{"paper":{"title":"Ultraviolet spectra of extreme nearby star-forming regions --- approaching a local reference sample for JWST","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aida Wofford, Alba Vidal-Garc\\'ia, Anna Feltre, Daniel P. Stark, Jacopo Chevallard, Julia Gutkin, Peter Senchyna, Ramesh Mainali, St\\'ephane Charlot, Tucker Jones","submitted_at":"2017-06-03T01:27:21Z","abstract_excerpt":"Nearby dwarf galaxies provide a unique laboratory in which to test stellar population models below $Z_\\odot/2$. Such tests are particularly important for interpreting the surprising high-ionization UV line emission detected at $z>6$ in recent years. We present HST/COS ultraviolet spectra of ten nearby metal-poor star-forming galaxies selected to show He II emission in SDSS optical spectra. The targets span nearly a dex in gas-phase oxygen abundance ($7.8<12+\\log\\mathrm{O/H}<8.5$) and present uniformly large specific star formation rates (sSFR $\\sim 10^2$ $\\mathrm{Gyr}^{-1}$). The UV spectra co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.00881","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"}