{"paper":{"title":"Variable broad lines and outflow in the weak blazar PBC J2333.9-2343","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bazzano, A. Malizia, E.F. Jim\\'enez-Andrade, E. Piconcelli, F. Panessa, G. Vietri, I. Saviane, L. Bassani, L. Hern\\'andez-Garc\\'ia, L. Monaco, M. Povi\\'c, N. Masetti, P. Ubertini, S. Cazzoli, V. Chavushyan","submitted_at":"2018-05-18T18:01:50Z","abstract_excerpt":"PBC J2333.9-2343 is a peculiar active nucleus with two giant radio lobes and a weak blazar-like nucleus at their center. In the present work we show new optical, UV, and X-ray data taken from the San Pedro M\\'artir telescope, the New Technology Telescope, NTT/EFOSC2, and the Swift/XRT satellite. The source is highly variable at all frequencies, in particular the strongest variations are found in the broad H$\\alpha$ component with a flux increase of 61$\\pm$4 per cent between 2009 and 2016, following the X-ray flux increase of 62$\\pm$6 per cent between 2010 and 2016. We also detected a broad H$\\"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1805.07366","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"}