{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:J5CZWJUZY7GLYN6NJY2R7EFPKK","short_pith_number":"pith:J5CZWJUZ","schema_version":"1.0","canonical_sha256":"4f459b2699c7ccbc37cd4e351f90af52bc6e6f9465af6ebc313377467eeac238","source":{"kind":"arxiv","id":"1009.5131","version":2},"attestation_state":"computed","paper":{"title":"Automatic Determination of Stellar Parameters via Asteroseismology of Stochastically Oscillating Stars: Comparison with Direct Measurements","license":"http://creativecommons.org/licenses/publicdomain/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"J. Christensen-Dalsgaard, P.-O. Quirion, T. Arentoft","submitted_at":"2010-09-26T21:35:49Z","abstract_excerpt":"Space-based projects are providing a wealth of high-quality asteroseismic data, including frequencies for a large number of stars showing solar-like oscillations. These data open the prospect for precise determinations of key stellar parameters, of particular value to the study of extra-solar planetary systems. Given the quantity of the available and expected data it is important to develop efficient and reliable techniques for analyzing them, including the determination of stellar parameters from the observed frequencies. Here we present the SEEK package developed for the analysis of asterose"},"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":"1009.5131","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/publicdomain/","primary_cat":"astro-ph.SR","submitted_at":"2010-09-26T21:35:49Z","cross_cats_sorted":["astro-ph.EP"],"title_canon_sha256":"2ecfc299552f8eb3c3fb3d9bb5e5e0a84820e1b5c8218e0ee2829abea3d5daac","abstract_canon_sha256":"52031012c6451c11f0b51b52fe1e0c72edd1a072491d56151a4db10cf0f597e9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:17.094695Z","signature_b64":"Wf9o2HjYqm+vUmnBMHhm5L1oxsFyEgbidzo9z2IreXmP9WnlYDH5sbwoFh7tO9arYTsb6dBhGJqlpx4GitFYCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4f459b2699c7ccbc37cd4e351f90af52bc6e6f9465af6ebc313377467eeac238","last_reissued_at":"2026-05-18T02:05:17.093910Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:17.093910Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Automatic Determination of Stellar Parameters via Asteroseismology of Stochastically Oscillating Stars: Comparison with Direct Measurements","license":"http://creativecommons.org/licenses/publicdomain/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"J. Christensen-Dalsgaard, P.-O. Quirion, T. Arentoft","submitted_at":"2010-09-26T21:35:49Z","abstract_excerpt":"Space-based projects are providing a wealth of high-quality asteroseismic data, including frequencies for a large number of stars showing solar-like oscillations. These data open the prospect for precise determinations of key stellar parameters, of particular value to the study of extra-solar planetary systems. Given the quantity of the available and expected data it is important to develop efficient and reliable techniques for analyzing them, including the determination of stellar parameters from the observed frequencies. Here we present the SEEK package developed for the analysis of asterose"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.5131","kind":"arxiv","version":2},"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":"1009.5131","created_at":"2026-05-18T02:05:17.093999+00:00"},{"alias_kind":"arxiv_version","alias_value":"1009.5131v2","created_at":"2026-05-18T02:05:17.093999+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.5131","created_at":"2026-05-18T02:05:17.093999+00:00"},{"alias_kind":"pith_short_12","alias_value":"J5CZWJUZY7GL","created_at":"2026-05-18T12:26:09.077623+00:00"},{"alias_kind":"pith_short_16","alias_value":"J5CZWJUZY7GLYN6N","created_at":"2026-05-18T12:26:09.077623+00:00"},{"alias_kind":"pith_short_8","alias_value":"J5CZWJUZ","created_at":"2026-05-18T12:26:09.077623+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/J5CZWJUZY7GLYN6NJY2R7EFPKK","json":"https://pith.science/pith/J5CZWJUZY7GLYN6NJY2R7EFPKK.json","graph_json":"https://pith.science/api/pith-number/J5CZWJUZY7GLYN6NJY2R7EFPKK/graph.json","events_json":"https://pith.science/api/pith-number/J5CZWJUZY7GLYN6NJY2R7EFPKK/events.json","paper":"https://pith.science/paper/J5CZWJUZ"},"agent_actions":{"view_html":"https://pith.science/pith/J5CZWJUZY7GLYN6NJY2R7EFPKK","download_json":"https://pith.science/pith/J5CZWJUZY7GLYN6NJY2R7EFPKK.json","view_paper":"https://pith.science/paper/J5CZWJUZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1009.5131&json=true","fetch_graph":"https://pith.science/api/pith-number/J5CZWJUZY7GLYN6NJY2R7EFPKK/graph.json","fetch_events":"https://pith.science/api/pith-number/J5CZWJUZY7GLYN6NJY2R7EFPKK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/J5CZWJUZY7GLYN6NJY2R7EFPKK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/J5CZWJUZY7GLYN6NJY2R7EFPKK/action/storage_attestation","attest_author":"https://pith.science/pith/J5CZWJUZY7GLYN6NJY2R7EFPKK/action/author_attestation","sign_citation":"https://pith.science/pith/J5CZWJUZY7GLYN6NJY2R7EFPKK/action/citation_signature","submit_replication":"https://pith.science/pith/J5CZWJUZY7GLYN6NJY2R7EFPKK/action/replication_record"}},"created_at":"2026-05-18T02:05:17.093999+00:00","updated_at":"2026-05-18T02:05:17.093999+00:00"}