{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:6GNI3L6BSJMNUBJLXTPPOA66FX","short_pith_number":"pith:6GNI3L6B","schema_version":"1.0","canonical_sha256":"f19a8dafc19258da052bbcdef703de2ddef675913b1f17e7bd27ab9ff2e773e0","source":{"kind":"arxiv","id":"1310.3965","version":1},"attestation_state":"computed","paper":{"title":"The magnetic characteristics of Galactic OB stars from the MiMeS survey of magnetism in massive stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. David-Uraz, C. Folsom, C. Neiner, D.A. Bohlender, E. Alecian, G.A. Wade, H.F. Henrichs, J. Grunhut, M. Auriere, O. Kochukhov, S. Mathis, S. Owocki, the MiMeS Collaboration, V. Petit","submitted_at":"2013-10-15T08:51:38Z","abstract_excerpt":"The Magnetism in Massive Stars (MiMeS) project represents the largest systematic survey of stellar magnetism ever undertaken. Based on a sample of over 550 Galactic B and O-type stars, the MiMeS project has derived the basic characteristics of magnetism in hot, massive stars. Herein we report preliminary results."},"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":"1310.3965","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-10-15T08:51:38Z","cross_cats_sorted":[],"title_canon_sha256":"e2c2d7f4ac910a528c0b94d04d5ddd59b902253636c4eb60a511976079bd1088","abstract_canon_sha256":"874353f4f30f9bec6bc009da12a5ae0343f38f47ab383c594036173921d38072"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:05.336929Z","signature_b64":"C0tCxnLeErPCOIy2j88JjEjXhL6rGWPindJ0FcxBhXwsoVDelnGLYWnqiy9Qhr9AtjjLPmphRC1UDTgB4k+6AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f19a8dafc19258da052bbcdef703de2ddef675913b1f17e7bd27ab9ff2e773e0","last_reissued_at":"2026-05-18T01:47:05.336311Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:05.336311Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The magnetic characteristics of Galactic OB stars from the MiMeS survey of magnetism in massive stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. David-Uraz, C. Folsom, C. Neiner, D.A. Bohlender, E. Alecian, G.A. Wade, H.F. Henrichs, J. Grunhut, M. Auriere, O. Kochukhov, S. Mathis, S. Owocki, the MiMeS Collaboration, V. Petit","submitted_at":"2013-10-15T08:51:38Z","abstract_excerpt":"The Magnetism in Massive Stars (MiMeS) project represents the largest systematic survey of stellar magnetism ever undertaken. Based on a sample of over 550 Galactic B and O-type stars, the MiMeS project has derived the basic characteristics of magnetism in hot, massive stars. Herein we report preliminary results."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.3965","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":"1310.3965","created_at":"2026-05-18T01:47:05.336421+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.3965v1","created_at":"2026-05-18T01:47:05.336421+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.3965","created_at":"2026-05-18T01:47:05.336421+00:00"},{"alias_kind":"pith_short_12","alias_value":"6GNI3L6BSJMN","created_at":"2026-05-18T12:27:36.564083+00:00"},{"alias_kind":"pith_short_16","alias_value":"6GNI3L6BSJMNUBJL","created_at":"2026-05-18T12:27:36.564083+00:00"},{"alias_kind":"pith_short_8","alias_value":"6GNI3L6B","created_at":"2026-05-18T12:27:36.564083+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/6GNI3L6BSJMNUBJLXTPPOA66FX","json":"https://pith.science/pith/6GNI3L6BSJMNUBJLXTPPOA66FX.json","graph_json":"https://pith.science/api/pith-number/6GNI3L6BSJMNUBJLXTPPOA66FX/graph.json","events_json":"https://pith.science/api/pith-number/6GNI3L6BSJMNUBJLXTPPOA66FX/events.json","paper":"https://pith.science/paper/6GNI3L6B"},"agent_actions":{"view_html":"https://pith.science/pith/6GNI3L6BSJMNUBJLXTPPOA66FX","download_json":"https://pith.science/pith/6GNI3L6BSJMNUBJLXTPPOA66FX.json","view_paper":"https://pith.science/paper/6GNI3L6B","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.3965&json=true","fetch_graph":"https://pith.science/api/pith-number/6GNI3L6BSJMNUBJLXTPPOA66FX/graph.json","fetch_events":"https://pith.science/api/pith-number/6GNI3L6BSJMNUBJLXTPPOA66FX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6GNI3L6BSJMNUBJLXTPPOA66FX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6GNI3L6BSJMNUBJLXTPPOA66FX/action/storage_attestation","attest_author":"https://pith.science/pith/6GNI3L6BSJMNUBJLXTPPOA66FX/action/author_attestation","sign_citation":"https://pith.science/pith/6GNI3L6BSJMNUBJLXTPPOA66FX/action/citation_signature","submit_replication":"https://pith.science/pith/6GNI3L6BSJMNUBJLXTPPOA66FX/action/replication_record"}},"created_at":"2026-05-18T01:47:05.336421+00:00","updated_at":"2026-05-18T01:47:05.336421+00:00"}