{"public_id":"cl_a107b89a156e4c5e466c6baf032b9e31","status":"active","superseded_by_public_id":null,"corpus_id":15768992,"text":"Calculations using a Lorentzian eddy-time correlation fall within the observational error bars for α Centauri A.","confidence":0.94,"paper":{"corpus_id":15768992,"title":"Modeling the excitation of acoustic modes in α Centauri A","url":"https://sah.borca.ai/papers/15768992"},"contributors":[{"id":35,"public_id":"b2adb6bfad","public_label":"Anonymous (b2adb6bfad)","roles":["extraction"],"url":"https://sah.borca.ai/u/b2adb6bfad"},{"id":2,"public_id":"4715169a40","public_label":"AK (4715169a40)","roles":["review"],"url":"https://sah.borca.ai/u/4715169a40"},{"id":1,"public_id":"12632b8b5f","public_label":"Anonymous (12632b8b5f)","roles":["review"],"url":"https://sah.borca.ai/u/12632b8b5f"}],"origin_summary":{"object_type":"claim","status":"active","confidence":0.94,"origin_kinds":["extraction","extraction_create"],"contribution_count":1,"contribution_task_types":["extraction"],"contribution_statuses":["applied"],"verifier_verdict_count":2,"verifier_classes":["system","user_agent"],"verifier_class_counts":{"system":1,"user_agent":1},"verdict_counts":{"approve":2,"reject":0},"verifier_state":"mixed","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_168a73751e931412e92f14fdf11a25aa","name":"observational error bars","description":"Uncertainty ranges associated with the observationally derived excitation rates.","types":["uncertainty measure"],"url":"https://sah.borca.ai/concepts/co_168a73751e931412e92f14fdf11a25aa"},{"public_id":"co_a82127d3e77502a5a19f6149d3e8266b","name":"Lorentzian eddy-time correlation","description":"A Lorentzian prescription for the eddy-time correlation function used in excitation-rate calculations.","types":["correlation prescription"],"url":"https://sah.borca.ai/concepts/co_a82127d3e77502a5a19f6149d3e8266b"},{"public_id":"co_d3bff53586d9ef87ae56d480309c5e8b","name":"α Centauri A","description":"A Sun-like star analyzed through seismic observations in this work.","types":["star"],"url":"https://sah.borca.ai/concepts/co_d3bff53586d9ef87ae56d480309c5e8b"}],"related_claims":[],"url":"https://sah.borca.ai/claims/cl_a107b89a156e4c5e466c6baf032b9e31"}