arXiv (All)
open access
Cluster connectivity in DES Y3 data: impact on galaxy properties
Connectivity, namely the number of cosmic filaments reaching out of groups or clusters, has recently emerged as an informative way to quantify environment. With the advent of wide-area photometric surveys, it becomes possible to measure connectivity on a statistically significant sample of clusters.
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
- Exploring non-Poisson satellite occupation in HOD models and its impact on 2- and 3-point galaxy clustering#1297150
- Exploring the dynamics of the Coma galaxy cluster by mapping its X-ray emission line profiles with XRISM#1160768
- Mixed Dark Matter and Galaxy Clustering: The Importance of Relative Perturbations#1343437
- Galaxy-multiplet clustering from DESI DR2#1341151
- Probing Projection Effects in Optically-Selected Clusters with Velocity Dispersions Outliers#985484
Record · ID 1446845
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