{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:OUOSZM6XIEOBPZK56KB5LNAFK7","short_pith_number":"pith:OUOSZM6X","schema_version":"1.0","canonical_sha256":"751d2cb3d7411c17e55df283d5b40557cc2b31a835523850bee7e0c09784dad9","source":{"kind":"arxiv","id":"2011.02049","version":1},"attestation_state":"computed","paper":{"title":"Atomic data for the Gaia-ESO Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.IM","authors_text":"Alessandro Lanzafame, Amelia Bayo Ar\\'an, Andreas J. Korn, Andrew R. Casey, Bengt Edvardsson, Carmela Lardo, Clare Worley, Elena Pancino, Francesco Damiani, Gerard F. Gilmore, Henrik J\\\"onsson, Juliet C. Pickering, Karin Lind, Laura Magrini, Lorenzo Monaco, Lorenzo Morbidelli, Maria Bergemann, Martin Asplund, Nils Ryde, Patrick de Laverny, Paula Jofr\\'e, Paul S. Barklem, Rodolfo Smiljanic, Simone Zaggia, Sofia Feltzing, Sofia Randich, Thomas Bensby, Thomas Masseron, Ulrike Heiter, \\v{S}arunas Mikolaitis","submitted_at":"2020-11-03T22:51:36Z","abstract_excerpt":"We describe the atomic and molecular data that were used for the abundance analyses of FGK-type stars carried out within the Gaia-ESO Survey. We present an unprecedented effort to create a homogeneous line list, which was used by several abundance analysis groups to calculate synthetic spectra and equivalent widths. The atomic data are accompanied by quality indicators and detailed references to the sources. The atomic and molecular data are made publicly available in electronic form. In general experimental transition probabilities were preferred but theoretical values were also used. Astroph"},"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":"2011.02049","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2020-11-03T22:51:36Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"2b9f383c9d17d13a44b8d59906a3d9dda084a0877f289ea6c4ef5d5ab61f8c03","abstract_canon_sha256":"a5bac81205f1e92ba7ef499bdf2a48ab05c003e038509f70abc15a4b0482688b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:09:49.958779Z","signature_b64":"RD7eTwhwaL2DKDy/dAYnqAlAbbEzwfOT0tDphSAqM6TxJ9BILwBrz+yD5rfxugLd+UT8qGfkXps6Tsb7dvM/Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"751d2cb3d7411c17e55df283d5b40557cc2b31a835523850bee7e0c09784dad9","last_reissued_at":"2026-07-05T02:09:49.958334Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:09:49.958334Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Atomic data for the Gaia-ESO Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.IM","authors_text":"Alessandro Lanzafame, Amelia Bayo Ar\\'an, Andreas J. Korn, Andrew R. Casey, Bengt Edvardsson, Carmela Lardo, Clare Worley, Elena Pancino, Francesco Damiani, Gerard F. Gilmore, Henrik J\\\"onsson, Juliet C. Pickering, Karin Lind, Laura Magrini, Lorenzo Monaco, Lorenzo Morbidelli, Maria Bergemann, Martin Asplund, Nils Ryde, Patrick de Laverny, Paula Jofr\\'e, Paul S. Barklem, Rodolfo Smiljanic, Simone Zaggia, Sofia Feltzing, Sofia Randich, Thomas Bensby, Thomas Masseron, Ulrike Heiter, \\v{S}arunas Mikolaitis","submitted_at":"2020-11-03T22:51:36Z","abstract_excerpt":"We describe the atomic and molecular data that were used for the abundance analyses of FGK-type stars carried out within the Gaia-ESO Survey. We present an unprecedented effort to create a homogeneous line list, which was used by several abundance analysis groups to calculate synthetic spectra and equivalent widths. The atomic data are accompanied by quality indicators and detailed references to the sources. The atomic and molecular data are made publicly available in electronic form. In general experimental transition probabilities were preferred but theoretical values were also used. Astroph"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2011.02049","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/2011.02049/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":"2011.02049","created_at":"2026-07-05T02:09:49.958391+00:00"},{"alias_kind":"arxiv_version","alias_value":"2011.02049v1","created_at":"2026-07-05T02:09:49.958391+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2011.02049","created_at":"2026-07-05T02:09:49.958391+00:00"},{"alias_kind":"pith_short_12","alias_value":"OUOSZM6XIEOB","created_at":"2026-07-05T02:09:49.958391+00:00"},{"alias_kind":"pith_short_16","alias_value":"OUOSZM6XIEOBPZK5","created_at":"2026-07-05T02:09:49.958391+00:00"},{"alias_kind":"pith_short_8","alias_value":"OUOSZM6X","created_at":"2026-07-05T02:09:49.958391+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.09851","citing_title":"Benchmark Brown Dwarf Systems I: Chemical Abundance Analysis of FGK Stars with Wide-Separation Brown Dwarf Companions Using PEPSI","ref_index":250,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OUOSZM6XIEOBPZK56KB5LNAFK7","json":"https://pith.science/pith/OUOSZM6XIEOBPZK56KB5LNAFK7.json","graph_json":"https://pith.science/api/pith-number/OUOSZM6XIEOBPZK56KB5LNAFK7/graph.json","events_json":"https://pith.science/api/pith-number/OUOSZM6XIEOBPZK56KB5LNAFK7/events.json","paper":"https://pith.science/paper/OUOSZM6X"},"agent_actions":{"view_html":"https://pith.science/pith/OUOSZM6XIEOBPZK56KB5LNAFK7","download_json":"https://pith.science/pith/OUOSZM6XIEOBPZK56KB5LNAFK7.json","view_paper":"https://pith.science/paper/OUOSZM6X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2011.02049&json=true","fetch_graph":"https://pith.science/api/pith-number/OUOSZM6XIEOBPZK56KB5LNAFK7/graph.json","fetch_events":"https://pith.science/api/pith-number/OUOSZM6XIEOBPZK56KB5LNAFK7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OUOSZM6XIEOBPZK56KB5LNAFK7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OUOSZM6XIEOBPZK56KB5LNAFK7/action/storage_attestation","attest_author":"https://pith.science/pith/OUOSZM6XIEOBPZK56KB5LNAFK7/action/author_attestation","sign_citation":"https://pith.science/pith/OUOSZM6XIEOBPZK56KB5LNAFK7/action/citation_signature","submit_replication":"https://pith.science/pith/OUOSZM6XIEOBPZK56KB5LNAFK7/action/replication_record"}},"created_at":"2026-07-05T02:09:49.958391+00:00","updated_at":"2026-07-05T02:09:49.958391+00:00"}