arXiv (All)
open access
Mitigating prior-volume effects in galaxy clustering by adopting Mpc over Mpc/h units
We investigate prior-volume effects in Bayesian analyses of galaxy clustering based on state-of-the-art models, such as the EFT and the VDG$_\infty$ model. We show that these effects are largely driven by imposing priors on the model parameters defined in ${\rm Mpc}/h$ units, thereby introducing a s
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
- Exploring the AGN population in protoclusters: results from the TNG300 simulation and comparison with observations#987059
- Galaxy clustering and feedback#433127
- Anisotropic redshift distributions in photometric galaxy clustering and their cosmological impact#1109832
- The Clustering of Dark Matter, Haloes & Galaxies#231035
Record · ID 1218543
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