{"paper":{"title":"Constraining the transient high-energy activity of FRB180916.J0158+65 with Insight-HXMT followup observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"B.B. Wu, B. Li, B. Meng, B.S. Liu, B.Y. Wu, C. Cai, C.C. Guo, C. Guidorzi, C.K. Li, C.Wang, C.Z. Liu, D.K. Zhou, D.W. Han, E. Virgilli, F. Frontera, F.J. Lu, F. Zhang, G.C. Xiao, G.H. Gao, G. Li, G. Ou, H. Gao, H.M. Zhang, H.S. Zhao, H.W. Liu, H.X. Liu, J. Guan, J. Huo, J. Jin, J.L Qu, J.Y. Liao, J.Y. Nie, J. Zhang, L. Amati, L. Chen, L.D. Kong, L.J. Wang, L.M. Song, L. Nicastro, L. Sun, L. Tao, M. Gao, M. Orlandini, M. Wu, M.Y. Ge, N. Sai, P.J. Wang, P. Zhang, Q.B. Yi, Q.C. Bu, Q. Luo, Q.Q. Yin, R.C. Ma, R. Yang, S.J. Zheng, S.L. Xiong, S.M. Jia, S.N. Zhang, S. Xiao, S. Yang, S. Zhang, T. Luo, T.P. Li, T.X. Chen, W.C. Jiang, W.C. Zhang, W. Li, W.S. Wang, W.W. Cui, W. Zhang, X.B. Li, X.F. Li, X.F. Lu, X.F. Zhao, X.H. Liang, X.J. Liu, X.L. Cao, X. Li, X. Ma, X.Q. Ren, X.Y. Song, X.Y. Wen, Y. Chen, Y.D. Gu, Y.F. Zhang, Y.G. Zheng, Y. Huang, Y.H. Zhang, Y.J. Yang, Y.L. Tuo, Y. Nang, Y.P. Chen, Y.P. Xu, Y.S. Wang, Y. Tan, Y.Y. Du, Y. You, Z. Chang, Z.W. Li","submitted_at":"2020-08-27T07:41:17Z","abstract_excerpt":"A link between magnetars and fast radio burst (FRB) sources has finally been established. In this context, one of the open issues is whether/which sources of extra galactic FRBs exhibit X/gamma-ray outbursts and whether it is correlated with radio activity. We aim to constrain possible X/gamma-ray burst activity from one of the nearest extragalactic FRB sources currently known over a broad energy range, by looking for bursts over a range of timescales and energies that are compatible with being powerful flares from extragalactic magnetars. We followed up the as-yet nearest extragalactic FRB so"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2008.11965","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2008.11965/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"}