{"paper":{"title":"Fundamental Plane of Black Hole Activity in Quiescent Regime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Feng Yuan, Fu-Guo Xie","submitted_at":"2017-01-22T09:47:27Z","abstract_excerpt":"A correlation among the radio luminosity ($L_{\\rm R}$), X-ray luminosity ($L_{\\rm X}$), and black hole mass ($M_{\\rm BH}$) in active galactic nuclei (AGNs) and black hole binaries is known to exist and is called the \"Fundamental Plane\" of black hole activity. Yuan & Cui (2005) predicts that the radio/X-ray correlation index, $\\xi_{\\rm X}$, changes from $\\xi_{\\rm X}\\approx 0.6$ to $\\xi_{\\rm X}\\approx 1.2-1.3$ when $L_{\\rm X}/L_{\\rm Edd}$ decreases below a critical value $\\sim 10^{-6}$. While many works favor such a change, there are also several works claiming the opposite. In this paper, we ga"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.06143","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"}