{"paper":{"title":"The Radio and $\\gamma$-ray Variability Analysis of S5 0716+714","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D. F. Guo, F. W. Lu, H. M. Zhang, H. Z. Li, J. Y. Ren, Q. G. Gao, T. F. Yi, X. Chen, Y. G. Jiang","submitted_at":"2018-01-20T09:00:47Z","abstract_excerpt":"We have studied the variability of \\object{S5 0716+714} at radio 15 GHz and $\\gamma$-ray band using three different methods. A possible periodicity of $P_{15 GHz}=266.0\\pm11.5$ and $P_{\\gamma}=344.0\\pm16.4$ days are obtained for radio 15 GHz and $\\gamma$-ray light curves, respectively. The variability may be related to the intrinsically emission mechanism. The difference between the variability timescales of radio 15 GHz and $\\gamma$-ray may be due to that the emission of radio 15 GHz is produced via the synchrotron process, while the $\\gamma$-ray is produced by both the SSC and EC processes."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.06640","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"}