{"paper":{"title":"Dependence of galaxy clustering on UV-luminosity and stellar mass at $z \\sim 4 - 7$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Garth D. Illingworth, Ivo Labb\\'e, J. Stuart B. Wyithe, Mauro Stefanon, Pascal A. Oesch, Rychard J. Bouwens, Simon J. Mutch, Yisheng Qiu, YuXiang Qin","submitted_at":"2018-09-26T18:02:38Z","abstract_excerpt":"We investigate the dependence of galaxy clustering at $z \\sim 4 - 7$ on UV-luminosity and stellar mass. Our sample consists of $\\sim$ 10,000 Lyman-break galaxies (LBGs) in the XDF and CANDELS fields. As part of our analysis, the $M_\\star - M_{\\rm UV}$ relation is estimated for the sample, which is found to have a nearly linear slope of $d\\log_{10} M_\\star / d M_{\\rm UV} \\sim 0.44$. We subsequently measure the angular correlation function and bias in different stellar mass and luminosity bins. We focus on comparing the clustering dependence on these two properties. While UV-luminosity is only r"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1809.10161","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"}