arXiv (All)
open access
Euclid preparation. Testing template-fitting models for the multipoles of the two-point clustering of galaxy clusters
The Euclid satellite will deliver a catalogue of optically selected galaxy clusters spanning from around 2000 deg$^2$ in Data Release (DR) 1 to around $14\,000$ deg$^2$ in DR3. In this work, we assess the validity of cluster clustering (CC) models for template-fitting, which complements the full-sha
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
- ISO far-infrared observations of rich galaxy clusters II. Sersic 159-03#639553
- Euclid preparation. XCI. Validation method for the detections in the Euclid Catalogue of Galaxy Clusters using external data#799883
- CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles#677830
- Galaxy clustering and feedback#433127
- Constraining the galaxy-halo connection at $z>10$ using the neighbors of UV-bright galaxies#1118890
Record · ID 800014
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