{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2012:ZJVLA5AYF3TO64SOD5WSWJE3XM","short_pith_number":"pith:ZJVLA5AY","canonical_record":{"source":{"id":"1203.4307","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-03-20T01:54:40Z","cross_cats_sorted":[],"title_canon_sha256":"f7a25b72589b024687a605dd1de0d975ea84d5f9408b6508bcbe0100e3b4c6d1","abstract_canon_sha256":"371adaecc0a5aa1f28efb45f2ae20596de71a6562156819fe165aee8c9bd792f"},"schema_version":"1.0"},"canonical_sha256":"ca6ab074182ee6ef724e1f6d2b249bbb1b80a4cdda17ebb3c6030077170d0d41","source":{"kind":"arxiv","id":"1203.4307","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1203.4307","created_at":"2026-05-18T01:58:05Z"},{"alias_kind":"arxiv_version","alias_value":"1203.4307v1","created_at":"2026-05-18T01:58:05Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1203.4307","created_at":"2026-05-18T01:58:05Z"},{"alias_kind":"pith_short_12","alias_value":"ZJVLA5AYF3TO","created_at":"2026-05-18T12:27:30Z"},{"alias_kind":"pith_short_16","alias_value":"ZJVLA5AYF3TO64SO","created_at":"2026-05-18T12:27:30Z"},{"alias_kind":"pith_short_8","alias_value":"ZJVLA5AY","created_at":"2026-05-18T12:27:30Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2012:ZJVLA5AYF3TO64SOD5WSWJE3XM","target":"record","payload":{"canonical_record":{"source":{"id":"1203.4307","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-03-20T01:54:40Z","cross_cats_sorted":[],"title_canon_sha256":"f7a25b72589b024687a605dd1de0d975ea84d5f9408b6508bcbe0100e3b4c6d1","abstract_canon_sha256":"371adaecc0a5aa1f28efb45f2ae20596de71a6562156819fe165aee8c9bd792f"},"schema_version":"1.0"},"canonical_sha256":"ca6ab074182ee6ef724e1f6d2b249bbb1b80a4cdda17ebb3c6030077170d0d41","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:05.755163Z","signature_b64":"VhpKA0fbBMeDVzTBHiVVWzfioyp6K8/1lld7ii1IYde/8SvDhw5Ju8K8Zu0uPwGzGBQ1halAp7QBl5x3DEnCDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ca6ab074182ee6ef724e1f6d2b249bbb1b80a4cdda17ebb3c6030077170d0d41","last_reissued_at":"2026-05-18T01:58:05.754720Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:05.754720Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1203.4307","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":"2026-05-18T01:58:05Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"MqnREP3UrjxZqhR3GyKec6GdB8UsABgCu5IUClXtr+1XPsv6Ukb/XNVGLGUMQWVPVMO5WqE7/bx8p6hl5k0iCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-03T12:41:38.222805Z"},"content_sha256":"b9fbc8f7fdf3ec6afc2fdbf5e6fb5c0e2de988b813fb0045288153aa5195c6bf","schema_version":"1.0","event_id":"sha256:b9fbc8f7fdf3ec6afc2fdbf5e6fb5c0e2de988b813fb0045288153aa5195c6bf"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2012:ZJVLA5AYF3TO64SOD5WSWJE3XM","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Spectroscopic Pulsational Frequency Identification and Mode Determination of Gamma Doradus Star HD135825","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"D. J. Wright, E. Brunsden, K. R. Pollard, P. De Cat, P. L. Cottrell, P. M. Kilmartin","submitted_at":"2012-03-20T01:54:40Z","abstract_excerpt":"We present the mode identification of frequencies found in spectroscopic observations of the Gamma Doradus star HD135825. Four frequencies were successfully identified: 1.3150 +/- 0.0003 1/d; 0.2902 +/- 0.0004 1/d; 1.4045 +/- 0.0005 1/d; and 1.8829 +/- 0.0005 1/d. These correspond to (l, m) modes of (1,1), (2,-2), (4,0) and (1,1) respectively. Additional frequencies were found but they were below the signal-to-noise limit of the Fourier spectrum and not suitable for mode identification. The rotational axis inclination and vsini of the star were determined to be 87 degrees (nearly edge-on) and "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.4307","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":"2026-05-18T01:58:05Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"QUNCu0e0KFgoyYICrQe/QQVMtENJZgHpUmLWzlOOrjlsVLDw46OlzyimyLGToPtBMJ0U9CcpvazSGuJyEzv9AQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-03T12:41:38.223157Z"},"content_sha256":"8a07745217d07ba01da2dadc77244e22c15665dd5597c6957a3babcc0996e1a2","schema_version":"1.0","event_id":"sha256:8a07745217d07ba01da2dadc77244e22c15665dd5597c6957a3babcc0996e1a2"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/ZJVLA5AYF3TO64SOD5WSWJE3XM/bundle.json","state_url":"https://pith.science