{"paper":{"title":"Signatures of the disk-jet coupling in the Broad-line Radio Quasar 4C+74.26","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. A. Zdziarski, A. Kuzmicz, A. Markowitz, B. Debski, D. B. Caton, D. Koziel-Wierzbowska, G. Bhatta, G. Stachowski, J. Machalski, K. Balasubramaniam, L. Stawarz, M. Drozdz, M. Jamrozy, M. Ostrowski, M. Siwak, S. Zola, T. Kundera, V. S. Paliya, W. Ogloza","submitted_at":"2018-05-17T20:19:47Z","abstract_excerpt":"Here we explore the disk-jet connection in the broad-line radio quasar 4C+74.26, utilizing the results of the multiwavelength monitoring of the source. The target is unique in that its radiative output at radio wavelengths is dominated by a moderately-beamed nuclear jet, at optical frequencies by the accretion disk, and in the hard X-ray range by the disk corona. Our analysis reveals a correlation (local and global significance of 96\\% and 98\\%, respectively) between the optical and radio bands, with the disk lagging behind the jet by $250 \\pm 42$ days. We discuss the possible explanation for "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1805.06957","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"}