{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:E2ECBRB77TOAZQGWNWW7Z56UWU","short_pith_number":"pith:E2ECBRB7","schema_version":"1.0","canonical_sha256":"268820c43ffcdc0cc0d66dadfcf7d4b51667566d655fcf03a3d66c6ff742bb34","source":{"kind":"arxiv","id":"2506.10400","version":1},"attestation_state":"computed","paper":{"title":"Stellar Ancestry Unlocked: Chemical and Orbital Clues Link Metal Poor Stars to Globular Clusters and the Galaxy's Thick Disk","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Gizay Yolalan, Olcay Plevne, Sel\\c{c}uk Bilir, Timur \\c{S}ahin","submitted_at":"2025-06-12T06:47:43Z","abstract_excerpt":"This study presents a detailed chemical, kinematic, and orbital dynamic analysis of five metal poor stars in the solar neighborhood: HD 2665, HD 5916, HD 122956, HD 189349, and HD 218857. Using high-resolution spectroscopic data from the ELODIE and ESPaDOnS instruments, we derived elemental abundances for 29 species (25 elements: C, O, Na, Mg, Al, Si, S, Ca, Sc, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn, Sr, Y, Zr, Ba, Ce, Nd, and Sm) via LTE based analysis with ATLAS9 model atmospheres. Notably, we report first time detections of Ce and Nd in HD2665; Al, V, Sm, and Mn in HD5916; Al in HD 122956; and "},"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":"2506.10400","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-06-12T06:47:43Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"4a76ac3ffc5026853f5ec5094f886645e6fff85a4d4d2ad4acc04a5b2f352dbe","abstract_canon_sha256":"ae3b3fba6fcba0457887c504c2af4f42f151eddba4483acd37c14f67d64affdf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:20:22.770100Z","signature_b64":"4gDsV1v3y1JYzF1uRHQcuBgMVLrGP8i7QKPfDHItozv7taQit2tGQPWhAZDVzA1Q7VRJgw5N6deLrcLq4w1ZAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"268820c43ffcdc0cc0d66dadfcf7d4b51667566d655fcf03a3d66c6ff742bb34","last_reissued_at":"2026-07-05T11:20:22.769611Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:20:22.769611Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stellar Ancestry Unlocked: Chemical and Orbital Clues Link Metal Poor Stars to Globular Clusters and the Galaxy's Thick Disk","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Gizay Yolalan, Olcay Plevne, Sel\\c{c}uk Bilir, Timur \\c{S}ahin","submitted_at":"2025-06-12T06:47:43Z","abstract_excerpt":"This study presents a detailed chemical, kinematic, and orbital dynamic analysis of five metal poor stars in the solar neighborhood: HD 2665, HD 5916, HD 122956, HD 189349, and HD 218857. Using high-resolution spectroscopic data from the ELODIE and ESPaDOnS instruments, we derived elemental abundances for 29 species (25 elements: C, O, Na, Mg, Al, Si, S, Ca, Sc, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn, Sr, Y, Zr, Ba, Ce, Nd, and Sm) via LTE based analysis with ATLAS9 model atmospheres. Notably, we report first time detections of Ce and Nd in HD2665; Al, V, Sm, and Mn in HD5916; Al in HD 122956; and "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.10400","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2506.10400/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2506.10400","created_at":"2026-07-05T11:20:22.769671+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.10400v1","created_at":"2026-07-05T11:20:22.769671+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.10400","created_at":"2026-07-05T11:20:22.769671+00:00"},{"alias_kind":"pith_short_12","alias_value":"E2ECBRB77TOA","created_at":"2026-07-05T11:20:22.769671+00:00"},{"alias_kind":"pith_short_16","alias_value":"E2ECBRB77TOAZQGW","created_at":"2026-07-05T11:20:22.769671+00:00"},{"alias_kind":"pith_short_8","alias_value":"E2ECBRB7","created_at":"2026-07-05T11:20:22.769671+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/E2ECBRB77TOAZQGWNWW7Z56UWU","json":"https://pith.science/pith/E2ECBRB77TOAZQGWNWW7Z56UWU.json","graph_json":"https://pith.science/api/pith-number/E2ECBRB77TOAZQGWNWW7Z56UWU/graph.json","events_json":"https://pith.science/api/pith-number/E2ECBRB77TOAZQGWNWW7Z56UWU/events.json","paper":"https://pith.science/paper/E2ECBRB7"},"agent_actions":{"view_html":"https://pith.science/pith/E2ECBRB77TOAZQGWNWW7Z56UWU","download_json":"https://pith.science/pith/E2ECBRB77TOAZQGWNWW7Z56UWU.json","view_paper":"https://pith.science/paper/E2ECBRB7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.10400&json=true","fetch_graph":"https://pith.science/api/pith-number/E2ECBRB77TOAZQGWNWW7Z56UWU/graph.json","fetch_events":"https://pith.science/api/pith-number/E2ECBRB77TOAZQGWNWW7Z56UWU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/E2ECBRB77TOAZQGWNWW7Z56UWU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/E2ECBRB77TOAZQGWNWW7Z56UWU/action/storage_attestation","attest_author":"https://pith.science/pith/E2ECBRB77TOAZQGWNWW7Z56UWU/action/author_attestation","sign_citation":"https://pith.science/pith/E2ECBRB77TOAZQGWNWW7Z56UWU/action/citation_signature","submit_replication":"https://pith.science/pith/E2ECBRB77TOAZQGWNWW7Z56UWU/action/replication_record"}},"created_at":"2026-07-05T11:20:22.769671+00:00","updated_at":"2026-07-05T11:20:22.769671+00:00"}