{"paper":{"title":"The Copernicus Complexio: a high-resolution view of the small-scale Universe","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Adrian Jenkins (Durham), Carlos S. Frenk (Durham), John Helly (Durham), Maciej Cytowski (Warsaw), Marius Cautun (Durham), Sownak Bose (Durham), Till Sawala (Durham), Warsaw), Wojciech A. Hellwing (Durham","submitted_at":"2015-05-24T13:14:33Z","abstract_excerpt":"We introduce Copernicus Complexio (COCO), a high-resolution cosmological N-body simulation of structure formation in the $\\Lambda{\\rm CDM}{}$ model. COCO follows an approximately spherical region of radius $\\sim 17.4h^{-1}\\,{\\rm Mpc}$ embedded in a much larger periodic cube that is followed at lower resolution. The high resolution volume has a particle mass of $1.135\\times10^5h^{-1}{\\rm M}_{\\odot}$ (60 times higher than the Millennium-II simulation). COCO gives the dark matter halo mass function over eight orders of magnitude in halo mass; it forms $\\sim 60$ haloes of galactic size, each resol"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1505.06436","kind":"arxiv","version":2},"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"}