{"id":"W2131260550","doi":"10.1051/0004-6361:20054185","title":"The Supernova Legacy Survey: measurement of $\\Omega_{\\mathsf{M}}$, $\\Omega_\\mathsf{\\Lambda}$ and<i>w</i>from the first year data set","year":2006,"lang":"en","type":"article","venue":"Astronomy and Astrophysics","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":2459,"is_retracted":false,"has_abstract":true,"ca_institutions":"University of Toronto; University of Victoria","funders":"Institut National de Physique Nucléaire et de Physique des Particules; Institut national des sciences de l'Univers; Comisión Nacional de Investigación Científica y Tecnológica; Fundação para a Ciência e a Tecnologia; Australian Research Council; Nuclear Physics; Natural Sciences and Engineering Research Council of Canada; France-Berkeley Fund; Centre National de la Recherche Scientifique; European Southern Observatory; Conselho Nacional de Desenvolvimento Científico e Tecnológico; California Institute of Technology; U.S. Department of Energy; Consejo Nacional de Investigaciones Científicas y Técnicas; Office of Science; National Science Foundation","keywords":"Physics; Omega; Hubble's law; Dark energy; Astrophysics; Redshift; Sky; Supernova; Cosmology; Cosmic distance ladder; Baryon acoustic oscillations; Photometry (optics); Lambda; Astronomy; Baryon; Galaxy; Stars; Optics","routes":{"ca_aff":true,"ca_fund":true,"ca_venue":false,"about_ca":true,"invisible_to_affiliation_only":false},"retraction":null,"screen":null,"machine_scores":{"provisional":true,"baseline":true,"maturity_gate_passed":false,"score_opus":0.02616750270020374,"score_gpt":0.2206994096423309,"score_spread":0.1945319069421272,"validation_status":"score_only:v0-immature-baseline","note":"Baseline scores from an immature model (maturity gate not passed). Scores rank; they never assert a category."}}