{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:D3D5UX2LXPPW7VFJ6YJFX3HUA7","short_pith_number":"pith:D3D5UX2L","schema_version":"1.0","canonical_sha256":"1ec7da5f4bbbdf6fd4a9f6125becf407dcee2259fcd2b1fb3b00da7ae5abe154","source":{"kind":"arxiv","id":"2405.06153","version":1},"attestation_state":"computed","paper":{"title":"Abundances in eight bulge stars from the optical and near-infrared","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"B. Barbuy, D. Gonz\\'alez-D\\'iaz, H. Ernandes, J. G. Fern\\'andez-Trincado, Patr\\'icia da Silva, S. O. Souza","submitted_at":"2024-05-10T00:22:14Z","abstract_excerpt":"Context: The abundances of the $\\alpha$-elements are key for understanding the early chemical enrichment of the Galactic bulge. The elements of interest present lines in different wavelength regions, and some of them show lines only in part of the spectra. In the present work, the CNO trio, the alpha-elements Mg, Si, Ca, and Ti, and odd-Z Na and Al are examined as measured from optical and H-band lines.\n  Aims: The aim of this work is to carry out a detailed comparison of stellar parameters and abundances derived in the optical and near-infrared (H-band). We also inspect the best available lin"},"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":"2405.06153","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2024-05-10T00:22:14Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"8872f163b5dad9b2c0e509b86171bf29bed87c1dbed014b4b8f8632eaa2c9427","abstract_canon_sha256":"16e026744e2553bdc3d31592064bae7448aeec162601cf0b52a2096eda728412"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:17:36.428301Z","signature_b64":"6nm+ZIPUZ1vY71Qrms9hl8XkkiB0snjOWuPq8QNe/IK799JWEjLB3iM6nNTrjmwi/vgamlbFX77uVN+HPeNaCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1ec7da5f4bbbdf6fd4a9f6125becf407dcee2259fcd2b1fb3b00da7ae5abe154","last_reissued_at":"2026-07-05T08:17:36.427889Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:17:36.427889Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Abundances in eight bulge stars from the optical and near-infrared","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"B. Barbuy, D. Gonz\\'alez-D\\'iaz, H. Ernandes, J. G. Fern\\'andez-Trincado, Patr\\'icia da Silva, S. O. Souza","submitted_at":"2024-05-10T00:22:14Z","abstract_excerpt":"Context: The abundances of the $\\alpha$-elements are key for understanding the early chemical enrichment of the Galactic bulge. The elements of interest present lines in different wavelength regions, and some of them show lines only in part of the spectra. In the present work, the CNO trio, the alpha-elements Mg, Si, Ca, and Ti, and odd-Z Na and Al are examined as measured from optical and H-band lines.\n  Aims: The aim of this work is to carry out a detailed comparison of stellar parameters and abundances derived in the optical and near-infrared (H-band). We also inspect the best available lin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.06153","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/2405.06153/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":"2405.06153","created_at":"2026-07-05T08:17:36.427943+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.06153v1","created_at":"2026-07-05T08:17:36.427943+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.06153","created_at":"2026-07-05T08:17:36.427943+00:00"},{"alias_kind":"pith_short_12","alias_value":"D3D5UX2LXPPW","created_at":"2026-07-05T08:17:36.427943+00:00"},{"alias_kind":"pith_short_16","alias_value":"D3D5UX2LXPPW7VFJ","created_at":"2026-07-05T08:17:36.427943+00:00"},{"alias_kind":"pith_short_8","alias_value":"D3D5UX2L","created_at":"2026-07-05T08:17:36.427943+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/D3D5UX2LXPPW7VFJ6YJFX3HUA7","json":"https://pith.science/pith/D3D5UX2LXPPW7VFJ6YJFX3HUA7.json","graph_json":"https://pith.science/api/pith-number/D3D5UX2LXPPW7VFJ6YJFX3HUA7/graph.json","events_json":"https://pith.science/api/pith-number/D3D5UX2LXPPW7VFJ6YJFX3HUA7/events.json","paper":"https://pith.science/paper/D3D5UX2L"},"agent_actions":{"view_html":"https://pith.science/pith/D3D5UX2LXPPW7VFJ6YJFX3HUA7","download_json":"https://pith.science/pith/D3D5UX2LXPPW7VFJ6YJFX3HUA7.json","view_paper":"https://pith.science/paper/D3D5UX2L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.06153&json=true","fetch_graph":"https://pith.science/api/pith-number/D3D5UX2LXPPW7VFJ6YJFX3HUA7/graph.json","fetch_events":"https://pith.science/api/pith-number/D3D5UX2LXPPW7VFJ6YJFX3HUA7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/D3D5UX2LXPPW7VFJ6YJFX3HUA7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/D3D5UX2LXPPW7VFJ6YJFX3HUA7/action/storage_attestation","attest_author":"https://pith.science/pith/D3D5UX2LXPPW7VFJ6YJFX3HUA7/action/author_attestation","sign_citation":"https://pith.science/pith/D3D5UX2LXPPW7VFJ6YJFX3HUA7/action/citation_signature","submit_replication":"https://pith.science/pith/D3D5UX2LXPPW7VFJ6YJFX3HUA7/action/replication_record"}},"created_at":"2026-07-05T08:17:36.427943+00:00","updated_at":"2026-07-05T08:17:36.427943+00:00"}