{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:Q4E7HNNFBFADAFV4UJO6R22AZ5","short_pith_number":"pith:Q4E7HNNF","schema_version":"1.0","canonical_sha256":"8709f3b5a509403016bca25de8eb40cf6faa10c09fb437a98422a4b1afe61a00","source":{"kind":"arxiv","id":"1610.00193","version":1},"attestation_state":"computed","paper":{"title":"Systematic non-LTE study of the $-2.6 \\le$ [Fe/H] $\\le 0.2$ F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Eu","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Kobayashi, F. Liu, G. Zhao, H. L. Yan, H. W. Zhang, J. B. Zhang, J. R. Shi, K. F. Tan, L. Mashonkina, M. Bolte, M. Zhai, S. Alexeeva, T. Sitnova, X. Li, Y. Q. Chen, Yu. Pakhomov, Z. M. Zhou","submitted_at":"2016-10-01T21:40:58Z","abstract_excerpt":"For the first time, we present an extensive study of stars with individual non-local thermodynamic equilibrium (NLTE) abundances for 17 chemical elements from Li to Eu in a sample of stars uniformly distributed over the $-2.62 \\le$ [Fe/H] $\\le +0.24$ metallicity range that is suitable for the Galactic chemical evolution research. The star sample has been kinematically selected to trace the Galactic thin and thick disks and halo. We find new and improve earlier results as follows. (i) The element-to-iron ratios for Mg, Si, Ca, and Ti form a MP plateau at a similar height of 0.3~dex, and the kne"},"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":"1610.00193","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-01T21:40:58Z","cross_cats_sorted":[],"title_canon_sha256":"88da7aa803435192c0d0ed56be5e0adb8ddf7dd957419727fafa1650c835002f","abstract_canon_sha256":"ae9c6af85d6e12324cde7ae3bdbcf9d1a1750258a41c32ad8185498c2ca33a91"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:53:58.526508Z","signature_b64":"hr6EdpHb0ONZjR7fE7lGJZPM3V+gqPfR1Qd8H+NsiBebuJwLmqr4Ie2yVJjs9pnuKFxAYMEL5uXx3PwIXXkzBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8709f3b5a509403016bca25de8eb40cf6faa10c09fb437a98422a4b1afe61a00","last_reissued_at":"2026-05-18T00:53:58.525977Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:53:58.525977Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Systematic non-LTE study of the $-2.6 \\le$ [Fe/H] $\\le 0.2$ F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Eu","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"C. Kobayashi, F. Liu, G. Zhao, H. L. Yan, H. W. Zhang, J. B. Zhang, J. R. Shi, K. F. Tan, L. Mashonkina, M. Bolte, M. Zhai, S. Alexeeva, T. Sitnova, X. Li, Y. Q. Chen, Yu. Pakhomov, Z. M. Zhou","submitted_at":"2016-10-01T21:40:58Z","abstract_excerpt":"For the first time, we present an extensive study of stars with individual non-local thermodynamic equilibrium (NLTE) abundances for 17 chemical elements from Li to Eu in a sample of stars uniformly distributed over the $-2.62 \\le$ [Fe/H] $\\le +0.24$ metallicity range that is suitable for the Galactic chemical evolution research. The star sample has been kinematically selected to trace the Galactic thin and thick disks and halo. We find new and improve earlier results as follows. (i) The element-to-iron ratios for Mg, Si, Ca, and Ti form a MP plateau at a similar height of 0.3~dex, and the kne"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.00193","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":"1610.00193","created_at":"2026-05-18T00:53:58.526067+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.00193v1","created_at":"2026-05-18T00:53:58.526067+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.00193","created_at":"2026-05-18T00:53:58.526067+00:00"},{"alias_kind":"pith_short_12","alias_value":"Q4E7HNNFBFAD","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_16","alias_value":"Q4E7HNNFBFADAFV4","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_8","alias_value":"Q4E7HNNF","created_at":"2026-05-18T12:30:39.010887+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2606.08782","citing_title":"JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe","ref_index":52,"is_internal_anchor":true},{"citing_arxiv_id":"2605.11074","citing_title":"Observational Signatures and Constraints on the Intermediate Neutron-Capture Process. The Case of the CEMP star TYC 6044-714-1 (RAVE J094921.8-161722)","ref_index":125,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Q4E7HNNFBFADAFV4UJO6R22AZ5","json":"https://pith.science/pith/Q4E7HNNFBFADAFV4UJO6R22AZ5.json","graph_json":"https://pith.science/api/pith-number/Q4E7HNNFBFADAFV4UJO6R22AZ5/graph.json","events_json":"https://pith.science/api/pith-number/Q4E7HNNFBFADAFV4UJO6R22AZ5/events.json","paper":"https://pith.science/paper/Q4E7HNNF"},"agent_actions":{"view_html":"https://pith.science/pith/Q4E7HNNFBFADAFV4UJO6R22AZ5","download_json":"https://pith.science/pith/Q4E7HNNFBFADAFV4UJO6R22AZ5.json","view_paper":"https://pith.science/paper/Q4E7HNNF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.00193&json=true","fetch_graph":"https://pith.science/api/pith-number/Q4E7HNNFBFADAFV4UJO6R22AZ5/graph.json","fetch_events":"https://pith.science/api/pith-number/Q4E7HNNFBFADAFV4UJO6R22AZ5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Q4E7HNNFBFADAFV4UJO6R22AZ5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Q4E7HNNFBFADAFV4UJO6R22AZ5/action/storage_attestation","attest_author":"https://pith.science/pith/Q4E7HNNFBFADAFV4UJO6R22AZ5/action/author_attestation","sign_citation":"https://pith.science/pith/Q4E7HNNFBFADAFV4UJO6R22AZ5/action/citation_signature","submit_replication":"https://pith.science/pith/Q4E7HNNFBFADAFV4UJO6R22AZ5/action/replication_record"}},"created_at":"2026-05-18T00:53:58.526067+00:00","updated_at":"2026-05-18T00:53:58.526067+00:00"}