{"paper":{"title":"Spectroscopy of the Type Ic Supernova SN\\,2017iuk Associated with Low-redshift GRB\\,171205A","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D. Xu, H. J. Wang, J. B. Zhang, J. S. Deng, J. Wang, J. Y. Wei, L. P. Xin, P. Qiu, Y. L. Qiu, Z. P. Zhu","submitted_at":"2018-10-08T02:39:12Z","abstract_excerpt":"We here report a spectroscopic monitor for the supernova SN\\,2017iuk associated with the long-duration low-luminosity gamma-ray burst GRB\\,171205A at a redshift of 0.037, which is up to now the third GRB-SN event away from us. Our spectroscopic observations and spectral analysis allow us to identify SN\\,2017iuk as a typical broad-line type Ic SN. A comparison study suggests that the type-IcBL SN\\,2017iuk resembles to SN\\,2006aj in following aspects: 1) similar spectra at the nearby epochs, 2) comparable evolution of the photospheric velocity obtained from the measurements based on both \\ion{Si"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1810.03250","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"}