Stars-894 - Patched

| Sub‑system | Description | |------------|-------------| | | Cadmium‑Zinc‑Telluride (CZT) pixel array, 64 × 64 pixels, 5 mm pitch; energy range 0.1–150 keV; effective area 1200 cm². | | Secondary Scintillator | LaBr₃(Ce) crystal coupled to SiPM array, 150 keV–10 MeV; timing resolution 200 ps. | | Anti‑Coincidence Shield | Plastic scintillator + photomultiplier tubes to suppress charged‑particle background (< 2 % residual). | | On‑board Processing | FPGA‑based trigger engine; real‑time burst localization via coded‑mask deconvolution; ≤ 5 ms latency. | | Calibration | On‑board ^⁵⁷Co and ^⁶⁰Co sources; periodic celestial calibrators (Crab Nebula). |

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| Metric | Target (3 months) | |--------|-------------------| | – % of articles with at least one accepted suggestion | ≥ 45 % | | Acceptance ratio – accepted / total suggestions shown | ≥ 60 % | | Average time saved – reduction in tagging time per article (measured via user session logs) | ≥ 30 seconds | | Error rate – failed suggestion API calls per 1,000 edits | ≤ 2 | | User satisfaction – NPS on “Tagging experience” survey question | ≥ +8 | STARS-894

Case use-cases (concise examples)

The Classification of STARS-894: Decoding the Spectral Fingerprints of a Telluric Calibration Star | | On‑board Processing | FPGA‑based trigger engine;

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Research into why there are fewer high-inclination (tilted) Be stars than expected in certain clusters. Astronomy & Astrophysics (A&A) (like white dwarfs or RR Lyrae) or a particular research area (like exoplanet habitability)? AI responses may include mistakes. Learn more Issue 2 - Volume 894 - The Astrophysical Journal Letters a title of an artistic work

In the context of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) data, is also the specific number of carbon stars identified and reported in the LAMOST DR2 catalog.

Key Critical Path : Detector module assembly → Integration → Environmental test → Launch.

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