{"paper":{"title":"GRB 130606A within a sub-DLA at redshift 5.91","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"1), 16), 2), 20), 20) ((1) IAA-CSIC, (26) \\.Istanbul Uni, 6, 7), A. J. Castro-Tirado (1, A. Mart\\'in-Carrillo (4), A. S. Pozanenko (12), A. Tejero (19, Austin, A. Volnova (12), Bilbao, C. \\'Alvarez-Iglesias (19, Canada. (4) Uni. College Dublin, Czech Republic. (16) Czech Technical Uni. Czech Republic. (17) Fyzik\\'aln\\'i \\'ustav Czech Republic. (18) Uni. de Ja\\'en, D. P\\'erez-Ram\\'irez (18), E. G\\\"o\\u{g}\\\"u\\c{s} (25), E. Sonbas (11), France. (9) Aryabhatta Research Institute of Observational Sciences, Georgia Republic. (22) SRI, Germany. (24) ESAC, I. H. Park (27), India. (10) Nikolaev National Uni. Ukraine. (11) Uni. of Adiyaman, Ireland. (5) Uni. of Texas, J. Cepa (19, J. Gorosabel (1, J. M. Castro Cer\\'on (24), J. M. Winters (8), J. \\v{S}trobl (15, Korea. (28) INTA, L. Hanlon (4), L. Sabau-Graziati (28), M. Bremer (8), M. Jel\\'inek (1), M. Topinka (4), N. Gehrels (14), O. Lara-Gil (1), \\\"O. \\\"Onal Ta\\c{s} (26), P. Ferrero (1), P. Kub\\'anek (17), R. Cunniffe (1), R. Fern\\'andez-Mu\\~noz (13), R. Hudec (15, R. Inasaridze (21), R. S\\'anchez-Ram\\'irez (1), Russia. (13) UMA-CSIC, S. B. Pandey (9), S. Guziy (10, S. Hellmich (23), S. Jeong (1), S. L. Ellison (3), S. Meegan (4), S. Mottola (23), Spain), Spain. (14) NASA/GSFC, Spain. (19) IAC, Spain. (20) Uni. La Laguna, Spain. (21) Ilia State Uni., Spain. (25) Sabanc{\\i} Uni. Turkey, Spain. (2) Uni. M\\'alaga, Spain. (3) Uni. of Victoria, Spain. (7) Ikerbasque, Spain. (8) IRAM, T. G\\\"uver (26), Turkey. (12) RAS, Turkey. (27) Sungkyunkwan Uni, Ukraine. (23) DLR, USA. (15) Astronomical Institute, USA. (6) UPV/EHU-IAA/CSIC, V. Bromm (5), V. F. Mu\\~noz-Mart\\'inez (2), V. Rumyantsev (22)","submitted_at":"2013-12-19T16:49:36Z","abstract_excerpt":"Events such as GRB130606A at z=5.91, offer an exciting new window into pre-galactic metal enrichment in these very high redshift host galaxies. We study the environment and host galaxy of GRB 130606A, a high-z event, in the context of a high redshift population of GRBs. We have obtained multiwavelength observations from radio to gamma-ray, concentrating particularly on the X-ray evolution as well as the optical photometric and spectroscopic data analysis. With an initial Lorentz bulk factor in the range \\Gamma_0 ~ 65-220, the X-ray afterglow evolution can be explained by a time-dependent photo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.5631","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"}