{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:LC34HBFDBVPJRUCTKMCAMFN6HM","short_pith_number":"pith:LC34HBFD","canonical_record":{"source":{"id":"1004.0609","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-04-05T10:57:54Z","cross_cats_sorted":[],"title_canon_sha256":"d631c2b4c10317d8d2f54e59f323a307a9ea855a426183938cf348cb470cdc4e","abstract_canon_sha256":"57f0d2edbab39e23bb6c2d79335679f3de0b53db5fde90998388c58657cd0f84"},"schema_version":"1.0"},"canonical_sha256":"58b7c384a30d5e98d05353040615be3b3434f707b9fecb0ad120e038a77d7834","source":{"kind":"arxiv","id":"1004.0609","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1004.0609","created_at":"2026-05-18T02:08:14Z"},{"alias_kind":"arxiv_version","alias_value":"1004.0609v1","created_at":"2026-05-18T02:08:14Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1004.0609","created_at":"2026-05-18T02:08:14Z"},{"alias_kind":"pith_short_12","alias_value":"LC34HBFDBVPJ","created_at":"2026-05-18T12:26:10Z"},{"alias_kind":"pith_short_16","alias_value":"LC34HBFDBVPJRUCT","created_at":"2026-05-18T12:26:10Z"},{"alias_kind":"pith_short_8","alias_value":"LC34HBFD","created_at":"2026-05-18T12:26:10Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:LC34HBFDBVPJRUCTKMCAMFN6HM","target":"record","payload":{"canonical_record":{"source":{"id":"1004.0609","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-04-05T10:57:54Z","cross_cats_sorted":[],"title_canon_sha256":"d631c2b4c10317d8d2f54e59f323a307a9ea855a426183938cf348cb470cdc4e","abstract_canon_sha256":"57f0d2edbab39e23bb6c2d79335679f3de0b53db5fde90998388c58657cd0f84"},"schema_version":"1.0"},"canonical_sha256":"58b7c384a30d5e98d05353040615be3b3434f707b9fecb0ad120e038a77d7834","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:08:14.447702Z","signature_b64":"aBC4nLhomLszKGsnw/33L2h3jGVJbK9+lj1sPhvAR90ynENtIs8vsiPpix+Ng2Cm2j1DKoiz05MHVFYE9SgCCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"58b7c384a30d5e98d05353040615be3b3434f707b9fecb0ad120e038a77d7834","last_reissued_at":"2026-05-18T02:08:14.447301Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:08:14.447301Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1004.0609","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":"2026-05-18T02:08:14Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"2SOgfRJxCkmPWgWZNDZKTnxbyqqlgESTkcqlHKhgHarLXAKt9u4aa9LgEd9bFKUqQo20QJve1BVe1YXWHqxqCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T17:34:25.357368Z"},"content_sha256":"5214b1b9568c439161dd8469cbff28573b4943611b42b855b9216ca9b903f44b","schema_version":"1.0","event_id":"sha256:5214b1b9568c439161dd8469cbff28573b4943611b42b855b9216ca9b903f44b"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:LC34HBFDBVPJRUCTKMCAMFN6HM","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"On the use of rotational splitting asymmetries to probe the internal rotation profile of stars. Application to $\\beta$ Cephei stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"(2)Instituo de Astronomia, (3)LESIA, E. Janot-Pacheco(2) ((1)Instituto de Astrof\\'isica de Andaluc\\'ia (CSIC)Granada-Spain, France), Geof\\'isica e Ci\\^encias Atmosf\\'ericas da Universidade de S\\~ao Paulo (IAG-USP)Brazil, J.C.Su\\'arez (1), L.Andrade (2), Meudon, M.J. Goupil (3), Observatoire de Paris-Meudon, UMR8109","submitted_at":"2010-04-05T10:57:54Z","abstract_excerpt":"Rotationally-split modes can provide valuable information about the internal rotation profile of stars. This has been used for years to infer the internal rotation behavior of the Sun. The present work discusses the potential additional information that rotationally splitting asymmetries may provide when studying the internal rotation profile of stars. We present here some preliminary results of a method, currently under development, which intends: 1) to understand the variation of the rotational splitting asymmetries in terms of physical processes acting on the angular momentum distribution