arXiv (All)
open access
IceCube Upgrade status and perspectives
The IceCube Neutrino Observatory instruments one cubic kilometer of deep-glacial ice between 1450 m and 2450 m below the surface at the geographic South Pole to detect neutrinos via Cherenkov radiation of relativistic charged particles produced in their interactions. This detector is responsible for
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
- In situ estimation of ice crystal properties at the South Pole using LED calibration data from the IceCube Neutrino Observatory#1157711
- IceCube neutrino point-source searches in the direction of the KM3NeT ultra-high-energy event#998505
- Time-Integrated Searches for Sub-TeV Neutrino Sources with IceCube-DeepCore#1000028
- Study of Supernova Neutrinos at ESSnuSB#785189
- Study of Supernova Neutrinos at ESSnuSB#783599
Record · ID 1050566
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