arXiv (All)
open access
Characterization and on-sky testing of photonic, AWG-based astronomical spectrographs
Astrophotonics is a field that intends to meet the needs of next-generation instruments at a small footprint, low cost, and high stability, compared to bulk-optics-based alternatives. Much development effort is driven by the stringent requirements of direct detection and characterization of exoplane
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
- Characterizing exoplanets atmospheres with space photometry at optical wavelengths#153708
- Highly bipolar planetary nebula Hen 2-57 and its possible symbiotic core#1014921
- PHAROS: Panchromatic spectral energy distributions of solar-like stars across evolutionary stages#1131002
- TSD: An inverse problem approach for recovering the exoplanetary atmosphere transmission spectrum from high-resolution spectroscopy#1062794
- Fusion de données hyperspectrales et séparation de sources pour l'imagerie X en astrophysique#241997
Record · ID 1129344
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