{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2026:25OQX3IZ2ASDVDRDSTJLIFZOCV","short_pith_number":"pith:25OQX3IZ","canonical_record":{"source":{"id":"2604.11106","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-04-13T07:23:08Z","cross_cats_sorted":[],"title_canon_sha256":"c8140b9968a5f5a47b86c2fc3dfd968c1018ddaae0b21fd13909d140bd8f4783","abstract_canon_sha256":"a627af07d30ccae6d95031d66f1a50288fa3333dd8e3fc4301186d080a12d983"},"schema_version":"1.0"},"canonical_sha256":"d75d0bed19d0243a8e2394d2b4172e154f7eeca24ac5965444b11ae80111537e","source":{"kind":"arxiv","id":"2604.11106","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2604.11106","created_at":"2026-05-25T02:01:19Z"},{"alias_kind":"arxiv_version","alias_value":"2604.11106v2","created_at":"2026-05-25T02:01:19Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2604.11106","created_at":"2026-05-25T02:01:19Z"},{"alias_kind":"pith_short_12","alias_value":"25OQX3IZ2ASD","created_at":"2026-05-25T02:01:19Z"},{"alias_kind":"pith_short_16","alias_value":"25OQX3IZ2ASDVDRD","created_at":"2026-05-25T02:01:19Z"},{"alias_kind":"pith_short_8","alias_value":"25OQX3IZ","created_at":"2026-05-25T02:01:19Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2026:25OQX3IZ2ASDVDRDSTJLIFZOCV","target":"record","payload":{"canonical_record":{"source":{"id":"2604.11106","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-04-13T07:23:08Z","cross_cats_sorted":[],"title_canon_sha256":"c8140b9968a5f5a47b86c2fc3dfd968c1018ddaae0b21fd13909d140bd8f4783","abstract_canon_sha256":"a627af07d30ccae6d95031d66f1a50288fa3333dd8e3fc4301186d080a12d983"},"schema_version":"1.0"},"canonical_sha256":"d75d0bed19d0243a8e2394d2b4172e154f7eeca24ac5965444b11ae80111537e","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-25T02:01:19.379574Z","signature_b64":"s43bWG9puGlCGjQlRcVrw22qzWK8Sh4L4McEXqRTxEwVcSz6dG9LOWyVMj6IFhoQF6AdNia9TaHyMlWkiklBCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d75d0bed19d0243a8e2394d2b4172e154f7eeca24ac5965444b11ae80111537e","last_reissued_at":"2026-05-25T02:01:19.378618Z","signature_status":"signed_v1","first_computed_at":"2026-05-25T02:01:19.378618Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"2604.11106","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-25T02:01:19Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"AjAejULIL421G0CjkG4zsZbzr9UljfeW6jQBijybTdd7EtgFsJiYY9EiVUgpUW9KhyWd00EIKO84xn5gnAeXBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-10T08:07:09.059458Z"},"content_sha256":"0e756f4ec43cc3a821f600d7c0b37f6b4a68f0e6950a7659e95a95f1b511bed9","schema_version":"1.0","event_id":"sha256:0e756f4ec43cc3a821f600d7c0b37f6b4a68f0e6950a7659e95a95f1b511bed9"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2026:25OQX3IZ2ASDVDRDSTJLIFZOCV","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"On the origin of the BAOtr-DESI tension","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"BAOtr and DESI BAO datasets cannot be fit simultaneously by any CMB-consistent CPL dark energy model.","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Ioannis Pantos, Leandros Perivolaropoulos","submitted_at":"2026-04-13T07:23:08Z","abstract_excerpt":"The fiducial-independent angular/transverse BAO dataset, obtained from two-point angular correlation functions in thin redshift shells (hereafter BAOtr), systematically prefers smaller comoving distance ratios $D_{\\rm M}/r_{\\rm d}$ than the DESI DR2 three-dimensional BAO measurements at $z \\lesssim 0.65$, driving dataset-dependent CPL dark-energy inferences and conflicting conclusions about the Hubble tension. We investigate whether this disagreement can be attributed to the $\\Lambda$CDM fiducial assumed in the 3D BAO pipeline, or resolved within the CPL parametrisation. We show that the publi"},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"No CMB-consistent CPL model fits both datasets simultaneously. The direct comparison at z = 0.510 sets an irreducible tension floor that no smooth modification of D_M(z) can remove.