arXiv (All)
open access
An analytical model for non-local stochastic field-level galaxy bias on the sphere
We present the `Bias of Overdensities in Large-scale Tracers on the Sphere' (BOLTS) model, a novel analytic galaxy bias model for projected fields on the sphere that incorporates stochasticity and non-locality already at linear order while enforcing physicality and statistical isotropy. Rather than
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
- Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation#670421
- Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation#668356
- RZS Series - Primordial Non-Gaussian Fluctuations: Addressing High-Redshift Galaxy Abundances via Variance-Preserving Modulated Kernels#109296
- Exploring non-Poisson satellite occupation in HOD models and its impact on 2- and 3-point galaxy clustering#1297150
- Host Dependence and Line-of-Sight Effects on Galaxy-Galaxy Strong Lensing in Clusters#799313
Record · ID 1249683
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