Science-Driven Performance Requirements for UV Coronagraph Design: Implications for O 3 Detection in Earth-like Atmospheres

arXiv:2610.19081 · astro-ph.EP, astro-ph.IM · Submitted 2026-10-13 · Read on arXiv

astro-ph.EP, astro-ph.IM

Submitted: 2026-10-13

Updated: 2026-10-13

Comments: 34 pages, 10 figures, Accepted for publication to SPIE JATIS

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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