{"paper":{"title":"The Extreme Ultraviolet Deficit - Jet Connection in the Quasar 1442+101","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Brian Punsly, Christopher P. O'Dea, Marianne Vestergaard, Paola Marziani, Preeti Kharb","submitted_at":"2015-09-09T03:06:47Z","abstract_excerpt":"In previous studies, it has been shown that the long term time average jet power, $\\overline{Q}$, is correlated with the spectral index in the extreme ultraviolet (EUV), $\\alpha_{EUV}$ (defined by $F_{\\nu} \\sim \\nu^{-\\alpha_{EUV}}$ computed between 700\\AA\\, and 1100\\AA\\,). Larger $\\overline{Q}$ tends to decrease the EUV emission. This is a curious relationship because it connects a long term average over $\\sim 10^{6}$ years with an instantaneous measurement of the EUV. The EUV appears to be emitted adjacent to the central supermassive black hole and the most straightforward explanation of the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1509.02619","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"}