| # Repair a scientific dark-matter map workflow |
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| This task contains a pinned source snapshot of Gammapy and an offline |
| reproduction of a dark-matter line-of-sight calculation. A map that is valid |
| for a small field of view becomes unusable for a wider field, and calculations |
| that do complete must still represent the intended astrophysical integral. |
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| Inspect the relevant source documentation and call graph, then repair the |
| implementation so that the dark-matter spatial calculation remains |
| scientifically valid across the supported geometries, profiles, units, and |
| annihilation/decay modes. |
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| The goal is one general scientific repair. Preserve the existing public API and |
| do not hard-code the public map, a particular profile, an angular width, a |
| matrix shape, or expected numerical values. Keep the repair inside the source |
| snapshot and do not modify the test harness. |
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| Run the public symptom reproduction with: |
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| ```bash |
| python reproduce.py |
| ``` |
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| The evaluator is offline. Do not download catalogs, query remote services, or |
| depend on a local absolute path. Generated reports belong under `outputs/`. |
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