{"id":"W1993246016","doi":"10.1093/mnras/sts535","title":"Cosmological simulations with self-interacting dark matter – II. Halo shapes versus observations","year":2013,"lang":"en","type":"article","venue":"Monthly Notices of the Royal Astronomical Society","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":513,"is_retracted":false,"has_abstract":true,"ca_institutions":"","funders":"University of California, Irvine; Institut Périmètre de physique théorique; Industry Canada; Consejo Nacional de Ciencia y Tecnología; National Science Foundation; Government of Canada; Ministero dello Sviluppo Economico; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; National Aeronautics and Space Administration","keywords":"Physics; Dark matter; Halo; Astrophysics; Galaxy cluster; Cluster (spacecraft); Galaxy; Dark matter halo; Weak gravitational lensing; Cuspy halo problem; Cold dark matter; Redshift","routes":{"ca_aff":false,"ca_fund":true,"ca_venue":false,"about_ca":false,"invisible_to_affiliation_only":true},"retraction":null,"screen":null,"machine_scores":{"provisional":true,"baseline":true,"maturity_gate_passed":false,"score_opus":0.01245707121658018,"score_gpt":0.2066315807846246,"score_spread":0.1941745095680444,"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."}}