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"That the CPL parametrization is sufficiently flexible to describe any smooth dark energy evolution consistent with the data, and that residual fiducial dependence in the published DESI distances is truly negligible at the 0.3% level.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"No CMB-consistent CPL dark energy model can simultaneously fit both the BAOtr and DESI datasets; the 3.7-sigma disagreement at z=0.51 sets an irreducible floor.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"BAOtr and DESI BAO datasets cannot be fit simultaneously by any CMB-consistent CPL dark energy model.","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"d5886926ab357386b4b9ddd5e918446267e49808669f4807b4b9e7b539848410"},"source":{"id":"2604.11106","kind":"arxiv","version":2},"verdict":{"id":"ebf8af75-f57c-4375-a0ad-312d0550d7fe","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-10T15:50:55.626909Z","strongest_claim":"No CMB-consistent CPL model fits both datasets simultaneously. The direct comparison at z = 0.510 sets an irreducible tension floor that no smooth modification of D_M(z) can remove.","one_line_summary":"No CMB-consistent CPL dark energy model can simultaneously fit both the BAOtr and DESI datasets; the 3.7-sigma disagreement at z=0.51 sets an irreducible floor.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"That the CPL parametrization is sufficiently flexible to describe any smooth dark energy evolution consistent with the data, and that residual fiducial dependence in the published DESI distances is truly negligible at the 0.3% level.","pith_extraction_headline":"BAOtr and DESI BAO datasets cannot be fit simultaneously by any CMB-consistent CPL dark energy model."},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2604.11106/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":85,"sample":[{"doi":"","year":1998,"title":"D. J. Eisenstein, W. Hu, M. Tegmark, Cosmic complementarity:H 0 andΩ m from combining CMB experiments and redshift surveys, Astro- phys. J. 504 (1998) L57–L60.arXiv:astro-ph/9805239,doi:10.1086/ 31158","work_id":"a5e8beed-40d8-4428-a0f2-809d8e001c87","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2005,"title":"Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies","work_id":"ce6a8c9a-70a6-448e-9706-59019b463903","ref_index":2,"cited_arxiv_id":"astro-ph/0501171","is_internal_anchor":false},{"doi":"10.1046/j.1365-8711.1999.02369.x","year":1999,"title":"1999, MNRAS, 302, 81, doi: 10.1046/j.1365-8711.1999.02083.x","work_id":"4f7e2990-d16b-4b19-8801-2137d127eb2e","ref_index":3,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"10.1086/376983","year":2003,"title":"Probing dark energy using baryonic oscillations in the galaxy power spectrum as a cosmological ruler","work_id":"4ef2e2a0-34b5-4af2-ae19-a22d39b02cef","ref_index":4,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"10.1086/379122","year":2003,"title":"Probing dark energy with baryonic acoustic oscillations from future large galaxy redshift surveys","work_id":"995f6aed-c552-4267-a5d3-e0f105d7f1fe","ref_index":5,"cited_arxiv_id":"","is_internal_anchor":false}],"resolved_work":85,"snapshot_sha256":"0fa09ee28760f228156d3f5c33e0c12f9bb43c1cd50e6eee1bcb09e28936135d","internal_anchors":5},"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":"ebf8af75-f57c-4375-a0ad-312d0550d7fe"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-25T02:01:19Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"KWSIDGE/qUcHVtiEs0QNieLnnd/hoN2mqObGL5QmKo9/jI0u5Fnj09hhQ2TUVlolnqRM8TyXCrgNDinUFIItDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-10T08:07:09.060779Z"},"content_sha256":"c225c6ebc2823405ff906699