{"paper":{"title":"Connecting Faint End Slopes of the Lyman-$\\alpha$ emitter and Lyman-break Galaxy Luminosity Functions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Mark Dijkstra, Max Gronke, Michele Trenti, Stuart Wyithe","submitted_at":"2015-01-30T21:32:33Z","abstract_excerpt":"We predict Lyman-$\\alpha$ (Ly$\\alpha$) luminosity functions (LFs) of Ly$\\alpha$-selected galaxies (Ly$\\alpha$ emitters, or LAEs) at $z=3-6$ using the phenomenological model of Dijkstra & Wyithe (2012). This model combines observed UV-LFs of Lyman-break galaxies (LBGs, or drop out galaxies), with constraints on their distribution of Ly$\\alpha$ line strengths as a function of UV-luminosity and redshift. Our analysis shows that while Ly$\\alpha$ LFs of LAEs are generally not Schechter functions, these provide a good description over the luminosity range of $\\log_{10}( L_{\\alpha}/{\\rm erg}\\,{\\rm s}"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1502.00022","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"}