{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:ACQYXHCXWVACEINHUMRED56VIJ","short_pith_number":"pith:ACQYXHCX","schema_version":"1.0","canonical_sha256":"00a18b9c57b5402221a7a32241f7d54252ca24c2eb8e628214a05b398915b79d","source":{"kind":"arxiv","id":"1009.3246","version":1},"attestation_state":"computed","paper":{"title":"Discovery of the most rapidly-rotating, non-degenerate, magnetic massive star by the MiMeS collaboration","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"G.A. Wade, J.H. Grunhut, R.H.D. Townsend, the MiMeS Collaboration, T. Rivinius, W.L.F. Marcolino","submitted_at":"2010-09-16T19:00:38Z","abstract_excerpt":"We discuss the recent detection of a strong, organized magnetic field in the bright, broad-line B2V star, HD 142184, using the ESPaDOnS spectropolarimeter on the CFHT as part of the Magnetism in Massive Stars (MiMeS) survey. We find a rotational period of 0.50833 days, making it the fastest-rotating, non-degenerate magnetic star ever detected. Like the previous rapid-rotation record holder HR 7355 (also discovered by MiMeS: Oksala et al. 2010, Rivinius et al. 2010), this star shows emission line variability that is diagnostic of a structured magnetosphere."},"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":"1009.3246","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-09-16T19:00:38Z","cross_cats_sorted":[],"title_canon_sha256":"dae40368650230f30261f6840a4f1ab011aa4feb76b194b8e413d6a0e6556fcc","abstract_canon_sha256":"7ddaec0b9677ed18bc6f55ea02b937587272ef09f13d0cd30247b40a408a09e7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:27.304962Z","signature_b64":"pdu3qOpyVno7J6HYsXgTUexavN7J2b8+aVOzR2hJZzipyma5pVA5x9TAUN5JaB9gLzGckQ6YkLgB1PU9MbTwCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"00a18b9c57b5402221a7a32241f7d54252ca24c2eb8e628214a05b398915b79d","last_reissued_at":"2026-05-18T02:05:27.304224Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:27.304224Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Discovery of the most rapidly-rotating, non-degenerate, magnetic massive star by the MiMeS collaboration","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"G.A. Wade, J.H. Grunhut, R.H.D. Townsend, the MiMeS Collaboration, T. Rivinius, W.L.F. Marcolino","submitted_at":"2010-09-16T19:00:38Z","abstract_excerpt":"We discuss the recent detection of a strong, organized magnetic field in the bright, broad-line B2V star, HD 142184, using the ESPaDOnS spectropolarimeter on the CFHT as part of the Magnetism in Massive Stars (MiMeS) survey. We find a rotational period of 0.50833 days, making it the fastest-rotating, non-degenerate magnetic star ever detected. Like the previous rapid-rotation record holder HR 7355 (also discovered by MiMeS: Oksala et al. 2010, Rivinius et al. 2010), this star shows emission line variability that is diagnostic of a structured magnetosphere."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.3246","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":""},"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":"1009.3246","created_at":"2026-05-18T02:05:27.304332+00:00"},{"alias_kind":"arxiv_version","alias_value":"1009.3246v1","created_at":"2026-05-18T02:05:27.304332+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.3246","created_at":"2026-05-18T02:05:27.304332+00:00"},{"alias_kind":"pith_short_12","alias_value":"ACQYXHCXWVAC","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_16","alias_value":"ACQYXHCXWVACEINH","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_8","alias_value":"ACQYXHCX","created_at":"2026-05-18T12:26:05.355336+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ACQYXHCXWVACEINHUMRED56VIJ","json":"https://pith.science/pith/ACQYXHCXWVACEINHUMRED56VIJ.json","graph_json":"https://pith.science/api/pith-number/ACQYXHCXWVACEINHUMRED56VIJ/graph.json","events_json":"https://pith.science/api/pith-number/ACQYXHCXWVACEINHUMRED56VIJ/events.json","paper":"https://pith.science/paper/ACQYXHCX"},"agent_actions":{"view_html":"https://pith.science/pith/ACQYXHCXWVACEINHUMRED56VIJ","download_json":"https://pith.science/pith/ACQYXHCXWVACEINHUMRED56VIJ.json","view_paper":"https://pith.science/paper/ACQYXHCX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1009.3246&json=true","fetch_graph":"https://pith.science/api/pith-number/ACQYXHCXWVACEINHUMRED56VIJ/graph.json","fetch_events":"https://pith.science/api/pith-number/ACQYXHCXWVACEINHUMRED56VIJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ACQYXHCXWVACEINHUMRED56VIJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ACQYXHCXWVACEINHUMRED56VIJ/action/storage_attestation","attest_author":"https://pith.science/pith/ACQYXHCXWVACEINHUMRED56VIJ/action/author_attestation","sign_citation":"https://pith.science/pith/ACQYXHCXWVACEINHUMRED56VIJ/action/citation_signature","submit_replication":"https://pith.science/pith/ACQYXHCXWVACEINHUMRED56VIJ/action/replication_record"}},"created_at":"2026-05-18T02:05:27.304332+00:00","updated_at":"2026-05-18T02:05:27.304332+00:00"}