{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:TSUI2TD6XREMGKP3D55NZH6J5C","short_pith_number":"pith:TSUI2TD6","schema_version":"1.0","canonical_sha256":"9ca88d4c7ebc48c329fb1f7adc9fc9e8ae65355f48d0828d9222f25242e174ce","source":{"kind":"arxiv","id":"2501.14247","version":1},"attestation_state":"computed","paper":{"title":"A flaring radio counterpart to a fast radio burst reveals a newborn magnetized engine","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Bing Zhang, Wenfei Yu, Xian Zhang, Yi Xing, Zhen Yan","submitted_at":"2025-01-24T05:19:24Z","abstract_excerpt":"Fast Radio Bursts (FRBs) are energetic millisecond radio bursts at cosmological distances, whose underlying engine is not identified. Among a sub-population that emit repeated radio bursts, a handful were associated with a persistent radio source (PRS) whose origin is unknown. Here we report the discovery of a compact flaring radio source (FRS) associated with a newly-active repeating FRB within one month after the first radio burst was detected. Its temporal and spectral characteristics differ from those of the PRSs but are similar to those of engine-powered supernovae and low-luminosity acti"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2501.14247","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-01-24T05:19:24Z","cross_cats_sorted":[],"title_canon_sha256":"d52f8e56d94d2d42d0326c5e0b47e8eff32beeff872dd29dd54a988904f75d81","abstract_canon_sha256":"05d40646ccf6fbbaf7288921a7a4b6c9a811f6a8eebe9cc98c09791aafab3a15"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:04:47.809639Z","signature_b64":"l5uz4L8y08kx6GnHA6aMzZ+JkLFR6is0rwNtQHEEVGQxMB7dfpEtI0g2kgrFgm550lWfzKEDV3ajYl0yZKIZAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9ca88d4c7ebc48c329fb1f7adc9fc9e8ae65355f48d0828d9222f25242e174ce","last_reissued_at":"2026-07-05T10:04:47.809171Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:04:47.809171Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A flaring radio counterpart to a fast radio burst reveals a newborn magnetized engine","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Bing Zhang, Wenfei Yu, Xian Zhang, Yi Xing, Zhen Yan","submitted_at":"2025-01-24T05:19:24Z","abstract_excerpt":"Fast Radio Bursts (FRBs) are energetic millisecond radio bursts at cosmological distances, whose underlying engine is not identified. Among a sub-population that emit repeated radio bursts, a handful were associated with a persistent radio source (PRS) whose origin is unknown. Here we report the discovery of a compact flaring radio source (FRS) associated with a newly-active repeating FRB within one month after the first radio burst was detected. Its temporal and spectral characteristics differ from those of the PRSs but are similar to those of engine-powered supernovae and low-luminosity acti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.14247","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2501.14247/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2501.14247","created_at":"2026-07-05T10:04:47.809233+00:00"},{"alias_kind":"arxiv_version","alias_value":"2501.14247v1","created_at":"2026-07-05T10:04:47.809233+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2501.14247","created_at":"2026-07-05T10:04:47.809233+00:00"},{"alias_kind":"pith_short_12","alias_value":"TSUI2TD6XREM","created_at":"2026-07-05T10:04:47.809233+00:00"},{"alias_kind":"pith_short_16","alias_value":"TSUI2TD6XREMGKP3","created_at":"2026-07-05T10:04:47.809233+00:00"},{"alias_kind":"pith_short_8","alias_value":"TSUI2TD6","created_at":"2026-07-05T10:04:47.809233+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.07087","citing_title":"A series of unfortunate events: CHIME/FRB misclassification of a Galactic pulsar as a periodic fast radio burst","ref_index":269,"is_internal_anchor":false},{"citing_arxiv_id":"2604.12791","citing_title":"The spectrum of the persistent radio source associated with FRB 20190417A","ref_index":58,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TSUI2TD6XREMGKP3D55NZH6J5C","json":"https://pith.science/pith/TSUI2TD6XREMGKP3D55NZH6J5C.json","graph_json":"https://pith.science/api/pith-number/TSUI2TD6XREMGKP3D55NZH6J5C/graph.json","events_json":"https://pith.science/api/pith-number/TSUI2TD6XREMGKP3D55NZH6J5C/events.json","paper":"https://pith.science/paper/TSUI2TD6"},"agent_actions":{"view_html":"https://pith.science/pith/TSUI2TD6XREMGKP3D55NZH6J5C","download_json":"https://pith.science/pith/TSUI2TD6XREMGKP3D55NZH6J5C.json","view_paper":"https://pith.science/paper/TSUI2TD6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2501.14247&json=true","fetch_graph":"https://pith.science/api/pith-number/TSUI2TD6XREMGKP3D55NZH6J5C/graph.json","fetch_events":"https://pith.science/api/pith-number/TSUI2TD6XREMGKP3D55NZH6J5C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TSUI2TD6XREMGKP3D55NZH6J5C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TSUI2TD6XREMGKP3D55NZH6J5C/action/storage_attestation","attest_author":"https://pith.science/pith/TSUI2TD6XREMGKP3D55NZH6J5C/action/author_attestation","sign_citation":"https://pith.science/pith/TSUI2TD6XREMGKP3D55NZH6J5C/action/citation_signature","submit_replication":"https://pith.science/pith/TSUI2TD6XREMGKP3D55NZH6J5C/action/replication_record"}},"created_at":"2026-07-05T10:04:47.809233+00:00","updated_at":"2026-07-05T10:04:47.809233+00:00"}