{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:HSLXB5UJJFJW5B2VMQQLYQ34TM","short_pith_number":"pith:HSLXB5UJ","schema_version":"1.0","canonical_sha256":"3c9770f68949536e87556420bc437c9b1b2d4925f1248dc94fb1429dd8dae6eb","source":{"kind":"arxiv","id":"1206.3841","version":1},"attestation_state":"computed","paper":{"title":"A pulsation zoo in the hot subdwarf B star KIC 10139564 observed by Kepler","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. S. Baran, B.D. Clarke, D. Stello, E. Pakstiene, H. Hu, J.H. Telting, J. van Cleve, M. D. Reed, P. Degroote, R.H. Ostensen, R. Silvotti, S. Bloemen, S.D. Kawaler, S.E. Thompson, S. J. O'Toole, V. Van Grootel","submitted_at":"2012-06-18T07:09:20Z","abstract_excerpt":"We present our analyses of 15 months of Kepler data on KIC 10139564. We detected 57 periodicities with a variety of properties not previously observed all together in one pulsating subdwarf B star. Ten of the periodicities were found in the low-frequency region, and we associate them with nonradial g-modes. The other periodicities were found in the high-frequency region, which are likely p-modes. We discovered that most of the periodicities are components of multiplets with a common spacing. Assuming that multiplets are caused by rotation, we derive a rotation period of 25.6(1.8) days. The mul"},"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":"1206.3841","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-06-18T07:09:20Z","cross_cats_sorted":[],"title_canon_sha256":"54015c121614eef88540388133bea14ecc1eaa63c7f527fde867d6654c88624e","abstract_canon_sha256":"59b3ba22e49c188bbe127698c0fae60f41af1d14a576acc18e603dd95a0e7f7d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:56:51.906914Z","signature_b64":"01O4ceiALiB7/qVxNFFQekn1D84EcKhrftjlNlnOqbj4lqQvsLrqFtR6TQ5EqVjDogZ0OpwKfA9WqxK2XaZoDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3c9770f68949536e87556420bc437c9b1b2d4925f1248dc94fb1429dd8dae6eb","last_reissued_at":"2026-05-18T01:56:51.906220Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:56:51.906220Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A pulsation zoo in the hot subdwarf B star KIC 10139564 observed by Kepler","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. S. Baran, B.D. Clarke, D. Stello, E. Pakstiene, H. Hu, J.H. Telting, J. van Cleve, M. D. Reed, P. Degroote, R.H. Ostensen, R. Silvotti, S. Bloemen, S.D. Kawaler, S.E. Thompson, S. J. O'Toole, V. Van Grootel","submitted_at":"2012-06-18T07:09:20Z","abstract_excerpt":"We present our analyses of 15 months of Kepler data on KIC 10139564. We detected 57 periodicities with a variety of properties not previously observed all together in one pulsating subdwarf B star. Ten of the periodicities were found in the low-frequency region, and we associate them with nonradial g-modes. The other periodicities were found in the high-frequency region, which are likely p-modes. We discovered that most of the periodicities are components of multiplets with a common spacing. Assuming that multiplets are caused by rotation, we derive a rotation period of 25.6(1.8) days. The mul"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1206.3841","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":"1206.3841","created_at":"2026-05-18T01:56:51.906361+00:00"},{"alias_kind":"arxiv_version","alias_value":"1206.3841v1","created_at":"2026-05-18T01:56:51.906361+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1206.3841","created_at":"2026-05-18T01:56:51.906361+00:00"},{"alias_kind":"pith_short_12","alias_value":"HSLXB5UJJFJW","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_16","alias_value":"HSLXB5UJJFJW5B2V","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_8","alias_value":"HSLXB5UJ","created_at":"2026-05-18T12:27:09.501522+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/HSLXB5UJJFJW5B2VMQQLYQ34TM","json":"https://pith.science/pith/HSLXB5UJJFJW5B2VMQQLYQ34TM.json","graph_json":"https://pith.science/api/pith-number/HSLXB5UJJFJW5B2VMQQLYQ34TM/graph.json","events_json":"https://pith.science/api/pith-number/HSLXB5UJJFJW5B2VMQQLYQ34TM/events.json","paper":"https://pith.science/paper/HSLXB5UJ"},"agent_actions":{"view_html":"https://pith.science/pith/HSLXB5UJJFJW5B2VMQQLYQ34TM","download_json":"https://pith.science/pith/HSLXB5UJJFJW5B2VMQQLYQ34TM.json","view_paper":"https://pith.science/paper/HSLXB5UJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1206.3841&json=true","fetch_graph":"https://pith.science/api/pith-number/HSLXB5UJJFJW5B2VMQQLYQ34TM/graph.json","fetch_events":"https://pith.science/api/pith-number/HSLXB5UJJFJW5B2VMQQLYQ34TM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HSLXB5UJJFJW5B2VMQQLYQ34TM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HSLXB5UJJFJW5B2VMQQLYQ34TM/action/storage_attestation","attest_author":"https://pith.science/pith/HSLXB5UJJFJW5B2VMQQLYQ34TM/action/author_attestation","sign_citation":"https://pith.science/pith/HSLXB5UJJFJW5B2VMQQLYQ34TM/action/citation_signature","submit_replication":"https://pith.science/pith/HSLXB5UJJFJW5B2VMQQLYQ34TM/action/replication_record"}},"created_at":"2026-05-18T01:56:51.906361+00:00","updated_at":"2026-05-18T01:56:51.906361+00:00"}