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The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) Observatory

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arxiv 2012.07945 v3 pith:ARQ4MDS4 submitted 2020-12-14 astro-ph.IM astro-ph.HEhep-ex

The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) Observatory

classification astro-ph.IM astro-ph.HEhep-ex
keywords poemmaastrophysicsmulti-messengerneutrinosobservewillabovecamera
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) is designed to accurately observe ultra-high-energy cosmic rays (UHECRs) and cosmic neutrinos from space with sensitivity over the full celestial sky. POEMMA will observe the extensive air showers (EASs) from UHECRs and UHE neutrinos above 20 EeV via air fluorescence. Additionally, POEMMA will observe the Cherenkov signal from upward-moving EASs induced by Earth-interacting tau neutrinos above 20 PeV. The POEMMA spacecraft are designed to quickly re-orientate to follow up transient neutrino sources and obtain unparalleled neutrino flux sensitivity. Developed as a NASA Astrophysics Probe-class mission, POEMMA consists of two identical satellites flying in loose formation in 525 km altitude orbits. Each POEMMA instrument incorporates a wide field-of-view (45$^\circ$) Schmidt telescope with over 6 m$^2$ of collecting area. The hybrid focal surface of each telescope includes a fast (1~$\mu$s) near-ultraviolet camera for EAS fluorescence observations and an ultrafast (10~ns) optical camera for Cherenkov EAS observations. In a 5-year mission, POEMMA will provide measurements that open new multi-messenger windows onto the most energetic events in the universe, enabling the study of new astrophysics and particle physics at these otherwise inaccessible energies.

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