{"paper":{"title":"The VLT LBG Redshift Survey - V. Characterising the z = 3.1 Lyman Alpha Emitter Population","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Orsi (CEFCA), E. Ba\\~nados (PUC, H. Francke (ALMA), Jorge Gonz\\'alez-L\\'opez (PUC), Khon Kaen), L. Infante (PUC), MPIA), N. H. M. Crighton (Swinburne), P. Tummuangpak (Durham, R. M. Bielby (Durham), T. Shanks (Durham)","submitted_at":"2015-01-06T16:11:21Z","abstract_excerpt":"We present a survey of $z\\sim3$ Ly$\\alpha$ emitters (LAEs) within the fields of the VLT LBG Redshift Survey. The data encompasses 5 independent survey fields co-spatial with spectroscopic LBG data and covering a larger total area than previously analysed for LAE number counts and clustering. This affords an improved analysis over previous work by minimising the effects of cosmic variance and allowing the cross-clustering analysis of LAEs and LBGs. Our photometric sample consists of $\\approx600$ LAE candidates, over an area of 1.07~deg$^2$, with equivalent widths of $\\gtrsim65$~\\AA\\ and a flux "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.01215","kind":"arxiv","version":2},"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"}