{"paper":{"title":"The Highly Energetic Expansion of SN2010bh Associated with GRB 100316D","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alberto J. Castro-Tirado, Alexei V. Filippenko, Andrew J. Levan, Antonio de Ugarte Postigo, Bo Milvang-Jensen, Daniele Malesani, Daniel E. Reichart, David Bersier, Elena Pian, Eliana Palazzi, Enrico Cappellaro, Felix I. Mirabel, Filomena Bufano (1), Francois Hammer, Gianpiero Tagliaferri, Giuliano Pignata, Giulia Stratta, Guido Chincarini, Javier Gorosabel, Jens Hjorth, Jesper Sollerman, Jinsong Deng, Jochen Greiner, Johan Fynbo, Keiichi Maeda, Kenichi Nomoto, Klass Wiersema, Koji S. Kawabata, Lex Kaper, Lorenzo Amati, Masaomi Tanaka, Massimo Della Valle, Massimo Turatto, Nial R. Tanvir, Nicola Masetti, Palle Moller, Pall Jakobsson, Paolo A. Mazzali, Paolo D'Avanzo, Paolo Goldoni, Patrizia Ferrero, Ralph A.M.J. Wijers ((1) INAF-Osservatorio Astronomico di Catania), Rhaana L. C. Starling, Ruben Salvaterra, Sergio Campana, Silvia Piranomonte, Stefano Benetti, Stefano Covino, Stefano Valenti, Susanna D. Vergani, Sylvio Klose, Valerio D'Elia, Zach Cano","submitted_at":"2011-11-19T03:03:53Z","abstract_excerpt":"We present the spectroscopic and photometric evolution of the nearby (z = 0.059) spectroscopically confirmed type Ic supernova, SN 2010bh, associated with the soft, long-duration gamma-ray burst (X-ray flash) GRB 100316D. Intensive follow-up observations of SN 2010bh were performed at the ESO Very Large Telescope (VLT) using the X-shooter and FORS2 instruments. Owing to the detailed temporal coverage and the extended wavelength range (3000--24800 A), we obtained an unprecedentedly rich spectral sequence among the hypernovae, making SN 2010bh one of the best studied representatives of this SN c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1111.4527","kind":"arxiv","version":2},"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"}