{"paper":{"title":"Unveiling slim accretion disc in AGN through X-ray and Infrared observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Chen Hu, Hagai Netzer, Jian-Min Wang, Jin-Ming Bai, Luis C. Ho, N\\'uria Castell\\'o-Mor, Pu Du, Shai Kaspi, Wei-Hao Bian, Ye-Fei Yuan","submitted_at":"2017-01-30T19:01:25Z","abstract_excerpt":"In this work, which is a continuation of Castell\\'o-Mor et al. (2016), we present new X-ray and infrared (IR) data for a sample of active galactic nuclei (AGN) covering a wide range in Eddington ratio over a small luminosity range. In particular, we rigorously explore the dependence of the optical-to-X-ray spectral index $\\alpha_{OX}$ and the IR-to-optical spectral index on the dimensionless accretion rate, $\\dot{\\mathcal{M}}=\\dot{m}/\\eta$ where $\\dot{m}=L_{AGN}/L_{Edd}$ and $\\eta$ is the mass-to-radiation conversion efficiency, in low and high accretion rate sources. We find that the SED of t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.08781","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"}