{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:DN5BWKGIFTJNP2WJYZOWBZMAVM","short_pith_number":"pith:DN5BWKGI","schema_version":"1.0","canonical_sha256":"1b7a1b28c82cd2d7eac9c65d60e580ab25a89bf9814fecea976c8bf0dc81896a","source":{"kind":"arxiv","id":"1801.10589","version":1},"attestation_state":"computed","paper":{"title":"Asteroseismology of ZZ Ceti stars with full evolutionary white dwarf models. II. The impact of AGB thermal pulses on the asteroseismic inferences of ZZ Ceti stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Alejandra D. Romero, Alejandro H. C\\'orsico, Francisco C. De Ger\\'onimo, Leandro G. Althaus, S.O. Kepler","submitted_at":"2018-01-31T18:23:22Z","abstract_excerpt":"The thermally pulsing phase on the asymptotic giant branch (TP-AGB) is the last nuclear burning phase experienced by most of low and intermediate mass stars. During this phase, the outer chemical stratification above the C/O core of the emerging white dwarf is built up. The chemical structure resulting from progenitor evolution strongly impacts the whole pulsation spectrum exhibited by ZZ Ceti stars, which are pulsating C/O core white dwarfs located on an narrow instability strip at T eff \\sim 12000 K. Several physical processes occurring during progenitor evolution strongly affect the chemica"},"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":"1801.10589","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-01-31T18:23:22Z","cross_cats_sorted":[],"title_canon_sha256":"646ad7fa411c0a79a0ab0d3df059c72b0c67821984c338007cbd23da067a7039","abstract_canon_sha256":"a4db981986feacfce54c04e36f10a06ccdfbf25e6ea90740e5ae6d5d9c0a0df2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:13:28.105784Z","signature_b64":"pYIPIVvF1pY4LrR7AS0N/d0eW2nj2Cy7pzGdZQa7w/qN2vm3HO0LHlg/IvQU8ZzkuNoNt59+d8huHlSq7sr8BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1b7a1b28c82cd2d7eac9c65d60e580ab25a89bf9814fecea976c8bf0dc81896a","last_reissued_at":"2026-05-18T00:13:28.105167Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:13:28.105167Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Asteroseismology of ZZ Ceti stars with full evolutionary white dwarf models. II. The impact of AGB thermal pulses on the asteroseismic inferences of ZZ Ceti stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Alejandra D. Romero, Alejandro H. C\\'orsico, Francisco C. De Ger\\'onimo, Leandro G. Althaus, S.O. Kepler","submitted_at":"2018-01-31T18:23:22Z","abstract_excerpt":"The thermally pulsing phase on the asymptotic giant branch (TP-AGB) is the last nuclear burning phase experienced by most of low and intermediate mass stars. During this phase, the outer chemical stratification above the C/O core of the emerging white dwarf is built up. The chemical structure resulting from progenitor evolution strongly impacts the whole pulsation spectrum exhibited by ZZ Ceti stars, which are pulsating C/O core white dwarfs located on an narrow instability strip at T eff \\sim 12000 K. Several physical processes occurring during progenitor evolution strongly affect the chemica"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.10589","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":"1801.10589","created_at":"2026-05-18T00:13:28.105255+00:00"},{"alias_kind":"arxiv_version","alias_value":"1801.10589v1","created_at":"2026-05-18T00:13:28.105255+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1801.10589","created_at":"2026-05-18T00:13:28.105255+00:00"},{"alias_kind":"pith_short_12","alias_value":"DN5BWKGIFTJN","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_16","alias_value":"DN5BWKGIFTJNP2WJ","created_at":"2026-05-18T12:32:19.392346+00:00"},{"alias_kind":"pith_short_8","alias_value":"DN5BWKGI","created_at":"2026-05-18T12:32:19.392346+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/DN5BWKGIFTJNP2WJYZOWBZMAVM","json":"https://pith.science/pith/DN5BWKGIFTJNP2WJYZOWBZMAVM.json","graph_json":"https://pith.science/api/pith-number/DN5BWKGIFTJNP2WJYZOWBZMAVM/graph.json","events_json":"https://pith.science/api/pith-number/DN5BWKGIFTJNP2WJYZOWBZMAVM/events.json","paper":"https://pith.science/paper/DN5BWKGI"},"agent_actions":{"view_html":"https://pith.science/pith/DN5BWKGIFTJNP2WJYZOWBZMAVM","download_json":"https://pith.science/pith/DN5BWKGIFTJNP2WJYZOWBZMAVM.json","view_paper":"https://pith.science/paper/DN5BWKGI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1801.10589&json=true","fetch_graph":"https://pith.science/api/pith-number/DN5BWKGIFTJNP2WJYZOWBZMAVM/graph.json","fetch_events":"https://pith.science/api/pith-number/DN5BWKGIFTJNP2WJYZOWBZMAVM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DN5BWKGIFTJNP2WJYZOWBZMAVM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DN5BWKGIFTJNP2WJYZOWBZMAVM/action/storage_attestation","attest_author":"https://pith.science/pith/DN5BWKGIFTJNP2WJYZOWBZMAVM/action/author_attestation","sign_citation":"https://pith.science/pith/DN5BWKGIFTJNP2WJYZOWBZMAVM/action/citation_signature","submit_replication":"https://pith.science/pith/DN5BWKGIFTJNP2WJYZOWBZMAVM/action/replication_record"}},"created_at":"2026-05-18T00:13:28.105255+00:00","updated_at":"2026-05-18T00:13:28.105255+00:00"}