{"paper":{"title":"Stellar atmospheric parameters and chemical abundances of about 5 million stars from S-PLUS multi-band photometry","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":["astro-ph.IM","astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"A. Alvarez-Candal, A. Kanaan, A. R. Lopes, A. V. Smith Castelli, B. Cubillos Palma, B. Dias, C. E. Ferreira Lopes, C. J. Bonatto, C. Mendes de Oliveira, C. R. Bom, D. Hazarika, D. R. Gon\\c{c}alves, E. Machado-Pereira, F. Almeida-Fernandes, G. B. Oliveira Schwarz, G. Limberg, H. D. Perottoni, J. Alonso-Garc\\'ia, L. A. Guti\\'errez-Soto, M. Borges Fernandes, M. Catelan, M. E. De Rossi, M. Jaque Arancibia, N. G. de Is\\'idio, N. Monsalves, P. K. Humire, R. C. Thom de Souza, S. Akras, S. Daflon, V. Cordeiro, V. M. Placco, V. S. Ferreira Alberice, W. Schoenell","submitted_at":"2024-11-27T20:50:40Z","abstract_excerpt":"Context. Spectroscopic surveys like APOGEE, GALAH, and LAMOST have significantly advanced our understanding of the Milky Way by providing extensive stellar parameters and chemical abundances. Complementing these, photometric surveys with narrow/medium-band filters, such as the Southern Photometric Local Universe Survey (S-PLUS), offer the potential to estimate stellar parameters and abundances for a much larger number of stars.\n  Aims. This work develops methodologies to extract stellar atmospheric parameters and selected chemical abundances from S-PLUS photometric data, which spans ~3000 squa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.18748","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2411.18748/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"}