{"paper":{"title":"BlueTides simulation: establishing black hole-galaxy relations at high-redshift","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aklant K. Bhowmick, Chung-Pei Ma, Kuan-Wei Huang, Tiziana Di Matteo, Yu Feng","submitted_at":"2018-01-15T19:07:06Z","abstract_excerpt":"The scaling relations between the mass of supermassive black holes ($M_{\\bullet}$) and host galaxy properties (stellar mass, $M_{\\star}$, and velocity dispersion, $\\sigma$), provide a link between the growth of black holes (BHs) and that of their hosts. Here we investigate if and how the BH-galaxy relations are established in the high-$z$ universe using \\textsc{BlueTides}, a high-resolution large volume cosmological hydrodynamic simulation. We find the $M_{\\bullet}-M_{\\star}$ and $M_{\\bullet}-\\sigma$ relations at $z=8$: $\\log_{10}(M_{\\bullet}) = 8.25 + 1.10 \\ \\log_{10}(M_{\\star}/10^{11}M_{\\odo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.04951","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"}