{"paper":{"title":"The Evolution Of The Faint End Of The UV Luminosity Function During The Peak Epoch Of Star Formation (1<z<3)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"(10) University of California Santa Cruz, (11) Steward Observatory University of Arizona, (12) Infrared Processing, (2) Centre de Recherche Astrophysique de Lyon, (3) Goddard Space Flight Center, 4), (4) STScI (5) Centre for Extragalactic Astronomy Durham, 6, (6) Institute for Computational Cosmology Durham University, 7), (7) Astrophysics, (8) Laboratoire d\\'eAstrophysique de Marseille-LAM, (9) Minnesota Institute for Astrophysics, Anahita Alavi (1), Analysis Center Caltech), Brant Robertson (10), Brian Siana (1), Claudia Scarlata (9), Cosmology Research Unit University of KwaZulu-Natal, Daniel P. Stark (11), Harry I. Teplitz (12), Johan Richard (2), Marceau Limousin (8), Marc Rafelski (3, Mathilde Jauzac (5, Vandana Desai (12) ((1) University Of California Riverside, William R. Freeman (1)","submitted_at":"2016-06-01T21:04:48Z","abstract_excerpt":"[Abridged] We present a robust measurement of the rest-frame UV luminosity function (LF) and its evolution during the peak epoch of cosmic star formation at 1<z<3. We use our deep near ultraviolet imaging from WFC3/UVIS on the Hubble Space Telescope (HST) and existing ACS/WFC and WFC3/IR imaging of three lensing galaxy clusters, Abell 2744 and MACSJ0717 from the Hubble Frontier Field survey and Abell 1689. We use photometric redshifts to identify 780 ultra-faint galaxies with $M_{UV}$<-12.5 AB mag at 1<z<3. From these samples, we identified 5 new, faint, multiply imaged systems in A1689. We co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.00469","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"}