arXiv (All)
open access
Far-Ultraviolet diffuse emission as a tracer of Galactic extinction at the North Galactic Pole
Interstellar extinction at high Galactic latitude is often traced by thermal dust emission, but the conversion from infrared surface brightness to reddening is sensitive to grain properties and temperature. We test dust-scattered far-ultraviolet (FUV) and near-ultraviolet (NUV) diffuse emission as a
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
- NOEMA probes the [CII] and dust content in a 2175Å UV Bump Galaxy at $z=7.1$#1000167
- Low-Metallicity Star Formation Survey in Sh2-284 (LZ-STAR): The Core Mass Function#1062971
- Exploring spatially resolved metallicities, dynamics, and outflows in low-mass galaxies at z ∼ 7.6#1065846
- Radio-dust connection in quasars driven by powerful ionised outflows#820662
- A Steep-Extinction Quasi-stellar Object at z=4.6: JWST Evidence for Abundant Small Dust Grains#684484
Record · ID 1129562
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