{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:YRDUW25YHL3GNZ4CDXV3GG7YRF","short_pith_number":"pith:YRDUW25Y","canonical_record":{"source":{"id":"1301.2499","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-01-11T13:56:57Z","cross_cats_sorted":[],"title_canon_sha256":"2115f80d36cdb3a5d0351e8f4349fb74ebd170e6002afc32756926fdb0390065","abstract_canon_sha256":"72f093ded85bc80ec213d948a169f514753afb80fcff2b2b8bccaaed810d0fa0"},"schema_version":"1.0"},"canonical_sha256":"c4474b6bb83af666e7821debb31bf889703b933262f365f407179835319cab47","source":{"kind":"arxiv","id":"1301.2499","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1301.2499","created_at":"2026-05-18T03:36:37Z"},{"alias_kind":"arxiv_version","alias_value":"1301.2499v1","created_at":"2026-05-18T03:36:37Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.2499","created_at":"2026-05-18T03:36:37Z"},{"alias_kind":"pith_short_12","alias_value":"YRDUW25YHL3G","created_at":"2026-05-18T12:28:09Z"},{"alias_kind":"pith_short_16","alias_value":"YRDUW25YHL3GNZ4C","created_at":"2026-05-18T12:28:09Z"},{"alias_kind":"pith_short_8","alias_value":"YRDUW25Y","created_at":"2026-05-18T12:28:09Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:YRDUW25YHL3GNZ4CDXV3GG7YRF","target":"record","payload":{"canonical_record":{"source":{"id":"1301.2499","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-01-11T13:56:57Z","cross_cats_sorted":[],"title_canon_sha256":"2115f80d36cdb3a5d0351e8f4349fb74ebd170e6002afc32756926fdb0390065","abstract_canon_sha256":"72f093ded85bc80ec213d948a169f514753afb80fcff2b2b8bccaaed810d0fa0"},"schema_version":"1.0"},"canonical_sha256":"c4474b6bb83af666e7821debb31bf889703b933262f365f407179835319cab47","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:36:37.751346Z","signature_b64":"3eJ5aBlogsEFgwyucBxwAXJvMqTK/Qybg8T/XXr4fst5uVeZpMZ8QEIuOdTwlHKXn8+CrwTfUaxIiTYWoAmEBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c4474b6bb83af666e7821debb31bf889703b933262f365f407179835319cab47","last_reissued_at":"2026-05-18T03:36:37.750889Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:36:37.750889Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1301.2499","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":"2026-05-18T03:36:37Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"kaPcA05lJBmyZw3B2crHdGeTwwuPeYTtVbcM1Qo5HqkWrmFsUqeiZKp6PURoZGxMl+PTafDjSSo177oD5uVoDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T06:03:25.030971Z"},"content_sha256":"2d4a439034c6fad15d77adcc28b1fd573fc5d7da0c4dce93babc319c8fe3b2be","schema_version":"1.0","event_id":"sha256:2d4a439034c6fad15d77adcc28b1fd573fc5d7da0c4dce93babc319c8fe3b2be"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:YRDUW25YHL3GNZ4CDXV3GG7YRF","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"2D non-perturbative modeling of oscillations in rapidly rotating stars","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"D.R. Reese, M-A. Dupret, M.J. Goupil, R-M. Ouazzani","submitted_at":"2013-01-11T13:56:57Z","abstract_excerpt":"We present and discuss results of a recently developped two dimensional non-perturbative method to compute accurate adiabatic oscillation modes of rapidly rotating stars . The 2D calculations fully take into account the centrifugal distorsion of the star while the non-perturbative method includes the full influence of the Coriolis acceleration. These characteristics allows us to compute oscillation modes of rapid rotators - from high order p-modes in $\\delta$Scuti stars, to low order p- and g-modes in $\\beta$ Cephei or Be stars."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.2499","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":"2026-05-18T03:36:37Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"45epWmTtZNpufWCZEExGLv/D6G2EaQ28bWoFMUyiPSivRguBUJKS7g4s/mbQCy3usatJWjf3BOhckX7FhEb3AQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T06:03:25.031442Z"},"content_sha256":"816f4649fb5de364a73bc63bbd7167685dadc5bacb5f5c41e03bc9e1e28ea97b","schema_version":"1.0","event_id":"sha256:816f4649fb5de364a73bc63bbd7167685dadc5bacb5f5c41e03bc9e1e28ea97b"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/YRDUW25YHL3GNZ4CDXV3GG7YRF/bundle.json","state_url":"https://pith.science/pith/YRDUW25YHL3GNZ4CDXV3GG7YRF/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