{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2015:ELOEYV7DPRVFWDWU7UZBURJSEF","short_pith_number":"pith:ELOEYV7D","canonical_record":{"source":{"id":"1506.03146","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-06-10T02:23:18Z","cross_cats_sorted":[],"title_canon_sha256":"ecd732e8f449904de1328a02e43d86b51c013cfb1cc165953c9a1ab1fc1946de","abstract_canon_sha256":"fd21dd5da718ae0f120d0de4318deeaae82fd0cb1b6dff6541814db62a71d7ef"},"schema_version":"1.0"},"canonical_sha256":"22dc4c57e37c6a5b0ed4fd321a4532217128f180c37826f4bd54b5ac606e4739","source":{"kind":"arxiv","id":"1506.03146","version":3},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1506.03146","created_at":"2026-07-04T21:41:18Z"},{"alias_kind":"arxiv_version","alias_value":"1506.03146v3","created_at":"2026-07-04T21:41:18Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.03146","created_at":"2026-07-04T21:41:18Z"},{"alias_kind":"pith_short_12","alias_value":"ELOEYV7DPRVF","created_at":"2026-07-04T21:41:18Z"},{"alias_kind":"pith_short_16","alias_value":"ELOEYV7DPRVFWDWU","created_at":"2026-07-04T21:41:18Z"},{"alias_kind":"pith_short_8","alias_value":"ELOEYV7D","created_at":"2026-07-04T21:41:18Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2015:ELOEYV7DPRVFWDWU7UZBURJSEF","target":"record","payload":{"canonical_record":{"source":{"id":"1506.03146","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-06-10T02:23:18Z","cross_cats_sorted":[],"title_canon_sha256":"ecd732e8f449904de1328a02e43d86b51c013cfb1cc165953c9a1ab1fc1946de","abstract_canon_sha256":"fd21dd5da718ae0f120d0de4318deeaae82fd0cb1b6dff6541814db62a71d7ef"},"schema_version":"1.0"},"canonical_sha256":"22dc4c57e37c6a5b0ed4fd321a4532217128f180c37826f4bd54b5ac606e4739","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T21:41:18.952330Z","signature_b64":"XFpDdOmsWAaiIUol2n7iEL6J3Uh4nBC9dIhh4MSExmrMEuSGhUo7c/L958kNXtD+NojE9hFvTEDXmZI0OvILDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"22dc4c57e37c6a5b0ed4fd321a4532217128f180c37826f4bd54b5ac606e4739","last_reissued_at":"2026-07-04T21:41:18.951785Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T21:41:18.951785Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1506.03146","source_version":3,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T21:41:18Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"eUPfsAjvpMglKbzmnzx//uF8+z95w8pE8CY7GuE8M2RLrf/F8AG03LhlFO9ay1go2EQRimeqNFvoMpXvJhYYCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-11T20:13:41.368100Z"},"content_sha256":"3a35de3ea2c088e97a87a62501adfabb08cb34d4244e8375999308d8dcfbb690","schema_version":"1.0","event_id":"sha256:3a35de3ea2c088e97a87a62501adfabb08cb34d4244e8375999308d8dcfbb690"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2015:ELOEYV7DPRVFWDWU7UZBURJSEF","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"MESA now evolves pairs of interacting stars and models massive star explosions from pre-main sequence through core collapse.","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Bill Paxton, Dean M. Townsley, Evan B. Bauer, F.X. Timmes, H. Hu, Josiah Schwab, Lars Bildsten, Luc Dessart, Matteo Cantiello, N. Langer, Pablo Marchant, R. Farmer, R.H.D. Townsend","submitted_at":"2015-06-10T02:23:18Z","abstract_excerpt":"We substantially update the capabilities of the open-source software instrument Modules for Experiments in Stellar Astrophysics (MESA). MESA can now simultaneously evolve an interacting pair of differentially rotating stars undergoing transfer and loss of mass and angular momentum, greatly enhancing the prior ability to model binary evolution. New MESA capabilities in fully coupled calculation of nuclear networks with hundreds of isotopes now allow MESA to accurately simulate advanced burning stages needed to construct supernova progenitor models. Implicit hydrodynamics with shocks can now be "},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"MESA can now simultaneously evolve an interacting pair of differentially rotating stars undergoing transfer and loss of mass and angular momentum, greatly enhancing the prior ability to model binary evolution. Implicit hydrodynamics with shocks can now be treated with MESA, enabling modeling of the entire massive star lifecycle, from pre-main sequence evolution to the onset of core collapse and nucleosynthesis from the resulting explosion.