{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:GAKDG72ZSYOSX7LLOJYNX6LNYL","short_pith_number":"pith:GAKDG72Z","schema_version":"1.0","canonical_sha256":"3014337f59961d2bfd6b7270dbf96dc2dabf51de0267aecbf2ead8921b31f143","source":{"kind":"arxiv","id":"1610.07139","version":1},"attestation_state":"computed","paper":{"title":"A Monte Carlo Study of Flux Ratios of Raman Scattered O~VI Features at 6825 \\AA\\ and 7082 \\AA\\ in Symbiotic Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Dae-Sub Lee, Hee-Won Lee, Jeong-Eun Heo, Seok-Jun Chang, Young-Min Lee","submitted_at":"2016-10-23T10:16:28Z","abstract_excerpt":"Symbiotic stars are regarded as wide binary systems consisting of a hot white dwarf and a mass losing giant. They exhibit unique spectral features at 6825 \\AA\\ and 7082 \\AA, which are formed via Raman scattering of \\ion{O}{6}$\\lambda\\lambda$ 1032 and 1038 with atomic hydrogen. We adopt a Monte Carlo technique to generate the same number of \\ion{O}{6}$\\lambda$1032 and $\\lambda$1038 line photons and compute the flux ratio $F(6825)/F(7082)$ of these Raman scattered \\ion{O}{6} features formed in neutral regions with a simple geometric shape as a function of \\ion{H}{1} column density $N_{HI}$. In c"},"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":"1610.07139","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-23T10:16:28Z","cross_cats_sorted":[],"title_canon_sha256":"4396cbe87e0a6972e4c9b09561c5746678073e576ff6217d1591007dea37e205","abstract_canon_sha256":"021032e525859e8fba419bdae652f97315f9d47b40ce59730783ce382d6890fb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:55:06.821326Z","signature_b64":"2mwzqRugcX6tszKUqwXncvBn0w5LMz4MPNAHWEv06H0qHF1SiDagAqoD13IFrH4rjVv5dvPuQHhthQg33CXkDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3014337f59961d2bfd6b7270dbf96dc2dabf51de0267aecbf2ead8921b31f143","last_reissued_at":"2026-05-18T00:55:06.820622Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:55:06.820622Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Monte Carlo Study of Flux Ratios of Raman Scattered O~VI Features at 6825 \\AA\\ and 7082 \\AA\\ in Symbiotic Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Dae-Sub Lee, Hee-Won Lee, Jeong-Eun Heo, Seok-Jun Chang, Young-Min Lee","submitted_at":"2016-10-23T10:16:28Z","abstract_excerpt":"Symbiotic stars are regarded as wide binary systems consisting of a hot white dwarf and a mass losing giant. They exhibit unique spectral features at 6825 \\AA\\ and 7082 \\AA, which are formed via Raman scattering of \\ion{O}{6}$\\lambda\\lambda$ 1032 and 1038 with atomic hydrogen. We adopt a Monte Carlo technique to generate the same number of \\ion{O}{6}$\\lambda$1032 and $\\lambda$1038 line photons and compute the flux ratio $F(6825)/F(7082)$ of these Raman scattered \\ion{O}{6} features formed in neutral regions with a simple geometric shape as a function of \\ion{H}{1} column density $N_{HI}$. In c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.07139","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":"1610.07139","created_at":"2026-05-18T00:55:06.820730+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.07139v1","created_at":"2026-05-18T00:55:06.820730+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.07139","created_at":"2026-05-18T00:55:06.820730+00:00"},{"alias_kind":"pith_short_12","alias_value":"GAKDG72ZSYOS","created_at":"2026-05-18T12:30:15.759754+00:00"},{"alias_kind":"pith_short_16","alias_value":"GAKDG72ZSYOSX7LL","created_at":"2026-05-18T12:30:15.759754+00:00"},{"alias_kind":"pith_short_8","alias_value":"GAKDG72Z","created_at":"2026-05-18T12:30:15.759754+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/GAKDG72ZSYOSX7LLOJYNX6LNYL","json":"https://pith.science/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL.json","graph_json":"https://pith.science/api/pith-number/GAKDG72ZSYOSX7LLOJYNX6LNYL/graph.json","events_json":"https://pith.science/api/pith-number/GAKDG72ZSYOSX7LLOJYNX6LNYL/events.json","paper":"https://pith.science/paper/GAKDG72Z"},"agent_actions":{"view_html":"https://pith.science/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL","download_json":"https://pith.science/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL.json","view_paper":"https://pith.science/paper/GAKDG72Z","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.07139&json=true","fetch_graph":"https://pith.science/api/pith-number/GAKDG72ZSYOSX7LLOJYNX6LNYL/graph.json","fetch_events":"https://pith.science/api/pith-number/GAKDG72ZSYOSX7LLOJYNX6LNYL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL/action/storage_attestation","attest_author":"https://pith.science/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL/action/author_attestation","sign_citation":"https://pith.science/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL/action/citation_signature","submit_replication":"https://pith.science/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL/action/replication_record"}},"created_at":"2026-05-18T00:55:06.820730+00:00","updated_at":"2026-05-18T00:55:06.820730+00:00"}