i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1004.0609","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":"2026-05-18T02:08:14Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"SvBg5004TVmbfdm7wniJ9oPlk8RlO5R6daLzMS2Zge9FUPoE3d+vWLGLwGWczq58LfNkFneP/TvrTOpOYy8lCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T17:34:25.358082Z"},"content_sha256":"bd71b072880ba4f008b80749e45922a2c7c2dcc4bb447b2216201f2aea6ae8af","schema_version":"1.0","event_id":"sha256:bd71b072880ba4f008b80749e45922a2c7c2dcc4bb447b2216201f2aea6ae8af"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/LC34HBFDBVPJRUCTKMCAMFN6HM/bundle.json","state_url":"https://pith.science/pith/LC34HBFDBVPJRUCTKMCAMFN6HM/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/LC34HBFDBVPJRUCTKMCAMFN6HM/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":"2026-05-25T17:34:25Z","links":{"resolver":"https://pith.science/pith/LC34HBFDBVPJRUCTKMCAMFN6HM","bundle":"https://pith.science/pith/LC34HBFDBVPJRUCTKMCAMFN6HM/bundle.json","state":"https://pith.science/pith/LC34HBFDBVPJRUCTKMCAMFN6HM/state.json","well_known_bundle":"https://pith.science/.well-known/pith/LC34HBFDBVPJRUCTKMCAMFN6HM/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:LC34HBFDBVPJRUCTKMCAMFN6HM","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":"57f0d2edbab39e23bb6c2d79335679f3de0b53db5fde90998388c58657cd0f84","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-04-05T10:57:54Z","title_canon_sha256":"d631c2b4c10317d8d2f54e59f323a307a9ea855a426183938cf348cb470cdc4e"},"schema_version":"1.0","source":{"id":"1004.0609","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1004.0609","created_at":"2026-05-18T02:08:14Z"},{"alias_kind":"arxiv_version","alias_value":"1004.0609v1","created_at":"2026-05-18T02:08:14Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1004.0609","created_at":"2026-05-18T02:08:14Z"},{"alias_kind":"pith_short_12","alias_value":"LC34HBFDBVPJ","created_at":"2026-05-18T12:26:10Z"},{"alias_kind":"pith_short_16","alias_value":"LC34HBFDBVPJRUCT","created_at":"2026-05-18T12:26:10Z"},{"alias_kind":"pith_short_8","alias_value":"LC34HBFD","created_at":"2026-05-18T12:26:10Z"}],"graph_snapshots":[{"event_id":"sha256:bd71b072880ba4f008b80749e45922a2c7c2dcc4bb447b2216201f2aea6ae8af","target":"graph","created_at":"2026-05-18T02:08:14Z","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":"Rotationally-split modes can provide valuable information about the internal rotation profile of stars. This has been used for years to infer the internal rotation behavior of the Sun. The present work discusses the potential additional information that rotationally splitting asymmetries may provide when studying the internal rotation profile of stars. We present here some preliminary results of a method, currently under development, which intends: 1) to understand the variation of the rotational splitting asymmetries in terms of physical processes acting on the angular momentum distribution i","authors_text":"(2)Instituo de Astronomia, (3)LESIA, E. Janot-Pacheco(2) ((1)Instituto de Astrof\\'isica de Andaluc\\'ia (CSIC)Granada-Spain, France), Geof\\'isica e Ci\\^encias Atmosf\\'ericas da Universidade de S\\~ao Paulo (IAG-USP)Brazil, J.C.Su\\'arez (1), L.Andrade (2), Meudon, M.J. Goupil (3), Observatoire de Paris-Meudon, UMR8109","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-04-05T10:57:54Z","title":"On the use of rotational splitting asymmetries to probe the internal rotation profile of stars. Application to $\\beta$ Cephei stars"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1004.0609","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":"sha256:5214b1b9568c439161dd8469cbff28573b4943611b42b855b9216ca9b903f44b","target":"record","created_at":"2026-05-18T02:08:14Z","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":"57f0d2edbab39e23bb6c2d79335679f3de0b53db5fde90998388c58657cd0f84","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-04-05T10:57:54Z","title_canon_sha256":"d631c2b4c10317d8d2f54e59f323a307a9ea855a426183938cf348cb470cdc4e"},"schema_version":"1.0","source":{"id":"1004.0609","kind":"arxiv","version":1}},"canonical_sha256":"58b7c384a30d5e98d05353040615be3b3434f707b9fecb0ad120e038a77d7834","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"58b7c384a30d5e98d05353040615be3b3434f707b9fecb0ad120e038a77d7834","first_computed_at":"2026-05-18T02:08:14.447301Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:08:14.447301Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"aBC4nLhomLszKGsnw/33L2h3jGVJbK9+lj1sPhvAR90ynENtIs8vsiPpix+Ng2Cm2j1DKoiz05MHVFYE9SgCCg==","signature_status":"signed_v1","signed_at":"2026-05-18T02:08:14.447702Z","signed_message":"canonical_sha256_bytes"},"source_id":"1004.0609","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:5214b1b9568c439161dd8469cbff28573b4943611b42b855b9216ca9b903f44b","sha256:bd71b072880ba4f008b80749e45922a2c7c2dcc4bb447b2216201f2aea6ae8af"],"state_sha256":"d8383ca7743a4e75b84c1284cc7e608f6f5a64d920b80dfe8106102fdfc53352"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"oCoh4Ntm66gh1Q3Qj1fIwAuMqfMf30iVainD9thryXl83OMt0HElnCQjBWHJwmLfwipzCaVpyTsPqBI8npVEBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T17:34:25.361756Z","bundle_sha256":"43890dcf9bd3f855934a032a8da509335549528e75683b7af71cd707a1ab3ff0"}}