arXiv (All)
open access
Inferring radio beams from sparse sampling patterns: a case study with the Murchison Widefield Array
Accurate primary-beam models are essential for high-dynamic-range radio experiments, particularly searches for the redshifted 21-cm signal from the Epoch of Reionisation, where beam errors can couple bright foreground emission into the faint cosmological measurement. Using reprocessed satellite obse
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
- Twenty-First-Century Statistical and Computational Challenges in Astrophysics#679166
- A VLBA survey of radio stars in the Orion Nebula Cluster: III. Inter-epoch variability analysis#1062357
- Biases from Astrophysical Environmental Effects in Standard-Siren Cosmology#1050650
- The GMRT CAT$z$1-COSMOS Survey: HI 21 cm emission from star-forming galaxies at $z\approx1$ in the COSMOS field#1071178
- Estimating galactic foreground with the population of resolved galactic binaries#1083076
Record · ID 1155401
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