{"paper":{"title":"The Nature of the Galactic Dark Matter","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"N.W.Evans","submitted_at":"1995-10-04T17:19:14Z","abstract_excerpt":"Disk-halo models of the Galaxy and LMC are constructed and used to analyse the microlensing data-set. Deflectors in the LMC bar, disk and halo provide an optical depth to microlensing of $\\sim 2 \\times 10^{-7}$. Deflectors in the Galactic disk and halo contribute $\\sim 5 \\times 10^{-7}$. The extent, flattening and velocity anisotropy of the dark objects in the Galactic halo are unknown. So, it is crucial to analyse the microlensing data-set with families of models that span the viable ranges of these structural parameters. Also uncertain is the contribution of the Galactic disk to the local ci"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9510016","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}