{"paper":{"title":"Extragalactic background light inferred from AEGIS galaxy SED-type fractions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Dominguez (Universidad de Sevilla/IAA-CSIC), C. J. Conselice (Nottingham), D. C. Koo (UCSC), D. J. Rosario (UCSC), F. Prada (IAA-Csic), J. A. Newman (Pittsburgh), J. R. Primack (UCSC), J.-S. Huang (CfA), M. A. Perez-Torres (IAA-CSIC), M. C. Cooper (Arizona), M. Davis (Berkeley), M. Lozano (Sevilla), P. Barmby (Western Ontario), P. Guhathakurta (UCSC), P. Perez-Gonzalez (Uni. Comp. de Madrid), R. C. Gilmore (SISSA), R. S. Somerville (STSCI), S. M. Faber (UCSC)","submitted_at":"2011-03-15T20:00:05Z","abstract_excerpt":"The extragalactic background light (EBL) is of fundamental importance both for understanding the entire process of galaxy evolution and for gamma-ray astronomy. However, the overall spectrum of the EBL between 0.1 and 1000 microns has never been determined directly neither from observed luminosity functions (LFs), over a wide redshift range, nor from any multiwavelength observation of galaxy spectral energy distributions (SEDs). The evolving, overall spectrum of the EBL is derived here utilizing a novel method based on observations only. The changing fractions of quiescent galaxies, star-formi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1103.4534","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"}