{"paper":{"title":"The P\\'egase.3 code of spectrochemical evolution of galaxies: documentation and complements","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.IM","authors_text":"2), (2) Sorbonne universit\\'e, 3) ((1) Institut d'Astrophysique de Paris, (3) Universit\\'e Paris-Sud), Brigitte Rocca-Volmerange (1, Michel Fioc (1","submitted_at":"2019-02-06T14:22:08Z","abstract_excerpt":"P\\'egase.3 is a Fortran 95 code modeling the spectral evolution of galaxies from the far-ultraviolet to submillimeter wavelengths. It also follows the chemical evolution of their stars, gas and dust.\n  For a given scenario (a set of parameters defining the history of mass assembly, the star formation law, the initial mass function...), P\\'egase.3 consistently computes the following:\n  * the star formation, infall, outflow and supernova rates from 0 to 20 Gyr;\n  * the stellar metallicity, the abundances of main elements in the gas and the composition of dust;\n  * the unattenuated stellar spectr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1902.02198","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"}