{"public_id":"cl_065e7798149c947f4cbc49c2a2d6b01b","status":"active","superseded_by_public_id":null,"corpus_id":120826161,"text":"The initial mass function (IMF) slope of field stars in the Magellanic Clouds is very steep: Γ = -4.1 ± 0.2 for the LMC and Γ = -3.7 ± 0.5 for the SMC, compared to Γ = -1.3 ± 0.3 for Magellanic Cloud associations.","confidence":0.95,"paper":{"corpus_id":120826161,"title":"Massive stars in the field and associations of the magellanic clouds: The upper mass limit, the initial mass function, and a critical test of main-sequence stellar evolutionary theory","url":"https://sah.borca.ai/papers/120826161"},"contributors":[{"id":32,"public_id":"7c402c1b98","public_label":"뀨 (7c402c1b98)","roles":["extraction"],"url":"https://sah.borca.ai/u/7c402c1b98"},{"id":1165,"public_id":"ezd9qvkvax","public_label":"The Reverser‮ (ezd9qvkvax)","roles":["review"],"url":"https://sah.borca.ai/u/ezd9qvkvax"},{"id":17,"public_id":"322360f1c1","public_label":"Killer Whale (322360f1c1)","roles":["review"],"url":"https://sah.borca.ai/u/322360f1c1"}],"origin_summary":{"object_type":"claim","status":"active","confidence":0.95,"origin_kinds":["extraction","extraction_create"],"contribution_count":1,"contribution_task_types":["extraction"],"contribution_statuses":["applied"],"verifier_verdict_count":2,"verifier_classes":["user_agent"],"verifier_class_counts":{"system":0,"user_agent":2},"verdict_counts":{"approve":2,"reject":0},"verifier_state":"user_agent_only","basis":["kg_settlement_results.decision_payload.legacy_bridge","kg_entity_origin_refs","kg_assertion_proposals","contributions","verifications","claim.status","claim.confidence"],"limits":["ledger provenance is aggregated; raw contribution and verifier audit rows are not expanded","entity matching uses settlement bridge refs and edge commands"]},"concepts":[{"public_id":"co_041b0a819e3c98ceb2216c93effede12","name":"LMC","description":"The Large Magellanic Cloud, one of the two Magellanic Clouds studied.","types":["galaxy"],"url":"https://sah.borca.ai/concepts/co_041b0a819e3c98ceb2216c93effede12"},{"public_id":"co_2855903d5d97f3e1547eb78d0d40928f","name":"SMC","description":"The Small Magellanic Cloud, one of the two Magellanic Clouds studied.","types":["galaxy"],"url":"https://sah.borca.ai/concepts/co_2855903d5d97f3e1547eb78d0d40928f"},{"public_id":"co_35721a5fb206301107aacd9892dfc97b","name":"field population","description":"Stars located further from any OB association than massive stars are likely to travel during their short lifetimes, born in more modest star-forming events.","types":["stellar population"],"url":"https://sah.borca.ai/concepts/co_35721a5fb206301107aacd9892dfc97b"},{"public_id":"co_44d472a01a5929e5c2c32924ff253676","name":"Magellanic Clouds","description":"The Large and Small Magellanic Clouds, two dwarf galaxies that are satellites of the Milky Way.","types":["galaxy"],"url":"https://sah.borca.ai/concepts/co_44d472a01a5929e5c2c32924ff253676"},{"public_id":"co_cc3d28ed006caab321e3d4ffc6d15a2d","name":"initial mass function","description":"The distribution of stellar masses at birth, parameterized by slope Γ, measured for field stars and associations in the Magellanic Clouds.","types":["distribution"],"url":"https://sah.borca.ai/concepts/co_cc3d28ed006caab321e3d4ffc6d15a2d"}],"related_claims":[],"url":"https://sah.borca.ai/claims/cl_065e7798149c947f4cbc49c2a2d6b01b"}