arXiv (All)
open access
Constraints on the Pop III Sky Surface Brightness from High-Redshift Caustic Transients in MACS0416
Population III (Pop III) stars are hypothetical zero-metallicity stellar structures formed from primordial hydrogen and helium. They are theorized to span a wide mass range, extending to several 100 solar masses, and may have played important roles in nucleosynthesis and reionization. Their expected
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
- Sown at Cosmic Dawn: Searching for Pop III Signatures in JWST JADES He II Selected Line Emitters#1034935
- ATLASGAL: The HCN-IR Star Formation Relation for the Milky Way#1105784
- First-star imprints in a metal-poor galaxy overdensity near the end of reionization#985158
- Stellar Yields of Rapidly Rotating Population III Stars for the High Redshift Universe#1036327
- Active galactic nucleus activity in brightest cluster galaxies at intermediate redshifts in Sunyaev-Zel'dovich--selected clusters#1123219
Record · ID 1014344
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