{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:6J3SNWQ3OPMXY6MIIROQC7BWBT","short_pith_number":"pith:6J3SNWQ3","schema_version":"1.0","canonical_sha256":"f27726da1b73d97c7988445d017c360cc6586a3efe66f35df24ba748a015a8a8","source":{"kind":"arxiv","id":"1701.05370","version":1},"attestation_state":"computed","paper":{"title":"How unique is Plaskett's star? A search for organized magnetic fields in short period, interacting or post-interaction massive binary systems","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Neiner (ObsPM), CNRS), E. Alecian (IPAG, G.A. Wade (RMC), G. Rauw (ULg), J. Grunhut (ESO, S. Bagnulo (Armagh Obs), the BinaMIcS collaboration, Toronto Univ), Y. Naze (ULg)","submitted_at":"2017-01-19T11:05:23Z","abstract_excerpt":"Amongst O-type stars with detected magnetic fields, the fast rotator in the close binary called Plaskett's star shows a variety of unusual properties. Since strong binary interactions are believed to have occurred in this system, one may wonder about their potential role in generating magnetic fields. Stokes V spectra collected with the low-resolution FORS2 and high-resolution ESPaDOnS and Narval spectropolarimeters were therefore used to search for magnetic fields in 15 interacting or post-interaction massive binaries. No magnetic field was detected in any of them, with 0G always being within"},"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":"1701.05370","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-01-19T11:05:23Z","cross_cats_sorted":[],"title_canon_sha256":"839033a33240bceaac99cffdcedc0a349803e41a5ef4a8e3a8c6dfdf5d9620cd","abstract_canon_sha256":"f83baf1576f92e099b2015f3f5d9eec15e30d54efb4914bcaef2773d7351cba3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:57:45.660000Z","signature_b64":"tmxmD4r5qHkWVjeLdjw+FNr3iaN2DtFG0SBKBQC6VuTpAb6bbb5F40CSOC06mNls7ttRUMSIz/DosutSyXrgBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f27726da1b73d97c7988445d017c360cc6586a3efe66f35df24ba748a015a8a8","last_reissued_at":"2026-07-05T01:57:45.659549Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:57:45.659549Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"How unique is Plaskett's star? A search for organized magnetic fields in short period, interacting or post-interaction massive binary systems","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Neiner (ObsPM), CNRS), E. Alecian (IPAG, G.A. Wade (RMC), G. Rauw (ULg), J. Grunhut (ESO, S. Bagnulo (Armagh Obs), the BinaMIcS collaboration, Toronto Univ), Y. Naze (ULg)","submitted_at":"2017-01-19T11:05:23Z","abstract_excerpt":"Amongst O-type stars with detected magnetic fields, the fast rotator in the close binary called Plaskett's star shows a variety of unusual properties. Since strong binary interactions are believed to have occurred in this system, one may wonder about their potential role in generating magnetic fields. Stokes V spectra collected with the low-resolution FORS2 and high-resolution ESPaDOnS and Narval spectropolarimeters were therefore used to search for magnetic fields in 15 interacting or post-interaction massive binaries. No magnetic field was detected in any of them, with 0G always being within"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.05370","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/1701.05370/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":"1701.05370","created_at":"2026-07-05T01:57:45.659606+00:00"},{"alias_kind":"arxiv_version","alias_value":"1701.05370v1","created_at":"2026-07-05T01:57:45.659606+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.05370","created_at":"2026-07-05T01:57:45.659606+00:00"},{"alias_kind":"pith_short_12","alias_value":"6J3SNWQ3OPMX","created_at":"2026-07-05T01:57:45.659606+00:00"},{"alias_kind":"pith_short_16","alias_value":"6J3SNWQ3OPMXY6MI","created_at":"2026-07-05T01:57:45.659606+00:00"},{"alias_kind":"pith_short_8","alias_value":"6J3SNWQ3","created_at":"2026-07-05T01:57:45.659606+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/6J3SNWQ3OPMXY6MIIROQC7BWBT","json":"https://pith.science/pith/6J3SNWQ3OPMXY6MIIROQC7BWBT.json","graph_json":"https://pith.science/api/pith-number/6J3SNWQ3OPMXY6MIIROQC7BWBT/graph.json","events_json":"https://pith.science/api/pith-number/6J3SNWQ3OPMXY6MIIROQC7BWBT/events.json","paper":"https://pith.science/paper/6J3SNWQ3"},"agent_actions":{"view_html":"https://pith.science/pith/6J3SNWQ3OPMXY6MIIROQC7BWBT","download_json":"https://pith.science/pith/6J3SNWQ3OPMXY6MIIROQC7BWBT.json","view_paper":"https://pith.science/paper/6J3SNWQ3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1701.05370&json=true","fetch_graph":"https://pith.science/api/pith-number/6J3SNWQ3OPMXY6MIIROQC7BWBT/graph.json","fetch_events":"https://pith.science/api/pith-number/6J3SNWQ3OPMXY6MIIROQC7BWBT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6J3SNWQ3OPMXY6MIIROQC7BWBT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6J3SNWQ3OPMXY6MIIROQC7BWBT/action/storage_attestation","attest_author":"https://pith.science/pith/6J3SNWQ3OPMXY6MIIROQC7BWBT/action/author_attestation","sign_citation":"https://pith.science/pith/6J3SNWQ3OPMXY6MIIROQC7BWBT/action/citation_signature","submit_replication":"https://pith.science/pith/6J3SNWQ3OPMXY6MIIROQC7BWBT/action/replication_record"}},"created_at":"2026-07-05T01:57:45.659606+00:00","updated_at":"2026-07-05T01:57:45.659606+00:00"}