters with Cosmological Models: Scales, Anisotropies, and Scientific Explanation#86429
- Anisotropic redshift distributions in photometric galaxy clustering and their cosmological impact#1109832
- Homogeneity scale in the local Universe: Model-independent estimate from S-PLUS iDR6 blue galaxies#1062809
- DESI 2024 VII: cosmological constraints from the full-shape modeling of clustering measurements#780528
- Dark Matter as Inertial Anomaly - Coherence-Depth Dependence of Inertia and the Flat Rotation Curve Problem#90313
Record · ID 1050901
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