Juq-245 Jun 2026

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| | Objective | Key Instruments | Timeline | |-----------|---------------|----------------------|--------------| | Verification | Confirm repeatability across all bands | DSA‑V3, RA4, Helios, JWST, IceCube (neutrino) | 6 months | | High‑Resolution Imaging | Map surface topology, detect possible apertures | Extremely Large Telescope (ELT), next‑gen interferometers | 1–2 years | | Spectral Deep Dive | Resolve exotic lattice signatures, search for modulated signals | JWST NIRSpec, ALMA, future Space‑Based X‑ray Array | 2–3 years | | Probe Mission Concept | Design a fly‑by probe capable of in‑situ analysis | International Mission Architecture (IMA) team | 5–10 years | | Theoretical Modelling | Simulate beacon physics, assess energy source | Global super‑computing consortium | Ongoing | JUQ-245

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