{"paper":{"title":"Investigating the origin of the Fe emission lines of the Seyfert 1 galaxy Mrk~205","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Matteo Guainazzi, Ritesh Ghosh, Shruti Tripathi, Sibasish Laha","submitted_at":"2019-04-13T04:11:10Z","abstract_excerpt":"We have investigated the nature and origin of the Fe K emission lines in Mrk~205 using observations with {\\it Suzaku} and {\\it XMM-Newton}, aiming to resolve the ambiguity between a broad emission line and multiple unresolved lines of higher ionization. We detect the presence of a narrow Fe K$\\alpha$ emission line along with a broad band Compton reflection hump at energies $E>10 \\rm \\, keV$. These are consistent with reflected emission of hard X-ray photons off a Compton thick material of $N_{\\rm H} \\ge 2.15\\times 10^{24} \\rm cm^{-2}$. In addition we detect a partially covering ionized absorpt"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1904.06476","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"}