{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:F62UOABM7OFD24YSFHMTGAUDLN","short_pith_number":"pith:F62UOABM","schema_version":"1.0","canonical_sha256":"2fb547002cfb8a3d731229d93302835b52c23f17cab37f57a0a619e2a1ee544b","source":{"kind":"arxiv","id":"astro-ph/0302127","version":1},"attestation_state":"computed","paper":{"title":"Asteroseismological studies of three Beta Cephei stars: IL Vel, V433 Car and KZ Mus","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"F. F. Vuthela, F. Rodler, G. Handler, L. A. Balona, R. R. Shobbrook, T. Tshenye","submitted_at":"2003-02-06T19:19:27Z","abstract_excerpt":"We have acquired between 127 and 150 h of time-resolved multicolour photometry for each of the three Beta Cephei stars IL Vel, V433 Car and KZ Mus over a time span of four months from two observatories. All three objects are multiperiodic with at least three modes of pulsation. Mode identification from the relative colour amplitudes is performed. We obtain unambiguous results for the two highest-amplitude modes of IL Vel (both are l=1) and the three strongest modes of KZ Mus (l=2,0 and 1), but none for V433 Car. Spectroscopy shows the latter star to be a fast rotator (v sin i = 240 km/s), wher"},"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":"astro-ph/0302127","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2003-02-06T19:19:27Z","cross_cats_sorted":[],"title_canon_sha256":"b89b68a5ca43cee94ecbfdf078a9ca14644e6ffbc8f76ca7cbddd18ea8cdd3b0","abstract_canon_sha256":"d58335706b2bd5779f508059dce94018f6ed5bd7d4bf27f431a8d6264992a86b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:18:04.389693Z","signature_b64":"9M0fBhonmP7eMYnCMzvpR5VZOqFPVBKD0PNvm7uh72/o9Tsqk0XzMNZuSAgSF406HFpsDA6zECGvtlfHR1TXBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2fb547002cfb8a3d731229d93302835b52c23f17cab37f57a0a619e2a1ee544b","last_reissued_at":"2026-07-04T15:18:04.389189Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:18:04.389189Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Asteroseismological studies of three Beta Cephei stars: IL Vel, V433 Car and KZ Mus","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"F. F. Vuthela, F. Rodler, G. Handler, L. A. Balona, R. R. Shobbrook, T. Tshenye","submitted_at":"2003-02-06T19:19:27Z","abstract_excerpt":"We have acquired between 127 and 150 h of time-resolved multicolour photometry for each of the three Beta Cephei stars IL Vel, V433 Car and KZ Mus over a time span of four months from two observatories. All three objects are multiperiodic with at least three modes of pulsation. Mode identification from the relative colour amplitudes is performed. We obtain unambiguous results for the two highest-amplitude modes of IL Vel (both are l=1) and the three strongest modes of KZ Mus (l=2,0 and 1), but none for V433 Car. Spectroscopy shows the latter star to be a fast rotator (v sin i = 240 km/s), wher"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0302127","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/astro-ph/0302127/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":"astro-ph/0302127","created_at":"2026-07-04T15:18:04.389246+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0302127v1","created_at":"2026-07-04T15:18:04.389246+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0302127","created_at":"2026-07-04T15:18:04.389246+00:00"},{"alias_kind":"pith_short_12","alias_value":"F62UOABM7OFD","created_at":"2026-07-04T15:18:04.389246+00:00"},{"alias_kind":"pith_short_16","alias_value":"F62UOABM7OFD24YS","created_at":"2026-07-04T15:18:04.389246+00:00"},{"alias_kind":"pith_short_8","alias_value":"F62UOABM","created_at":"2026-07-04T15:18:04.389246+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/F62UOABM7OFD24YSFHMTGAUDLN","json":"https://pith.science/pith/F62UOABM7OFD24YSFHMTGAUDLN.json","graph_json":"https://pith.science/api/pith-number/F62UOABM7OFD24YSFHMTGAUDLN/graph.json","events_json":"https://pith.science/api/pith-number/F62UOABM7OFD24YSFHMTGAUDLN/events.json","paper":"https://pith.science/paper/F62UOABM"},"agent_actions":{"view_html":"https://pith.science/pith/F62UOABM7OFD24YSFHMTGAUDLN","download_json":"https://pith.science/pith/F62UOABM7OFD24YSFHMTGAUDLN.json","view_paper":"https://pith.science/paper/F62UOABM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0302127&json=true","fetch_graph":"https://pith.science/api/pith-number/F62UOABM7OFD24YSFHMTGAUDLN/graph.json","fetch_events":"https://pith.science/api/pith-number/F62UOABM7OFD24YSFHMTGAUDLN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/F62UOABM7OFD24YSFHMTGAUDLN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/F62UOABM7OFD24YSFHMTGAUDLN/action/storage_attestation","attest_author":"https://pith.science/pith/F62UOABM7OFD24YSFHMTGAUDLN/action/author_attestation","sign_citation":"https://pith.science/pith/F62UOABM7OFD24YSFHMTGAUDLN/action/citation_signature","submit_replication":"https://pith.science/pith/F62UOABM7OFD24YSFHMTGAUDLN/action/replication_record"}},"created_at":"2026-07-04T15:18:04.389246+00:00","updated_at":"2026-07-04T15:18:04.389246+00:00"}