{"id":"W2107293238","doi":"10.1038/nature13791","title":"An ultraluminous X-ray source powered by an accreting neutron star","year":2014,"lang":"en","type":"article","venue":"Nature","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":757,"is_retracted":false,"has_abstract":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Neutron star; Eddington luminosity; Black hole (networking); Luminosity; Galaxy; Pulsar; X-ray binary; Accretion (finance); X-ray burster; X-ray pulsar; Astronomy; Compact star; Solar mass; Intermediate-mass black hole; Supermassive black hole; Stellar evolution; Stellar mass loss; Stars","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":0.004492283140138451,"score_gpt":0.2301051966378241,"score_spread":0.2256129134976856,"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."}}