410fc91661aa650af45f095e54017619c34ffec0","schema_version":"1.0","event_id":"sha256:c225c6ebc2823405ff906699410fc91661aa650af45f095e54017619c34ffec0"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/25OQX3IZ2ASDVDRDSTJLIFZOCV/bundle.json","state_url":"https://pith.science/pith/25OQX3IZ2ASDVDRDSTJLIFZOCV/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/25OQX3IZ2ASDVDRDSTJLIFZOCV/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":"2026-06-10T08:07:09Z","links":{"resolver":"https://pith.science/pith/25OQX3IZ2ASDVDRDSTJLIFZOCV","bundle":"https://pith.science/pith/25OQX3IZ2ASDVDRDSTJLIFZOCV/bundle.json","state":"https://pith.science/pith/25OQX3IZ2ASDVDRDSTJLIFZOCV/state.json","well_known_bundle":"https://pith.science/.well-known/pith/25OQX3IZ2ASDVDRDSTJLIFZOCV/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2026:25OQX3IZ2ASDVDRDSTJLIFZOCV","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":"a627af07d30ccae6d95031d66f1a50288fa3333dd8e3fc4301186d080a12d983","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-04-13T07:23:08Z","title_canon_sha256":"c8140b9968a5f5a47b86c2fc3dfd968c1018ddaae0b21fd13909d140bd8f4783"},"schema_version":"1.0","source":{"id":"2604.11106","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2604.11106","created_at":"2026-05-25T02:01:19Z"},{"alias_kind":"arxiv_version","alias_value":"2604.11106v2","created_at":"2026-05-25T02:01:19Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2604.11106","created_at":"2026-05-25T02:01:19Z"},{"alias_kind":"pith_short_12","alias_value":"25OQX3IZ2ASD","created_at":"2026-05-25T02:01:19Z"},{"alias_kind":"pith_short_16","alias_value":"25OQX3IZ2ASDVDRD","created_at":"2026-05-25T02:01:19Z"},{"alias_kind":"pith_short_8","alias_value":"25OQX3IZ","created_at":"2026-05-25T02:01:19Z"}],"graph_snapshots":[{"event_id":"sha256:c225c6ebc2823405ff906699410fc91661aa650af45f095e54017619c34ffec0","target":"graph","created_at":"2026-05-25T02:01:19Z","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":"No CMB-consistent CPL model fits both datasets simultaneously. The direct comparison at z = 0.510 sets an irreducible tension floor that no smooth modification of D_M(z) can remove."},{"attestation":"unclaimed","claim_id":"C2","kind":"weakest_assumption","source":"verdict.weakest_assumption","status":"machine_extracted","text":"That the CPL parametrization is sufficiently flexible to describe any smooth dark energy evolution consistent with the data, and that residual fiducial dependence in the published DESI distances is truly negligible at the 0.3% level."},{"attestation":"unclaimed","claim_id":"C3","kind":"one_line_summary","source":"verdict.one_line_summary","status":"machine_extracted","text":"No CMB-consistent CPL dark energy model can simultaneously fit both the BAOtr and DESI datasets; the 3.7-sigma disagreement at z=0.51 sets an irreducible floor."},{"attestation":"unclaimed","claim_id":"C4","kind":"headline","source":"verdict.pith_extraction.headline","status":"machine_extracted","text":"BAOtr and DESI BAO datasets cannot be fit simultaneously by any CMB-consistent CPL dark energy model."}],"snapshot_sha256":"d5886926ab357386b4b9ddd5e918446267e49808669f4807b4b9e7b539848410"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/2604.11106/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"The fiducial-independent angular/transverse BAO dataset, obtained from two-point angular correlation functions in thin redshift shells (hereafter BAOtr), systematically prefers smaller comoving distance ratios $D_{\\rm M}/r_{\\rm d}$ than the DESI DR2 three-dimensional BAO measurements at $z \\lesssim 0.65$, driving dataset-dependent CPL dark-energy inferences and conflicting conclusions about the Hubble tension. We investigate whether this disagreement can be attributed to the $\\Lambda$CDM fiducial assumed in the 3D BAO pipeline, or resolved