arXiv (All)
open access
Direct measures of black hole masses through cosmic time
Supermassive black holes (BHs) are thought to reside in all massive galaxies. They play a fundamental role in shaping galaxy evolution by suppressing star formation and halting the stellar growth of the most massive galaxies via feedback mechanisms. However, to date, measuring even their most basic
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
- Granular mass perturbations on the pulsar - supermassive black hole system#1216327
- Overmassive black holes and little red dots naturally form in simulations#1035369
- The Host Galaxies of Active Galactic Nuclei with Direct Black Hole Mass Measurements#921601
- Little Dots: the ULX Analogy#987064
- Probing binary supermassive black hole in quasars tough spectropolarimetry#1077370
Record · ID 1356860
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