arXiv (All)
open access
Disentangling constraints on $S_8$ from the high and low redshift CMB
The clustering of matter in the universe is quantified by $σ_8$, the RMS fluctuations today in linear theory in spheres of radius $8h^{-1}$ Mpc, where $h$ parametrizes the Hubble constant. Surveys of gravitational lensing and galaxy clustering best constrain $S_8\equiv (Ω_m/0.3)^{0.5} σ_8$, where $Ω
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
- Revisiting the Hubble Tension with DESI DR2 Baryon Acoustic Oscillation Observations and Machine Learning Methods#1232875
- Constraints on redshift-evolving Hubble constant models with early- and late-time diagnostics#1489499
- Cosmology with weak lensing surveys#1053363
- Sound-Horizon-Agnostic Forecast for Constraints on $H_0$ and $Σm_ν$ from BAO, CMB Lensing, Supernovae and LSST-like Galaxy Lensing#1424793
- (Re)Assessing Galaxy Clusters with Cosmological Models: Scales, Anisotropies, and Scientific Explanation#86429
Record · ID 1488544
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