{"id":"W2061710077","doi":"10.1086/382723","title":"[O<scp>ii</scp>] as a Star Formation Rate Indicator","year":2004,"lang":"en","type":"article","venue":"The Astronomical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":425,"is_retracted":false,"has_abstract":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Metallicity; Galaxy; Redshift; Star formation; Luminosity; Ionization; Interstellar medium; Doubly ionized oxygen; Spectral line; Astronomy; Emission spectrum","routes":{"ca_aff":false,"ca_fund":false,"ca_venue":false,"about_ca":true,"invisible_to_affiliation_only":true},"retraction":null,"screen":null,"machine_scores":{"provisional":true,"baseline":true,"maturity_gate_passed":false,"score_opus":0.006505128968869449,"score_gpt":0.2054823119805778,"score_spread":0.1989771830117084,"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."}}