arXiv (All)
open access
The MICADO first light imager for the ELT: Simulated Observations of Star Forming Clumps at Cosmic Noon
Galaxies at redshift z$\sim$2-6 exhibit prominent star-forming regions (clumps). Characterisation of these galactic structures requires both high sensitivity and spatial resolution of $\sim$100 pc or less. Currently, these spatial scales are achievable only with the aid of strong gravitational lensi
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Eliminating Dark Matter: Wave Geometry in the Time Field Model as an Alternative for Galactic Dynamics#721777
- Cosmology with the line-of-sight shear of strong gravitational lenses#1063851
- Triaxiality of the Milky Way dark matter halo and the microlensing optical depth towards the Large Magellanic Cloud#986601
- On the clumpy nature of super-early galaxies#1011396
- SQuIGG$\vec{L}$E: Spatially resolved NIRSpec Pa$α$ reveals that the most CO-luminous, $z\sim0.7$ post-starburst galaxies exhibit falling---but still active---star formation behind optically thick dust#1105865
Record · ID 984718
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