What the NOA-Star Simulation Reveals About Transient Classification
(Antonio V. Franco) A conventional Retrieval-Augmented Generation (RAG) system takes a set of retrieved documents, assembles them into a context window, and asks a large language model (LLM) to produce a classification. This approach works reasonably well until you reorder the same documents and watch the model change its mind. The same astronomical alert, the same collection of scientific papers, light curve templates, and stellar catalogs (with the correct document present in every permutation) can yield radically different classifications depending solely on the order in which the documents are presented. A supernova type Ia might emerge in one configuration, a kilonova in another, and an RR Lyrae variable star in a third. This phenomenon, which the Stable-RAG paper (Zhang et al., arXiv:2601.02993) calls permutation-induced hallucination, is more than a curiosity. In the field of transient astronomy, it means allocating precious telescope time to the wrong object, missing the electromagnetic counterpart of a gravitational wave signal, or polluting the Transient Name Server with misclassifications that confuse the entire community. The NOA-Star system was built precisely to solve this problem. ...