{"paper":{"title":"New Binary and Millisecond Pulsars from Arecibo Drift-Scan Searches","arxiv_id":"astro-ph/0404181","primary_cat":"astro-ph","submitted_at":"2004-04-08T10:37:51+00:00","version_compiled":"v1"},"notice":"Every quoted sentence is the authors' text from the arXiv listing abstract. Labels and probabilities are the outputs of classifier-1.13.0 on the question bank abstract-p1-20260923, exactly as returned. 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isolated.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.88,"main_claim_p":0.05,"quantitative":true,"quantitative_p":0.97,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.99,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.0}},{"i":2,"p":0.99,"id":"s2","own":true,"role":"result","text":"The 5.8-ms pulsar J1453+19 may have a low-mass companion.","hedge":{"p":1.0,"label":"hedged_possibility"},"own_p":0.8,"main_claim_p":0.05,"quantitative":true,"quantitative_p":0.88,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.99,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.01}},{"i":3,"p":0.78,"id":"s3","own":true,"role":"interpretation","text":"We discuss these pulsars in the context of isolated millisecond pulsar formation and the minimum spin period of neutron 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