arXiv (All)
open access
How bright can a galaxy be? Extreme value predictions for high-redshift survey observables
Assessing the significance of extreme galaxy candidates has typically relied on redshifts and stellar / halo masses inferred through inverse modelling, which carries substantial systematic uncertainty. We combine the halo mass function with a conditional model for galaxy emission and apply the Extre
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
- JADES: A Prominent Galaxy Overdensity Candidate within the First 500 Myr#1368982
- DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [O II] Luminosity#1358062
- RZS Series - Primordial Non-Gaussian Fluctuations: Addressing High-Redshift Galaxy Abundances via Variance-Preserving Modulated Kernels#109296
- Mitigating incoherent excess variance in high-redshift 21-cm observations with multi-output cross Gaussian process regression#1266320
- Non-linear halo bias for accurate modelling of cosmic infrared background anisotropies#1036467
Record · ID 1387305
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