arXiv (All)
open access
Improving cosmological distance measurements at high redshift using Lyman-Alpha forest BAO reconstruction
The Dark Energy Spectroscopic Instrument (DESI) measures baryon acoustic oscillations (BAO) in the Lyman-$α$ (Lyman-alpha) forest and provides a robust probe of the expansion history in the matter-dominated era. Yet, non-linear structure formation broadens and shifts the BAO peak. To undo these effe
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
- Constraints on neutrino physics from DESI DR2 BAO and DR1 full shape#1341193
- 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
- Baryon acoustic oscillation theory and modelling systematics for the DESI 2024 results#1015683
Record · ID 1469334
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