/YRDUW25YHL3GNZ4CDXV3GG7YRF/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":"2026-06-01T06:03:25Z","links":{"resolver":"https://pith.science/pith/YRDUW25YHL3GNZ4CDXV3GG7YRF","bundle":"https://pith.science/pith/YRDUW25YHL3GNZ4CDXV3GG7YRF/bundle.json","state":"https://pith.science/pith/YRDUW25YHL3GNZ4CDXV3GG7YRF/state.json","well_known_bundle":"https://pith.science/.well-known/pith/YRDUW25YHL3GNZ4CDXV3GG7YRF/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:YRDUW25YHL3GNZ4CDXV3GG7YRF","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":"72f093ded85bc80ec213d948a169f514753afb80fcff2b2b8bccaaed810d0fa0","cross_cats_sorted":[],"license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-01-11T13:56:57Z","title_canon_sha256":"2115f80d36cdb3a5d0351e8f4349fb74ebd170e6002afc32756926fdb0390065"},"schema_version":"1.0","source":{"id":"1301.2499","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1301.2499","created_at":"2026-05-18T03:36:37Z"},{"alias_kind":"arxiv_version","alias_value":"1301.2499v1","created_at":"2026-05-18T03:36:37Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.2499","created_at":"2026-05-18T03:36:37Z"},{"alias_kind":"pith_short_12","alias_value":"YRDUW25YHL3G","created_at":"2026-05-18T12:28:09Z"},{"alias_kind":"pith_short_16","alias_value":"YRDUW25YHL3GNZ4C","created_at":"2026-05-18T12:28:09Z"},{"alias_kind":"pith_short_8","alias_value":"YRDUW25Y","created_at":"2026-05-18T12:28:09Z"}],"graph_snapshots":[{"event_id":"sha256:816f4649fb5de364a73bc63bbd7167685dadc5bacb5f5c41e03bc9e1e28ea97b","target":"graph","created_at":"2026-05-18T03:36:37Z","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 and discuss results of a recently developped two dimensional non-perturbative method to compute accurate adiabatic oscillation modes of rapidly rotating stars . The 2D calculations fully take into account the centrifugal distorsion of the star while the non-perturbative method includes the full influence of the Coriolis acceleration. These characteristics allows us to compute oscillation modes of rapid rotators - from high order p-modes in $\\delta$Scuti stars, to low order p- and g-modes in $\\beta$ Cephei or Be stars.","authors_text":"D.R. Reese, M-A. Dupret, M.J. Goupil, R-M. Ouazzani","cross_cats":[],"headline":"","license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-01-11T13:56:57Z","title":"2D non-perturbative modeling of oscillations in rapidly rotating stars"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.2499","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":"sha256:2d4a439034c6fad15d77adcc28b1fd573fc5d7da0c4dce93babc319c8fe3b2be","target":"record","created_at":"2026-05-18T03:36:37Z","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":"72f093ded85bc80ec213d948a169f514753afb80fcff2b2b8bccaaed810d0fa0","cross_cats_sorted":[],"license":"http://creativecommons.org/licenses/by-nc-sa/3.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-01-11T13:56:57Z","title_canon_sha256":"2115f80d36cdb3a5d0351e8f4349fb74ebd170e6002afc32756926fdb0390065"},"schema_version":"1.0","source":{"id":"1301.2499","kind":"arxiv","version":1}},"canonical_sha256":"c4474b6bb83af666e7821debb31bf889703b933262f365f407179835319cab47","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"c4474b6bb83af666e7821debb31bf889703b933262f365f407179835319cab47","first_computed_at":"2026-05-18T03:36:37.750889Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T03:36:37.750889Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"3eJ5aBlogsEFgwyucBxwAXJvMqTK/Qybg8T/XXr4fst5uVeZpMZ8QEIuOdTwlHKXn8+CrwTfUaxIiTYWoAmEBA==","signature_status":"signed_v1","signed_at":"2026-05-18T03:36:37.751346Z","signed_message":"canonical_sha256_bytes"},"source_id":"1301.2499","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:2d4a439034c6fad15d77adcc28b1fd573fc5d7da0c4dce93babc319c8fe3b2be","sha256:816f4649fb5de364a73bc63bbd7167685dadc5bacb5f5c41e03bc9e1e28ea97b"],"state_sha256":"70b472483a209af51b1ba49238c696223e62c2eeec3d35cdc2082ff34ea68a60"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"9RJv0tFYSVTAUZOPfPWOxcih9HcEqIe1hDpIhZGz+apgHJ7Z7QyRwTTVfDryT+kDZHVmxkhxZDAt5jrP1npYDw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-01T06:03:25.033863Z","bundle_sha256":"75578d97ca1ca54635d6de13554390c41ab92e63881a3b556adaf5bff82db11b"}}