{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:V7ZHTORCI55VRGYWTRA5O75SSN","short_pith_number":"pith:V7ZHTORC","schema_version":"1.0","canonical_sha256":"aff279ba22477b589b169c41d77fb293542f8c746f18767c7804c618a55352d8","source":{"kind":"arxiv","id":"1204.3152","version":1},"attestation_state":"computed","paper":{"title":"Complex asteroseismology of the Slowly Pulsating B-type star HD74560","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Jadwiga Daszy\\'nska-Daszkiewicz, Przemys{\\l}aw Walczak, Wojciech Szewczuk","submitted_at":"2012-04-14T08:13:55Z","abstract_excerpt":"We present the results of complex seismic modelling of the Slowly Pulsating B-type star HD74560. The star pulsates in five frequencies detected in photometric observations. For all these frequencies, we identify the mode degree, $\\ell$. For two of them, found also in spectroscopic data, we are able to derived the empirical values of the complex nonadiabatic parameter $f$. We test effects of chemical composition and opacity data. Our results show that the properties of seismic models of SPB stars differ significantly from those of the more massive $\\beta$ Cephei 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":"1204.3152","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-04-14T08:13:55Z","cross_cats_sorted":[],"title_canon_sha256":"7484bf06134c1105560737e32552d9ee3051e1bf95760e4a00ea043e0aee5abe","abstract_canon_sha256":"672d4764e52b44b2eee4f7c2ad4fadee33d46d7a2ef1d8cfa20ff443ff8b6f5f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:52.508134Z","signature_b64":"Y7uop6rb8I5PYCznDPmTY1YqtcyOL3pi2XEwNX2LRxeJerskogel9CgEqpk7wNgXzYTlK9p88VAJGgJ2HSmQDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"aff279ba22477b589b169c41d77fb293542f8c746f18767c7804c618a55352d8","last_reissued_at":"2026-05-18T01:57:52.507763Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:52.507763Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Complex asteroseismology of the Slowly Pulsating B-type star HD74560","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Jadwiga Daszy\\'nska-Daszkiewicz, Przemys{\\l}aw Walczak, Wojciech Szewczuk","submitted_at":"2012-04-14T08:13:55Z","abstract_excerpt":"We present the results of complex seismic modelling of the Slowly Pulsating B-type star HD74560. The star pulsates in five frequencies detected in photometric observations. For all these frequencies, we identify the mode degree, $\\ell$. For two of them, found also in spectroscopic data, we are able to derived the empirical values of the complex nonadiabatic parameter $f$. We test effects of chemical composition and opacity data. Our results show that the properties of seismic models of SPB stars differ significantly from those of the more massive $\\beta$ Cephei stars."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1204.3152","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":"1204.3152","created_at":"2026-05-18T01:57:52.507815+00:00"},{"alias_kind":"arxiv_version","alias_value":"1204.3152v1","created_at":"2026-05-18T01:57:52.507815+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1204.3152","created_at":"2026-05-18T01:57:52.507815+00:00"},{"alias_kind":"pith_short_12","alias_value":"V7ZHTORCI55V","created_at":"2026-05-18T12:27:25.539911+00:00"},{"alias_kind":"pith_short_16","alias_value":"V7ZHTORCI55VRGYW","created_at":"2026-05-18T12:27:25.539911+00:00"},{"alias_kind":"pith_short_8","alias_value":"V7ZHTORC","created_at":"2026-05-18T12:27:25.539911+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/V7ZHTORCI55VRGYWTRA5O75SSN","json":"https://pith.science/pith/V7ZHTORCI55VRGYWTRA5O75SSN.json","graph_json":"https://pith.science/api/pith-number/V7ZHTORCI55VRGYWTRA5O75SSN/graph.json","events_json":"https://pith.science/api/pith-number/V7ZHTORCI55VRGYWTRA5O75SSN/events.json","paper":"https://pith.science/paper/V7ZHTORC"},"agent_actions":{"view_html":"https://pith.science/pith/V7ZHTORCI55VRGYWTRA5O75SSN","download_json":"https://pith.science/pith/V7ZHTORCI55VRGYWTRA5O75SSN.json","view_paper":"https://pith.science/paper/V7ZHTORC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1204.3152&json=true","fetch_graph":"https://pith.science/api/pith-number/V7ZHTORCI55VRGYWTRA5O75SSN/graph.json","fetch_events":"https://pith.science/api/pith-number/V7ZHTORCI55VRGYWTRA5O75SSN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/V7ZHTORCI55VRGYWTRA5O75SSN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/V7ZHTORCI55VRGYWTRA5O75SSN/action/storage_attestation","attest_author":"https://pith.science/pith/V7ZHTORCI55VRGYWTRA5O75SSN/action/author_attestation","sign_citation":"https://pith.science/pith/V7ZHTORCI55VRGYWTRA5O75SSN/action/citation_signature","submit_replication":"https://pith.science/pith/V7ZHTORCI55VRGYWTRA5O75SSN/action/replication_record"}},"created_at":"2026-05-18T01:57:52.507815+00:00","updated_at":"2026-05-18T01:57:52.507815+00:00"}