{"id":"W1630925398","doi":"10.1088/0004-637x/808/2/132","title":"CHEMICAL CARTOGRAPHY WITH APOGEE: METALLICITY DISTRIBUTION FUNCTIONS AND THE CHEMICAL STRUCTURE OF THE MILKY WAY DISK","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":613,"is_retracted":false,"has_abstract":true,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Ministerio de Economía y Competitividad; York University; Science and Technology Facilities Council; Carnegie Mellon University; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; University of Arizona; Office of Science; Alfred P. Sloan Foundation; University of Washington; Princeton University; College of Engineering, Michigan State University; Johns Hopkins University; University of Michigan; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; Brookhaven National Laboratory; U.S. Department of Energy; W. M. Keck Foundation; National Science Foundation","keywords":"Milky Way; Metallicity; Stars; RADIUS; Thick disk; Star count; Stellar kinematics; Distribution (mathematics)","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":0.006599589702912307,"score_gpt":0.191516869248521,"score_spread":0.1849172795456087,"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."}}