arXiv (All)
open access
Extending the Little Red Dot population at intermediate redshift with VIPERS
Little red dots (LRDs) are a recently identified population of compact, red sources characterised by a distinctive V-shaped UV-to-optical continuum and broad emission lines. Their physical structure and evolution remain uncertain, while their properties at intermediate redshifts are largely unexplor
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
- BlackTHUNDER – A non-stellar Balmer break in a black hole-dominated little red dot at z = 7.04#1065834
- Primordial Black Hole Seeds for Little Red Dots in $f(R)$ Gravity#798359
- Primordial Black Hole Seeds for Little Red Dots in $f(R)$ Gravity#796946
- BlackTHUNDER strikes twice: Balmer-line absorption in an overmassive Little Red Dot at z = 7.04#1065857
- Little Red Dots as a Transient Phase of Self-Interacting Dark Matter Assisted Black Hole Growth#1033802
Record · ID 997211
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