{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:MNKOV26WSWQZBBGIFSJLWUC4GE","short_pith_number":"pith:MNKOV26W","schema_version":"1.0","canonical_sha256":"6354eaebd695a19084c82c92bb505c3119ddd883919a98df5a78d57db2aecbae","source":{"kind":"arxiv","id":"1707.02082","version":1},"attestation_state":"computed","paper":{"title":"Semi-empirical seismic relations of A-F stars from CoRoT and Kepler legacy data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Garc\\'ia Hern\\'andez, A. Moya, J.C. Su\\'arez, M.A. Mendoza","submitted_at":"2017-07-07T09:05:37Z","abstract_excerpt":"Asteroseismology is witnessing a revolution thanks to high-precise asteroseismic space data (MOST, CoRoT, Kepler, BRITE), and their large ground-based follow-up programs. Those instruments have provided an unprecedented large amount of information, which allows us to scrutinize its statistical properties in the quest for hidden relations among pulsational and/or physical observables. This approach might be particularly useful for stars whose pulsation content is difficult to interpret. This is the case of intermediate-mass classical pulsating stars (i.e. gamma Dor, delta Scuti, hybrids) for wh"},"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":"1707.02082","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-07-07T09:05:37Z","cross_cats_sorted":[],"title_canon_sha256":"df186a04a9c235891629c4a1a10793835835aa7e3f47d05b31596b8ab62a6562","abstract_canon_sha256":"60df2767bb5aae93b528797d95f7d2776f866198378f5e6e7a7430e559ce4b7d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:37:18.162198Z","signature_b64":"JsLCbIMI6KQoBM8W+r4JJC+z0Iro97YdtMs1JW43JzbzroXSdGlnJ5R17VMefEiC8WMwbOn4c09Z7XZABLXVAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6354eaebd695a19084c82c92bb505c3119ddd883919a98df5a78d57db2aecbae","last_reissued_at":"2026-05-18T00:37:18.161507Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:37:18.161507Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Semi-empirical seismic relations of A-F stars from CoRoT and Kepler legacy data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Garc\\'ia Hern\\'andez, A. Moya, J.C. Su\\'arez, M.A. Mendoza","submitted_at":"2017-07-07T09:05:37Z","abstract_excerpt":"Asteroseismology is witnessing a revolution thanks to high-precise asteroseismic space data (MOST, CoRoT, Kepler, BRITE), and their large ground-based follow-up programs. Those instruments have provided an unprecedented large amount of information, which allows us to scrutinize its statistical properties in the quest for hidden relations among pulsational and/or physical observables. This approach might be particularly useful for stars whose pulsation content is difficult to interpret. This is the case of intermediate-mass classical pulsating stars (i.e. gamma Dor, delta Scuti, hybrids) for wh"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.02082","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":"1707.02082","created_at":"2026-05-18T00:37:18.161636+00:00"},{"alias_kind":"arxiv_version","alias_value":"1707.02082v1","created_at":"2026-05-18T00:37:18.161636+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1707.02082","created_at":"2026-05-18T00:37:18.161636+00:00"},{"alias_kind":"pith_short_12","alias_value":"MNKOV26WSWQZ","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_16","alias_value":"MNKOV26WSWQZBBGI","created_at":"2026-05-18T12:31:31.346846+00:00"},{"alias_kind":"pith_short_8","alias_value":"MNKOV26W","created_at":"2026-05-18T12:31:31.346846+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/MNKOV26WSWQZBBGIFSJLWUC4GE","json":"https://pith.science/pith/MNKOV26WSWQZBBGIFSJLWUC4GE.json","graph_json":"https://pith.science/api/pith-number/MNKOV26WSWQZBBGIFSJLWUC4GE/graph.json","events_json":"https://pith.science/api/pith-number/MNKOV26WSWQZBBGIFSJLWUC4GE/events.json","paper":"https://pith.science/paper/MNKOV26W"},"agent_actions":{"view_html":"https://pith.science/pith/MNKOV26WSWQZBBGIFSJLWUC4GE","download_json":"https://pith.science/pith/MNKOV26WSWQZBBGIFSJLWUC4GE.json","view_paper":"https://pith.science/paper/MNKOV26W","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1707.02082&json=true","fetch_graph":"https://pith.science/api/pith-number/MNKOV26WSWQZBBGIFSJLWUC4GE/graph.json","fetch_events":"https://pith.science/api/pith-number/MNKOV26WSWQZBBGIFSJLWUC4GE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MNKOV26WSWQZBBGIFSJLWUC4GE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MNKOV26WSWQZBBGIFSJLWUC4GE/action/storage_attestation","attest_author":"https://pith.science/pith/MNKOV26WSWQZBBGIFSJLWUC4GE/action/author_attestation","sign_citation":"https://pith.science/pith/MNKOV26WSWQZBBGIFSJLWUC4GE/action/citation_signature","submit_replication":"https://pith.science/pith/MNKOV26WSWQZBBGIFSJLWUC4GE/action/replication_record"}},"created_at":"2026-05-18T00:37:18.161636+00:00","updated_at":"2026-05-18T00:37:18.161636+00:00"}