eScholarship
metadata only
CC BY
HOD-dependent systematics for luminous red galaxies in the DESI 2024 BAO analysis
In this paper, we present the estimation of systematics related to the halo occupation distribution (HOD) modeling in the baryon acoustic oscillations (BAO) distance measurement of the Dark Energy Spectroscopic Instrument (DESI) 2024 analysis. This paper focuses on the study of HOD systematics for l
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
- Extensive analysis of reconstruction algorithms for DESI 2024 baryon acoustic oscillations#780518
- Baryon acoustic oscillation theory and modelling systematics for the DESI 2024 results#1015683
- Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data#998267
- DESI DR2 results. II. Measurements of baryon acoustic oscillations and cosmological constraints#642090
- Constraints on neutrino physics from DESI DR2 BAO and DR1 full shape#1341193
Record · ID 1366566
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