{"paper":{"title":"Stellar populations in the ELT perspective","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.IM","authors_text":"(10) NOAO-CTIO, 2), (2) INAF-OAR, 3), (3) INAF-OATe, (4) ESO, (5) IAC, (6) RSAA, (7) INAF-OAT, (8) DAO-HIA, (9) Obs. C\\^ote d'Azur, A. Milone (6), A. R. Walker (10) ((1) Univ. Rome Tor Vergata, Australia, Canada, Chile), France, F. Thev\\'enin (9), Garching, G. Bono (1, Germany, G. Iannicola (2), I. Ferraro (2), Italy, La Laguna, La Serena, L. Pulone (2), M. Fabrizio (3), M. Monelli (5), M. Nonino (7), Monte Porzio Catone, Nice, NRC, P.B. Stetson (8), R. Buonanno (1, R. Gilmozzi (4), Roma, Spain, Teramo, The Australian National University, Trieste, V. F. Braga (1), Victoria, Weston","submitted_at":"2014-01-22T20:25:37Z","abstract_excerpt":"We discuss the impact that the next generation of Extremely Large Telescopes will have on the open astrophysical problems of resolved stellar populations. In particular, we address the interplay between multiband photometry and spectroscopy."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1401.6372","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"}