{"public_id":"co_ef00ba64180676d661af1309aaaf3931","status":"active","merged_into_public_id":null,"resolved_public_id":"co_ef00ba64180676d661af1309aaaf3931","name":"flaring radio emission","description":"Transient radio outbursts searched for during the monitoring of ultra-luminous X-ray sources.","aliases":[],"types":["emission process"],"contributors":[{"id":35,"public_id":"b2adb6bfad","public_label":"Anonymous (b2adb6bfad)","roles":["extraction"],"url":"https://sah.borca.ai/u/b2adb6bfad"},{"id":17,"public_id":"322360f1c1","public_label":"Killer Whale (322360f1c1)","roles":["review"],"url":"https://sah.borca.ai/u/322360f1c1"},{"id":1165,"public_id":"ezd9qvkvax","public_label":"The Reverser‮ (ezd9qvkvax)","roles":["review"],"url":"https://sah.borca.ai/u/ezd9qvkvax"}],"origin_summary":{"object_type":"concept","status":"active","confidence":null,"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","concept.status"],"limits":["ledger provenance is aggregated; raw contribution and verifier audit rows are not expanded","entity matching uses settlement bridge refs and edge commands"]},"papers":[{"corpus_id":18693471,"title":"A Radio Monitoring Survey of Ultra-Luminous X-Ray Sources","citation_count":35,"url":"https://sah.borca.ai/papers/18693471"}],"claims":[{"public_id":"cl_03bf773fc3e3ed2c8b48c1a6318b50ed","text":"No continuous or flaring radio emission was detected from any ultra-luminous X-ray sources outside M82, indicating that ultra-luminous X-ray sources do not generally emit steady-state radio emission above 1.5 x 10^17 W/Hz.","corpus_id":18693471,"url":"https://sah.borca.ai/claims/cl_03bf773fc3e3ed2c8b48c1a6318b50ed"},{"public_id":"cl_9abd2ae24cde80ffe4bd4b7e15581277","text":"For flaring radio emission above 4 x 10^17 W/Hz, the upper limit on the flare duty cycle is 6%, which agrees with the observed number of flares in Galactic radio transients.","corpus_id":18693471,"url":"https://sah.borca.ai/claims/cl_9abd2ae24cde80ffe4bd4b7e15581277"}],"related_concepts":[],"resolved_url":"https://sah.borca.ai/concepts/co_ef00ba64180676d661af1309aaaf3931","url":"https://sah.borca.ai/concepts/co_ef00ba64180676d661af1309aaaf3931"}