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Real-time or high-cadence detection pipeline for early-phase astronomical transients (supernovae, kilonovae) using wide-field optical monitoring data.
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This project is a scientific research artifact (arXiv:2512.18157v1). While it has 0 stars, the 43 forks suggest a specific research group or academic collaboration is actively using/testing the code. It solves a highly domain-specific problem in astrophysics that requires deep expertise in astronomical data reduction and transient physics, making it irrelevant to frontier AI labs. Its defensibility lies in its niche scientific utility rather than software engineering complexity.
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