arXiv (All)
open access
The conditional colour-magnitude distribution: III. A study of galaxy colour- and luminosity-dependent counts-in-cells statistics
The conditional colour-magnitude distribution (CCMD) model connects the galaxy colour-luminosity distribution with dark matter halo mass, which has been constrained in Xu et al. by jointly modelling the two-point correlation functions of a large galaxy sample of the Sloan Digital Sky Survey (SDSS) i
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
- Halo mass, star formation, and morphology in galaxies: A morphology-dependent connection between halo environment and star formation activity#972670
- Diffuse Galactic Backgrounds with SPHEREx: A Pilot Study of Background Modeling and Its Impact on Extinction#1200431
- CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles#677830
- Partial-field inferability of galaxy overdensity structure: An information-geometric account of incomplete sky coverage#1062042
- The Merian Survey: A Statistical Census of Bright Satellites of Sub-Milky Way-Mass Galaxies#1199255
Record · ID 1247863
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