{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:T2HE52VUBDEC3JRZSX4AFAL7YF","short_pith_number":"pith:T2HE52VU","schema_version":"1.0","canonical_sha256":"9e8e4eeab408c82da63995f802817fc15fa5491f71a6509a6c6751412c0bf03d","source":{"kind":"arxiv","id":"1102.0252","version":1},"attestation_state":"computed","paper":{"title":"Open issues in probing interiors of solar-like oscillating main sequence stars: 2. Diversity in the HR diagram","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"J.P. Marques, J. Provost, M.J. Goupil, O. Benomar, S. Deheuvels, Y. Lebreton","submitted_at":"2011-02-01T19:04:27Z","abstract_excerpt":"We review some major open issues in the current modelling of low and intermediate mass, main sequence stars based on seismological studies. The solar case was discussed in a companion paper, here several issues specific to other stars than the Sun are illustrated with a few stars observed with CoRoT and expectations from Kepler data."},"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":"1102.0252","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-02-01T19:04:27Z","cross_cats_sorted":[],"title_canon_sha256":"7ed78d6547626c8b80a935407b67b2a70070a83c6f99ab99c1735294c009debf","abstract_canon_sha256":"2417b50b5d3691843ccc239a0b711321e672d2eaa3425cb726db246685105300"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:17.977535Z","signature_b64":"cYWxvHFjKyyl47ZXd+Lrxz7yv0zPmzYvARXRz1MllwLzklyRbXyTNjBIhLVPL58EcSizwZbTI+li+me2C5iODg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9e8e4eeab408c82da63995f802817fc15fa5491f71a6509a6c6751412c0bf03d","last_reissued_at":"2026-05-18T02:03:17.976959Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:17.976959Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Open issues in probing interiors of solar-like oscillating main sequence stars: 2. Diversity in the HR diagram","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"J.P. Marques, J. Provost, M.J. Goupil, O. Benomar, S. Deheuvels, Y. Lebreton","submitted_at":"2011-02-01T19:04:27Z","abstract_excerpt":"We review some major open issues in the current modelling of low and intermediate mass, main sequence stars based on seismological studies. The solar case was discussed in a companion paper, here several issues specific to other stars than the Sun are illustrated with a few stars observed with CoRoT and expectations from Kepler data."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1102.0252","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":"1102.0252","created_at":"2026-05-18T02:03:17.977051+00:00"},{"alias_kind":"arxiv_version","alias_value":"1102.0252v1","created_at":"2026-05-18T02:03:17.977051+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1102.0252","created_at":"2026-05-18T02:03:17.977051+00:00"},{"alias_kind":"pith_short_12","alias_value":"T2HE52VUBDEC","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_16","alias_value":"T2HE52VUBDEC3JRZ","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_8","alias_value":"T2HE52VU","created_at":"2026-05-18T12:26:41.206345+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/T2HE52VUBDEC3JRZSX4AFAL7YF","json":"https://pith.science/pith/T2HE52VUBDEC3JRZSX4AFAL7YF.json","graph_json":"https://pith.science/api/pith-number/T2HE52VUBDEC3JRZSX4AFAL7YF/graph.json","events_json":"https://pith.science/api/pith-number/T2HE52VUBDEC3JRZSX4AFAL7YF/events.json","paper":"https://pith.science/paper/T2HE52VU"},"agent_actions":{"view_html":"https://pith.science/pith/T2HE52VUBDEC3JRZSX4AFAL7YF","download_json":"https://pith.science/pith/T2HE52VUBDEC3JRZSX4AFAL7YF.json","view_paper":"https://pith.science/paper/T2HE52VU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1102.0252&json=true","fetch_graph":"https://pith.science/api/pith-number/T2HE52VUBDEC3JRZSX4AFAL7YF/graph.json","fetch_events":"https://pith.science/api/pith-number/T2HE52VUBDEC3JRZSX4AFAL7YF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/T2HE52VUBDEC3JRZSX4AFAL7YF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/T2HE52VUBDEC3JRZSX4AFAL7YF/action/storage_attestation","attest_author":"https://pith.science/pith/T2HE52VUBDEC3JRZSX4AFAL7YF/action/author_attestation","sign_citation":"https://pith.science/pith/T2HE52VUBDEC3JRZSX4AFAL7YF/action/citation_signature","submit_replication":"https://pith.science/pith/T2HE52VUBDEC3JRZSX4AFAL7YF/action/replication_record"}},"created_at":"2026-05-18T02:03:17.977051+00:00","updated_at":"2026-05-18T02:03:17.977051+00:00"}