{"paper":{"title":"The $\\rm{Y_{SZ,Planck} - Y_{SZ,XMM}}$ scaling relation and its difference between cool-core and non-cool-core clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Cheng-Kui Li, Hai-Hui Zhao, Shu-Mei Jia, Yong Chen, Yuan-Hao Wang, Yue Zhu","submitted_at":"2019-02-20T11:03:46Z","abstract_excerpt":"We construct a sample of 70 clusters using data from XMM-Newton and Planck to investigate the $Y_{\\rm SZ,Planck}-Y_{\\rm SZ, XMM}$ scaling relation and the cool-core influences on the relation. $Y_{\\rm SZ,XMM}$ is calculated by accurate de-projected temperature and electron number density profiles derived from XMM-Newton. $Y_{\\rm SZ,Planck}$ is the latest Planck data restricted to our precise X-ray size $\\theta_{\\rm 500}$. To study the cool-core influences on$Y_{\\rm SZ,Planck}-Y_{\\rm SZ, XMM}$ scaling relation, we apply two criteria, limits of central cooling time and classic mass deposition ra"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1902.07507","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"}