arXiv (All)
open access
Rubin LSST DP2 unveils almost-dark galaxies in the Virgo Cluster
Galaxies with the faintest surface brightness are currently known only in the Local Group. Similar objects should exist beyond our vicinity and are crucial for understanding galaxy evolution, structure, and dark matter content, yet surveys have not reached the depth required to detect them systemati
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
- Shape Degeneracies: the likely culprit for the differences between lens mass models of galaxy clusters#1063358
- The Next Generation Virgo Cluster Survey (NGVS). XXXV. First Kinematical Clues of Overly Massive Dark Matter Halos in Several Ultradiffuse Galaxies in the Virgo Cluster#453417
- Mapping Dark-Matter Clusters via Physics-Guided Diffusion Models#927254
- Eliminating Dark Matter: Wave Geometry in the Time Field Model as an Alternative for Galactic Dynamics#721777
- The Infrared Glow of Galactic Outskirts: A New Window with NASIM#1070383
Record · ID 1013844
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