{"id":"W2076246932","doi":"10.1093/mnras/stu1738","title":"Galaxies on FIRE (Feedback In Realistic Environments): stellar feedback explains cosmologically inefficient star formation","year":2014,"lang":"en","type":"article","venue":"Monthly Notices of the Royal Astronomical Society","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1458,"is_retracted":false,"has_abstract":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Smithsonian Astrophysical Observatory; Smithsonian Institution; University of California, San Diego; Johns Hopkins University; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Gordon and Betty Moore Foundation; Simons Foundation; California Institute of Technology; National Aeronautics and Space Administration; David and Lucile Packard Foundation; Ministerio de Ciencia e Innovación; National Science Foundation","keywords":"Physics; Astrophysics; Halo; Galaxy; Star formation; Supernova; Accretion (finance); Redshift; Galaxy formation and evolution; Stellar mass; Galactic halo; Radiative transfer; Astronomy","routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false,"invisible_to_affiliation_only":false},"retraction":null,"screen":null,"machine_scores":{"provisional":true,"baseline":true,"maturity_gate_passed":false,"score_opus":0.007755565867840401,"score_gpt":0.186592244881782,"score_spread":0.1788366790139416,"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."}}