{"paper":{"title":"On the multi-wavelength Emission from CTA 102","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D. Zargaryan, N. Sahakyan, S. Gasparyan, V. Baghmanyan","submitted_at":"2018-07-08T19:27:31Z","abstract_excerpt":"We report on broadband observations of CTA 102 ($z=1.037$) during the active states in 2016-2017. In the $\\gamma$-ray band, Fermi LAT observed several prominent flares which followed a harder-when-brighter behavior: the hardest photon index $\\Gamma=1.61\\pm 0.10$ being unusual for FSRQs. The peak $\\gamma$-ray flux above 100 MeV $(3.55\\pm0.55)\\times10^{-5}\\:{\\rm photon\\:cm^{-2}\\:s^{-1}}$ observed on MJD 57738.47 within 4.31 minutes, corresponds to an isotropic $\\gamma$-ray luminosity of $L_{\\gamma}=3.25\\times10^{50}\\:{\\rm erg\\:s^{-1}}$, comparable with the highest values observed from blazars so"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.02869","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"}