{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:ZEW6HWWKT2VZRVO3QIWLSSOGD5","short_pith_number":"pith:ZEW6HWWK","schema_version":"1.0","canonical_sha256":"c92de3daca9eab98d5db822cb949c61f7a769e2be2fddff86b715ae1c934f7be","source":{"kind":"arxiv","id":"1207.0615","version":1},"attestation_state":"computed","paper":{"title":"Solar-like oscillations in red giants observed with \\textit{Kepler}: influence of increased timespan on global oscillation parameters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"B. D. Clarke, B. Mosser, D. Stello, J. De Ridder, J. R. Hall, K. A. Ibrahim, R. A. Garcia, S. Hekker, T. Kallinger, W. J. Chaplin, Y. Elsworth","submitted_at":"2012-07-03T09:18:55Z","abstract_excerpt":"The length of the asteroseismic timeseries obtained from the Kepler satellite analysed here span 19 months. Kepler provides the longest continuous timeseries currently available, which calls for a study of the influence of the increased timespan on the accuracy and precision of the obtained results. We find that in general a minimum of the order of 400 day long timeseries are necessary to obtain reliable results for the global oscillation parameters in more than 95% of the stars, but this does depend on <dnu>. In a statistical sense the quoted uncertainties seem to provide a reasonable indicat"},"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":"1207.0615","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-07-03T09:18:55Z","cross_cats_sorted":[],"title_canon_sha256":"461b001e87a41b2f8f1f9bfe4d5ed926b50ed7c445b70d917a975ae7bf7544f4","abstract_canon_sha256":"4b60d459cb43297cc8946a9d8d2382b7dc76d018d5f2ff92f9f96661d6266e68"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:56:35.394264Z","signature_b64":"5MfuMx2Ytm6LJ46aln5ucDlJ8spNlm8cy4T8DYLocB3B9kgLEaKKZ9KD0HJf1eaHxxgFRMLaxictbGjmoW5CAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c92de3daca9eab98d5db822cb949c61f7a769e2be2fddff86b715ae1c934f7be","last_reissued_at":"2026-05-18T01:56:35.393788Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:56:35.393788Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Solar-like oscillations in red giants observed with \\textit{Kepler}: influence of increased timespan on global oscillation parameters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"B. D. Clarke, B. Mosser, D. Stello, J. De Ridder, J. R. Hall, K. A. Ibrahim, R. A. Garcia, S. Hekker, T. Kallinger, W. J. Chaplin, Y. Elsworth","submitted_at":"2012-07-03T09:18:55Z","abstract_excerpt":"The length of the asteroseismic timeseries obtained from the Kepler satellite analysed here span 19 months. Kepler provides the longest continuous timeseries currently available, which calls for a study of the influence of the increased timespan on the accuracy and precision of the obtained results. We find that in general a minimum of the order of 400 day long timeseries are necessary to obtain reliable results for the global oscillation parameters in more than 95% of the stars, but this does depend on <dnu>. In a statistical sense the quoted uncertainties seem to provide a reasonable indicat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1207.0615","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":"1207.0615","created_at":"2026-05-18T01:56:35.393867+00:00"},{"alias_kind":"arxiv_version","alias_value":"1207.0615v1","created_at":"2026-05-18T01:56:35.393867+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1207.0615","created_at":"2026-05-18T01:56:35.393867+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZEW6HWWKT2VZ","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZEW6HWWKT2VZRVO3","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZEW6HWWK","created_at":"2026-05-18T12:27:30.460161+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/ZEW6HWWKT2VZRVO3QIWLSSOGD5","json":"https://pith.science/pith/ZEW6HWWKT2VZRVO3QIWLSSOGD5.json","graph_json":"https://pith.science/api/pith-number/ZEW6HWWKT2VZRVO3QIWLSSOGD5/graph.json","events_json":"https://pith.science/api/pith-number/ZEW6HWWKT2VZRVO3QIWLSSOGD5/events.json","paper":"https://pith.science/paper/ZEW6HWWK"},"agent_actions":{"view_html":"https://pith.science/pith/ZEW6HWWKT2VZRVO3QIWLSSOGD5","download_json":"https://pith.science/pith/ZEW6HWWKT2VZRVO3QIWLSSOGD5.json","view_paper":"https://pith.science/paper/ZEW6HWWK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1207.0615&json=true","fetch_graph":"https://pith.science/api/pith-number/ZEW6HWWKT2VZRVO3QIWLSSOGD5/graph.json","fetch_events":"https://pith.science/api/pith-number/ZEW6HWWKT2VZRVO3QIWLSSOGD5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZEW6HWWKT2VZRVO3QIWLSSOGD5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZEW6HWWKT2VZRVO3QIWLSSOGD5/action/storage_attestation","attest_author":"https://pith.science/pith/ZEW6HWWKT2VZRVO3QIWLSSOGD5/action/author_attestation","sign_citation":"https://pith.science/pith/ZEW6HWWKT2VZRVO3QIWLSSOGD5/action/citation_signature","submit_replication":"https://pith.science/pith/ZEW6HWWKT2VZRVO3QIWLSSOGD5/action/replication_record"}},"created_at":"2026-05-18T01:56:35.393867+00:00","updated_at":"2026-05-18T01:56:35.393867+00:00"}