arXiv (All)
open access
Reconstructing orbits of galaxies in extreme regions (roger v2.0): an extension to intermediate mass systems
In this paper, we present an updated version of the roger code, called roger v2.0, developed to perform the orbital classification of galaxies residing in and around galaxy groups and clusters. In addition to the projected phase-space coordinates, the new version incorporates the host halo mass as a
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
- Fractal structures and the large scale distribution of galaxies#639463
- Shape Degeneracies: the likely culprit for the differences between lens mass models of galaxy clusters#1063358
- On the clumpy nature of super-early galaxies#1011396
- Galaxy-SMBH co-evolution in 2,435 DESI disk galaxies and merger-free BH growth in bulgeless disks#1037117
- Resolution to Galaxy Rotation Curves, Tully-Fisher, Radial Acceleration Relation, and Missing Satellites: Cosmological Coda V of the Principia Cybernetica#108956
Record · ID 1232828
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