{"paper":{"title":"GRB171010A / SN2017htp: a GRB-SN at z=0.33","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Breeveld, A. de Ugarte Postigo, A. Melandri, A. Rossi, A. Sagues Carracedo, C. Barbarino, C.C. Thone, C. Inserra, D.A. Kann, D. B. Malesani, D.H. Hartmann, D.R. Young, D. Xu, F. Hammer, F. Olivares E., G. Pugliese, G. Tagliaferri, J. Bolmer, J. Japelj, J. Kotilainen, J.P. Anderson, J.P.U. Fynbo, J. Sollerman, K.E. Heintz, K. Maguire, L. Izzo, L. Tomasella, M.B. Stone, M. Della Valle, M. De Pasquale, M. Gromadzki, M. Nicholl, N. Masetti, P. Calissendorff, P. D'Avanzo, P. Jakobsson, P. Schady, R. Carini, R. Salvaterra, S. Campana, S. Covino, S.D. Vergani, V. D'Elia, Z. Cano","submitted_at":"2019-10-30T22:21:32Z","abstract_excerpt":"The number of supernovae known to be connected with long-duration gamma-ray bursts is increasing and the link between these events is no longer exclusively found at low redshift ($z \\lesssim 0.3$) but is well established also at larger distances. We present a new case of such a liaison at $z = 0.33$ between GRB\\,171010A and SN\\,2017htp. It is the second closest GRB with an associated supernova of only three events detected by Fermi-LAT. The supernova is one of the few higher redshift cases where spectroscopic observations were possible and shows spectral similarities with the well-studied SN\\,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1910.14160","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/1910.14160/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"}