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"The newly implemented modules for binary mass transfer, hydrodynamics, and on-the-fly weak rates produce numerically stable and physically accurate results across the range of stellar conditions without requiring extensive user tuning.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"MESA gains simultaneous binary star evolution, large nuclear networks, implicit hydrodynamics, and GYRE pulsation coupling for better massive star and supernova modeling.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"MESA now evolves pairs of interacting stars and models massive star explosions from pre-main sequence through core collapse.","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"f88a23b201450487bc0445d14f0030daeb40831a7689e30419a8913ad591193b"},"source":{"id":"1506.03146","kind":"arxiv","version":3},"verdict":{"id":"0c02434b-0e49-411c-b106-44c7c781f513","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-13T19:24:04.254072Z","strongest_claim":"MESA can now simultaneously evolve an interacting pair of differentially rotating stars undergoing transfer and loss of mass and angular momentum, greatly enhancing the prior ability to model binary evolution. Implicit hydrodynamics with shocks can now be treated with MESA, enabling modeling of the entire massive star lifecycle, from pre-main sequence evolution to the onset of core collapse and nucleosynthesis from the resulting explosion.","one_line_summary":"MESA gains simultaneous binary star evolution, large nuclear networks, implicit hydrodynamics, and GYRE pulsation coupling for better massive star and supernova modeling.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"The newly implemented modules for binary mass transfer, hydrodynamics, and on-the-fly weak rates produce numerically stable and physically accurate results across the range of stellar conditions without requiring extensive user tuning.","pith_extraction_headline":"MESA now evolves pairs of interacting stars and models massive star explosions from pre-main sequence through core collapse."},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1506.03146/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":195,"sample":[{"doi":"","year":2010,"title":"Aerts, C., Christensen-Dalsgaard, J., & Kurtz, D. W. 2010, Asteroseismology (Springer Science+Business Media B.V)","work_id":"8875f23e-b645-4fa9-a832-e8cd178689b5","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2015,"title":"Aoyama, S., & Suzuki, T. K. 2015, ArXiv e-prints","work_id":"bf8cdb53-2e24-42ae-a040-499a72be6816","ref_index":2,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2010,"title":"F., & Woosley, S","work_id":"2b3a4f33-5cd3-429f-98e8-d2ac4ed717af","ref_index":3,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":1969,"title":"Arnett, W. D. 1969, Ap&SS, 5, 180","work_id":"cf765600-e824-4bf9-8bf9-ca0df2d864ca","ref_index":4,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2009,"title":"J., & Scott, P","work_id":"a8eb8263-ca5e-4103-8ae3-66ced6a7a453","ref_index":5,"cited_arxiv_id":"","is_internal_anchor":false}],"resolved_work":195,"snapshot_sha256":"8ce35f6ca47d4a5daa18eed43be17fb1e578122ad19b25429d5d1d7273b8f856","internal_anchors":0},"formal_canon":{"evidence_count":1,"snapshot_sha256":"725676c01e399e4403b85edc76db770b6ca9e2714966932c5dede7c46537a246"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"verdict_id":"0c02434b-0e49-411c-b106-44c7c781f513"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T21:41:18Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Qbxw4dbcOx9rrWA1gTLW+M7y7+SAFt/JmqgK8YSaUqBhNz5kjBw5EFjW18Pi24rdLCAoYdOQUvNyIzP97RYXAA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-11T20:13:41.369033Z"},"content_sha256":"5e0fbb483de7529c2c23fd60a566f9ac600d531ee5ef490f4c6749d707c84796","schema_version":"1.0","event_id":"sha256:5e0fbb483de7529c2c23fd60a566f9ac600d531ee5ef490f4c6749d707c84796"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/ELOEYV7DPRVFWDWU7UZBURJSEF/bundle.json","state_url":"https://pith.science/pith/ELOEYV7DPRVFWDWU7UZBURJSEF/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/ELOEYV7DPRVFWDWU7UZBURJSEF/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":"2026-08-11T20:13:41Z","links":{"resolver":"https://pith.science/pith/ELOEYV7DPRVFWDWU7UZBURJSEF","bundle":"https://pith.science/pith/ELOEYV7DPRVFWDWU7UZBURJSEF/bundle.json","state":"https://pith.science/pith/ELOEYV7DPRVFWDWU7UZBURJSEF/state.json","well_known_bundle":"https://pith.science/.well-known/pith/ELOEYV7DPRVFWDWU7UZBURJSEF/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2015:ELOEYV7DPRVFWDWU7UZBURJSEF","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":"fd21dd5da718ae0f120d0de4318deeaae82fd0cb1b6dff6541814db62a71d7ef","cross_cats_sorted":[],"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-06-10T02:23:18Z","title_canon_sha256":"ecd732e8f449904de1328a02e43d86b51c013cfb1cc165953c9a1ab1fc1946de"},"schema_version":"1.0","source":{"id":"1506.03146","kind":"arxiv","version":3}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1506.03146","created_at":"2026-07-04T21:41:18Z"},{"alias_kind":"arxiv_version","alias_value":"1506.03146v3","created_at":"2026-07-04T21:41:18Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.03146","created_at":"2026-07-04T21:41:18Z"},{"alias_kind":"pith_short_12","alias_value":"ELOEYV7DPRVF","created_at":"2026-07-04T21:41:18Z"},{"alias_kind":"pith_short_16","alias_value":"ELOEYV7DPRVFWDWU","created_at":"2026-07-04T21:41:18Z"},{"alias_kind":"pith_short_8","alias_value":"ELOEYV7D","created_at":"2026-07-04T21:41:18Z"}],"graph_snapshots":[{"event_id":"sha256:5e0fbb483de7529c2c23fd60a566f9ac600d531ee5ef490f4c6749d707c84796","target":"graph","created_at":"2026-07-04T21:41:18Z","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":4,"items":[{"attestation":"unclaimed","claim_id":"C1","kind":"strongest_claim","source":"verdict.strongest_claim","status":"machine_extracted","text":"MESA can now simultaneously evolve an interacting pair of differentially rotating stars undergoing transfer and loss of mass and angular momentum, greatly enhancing the prior ability to model binary evolution. Implicit hydrodynamics with shocks can now be treated with MESA, enabling modeling of the entire massive star lifecycle, from pre-main sequence evolution to the onset of core collapse and nucleosynthesis from the resulting explosion."},{"attestation":"unclaimed","claim_id":"C2","kind":"weakest_assumption","source":"verdict.weakest_assumption","status":"machine_extracted","text":"The newly implemented modules for binary mass transfer, hydrodynamics, and on-the-fly weak rates produce numerically stable and physically accurate results across the range of stellar conditions without requiring extensive user tuning."},{"attestation":"unclaimed","claim_id":"C3","kind":"one_line_summary","source":"verdict.one_line_summary","status":"machine_extracted","text":"MESA gains simultaneous binary star evolution, large nuclear networks, implicit hydrodynamics, and GYRE pulsation coupling for better massive star and supernova modeling."},{"attestation":"unclaimed","claim_id":"C4","kind":"headline","source":"verdict.pith_extraction.headline","status":"machine_extracted","text":"MESA now evolves pairs of interacting stars and models massive star explosions from pre-main sequence through core collapse."}],"snapshot_sha256":"f88a23b201450487bc0445d14f0030daeb40831a7689e30419a8913ad591193b"},"formal_canon":{"evidence_count":1,"snapshot_sha256":"725676c01e399e4403b85edc76db770b6ca9e2714966932c5dede7c46537a246"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/1506.03146/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"We substantially update the capabilities of the open-source software instrument Modules for Experiments in Stellar Astrophysics (MESA). MESA can now simultaneously evolve an interacting pair of differentially rotating stars undergoing transfer and loss of mass and angular momentum, greatly enhancing the prior ability to model binary evolution. New MESA capabilities in fully coupled calculation of nuclear networks with hundreds of isotopes now allow MESA to accurately simulate advanced burning stages needed to construct supernova progenitor models. Implicit hydrodynamics with shocks can now be ","authors_text":"Bill Paxton, Dean M. Townsley, Evan B. Bauer, F.X. Timmes, H. Hu, Josiah Schwab, Lars Bildsten, Luc Dessart, Matteo Cantiello, N. Langer, Pablo Marchant, R. Farmer, R.H.D. Townsend","cross_cats":[],"headline":"MESA now evolves pairs of interacting stars and models massive star explosions from pre-main sequence through