{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:T7XIUJI3XORO73SUKN73B5O6OU","short_pith_number":"pith:T7XIUJI3","schema_version":"1.0","canonical_sha256":"9fee8a251bbba2efee54537fb0f5de750d3c79870aebaf10800ab7e927e597ad","source":{"kind":"arxiv","id":"1407.6479","version":1},"attestation_state":"computed","paper":{"title":"Massive Star Asteroseismology in Action","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Conny Aerts","submitted_at":"2014-07-24T08:17:12Z","abstract_excerpt":"After highlighting the principle and power of asteroseismology for stellar  physics, we briefly emphasize some recent progress in this research for various  types of stars. We give an overview of high-precision high duty-cycle space  photometry of OB-type stars. Further, we update the overview of seismic estimates of stellar parameters of OB dwarfs, with specific emphasis on convective core overshoot. We discuss connections  between pulsational, rotational, and magnetic variability of massive stars and  end with future prospects for asteroseismology of evolved OB stars."},"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":"1407.6479","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-07-24T08:17:12Z","cross_cats_sorted":[],"title_canon_sha256":"e24c4f1b15a5173c47cb4c853510e97e22d50c268e9f2b8382ae34892841ec8a","abstract_canon_sha256":"b9a836823e62b158c1fc6cc03ac0f9df76bd945cd7be66465354419a5908408c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:32.306425Z","signature_b64":"fv5isVoRHZK/UcHxQs5N9tY12nYwIiFo9pbzZmA+I7GaE8Dxi4lOsgWjbf69qK2dLHuwErWM0u6EKEv/7t5LBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9fee8a251bbba2efee54537fb0f5de750d3c79870aebaf10800ab7e927e597ad","last_reissued_at":"2026-05-18T01:42:32.305766Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:32.305766Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Massive Star Asteroseismology in Action","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Conny Aerts","submitted_at":"2014-07-24T08:17:12Z","abstract_excerpt":"After highlighting the principle and power of asteroseismology for stellar  physics, we briefly emphasize some recent progress in this research for various  types of stars. We give an overview of high-precision high duty-cycle space  photometry of OB-type stars. Further, we update the overview of seismic estimates of stellar parameters of OB dwarfs, with specific emphasis on convective core overshoot. We discuss connections  between pulsational, rotational, and magnetic variability of massive stars and  end with future prospects for asteroseismology of evolved OB stars."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.6479","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":"1407.6479","created_at":"2026-05-18T01:42:32.305872+00:00"},{"alias_kind":"arxiv_version","alias_value":"1407.6479v1","created_at":"2026-05-18T01:42:32.305872+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.6479","created_at":"2026-05-18T01:42:32.305872+00:00"},{"alias_kind":"pith_short_12","alias_value":"T7XIUJI3XORO","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_16","alias_value":"T7XIUJI3XORO73SU","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_8","alias_value":"T7XIUJI3","created_at":"2026-05-18T12:28:49.207871+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/T7XIUJI3XORO73SUKN73B5O6OU","json":"https://pith.science/pith/T7XIUJI3XORO73SUKN73B5O6OU.json","graph_json":"https://pith.science/api/pith-number/T7XIUJI3XORO73SUKN73B5O6OU/graph.json","events_json":"https://pith.science/api/pith-number/T7XIUJI3XORO73SUKN73B5O6OU/events.json","paper":"https://pith.science/paper/T7XIUJI3"},"agent_actions":{"view_html":"https://pith.science/pith/T7XIUJI3XORO73SUKN73B5O6OU","download_json":"https://pith.science/pith/T7XIUJI3XORO73SUKN73B5O6OU.json","view_paper":"https://pith.science/paper/T7XIUJI3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1407.6479&json=true","fetch_graph":"https://pith.science/api/pith-number/T7XIUJI3XORO73SUKN73B5O6OU/graph.json","fetch_events":"https://pith.science/api/pith-number/T7XIUJI3XORO73SUKN73B5O6OU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/T7XIUJI3XORO73SUKN73B5O6OU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/T7XIUJI3XORO73SUKN73B5O6OU/action/storage_attestation","attest_author":"https://pith.science/pith/T7XIUJI3XORO73SUKN73B5O6OU/action/author_attestation","sign_citation":"https://pith.science/pith/T7XIUJI3XORO73SUKN73B5O6OU/action/citation_signature","submit_replication":"https://pith.science/pith/T7XIUJI3XORO73SUKN73B5O6OU/action/replication_record"}},"created_at":"2026-05-18T01:42:32.305872+00:00","updated_at":"2026-05-18T01:42:32.305872+00:00"}