{"paper":{"title":"ELT Observations of Supernovae at the Edge of the Universe","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2)European Southern Observatory, (3) ESA/Space Telescope Science Institute, (4)Institut d'Astrophysique de Paris - CNRS, 5, (5)Department of Astronomy, (6)European Southern Observatory, Astrophysics, Baltimore, Chile, Firenze, Garching, J.Bergeron (4), Largo E. Fermi, M. Della Valle (1), Munchen), N.Panagia (3), Paris, P.Dierickx (6) ((1)INAF-Arcetri Astrophysical Observatory, P.Madau (5) J.Spyromilio (2), R.Gilmozzi (2), Santa Cruz, Santiago, University of California","submitted_at":"2005-04-05T10:18:15Z","abstract_excerpt":"We discuss the possibility of using Supernovae as tracers of the star formation history of the Universe for the range of stellar masses $\\sim 3-30$ M$_\\odot$ and possibly beyond. We simulate the observations of 350 SNe, up to $z\\sim 15$, made with OWL (100m) telescope."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0504103","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"}