{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:GAKDG72ZSYOSX7LLOJYNX6LNYL","short_pith_number":"pith:GAKDG72Z","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"},"canonical_sha256":"3014337f59961d2bfd6b7270dbf96dc2dabf51de0267aecbf2ead8921b31f143","source":{"kind":"arxiv","id":"1610.07139","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1610.07139","created_at":"2026-05-18T00:55:06Z"},{"alias_kind":"arxiv_version","alias_value":"1610.07139v1","created_at":"2026-05-18T00:55:06Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.07139","created_at":"2026-05-18T00:55:06Z"},{"alias_kind":"pith_short_12","alias_value":"GAKDG72ZSYOS","created_at":"2026-05-18T12:30:15Z"},{"alias_kind":"pith_short_16","alias_value":"GAKDG72ZSYOSX7LL","created_at":"2026-05-18T12:30:15Z"},{"alias_kind":"pith_short_8","alias_value":"GAKDG72Z","created_at":"2026-05-18T12:30:15Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:GAKDG72ZSYOSX7LLOJYNX6LNYL","target":"record","payload":{"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"},"canonical_sha256":"3014337f59961d2bfd6b7270dbf96dc2dabf51de0267aecbf2ead8921b31f143","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"},"source_kind":"arxiv","source_id":"1610.07139","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:55:06Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"xuiGiJm01rD77pf4wZTYO3TdfM7yJi9OKDkQgrEGk8M8W+yV26JB12U5tcTJJNU8vgjapdm5+0HmGEItOZD2AA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T17:40:30.128240Z"},"content_sha256":"b044f7d5616684153ed5dc0a280b93b006abcc876803ba2e105491027f23e208","schema_version":"1.0","event_id":"sha256:b044f7d5616684153ed5dc0a280b93b006abcc876803ba2e105491027f23e208"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:GAKDG72ZSYOSX7LLOJYNX6LNYL","target":"graph","payload":{"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:55:06Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"v54KyBjkz09D91oJRDi/APKu0s/CbM4/p/4KYtUDF1l2xdAqqTQGnWbTNdiGHJ0BIcNRPTEs+M7rf3sireu5Dg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T17:40:30.128956Z"},"content_sha256":"66a327359e1c4b4eb9f77e209eede46f308a8d2e2f2d025a649d154beb7a15f1","schema_version":"1.0","event_id":"sha256:66a327359e1c4b4eb9f77e209eede46f308a8d2e2f2d025a649d154beb7a15f1"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL/bundle.json","state_url":"https://pith.science/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-25T17:40:30Z","links":{"resolver":"https://pith.science/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL","bundle":"https://pith.science/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL/bundle.json","state":"https://pith.science/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL/state.json","well_known_bundle":"https://pith.science/.well-known/pith/GAKDG72ZSYOSX7LLOJYNX6LNYL/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:GAKDG72ZSYOSX7LLOJYNX6LNYL","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"021032e525859e8fba419bdae652f97315f9d47b40ce59730783ce382d6890fb","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-23T10:16:28Z","title_canon_sha256":"4396cbe87e0a6972e4c9b09561c5746678073e576ff6217d1591007dea37e205"},"schema_version":"1.0","source":{"id":"1610.07139","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1610.07139","created_at":"2026-05-18T00:55:06Z"},{"alias_kind":"arxiv_version","alias_value":"1610.07139v1","created_at":"2026-05-18T00:55:06Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.07139","created_at":"2026-05-18T00:55:06Z"},{"alias_kind":"pith_short_12","alias_value":"GAKDG72ZSYOS","created_at":"2026-05-18T12:30:15Z"},{"alias_kind":"pith_short_16","alias_value":"GAKDG72ZSYOSX7LL","created_at":"2026-05-18T12:30:15Z"},{"alias_kind":"pith_short_8","alias_value":"GAKDG72Z","created_at":"2026-05-18T12:30:15Z"}],"graph_snapshots":[{"event_id":"sha256:66a327359e1c4b4eb9f77e209eede46f308a8d2e2f2d025a649d154beb7a15f1","target":"graph","created_at":"2026-05-18T00:55:06Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"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","authors_text":"Dae-Sub Lee, Hee-Won Lee, Jeong-Eun Heo, Seok-Jun Chang, Young-Min Lee","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-23T10:16:28Z","title":"A Monte Carlo Study of Flux Ratios of Raman Scattered O~VI Features at 6825 \\AA\\ and 7082 \\AA\\ in Symbiotic Stars"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.07139","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:b044f7d5616684153ed5dc0a280b93b006abcc876803ba2e105491027f23e208","target":"record","created_at":"2026-05-18T00:55:06Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"021032e525859e8fba419bdae652f97315f9d47b40ce59730783ce382d6890fb","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-23T10:16:28Z","title_canon_sha256":"4396cbe87e0a6972e4c9b09561c5746678073e576ff6217d1591007dea37e205"},"schema_version":"1.0","source":{"id":"1610.07139","kind":"arxiv","version":1}},"canonical_sha256":"3014337f59961d2bfd6b7270dbf96dc2dabf51de0267aecbf2ead8921b31f143","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"3014337f59961d2bfd6b7270dbf96dc2dabf51de0267aecbf2ead8921b31f143","first_computed_at":"2026-05-18T00:55:06.820622Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:55:06.820622Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"2mwzqRugcX6tszKUqwXncvBn0w5LMz4MPNAHWEv06H0qHF1SiDagAqoD13IFrH4rjVv5dvPuQHhthQg33CXkDA==","signature_status":"signed_v1","signed_at":"2026-05-18T00:55:06.821326Z","signed_message":"canonical_sha256_bytes"},"source_id":"1610.07139","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:b044f7d5616684153ed5dc0a280b93b006abcc876803ba2e105491027f23e208","sha256:66a327359e1c4b4eb9f77e209eede46f308a8d2e2f2d025a649d154beb7a15f1"],"state_sha256":"e6f41c5d2478c890d3a523adc42288a48a0c58e4583441a5c54736e2236a8d61"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"zg6CMsgGc7PfEsDRyljJytH46JfluAVqa7l9Ld2jy6Q/Sq3o1N5Y58ta4ZGKLbUxZULnBTLs0ItCHZrNrLkdDQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T17:40:30.132720Z","bundle_sha256":"0e58cfa5c15a130b3356eab460e0ef8161f4223d454732bb463947342b550625"}}