{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:CV5GDUD63VAJBGWLRYLD2OZFHJ","short_pith_number":"pith:CV5GDUD6","schema_version":"1.0","canonical_sha256":"157a61d07edd40909acb8e163d3b253a77efff70ea3ee3fa5ed566d2e633ca85","source":{"kind":"arxiv","id":"1510.08273","version":1},"attestation_state":"computed","paper":{"title":"NIR spectroscopy of the Sun and HD20010 - Compiling a new linelist in the NIR","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"B. Rojas-Ayala, D. T. Andreasen, E. Delgado Mena, M. Tsantaki, N. C. Santos, S. G. Sousa, V. Neves","submitted_at":"2015-10-28T11:58:58Z","abstract_excerpt":"Context: Effective temperature, surface gravity, and metallicity are basic spectroscopic stellar parameters necessary to characterize a star or a planetary system. Reliable atmospheric parameters for FGK stars have been obtained mostly from methods that relay on high resolution and high signal-to-noise optical spectroscopy. The advent of a new generation of high resolution near-IR spectrographs opens the possibility of using classic spectroscopic methods with high resolution and high signal-to-noise in the NIR spectral window. Aims: We aim to compile a new iron line list in the NIR from a sola"},"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":"1510.08273","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-10-28T11:58:58Z","cross_cats_sorted":[],"title_canon_sha256":"3391f0463f9ddee2133873e5edb08539f3235ea707334577dcc39ba80346e2b4","abstract_canon_sha256":"4fad8eeec9bebf0cef61393e35ec542bc62ee0021c4bea2e8cce9ddc45d6b4d7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:22:58.381241Z","signature_b64":"gVXpRxEEtfsog1qLbe1iBnMFB8OQop23/NXJ8CsFrYZ9EAsYACpf1Vzyo57dsWQpHIO83MH3oLCzGWIt6NQyCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"157a61d07edd40909acb8e163d3b253a77efff70ea3ee3fa5ed566d2e633ca85","last_reissued_at":"2026-05-18T01:22:58.380597Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:22:58.380597Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"NIR spectroscopy of the Sun and HD20010 - Compiling a new linelist in the NIR","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"B. Rojas-Ayala, D. T. Andreasen, E. Delgado Mena, M. Tsantaki, N. C. Santos, S. G. Sousa, V. Neves","submitted_at":"2015-10-28T11:58:58Z","abstract_excerpt":"Context: Effective temperature, surface gravity, and metallicity are basic spectroscopic stellar parameters necessary to characterize a star or a planetary system. Reliable atmospheric parameters for FGK stars have been obtained mostly from methods that relay on high resolution and high signal-to-noise optical spectroscopy. The advent of a new generation of high resolution near-IR spectrographs opens the possibility of using classic spectroscopic methods with high resolution and high signal-to-noise in the NIR spectral window. Aims: We aim to compile a new iron line list in the NIR from a sola"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.08273","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":"1510.08273","created_at":"2026-05-18T01:22:58.380683+00:00"},{"alias_kind":"arxiv_version","alias_value":"1510.08273v1","created_at":"2026-05-18T01:22:58.380683+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.08273","created_at":"2026-05-18T01:22:58.380683+00:00"},{"alias_kind":"pith_short_12","alias_value":"CV5GDUD63VAJ","created_at":"2026-05-18T12:29:17.054201+00:00"},{"alias_kind":"pith_short_16","alias_value":"CV5GDUD63VAJBGWL","created_at":"2026-05-18T12:29:17.054201+00:00"},{"alias_kind":"pith_short_8","alias_value":"CV5GDUD6","created_at":"2026-05-18T12:29:17.054201+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/CV5GDUD63VAJBGWLRYLD2OZFHJ","json":"https://pith.science/pith/CV5GDUD63VAJBGWLRYLD2OZFHJ.json","graph_json":"https://pith.science/api/pith-number/CV5GDUD63VAJBGWLRYLD2OZFHJ/graph.json","events_json":"https://pith.science/api/pith-number/CV5GDUD63VAJBGWLRYLD2OZFHJ/events.json","paper":"https://pith.science/paper/CV5GDUD6"},"agent_actions":{"view_html":"https://pith.science/pith/CV5GDUD63VAJBGWLRYLD2OZFHJ","download_json":"https://pith.science/pith/CV5GDUD63VAJBGWLRYLD2OZFHJ.json","view_paper":"https://pith.science/paper/CV5GDUD6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1510.08273&json=true","fetch_graph":"https://pith.science/api/pith-number/CV5GDUD63VAJBGWLRYLD2OZFHJ/graph.json","fetch_events":"https://pith.science/api/pith-number/CV5GDUD63VAJBGWLRYLD2OZFHJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CV5GDUD63VAJBGWLRYLD2OZFHJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CV5GDUD63VAJBGWLRYLD2OZFHJ/action/storage_attestation","attest_author":"https://pith.science/pith/CV5GDUD63VAJBGWLRYLD2OZFHJ/action/author_attestation","sign_citation":"https://pith.science/pith/CV5GDUD63VAJBGWLRYLD2OZFHJ/action/citation_signature","submit_replication":"https://pith.science/pith/CV5GDUD63VAJBGWLRYLD2OZFHJ/action/replication_record"}},"created_at":"2026-05-18T01:22:58.380683+00:00","updated_at":"2026-05-18T01:22:58.380683+00:00"}