{"paper":{"title":"Spectroscopic Discovery of the Supernova 2003dh Associated with GRB 030329","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B. Pindor, D. Bersier, D. J. Eisenstein, E. W. Olszewski, J. C. Lee, K. Krisciunas, K. Z. Stanek, L. Echevarria, M. L. Calkins, N. Caldwell, N. Hathi, P. Berlind, P. Challis, P. Harding, P. Martini, P. M. Garnavich, R. A. Jansen, R. Schild, R. Windhorst, S. T. Holland, T. Matheson, W. R. Brown","submitted_at":"2003-04-10T02:30:13Z","abstract_excerpt":"We present early observations of the afterglow of the Gamma-Ray Burst (GRB) 030329 and the spectroscopic discovery of its associated supernova SN 2003dh. We obtained spectra of the afterglow of GRB 030329 each night from March 30.12 (0.6 days after the burst) to April 8.13 (UT) (9.6 days after the burst). The spectra cover a wavelength range of 350 nm to 850 nm. The early spectra consist of a power-law continuum (F_nu ~ nu^{-0.9}) with narrow emission lines originating from HII regions in the host galaxy, indicating a low redshift of z=0.1687. However, our spectra taken after 2003 Apr. 5 show "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0304173","kind":"arxiv","version":4},"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"}