{"paper":{"title":"Clues on High Energy Emission Mechanism from Blazar 3C 454.3 during 2015 August Flare","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Naseer Iqbal, Nijil Mankuzhiyil, Pankaj Kushwaha, Ranjeev Misra, S. Sahayanathan, Zahir Shah","submitted_at":"2017-05-17T14:43:16Z","abstract_excerpt":"We perform a detailed spectral study of a recent flaring activity from the Flat Spectrum Radio Quasar (FSRQ), 3C\\,454.3, observed simultaneously in optical, UV, X-ray and $\\gamma$-ray energies during 16 to 28 August, 2015. The source reached its peak $\\gamma$-ray flux of $(1.9\\pm0.2)\\times\\,10^{-05} \\; {\\rm ph\\,cm^{-2}\\,s^{-1}}$ on 22 August. The time averaged broadband spectral energy distribution (SED) is obtained for three time periods, namely \"flaring state\"; covering the peak $\\gamma$-ray flux, \"post flaring state\"; immediately following the peak flare and \"quiescent state\"; separated fro"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.06185","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"}