arXiv (All)
open access
Toward a Complete Interpretation of Global 21 cm Absorption Signals Using the Radio CMB
The global 21 cm signal is among the most direct probes of cosmic dawn, encoding information about when the first stars formed and how efficiently they heated their surroundings. However, such measurements are limited by bright Galactic foregrounds, ionospheric effects, and instrumental systematics.
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
- Mitigating incoherent excess variance in high-redshift 21-cm observations with multi-output cross Gaussian process regression#1266320
- Medium bands, mega science: A JWST/NIRCam medium-band imaging survey of A2744#1480120
- The RAdio Galaxy Environment Reference Survey (RAGERS) Evidence of an anisotropic distribution of submillimeter galaxies in the 4C 23.56 protocluster at z=2.48#1290960
- EPOCHS-DR2 I: Expanded data release and properties of $6.5<z<16.5$ photometrically selected galaxies across NIRCam deep fields covering $\sim700\,\rm arcmin^2$ with the galfind software#1051379
- MUSE-ALMA Haloes XVI: a census of the condensed baryons in z~0.5 HI absorption-selected galaxies#1234484
Record · ID 1491908
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