{"paper":{"title":"A multi-wavelength study of z = 3.15 Lyman-alpha emitters in the GOODS South Field","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"((1) ESO-Garching, 2), (2) DARK Cosmology Centre, (3) MPA, (4) ESO-Chile), C. Ledoux (4), D. Watson (2), J.P.U. Fynbo (2), Kim K. Nilsson (1, K. Pedersen (2), L.F. Grove (2), M.J. Michalowski (2), O. Moeller (3), P. Moeller (1), P. Rosati (1)","submitted_at":"2007-06-07T20:15:34Z","abstract_excerpt":"Context: Ly-alpha-emitters have proven to be excellent probes of faint, star-forming galaxies in the high redshift universe. However, although the sample of known emitters is increasingly growing, their nature (e.g. stellar masses, ages, metallicities, star-formation rates) is still poorly constrained.\n  Aims: We aim to study the nature of Ly-alpha-emitters, to find the properties of a typical Ly-alpha-emitting galaxy and to compare these properties with the properties of other galaxies at similar redshift, in particular Lyman-break galaxies.\n  Methods: We have performed narrow-band imaging at"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0706.1070","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"}