core collapse.","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-06-10T02:23:18Z","title":"Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions"},"references":{"count":195,"internal_anchors":0,"resolved_work":195,"sample":[{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":1,"title":"Aerts, C., Christensen-Dalsgaard, J., & Kurtz, D. W. 2010, Asteroseismology (Springer Science+Business Media B.V)","work_id":"8875f23e-b645-4fa9-a832-e8cd178689b5","year":2010},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":2,"title":"Aoyama, S., & Suzuki, T. K. 2015, ArXiv e-prints","work_id":"bf8cdb53-2e24-42ae-a040-499a72be6816","year":2015},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":3,"title":"F., & Woosley, S","work_id":"2b3a4f33-5cd3-429f-98e8-d2ac4ed717af","year":2010},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":4,"title":"Arnett, W. D. 1969, Ap&SS, 5, 180","work_id":"cf765600-e824-4bf9-8bf9-ca0df2d864ca","year":1969},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":5,"title":"J., & Scott, P","work_id":"a8eb8263-ca5e-4103-8ae3-66ced6a7a453","year":2009}],"snapshot_sha256":"8ce35f6ca47d4a5daa18eed43be17fb1e578122ad19b25429d5d1d7273b8f856"},"source":{"id":"1506.03146","kind":"arxiv","version":3},"verdict":{"created_at":"2026-05-13T19:24:04.254072Z","id":"0c02434b-0e49-411c-b106-44c7c781f513","model_set":{"reader":"grok-4.3"},"one_line_summary":"MESA gains simultaneous binary star evolution, large nuclear networks, implicit hydrodynamics, and GYRE pulsation coupling for better massive star and supernova modeling.","pipeline_version":"pith-pipeline@v0.9.0","pith_extraction_headline":"MESA now evolves pairs of interacting stars and models massive star explosions from pre-main sequence through core collapse.","strongest_claim":"MESA can now simultaneously evolve an interacting pair of differentially rotating stars undergoing transfer and loss of mass and angular momentum, greatly enhancing the prior ability to model binary evolution. Implicit hydrodynamics with shocks can now be treated with MESA, enabling modeling of the entire massive star lifecycle, from pre-main sequence evolution to the onset of core collapse and nucleosynthesis from the resulting explosion.","weakest_assumption":"The newly implemented modules for binary mass transfer, hydrodynamics, and on-the-fly weak rates produce numerically stable and physically accurate results across the range of stellar conditions without requiring extensive user tuning."}},"verdict_id":"0c02434b-0e49-411c-b106-44c7c781f513"}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:3a35de3ea2c088e97a87a62501adfabb08cb34d4244e8375999308d8dcfbb690","target":"record","created_at":"2026-07-04T21:41:18Z","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":"fd21dd5da718ae0f120d0de4318deeaae82fd0cb1b6dff6541814db62a71d7ef","cross_cats_sorted":[],"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-06-10T02:23:18Z","title_canon_sha256":"ecd732e8f449904de1328a02e43d86b51c013cfb1cc165953c9a1ab1fc1946de"},"schema_version":"1.0","source":{"id":"1506.03146","kind":"arxiv","version":3}},"canonical_sha256":"22dc4c57e37c6a5b0ed4fd321a4532217128f180c37826f4bd54b5ac606e4739","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"22dc4c57e37c6a5b0ed4fd321a4532217128f180c37826f4bd54b5ac606e4739","first_computed_at":"2026-07-04T21:41:18.951785Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-04T21:41:18.951785Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"XFpDdOmsWAaiIUol2n7iEL6J3Uh4nBC9dIhh4MSExmrMEuSGhUo7c/L958kNXtD+NojE9hFvTEDXmZI0OvILDg==","signature_status":"signed_v1","signed_at":"2026-07-04T21:41:18.952330Z","signed_message":"canonical_sha256_bytes"},"source_id":"1506.03146","source_kind":"arxiv","source_version":3}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:3a35de3ea2c088e97a87a62501adfabb08cb34d4244e8375999308d8dcfbb690","sha256:5e0fbb483de7529c2c23fd60a566f9ac600d531ee5ef490f4c6749d707c84796"],"state_sha256":"98c382057bc264949a9b36fca6c98dd03aa070bb33deb87898336df9727070bc"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"UfQI6clWxKgamUhL/A4oBwDibJ2WKT5KRDsNNku1Oz65W+Pni2x3/7V9x0LWYJFkMNgvs9E+ND1z5bSX2jTkDQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-11T20:13:41.374148Z","bundle_sha256":"24becac52ecdcf0562de207a01220f5b5898b5f3091f67f45d76ba605736dff5"}}