/pith/ZJVLA5AYF3TO64SOD5WSWJE3XM/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/ZJVLA5AYF3TO64SOD5WSWJE3XM/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":"2026-06-03T12:41:38Z","links":{"resolver":"https://pith.science/pith/ZJVLA5AYF3TO64SOD5WSWJE3XM","bundle":"https://pith.science/pith/ZJVLA5AYF3TO64SOD5WSWJE3XM/bundle.json","state":"https://pith.science/pith/ZJVLA5AYF3TO64SOD5WSWJE3XM/state.json","well_known_bundle":"https://pith.science/.well-known/pith/ZJVLA5AYF3TO64SOD5WSWJE3XM/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2012:ZJVLA5AYF3TO64SOD5WSWJE3XM","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":"371adaecc0a5aa1f28efb45f2ae20596de71a6562156819fe165aee8c9bd792f","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-03-20T01:54:40Z","title_canon_sha256":"f7a25b72589b024687a605dd1de0d975ea84d5f9408b6508bcbe0100e3b4c6d1"},"schema_version":"1.0","source":{"id":"1203.4307","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1203.4307","created_at":"2026-05-18T01:58:05Z"},{"alias_kind":"arxiv_version","alias_value":"1203.4307v1","created_at":"2026-05-18T01:58:05Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1203.4307","created_at":"2026-05-18T01:58:05Z"},{"alias_kind":"pith_short_12","alias_value":"ZJVLA5AYF3TO","created_at":"2026-05-18T12:27:30Z"},{"alias_kind":"pith_short_16","alias_value":"ZJVLA5AYF3TO64SO","created_at":"2026-05-18T12:27:30Z"},{"alias_kind":"pith_short_8","alias_value":"ZJVLA5AY","created_at":"2026-05-18T12:27:30Z"}],"graph_snapshots":[{"event_id":"sha256:8a07745217d07ba01da2dadc77244e22c15665dd5597c6957a3babcc0996e1a2","target":"graph","created_at":"2026-05-18T01:58:05Z","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":"We present the mode identification of frequencies found in spectroscopic observations of the Gamma Doradus star HD135825. Four frequencies were successfully identified: 1.3150 +/- 0.0003 1/d; 0.2902 +/- 0.0004 1/d; 1.4045 +/- 0.0005 1/d; and 1.8829 +/- 0.0005 1/d. These correspond to (l, m) modes of (1,1), (2,-2), (4,0) and (1,1) respectively. Additional frequencies were found but they were below the signal-to-noise limit of the Fourier spectrum and not suitable for mode identification. The rotational axis inclination and vsini of the star were determined to be 87 degrees (nearly edge-on) and ","authors_text":"D. J. Wright, E. Brunsden, K. R. Pollard, P. De Cat, P. L. Cottrell, P. M. Kilmartin","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-03-20T01:54:40Z","title":"Spectroscopic Pulsational Frequency Identification and Mode Determination of Gamma Doradus Star HD135825"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.4307","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:b9fbc8f7fdf3ec6afc2fdbf5e6fb5c0e2de988b813fb0045288153aa5195c6bf","target":"record","created_at":"2026-05-18T01:58:05Z","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":"371adaecc0a5aa1f28efb45f2ae20596de71a6562156819fe165aee8c9bd792f","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-03-20T01:54:40Z","title_canon_sha256":"f7a25b72589b024687a605dd1de0d975ea84d5f9408b6508bcbe0100e3b4c6d1"},"schema_version":"1.0","source":{"id":"1203.4307","kind":"arxiv","version":1}},"canonical_sha256":"ca6ab074182ee6ef724e1f6d2b249bbb1b80a4cdda17ebb3c6030077170d0d41","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"ca6ab074182ee6ef724e1f6d2b249bbb1b80a4cdda17ebb3c6030077170d0d41","first_computed_at":"2026-05-18T01:58:05.754720Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:58:05.754720Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"VhpKA0fbBMeDVzTBHiVVWzfioyp6K8/1lld7ii1IYde/8SvDhw5Ju8K8Zu0uPwGzGBQ1halAp7QBl5x3DEnCDg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:58:05.755163Z","signed_message":"canonical_sha256_bytes"},"source_id":"1203.4307","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:b9fbc8f7fdf3ec6afc2fdbf5e6fb5c0e2de988b813fb0045288153aa5195c6bf","sha256:8a07745217d07ba01da2dadc77244e22c15665dd5597c6957a3babcc0996e1a2"],"state_sha256":"827440f79be2685e6008e9c62412a056c8e8c127d718bf54015602bf5a3c2b30"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"2UKW8qvhvL1NncshwbbdHc0ndL+ZsCgoNcsBP8dbrmqycVicVTwTPSNk9t2OUVwoyA6sdkROviesg6d+/fwxBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-03T12:41:38.224999Z","bundle_sha256":"4e451d5f9f2c1f8f4302193658ecd6b9ec75bf69e4291cb02528445132f11b8d"}}