{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:3GHED6DKD4ODZE2SBEENXMX5KG","short_pith_number":"pith:3GHED6DK","schema_version":"1.0","canonical_sha256":"d98e41f86a1f1c3c93520908dbb2fd51ab372381971639a51dc8469e558fe6f5","source":{"kind":"arxiv","id":"astro-ph/0509239","version":1},"attestation_state":"computed","paper":{"title":"Non-LTE Line-Formation and Abundances of Sulfur and Zinc in F, G, and K Stars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Hikaru Taguchi, Kazuo Yoshioka, Masahide Takada-Hidai, Osamu Hashimoto, Satoshi Honda, Yoichi Takeda, Yuji Saito","submitted_at":"2005-09-09T02:23:14Z","abstract_excerpt":"Extensive statistical-equilibrium calculations on neutral sulfur and zinc were carried out, in order to investigate how the non-LTE effect plays a role in the determination of S and Zn abundances in F, G, and K stars. Having checked on the spectra of representative F-type stars (Polaris, Procyon, and alpha Per) and the Sun that our non-LTE corrections yield a reasonable consistency between the abundances derived from different lines, we tried an extensive non-LTE reanalysis of published equivalent-width data of S I and Zn I lines for metal-poor halo/disk stars. According to our calculations, S"},"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":"astro-ph/0509239","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-09-09T02:23:14Z","cross_cats_sorted":[],"title_canon_sha256":"de6f2b9589ef98717015dd83b2cd59fb8bcb35b5ba0ef8fb83e0daa060a7a199","abstract_canon_sha256":"22dc46453e26f2fa1d7250076a30af7a7a47f2c14b0bb241aa70fb5579a5cba7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:33.508361Z","signature_b64":"o//9SETey/8nZkxPmKDe1Y8nSDjGguroMZzWpDDkFQuHfP/jKu+Z7OqoEoU9lIDSqoMMc3SEVVXOzyK8yBnxCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d98e41f86a1f1c3c93520908dbb2fd51ab372381971639a51dc8469e558fe6f5","last_reissued_at":"2026-05-18T01:40:33.507612Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:33.507612Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-LTE Line-Formation and Abundances of Sulfur and Zinc in F, G, and K Stars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Hikaru Taguchi, Kazuo Yoshioka, Masahide Takada-Hidai, Osamu Hashimoto, Satoshi Honda, Yoichi Takeda, Yuji Saito","submitted_at":"2005-09-09T02:23:14Z","abstract_excerpt":"Extensive statistical-equilibrium calculations on neutral sulfur and zinc were carried out, in order to investigate how the non-LTE effect plays a role in the determination of S and Zn abundances in F, G, and K stars. Having checked on the spectra of representative F-type stars (Polaris, Procyon, and alpha Per) and the Sun that our non-LTE corrections yield a reasonable consistency between the abundances derived from different lines, we tried an extensive non-LTE reanalysis of published equivalent-width data of S I and Zn I lines for metal-poor halo/disk stars. According to our calculations, S"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0509239","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":"astro-ph/0509239","created_at":"2026-05-18T01:40:33.507733+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0509239v1","created_at":"2026-05-18T01:40:33.507733+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0509239","created_at":"2026-05-18T01:40:33.507733+00:00"},{"alias_kind":"pith_short_12","alias_value":"3GHED6DKD4OD","created_at":"2026-05-18T12:25:52.687210+00:00"},{"alias_kind":"pith_short_16","alias_value":"3GHED6DKD4ODZE2S","created_at":"2026-05-18T12:25:52.687210+00:00"},{"alias_kind":"pith_short_8","alias_value":"3GHED6DK","created_at":"2026-05-18T12:25:52.687210+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2105.01661","citing_title":"The chemical make-up of the Sun: A 2020 vision","ref_index":154,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3GHED6DKD4ODZE2SBEENXMX5KG","json":"https://pith.science/pith/3GHED6DKD4ODZE2SBEENXMX5KG.json","graph_json":"https://pith.science/api/pith-number/3GHED6DKD4ODZE2SBEENXMX5KG/graph.json","events_json":"https://pith.science/api/pith-number/3GHED6DKD4ODZE2SBEENXMX5KG/events.json","paper":"https://pith.science/paper/3GHED6DK"},"agent_actions":{"view_html":"https://pith.science/pith/3GHED6DKD4ODZE2SBEENXMX5KG","download_json":"https://pith.science/pith/3GHED6DKD4ODZE2SBEENXMX5KG.json","view_paper":"https://pith.science/paper/3GHED6DK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0509239&json=true","fetch_graph":"https://pith.science/api/pith-number/3GHED6DKD4ODZE2SBEENXMX5KG/graph.json","fetch_events":"https://pith.science/api/pith-number/3GHED6DKD4ODZE2SBEENXMX5KG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3GHED6DKD4ODZE2SBEENXMX5KG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3GHED6DKD4ODZE2SBEENXMX5KG/action/storage_attestation","attest_author":"https://pith.science/pith/3GHED6DKD4ODZE2SBEENXMX5KG/action/author_attestation","sign_citation":"https://pith.science/pith/3GHED6DKD4ODZE2SBEENXMX5KG/action/citation_signature","submit_replication":"https://pith.science/pith/3GHED6DKD4ODZE2SBEENXMX5KG/action/replication_record"}},"created_at":"2026-05-18T01:40:33.507733+00:00","updated_at":"2026-05-18T01:40:33.507733+00:00"}