{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:CFBWBFZQCGDCARWNM2272BTJVH","short_pith_number":"pith:CFBWBFZQ","schema_version":"1.0","canonical_sha256":"114360973011862046cd66b5fd0669a9cee5a6a5aae4aaff23f4cae69db92078","source":{"kind":"arxiv","id":"1508.00955","version":4},"attestation_state":"computed","paper":{"title":"A Large Convective-Core Overshoot in \\textit{Kepler} Target KIC 11081729","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Wuming Yang","submitted_at":"2015-08-05T02:11:30Z","abstract_excerpt":"The frequency ratios $r_{01}$ and $r_{10}$ of KIC 11081729 decrease firstly and then increase with the increase in frequency. For different spectroscopic constraints, all models with overshooting parameter $\\delta_{\\mathrm{ov}}$ less than 1.7 can not reproduce the distributions of the ratios. However, the distributions of the ratios can be directly reproduced by models with $\\delta_{\\mathrm{ov}}$ in the range of about $1.7-1.8$. The estimations of mass and age of the star can be affected by spectroscopic results, but the determination of the $\\delta_{\\mathrm{ov}}$ is not dependent on the spect"},"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":"1508.00955","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-08-05T02:11:30Z","cross_cats_sorted":[],"title_canon_sha256":"549dac5dcbcd609a1d7c1e95ca7f20778f2baa0d0fb4b30a48059fe472c8246c","abstract_canon_sha256":"dec81b4b88e88554ca4dfed2825b9ae6931cfd54b10c228219f8051660c9a5ee"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:17:08.050122Z","signature_b64":"R+T1PjWL0wSNoyKLgrXi1lP08uahZYl2ONWEO8n3ztZ3D70t/sYZ9Xmsh4dQ9aBBIDWCEY1Lgqn5qSXZVRgUBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"114360973011862046cd66b5fd0669a9cee5a6a5aae4aaff23f4cae69db92078","last_reissued_at":"2026-05-18T01:17:08.049406Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:17:08.049406Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Large Convective-Core Overshoot in \\textit{Kepler} Target KIC 11081729","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Wuming Yang","submitted_at":"2015-08-05T02:11:30Z","abstract_excerpt":"The frequency ratios $r_{01}$ and $r_{10}$ of KIC 11081729 decrease firstly and then increase with the increase in frequency. For different spectroscopic constraints, all models with overshooting parameter $\\delta_{\\mathrm{ov}}$ less than 1.7 can not reproduce the distributions of the ratios. However, the distributions of the ratios can be directly reproduced by models with $\\delta_{\\mathrm{ov}}$ in the range of about $1.7-1.8$. The estimations of mass and age of the star can be affected by spectroscopic results, but the determination of the $\\delta_{\\mathrm{ov}}$ is not dependent on the spect"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1508.00955","kind":"arxiv","version":4},"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":"1508.00955","created_at":"2026-05-18T01:17:08.049510+00:00"},{"alias_kind":"arxiv_version","alias_value":"1508.00955v4","created_at":"2026-05-18T01:17:08.049510+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1508.00955","created_at":"2026-05-18T01:17:08.049510+00:00"},{"alias_kind":"pith_short_12","alias_value":"CFBWBFZQCGDC","created_at":"2026-05-18T12:29:14.074870+00:00"},{"alias_kind":"pith_short_16","alias_value":"CFBWBFZQCGDCARWN","created_at":"2026-05-18T12:29:14.074870+00:00"},{"alias_kind":"pith_short_8","alias_value":"CFBWBFZQ","created_at":"2026-05-18T12:29:14.074870+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/CFBWBFZQCGDCARWNM2272BTJVH","json":"https://pith.science/pith/CFBWBFZQCGDCARWNM2272BTJVH.json","graph_json":"https://pith.science/api/pith-number/CFBWBFZQCGDCARWNM2272BTJVH/graph.json","events_json":"https://pith.science/api/pith-number/CFBWBFZQCGDCARWNM2272BTJVH/events.json","paper":"https://pith.science/paper/CFBWBFZQ"},"agent_actions":{"view_html":"https://pith.science/pith/CFBWBFZQCGDCARWNM2272BTJVH","download_json":"https://pith.science/pith/CFBWBFZQCGDCARWNM2272BTJVH.json","view_paper":"https://pith.science/paper/CFBWBFZQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1508.00955&json=true","fetch_graph":"https://pith.science/api/pith-number/CFBWBFZQCGDCARWNM2272BTJVH/graph.json","fetch_events":"https://pith.science/api/pith-number/CFBWBFZQCGDCARWNM2272BTJVH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CFBWBFZQCGDCARWNM2272BTJVH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CFBWBFZQCGDCARWNM2272BTJVH/action/storage_attestation","attest_author":"https://pith.science/pith/CFBWBFZQCGDCARWNM2272BTJVH/action/author_attestation","sign_citation":"https://pith.science/pith/CFBWBFZQCGDCARWNM2272BTJVH/action/citation_signature","submit_replication":"https://pith.science/pith/CFBWBFZQCGDCARWNM2272BTJVH/action/replication_record"}},"created_at":"2026-05-18T01:17:08.049510+00:00","updated_at":"2026-05-18T01:17:08.049510+00:00"}