{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:R4TZFD3N2MRA2355EIUVXY3FG4","short_pith_number":"pith:R4TZFD3N","schema_version":"1.0","canonical_sha256":"8f27928f6dd3220d6fbd22295be36537259f36a097790cc2febb81ac326450e7","source":{"kind":"arxiv","id":"astro-ph/0605029","version":1},"attestation_state":"computed","paper":{"title":"High Resolution Irradiance Spectrum from 300 to 1000 nm","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Robert L. Kurucz (Harvard-Smithsonian Center for Astrophysics)","submitted_at":"2006-05-01T16:02:06Z","abstract_excerpt":"The FTS scans that made up the Kitt Peak Solar Flux Atlas by Kurucz, Furenlid, Brault, and Testerman (1984) have been re-reduced. An approximate telluric atmospheric model was determined for each FTS scan. Large-scale features produced by O3 and O2 dimer were computed and divided out. The solar continuum level was found by fitting a smooth curve to high points in each scan. The scans were normalized to the fitted continuum to produce a residual flux spectrum for each FTS scan. The telluric line spectrum was computed using HITRAN and other line data for H2O, O2, and CO2. The line parameters wer"},"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":"astro-ph/0605029","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-05-01T16:02:06Z","cross_cats_sorted":[],"title_canon_sha256":"3b35065975e555664abe4d00538dd0c09d94d86748014246dd4511f936d84ed6","abstract_canon_sha256":"c81810a7380c816c157e348d706b2be8cfe05610e2a802e0338513f2ab6ae5c3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T14:54:18.384713Z","signature_b64":"cHXW7OkwEmWuOfu91aNTMlMLkkJRlN47beA+2ds7VJbduXrurO9qOPyKD3ADQ7ZqQVjj9E0kBDG2ulWO/aGtDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8f27928f6dd3220d6fbd22295be36537259f36a097790cc2febb81ac326450e7","last_reissued_at":"2026-07-04T14:54:18.384344Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T14:54:18.384344Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High Resolution Irradiance Spectrum from 300 to 1000 nm","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Robert L. Kurucz (Harvard-Smithsonian Center for Astrophysics)","submitted_at":"2006-05-01T16:02:06Z","abstract_excerpt":"The FTS scans that made up the Kitt Peak Solar Flux Atlas by Kurucz, Furenlid, Brault, and Testerman (1984) have been re-reduced. An approximate telluric atmospheric model was determined for each FTS scan. Large-scale features produced by O3 and O2 dimer were computed and divided out. The solar continuum level was found by fitting a smooth curve to high points in each scan. The scans were normalized to the fitted continuum to produce a residual flux spectrum for each FTS scan. The telluric line spectrum was computed using HITRAN and other line data for H2O, O2, and CO2. The line parameters wer"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0605029","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/astro-ph/0605029/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":"astro-ph/0605029","created_at":"2026-07-04T14:54:18.384409+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0605029v1","created_at":"2026-07-04T14:54:18.384409+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0605029","created_at":"2026-07-04T14:54:18.384409+00:00"},{"alias_kind":"pith_short_12","alias_value":"R4TZFD3N2MRA","created_at":"2026-07-04T14:54:18.384409+00:00"},{"alias_kind":"pith_short_16","alias_value":"R4TZFD3N2MRA2355","created_at":"2026-07-04T14:54:18.384409+00:00"},{"alias_kind":"pith_short_8","alias_value":"R4TZFD3N","created_at":"2026-07-04T14:54:18.384409+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.10250","citing_title":"High Resolution Optical Methane Linelist from observations of Titan for Cross-Correlation studies","ref_index":24,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/R4TZFD3N2MRA2355EIUVXY3FG4","json":"https://pith.science/pith/R4TZFD3N2MRA2355EIUVXY3FG4.json","graph_json":"https://pith.science/api/pith-number/R4TZFD3N2MRA2355EIUVXY3FG4/graph.json","events_json":"https://pith.science/api/pith-number/R4TZFD3N2MRA2355EIUVXY3FG4/events.json","paper":"https://pith.science/paper/R4TZFD3N"},"agent_actions":{"view_html":"https://pith.science/pith/R4TZFD3N2MRA2355EIUVXY3FG4","download_json":"https://pith.science/pith/R4TZFD3N2MRA2355EIUVXY3FG4.json","view_paper":"https://pith.science/paper/R4TZFD3N","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0605029&json=true","fetch_graph":"https://pith.science/api/pith-number/R4TZFD3N2MRA2355EIUVXY3FG4/graph.json","fetch_events":"https://pith.science/api/pith-number/R4TZFD3N2MRA2355EIUVXY3FG4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R4TZFD3N2MRA2355EIUVXY3FG4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R4TZFD3N2MRA2355EIUVXY3FG4/action/storage_attestation","attest_author":"https://pith.science/pith/R4TZFD3N2MRA2355EIUVXY3FG4/action/author_attestation","sign_citation":"https://pith.science/pith/R4TZFD3N2MRA2355EIUVXY3FG4/action/citation_signature","submit_replication":"https://pith.science/pith/R4TZFD3N2MRA2355EIUVXY3FG4/action/replication_record"}},"created_at":"2026-07-04T14:54:18.384409+00:00","updated_at":"2026-07-04T14:54:18.384409+00:00"}