{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:4B3HOIW5PNCMYGMVQEL6RXMKGF","short_pith_number":"pith:4B3HOIW5","schema_version":"1.0","canonical_sha256":"e0767722dd7b44cc19958117e8dd8a316d7624f353c886044fc24db775389e15","source":{"kind":"arxiv","id":"2409.04910","version":1},"attestation_state":"computed","paper":{"title":"Spectral energy distribution of late stage stars","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"A. M. Tatarnikov, E. D. Malik, S. G. Zheltoukhov","submitted_at":"2024-09-07T21:10:32Z","abstract_excerpt":"This paper presents a catalog of the energy distribution in the spectra of 263 stars in the wavelength range from 0.4 to 100 {\\mu}m, which are at late stages of evolution and have been observed by the ISO space observatory. For each object in the catalog, estimates of the observed bolometric fluxes were derived from smoothed energy distribution curves. The catalog is available at https://infra.sai.msu.ru/sai\\_lss\\_sed both as a table and in machine-readable format. It is shown that for the specified sample of objects their ISO SWS spectra in the range 2.4-45 {\\mu}m only 60% of cases correspond"},"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":"2409.04910","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2024-09-07T21:10:32Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"b5dfbc039c0911b74fa223e484950041d4457e1d1e9f89e70b3731a4f32be58b","abstract_canon_sha256":"e8a2763592da35ebcc892beffc8a2f7d717b368f110666e85afdbc0e375cdacb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:04:41.747053Z","signature_b64":"EBTbvrlgelVQciLEdQUshGF+GbD74h2BXVnKqeMACgkyP5IeRJpSA+BAXmIrvzvHg5tJDSD6RZQ/1Wjn7rW8BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e0767722dd7b44cc19958117e8dd8a316d7624f353c886044fc24db775389e15","last_reissued_at":"2026-07-05T09:04:41.746607Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:04:41.746607Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spectral energy distribution of late stage stars","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"A. M. Tatarnikov, E. D. Malik, S. G. Zheltoukhov","submitted_at":"2024-09-07T21:10:32Z","abstract_excerpt":"This paper presents a catalog of the energy distribution in the spectra of 263 stars in the wavelength range from 0.4 to 100 {\\mu}m, which are at late stages of evolution and have been observed by the ISO space observatory. For each object in the catalog, estimates of the observed bolometric fluxes were derived from smoothed energy distribution curves. The catalog is available at https://infra.sai.msu.ru/sai\\_lss\\_sed both as a table and in machine-readable format. It is shown that for the specified sample of objects their ISO SWS spectra in the range 2.4-45 {\\mu}m only 60% of cases correspond"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2409.04910","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/2409.04910/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":"2409.04910","created_at":"2026-07-05T09:04:41.746680+00:00"},{"alias_kind":"arxiv_version","alias_value":"2409.04910v1","created_at":"2026-07-05T09:04:41.746680+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2409.04910","created_at":"2026-07-05T09:04:41.746680+00:00"},{"alias_kind":"pith_short_12","alias_value":"4B3HOIW5PNCM","created_at":"2026-07-05T09:04:41.746680+00:00"},{"alias_kind":"pith_short_16","alias_value":"4B3HOIW5PNCMYGMV","created_at":"2026-07-05T09:04:41.746680+00:00"},{"alias_kind":"pith_short_8","alias_value":"4B3HOIW5","created_at":"2026-07-05T09:04:41.746680+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/4B3HOIW5PNCMYGMVQEL6RXMKGF","json":"https://pith.science/pith/4B3HOIW5PNCMYGMVQEL6RXMKGF.json","graph_json":"https://pith.science/api/pith-number/4B3HOIW5PNCMYGMVQEL6RXMKGF/graph.json","events_json":"https://pith.science/api/pith-number/4B3HOIW5PNCMYGMVQEL6RXMKGF/events.json","paper":"https://pith.science/paper/4B3HOIW5"},"agent_actions":{"view_html":"https://pith.science/pith/4B3HOIW5PNCMYGMVQEL6RXMKGF","download_json":"https://pith.science/pith/4B3HOIW5PNCMYGMVQEL6RXMKGF.json","view_paper":"https://pith.science/paper/4B3HOIW5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2409.04910&json=true","fetch_graph":"https://pith.science/api/pith-number/4B3HOIW5PNCMYGMVQEL6RXMKGF/graph.json","fetch_events":"https://pith.science/api/pith-number/4B3HOIW5PNCMYGMVQEL6RXMKGF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4B3HOIW5PNCMYGMVQEL6RXMKGF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4B3HOIW5PNCMYGMVQEL6RXMKGF/action/storage_attestation","attest_author":"https://pith.science/pith/4B3HOIW5PNCMYGMVQEL6RXMKGF/action/author_attestation","sign_citation":"https://pith.science/pith/4B3HOIW5PNCMYGMVQEL6RXMKGF/action/citation_signature","submit_replication":"https://pith.science/pith/4B3HOIW5PNCMYGMVQEL6RXMKGF/action/replication_record"}},"created_at":"2026-07-05T09:04:41.746680+00:00","updated_at":"2026-07-05T09:04:41.746680+00:00"}