{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:THZMDTPKXZUYXMKTL3PC2BDSLM","short_pith_number":"pith:THZMDTPK","schema_version":"1.0","canonical_sha256":"99f2c1cdeabe698bb1535ede2d04725b29a6488c62df1f9f3ac5be8713e15c99","source":{"kind":"arxiv","id":"2103.10112","version":1},"attestation_state":"computed","paper":{"title":"The APOGEE Data Release 16 Spectral Line List","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"Bertrand Plez, Carlos Allende Prieto, D. A. Garcia-Hernandez, Diogo Souto, Dmitry Bizyaev, Guy S. Stringfellow, Henrik Jonsson, Jennifer Sobeck, Jon Holtzman, Katia Cunha, Matthew D. Shetrone, Rachael L. Beaton, Sten Hasselquist, Steven R. Majewski, Szabolcs Meszaros, Thomas Masseron, Verne V. Smith, Yeisson Osorio","submitted_at":"2021-03-18T09:39:05Z","abstract_excerpt":"The updated H-band spectral line list (from \\lambda 15,000 - 17,000\\AA) adopted by the Apache Point Observatory Galactic Evolution Experiment (APOGEE) for the SDSS IV Data Release 16 (DR16) is presented here. The APOGEE line list is a combination of atomic and molecular lines with data from laboratory, theoretical, and astrophysical sources. Oscillator strengths and damping constants are adjusted using high signal-to-noise, high-resolution spectra of the Sun and alpha Boo (Arcturus) as \"standard stars\". Updates to the DR16 line list, when compared to the previous DR14 version, are the inclusio"},"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":"2103.10112","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2021-03-18T09:39:05Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"a5a7f1712d7185b6a4c7e93ee179e6690f026212ce9deede690c531f8399985a","abstract_canon_sha256":"1c56966767b7ccefa073208a5c8c5fedb186b299c3bddf86de9b286fc234f01d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:39:16.853724Z","signature_b64":"gKQbd43c31B/6XYc4r/0vhIcBcFl5EMeSUHtS2xaYpqvu5apwUI0NZm3CNLG1XojxY+t6CjyTOfpuANCwiieDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"99f2c1cdeabe698bb1535ede2d04725b29a6488c62df1f9f3ac5be8713e15c99","last_reissued_at":"2026-07-05T02:39:16.853248Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:39:16.853248Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The APOGEE Data Release 16 Spectral Line List","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"Bertrand Plez, Carlos Allende Prieto, D. A. Garcia-Hernandez, Diogo Souto, Dmitry Bizyaev, Guy S. Stringfellow, Henrik Jonsson, Jennifer Sobeck, Jon Holtzman, Katia Cunha, Matthew D. Shetrone, Rachael L. Beaton, Sten Hasselquist, Steven R. Majewski, Szabolcs Meszaros, Thomas Masseron, Verne V. Smith, Yeisson Osorio","submitted_at":"2021-03-18T09:39:05Z","abstract_excerpt":"The updated H-band spectral line list (from \\lambda 15,000 - 17,000\\AA) adopted by the Apache Point Observatory Galactic Evolution Experiment (APOGEE) for the SDSS IV Data Release 16 (DR16) is presented here. The APOGEE line list is a combination of atomic and molecular lines with data from laboratory, theoretical, and astrophysical sources. Oscillator strengths and damping constants are adjusted using high signal-to-noise, high-resolution spectra of the Sun and alpha Boo (Arcturus) as \"standard stars\". Updates to the DR16 line list, when compared to the previous DR14 version, are the inclusio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2103.10112","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/2103.10112/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":"2103.10112","created_at":"2026-07-05T02:39:16.853313+00:00"},{"alias_kind":"arxiv_version","alias_value":"2103.10112v1","created_at":"2026-07-05T02:39:16.853313+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2103.10112","created_at":"2026-07-05T02:39:16.853313+00:00"},{"alias_kind":"pith_short_12","alias_value":"THZMDTPKXZUY","created_at":"2026-07-05T02:39:16.853313+00:00"},{"alias_kind":"pith_short_16","alias_value":"THZMDTPKXZUYXMKT","created_at":"2026-07-05T02:39:16.853313+00:00"},{"alias_kind":"pith_short_8","alias_value":"THZMDTPK","created_at":"2026-07-05T02:39:16.853313+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/THZMDTPKXZUYXMKTL3PC2BDSLM","json":"https://pith.science/pith/THZMDTPKXZUYXMKTL3PC2BDSLM.json","graph_json":"https://pith.science/api/pith-number/THZMDTPKXZUYXMKTL3PC2BDSLM/graph.json","events_json":"https://pith.science/api/pith-number/THZMDTPKXZUYXMKTL3PC2BDSLM/events.json","paper":"https://pith.science/paper/THZMDTPK"},"agent_actions":{"view_html":"https://pith.science/pith/THZMDTPKXZUYXMKTL3PC2BDSLM","download_json":"https://pith.science/pith/THZMDTPKXZUYXMKTL3PC2BDSLM.json","view_paper":"https://pith.science/paper/THZMDTPK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2103.10112&json=true","fetch_graph":"https://pith.science/api/pith-number/THZMDTPKXZUYXMKTL3PC2BDSLM/graph.json","fetch_events":"https://pith.science/api/pith-number/THZMDTPKXZUYXMKTL3PC2BDSLM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/THZMDTPKXZUYXMKTL3PC2BDSLM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/THZMDTPKXZUYXMKTL3PC2BDSLM/action/storage_attestation","attest_author":"https://pith.science/pith/THZMDTPKXZUYXMKTL3PC2BDSLM/action/author_attestation","sign_citation":"https://pith.science/pith/THZMDTPKXZUYXMKTL3PC2BDSLM/action/citation_signature","submit_replication":"https://pith.science/pith/THZMDTPKXZUYXMKTL3PC2BDSLM/action/replication_record"}},"created_at":"2026-07-05T02:39:16.853313+00:00","updated_at":"2026-07-05T02:39:16.853313+00:00"}