within the CPL parametrisation. We show that the publi","authors_text":"Ioannis Pantos, Leandros Perivolaropoulos","cross_cats":[],"headline":"BAOtr and DESI BAO datasets cannot be fit simultaneously by any CMB-consistent CPL dark energy model.","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-04-13T07:23:08Z","title":"On the origin of the BAOtr-DESI tension"},"references":{"count":85,"internal_anchors":5,"resolved_work":85,"sample":[{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":1,"title":"D. J. Eisenstein, W. Hu, M. Tegmark, Cosmic complementarity:H 0 andΩ m from combining CMB experiments and redshift surveys, Astro- phys. J. 504 (1998) L57–L60.arXiv:astro-ph/9805239,doi:10.1086/ 31158","work_id":"a5e8beed-40d8-4428-a0f2-809d8e001c87","year":1998},{"cited_arxiv_id":"astro-ph/0501171","doi":"","is_internal_anchor":false,"ref_index":2,"title":"Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies","work_id":"ce6a8c9a-70a6-448e-9706-59019b463903","year":2005},{"cited_arxiv_id":"","doi":"10.1046/j.1365-8711.1999.02369.x","is_internal_anchor":false,"ref_index":3,"title":"1999, MNRAS, 302, 81, doi: 10.1046/j.1365-8711.1999.02083.x","work_id":"4f7e2990-d16b-4b19-8801-2137d127eb2e","year":1999},{"cited_arxiv_id":"","doi":"10.1086/376983","is_internal_anchor":false,"ref_index":4,"title":"Probing dark energy using baryonic oscillations in the galaxy power spectrum as a cosmological ruler","work_id":"4ef2e2a0-34b5-4af2-ae19-a22d39b02cef","year":2003},{"cited_arxiv_id":"","doi":"10.1086/379122","is_internal_anchor":false,"ref_index":5,"title":"Probing dark energy with baryonic acoustic oscillations from future large galaxy redshift surveys","work_id":"995f6aed-c552-4267-a5d3-e0f105d7f1fe","year":2003}],"snapshot_sha256":"0fa09ee28760f228156d3f5c33e0c12f9bb43c1cd50e6eee1bcb09e28936135d"},"source":{"id":"2604.11106","kind":"arxiv","version":2},"verdict":{"created_at":"2026-05-10T15:50:55.626909Z","id":"ebf8af75-f57c-4375-a0ad-312d0550d7fe","model_set":{"reader":"grok-4.3"},"one_line_summary":"No CMB-consistent CPL dark energy model can simultaneously fit both the BAOtr and DESI datasets; the 3.7-sigma disagreement at z=0.51 sets an irreducible floor.","pipeline_version":"pith-pipeline@v0.9.0","pith_extraction_headline":"BAOtr and DESI BAO datasets cannot be fit simultaneously by any CMB-consistent CPL dark energy model.","strongest_claim":"No CMB-consistent CPL model fits both datasets simultaneously. The direct comparison at z = 0.510 sets an irreducible tension floor that no smooth modification of D_M(z) can remove.","weakest_assumption":"That the CPL parametrization is sufficiently flexible to describe any smooth dark energy evolution consistent with the data, and that residual fiducial dependence in the published DESI distances is truly negligible at the 0.3% level."}},"verdict_id":"ebf8af75-f57c-4375-a0ad-312d0550d7fe"}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:0e756f4ec43cc3a821f600d7c0b37f6b4a68f0e6950a7659e95a95f1b511bed9","target":"record","created_at":"2026-05-25T02:01:19Z","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":"a627af07d30ccae6d95031d66f1a50288fa3333dd8e3fc4301186d080a12d983","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-04-13T07:23:08Z","title_canon_sha256":"c8140b9968a5f5a47b86c2fc3dfd968c1018ddaae0b21fd13909d140bd8f4783"},"schema_version":"1.0","source":{"id":"2604.11106","kind":"arxiv","version":2}},"canonical_sha256":"d75d0bed19d0243a8e2394d2b4172e154f7eeca24ac5965444b11ae80111537e","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"d75d0bed19d0243a8e2394d2b4172e154f7eeca24ac5965444b11ae80111537e","first_computed_at":"2026-05-25T02:01:19.378618Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-25T02:01:19.378618Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"s43bWG9puGlCGjQlRcVrw22qzWK8Sh4L4McEXqRTxEwVcSz6dG9LOWyVMj6IFhoQF6AdNia9TaHyMlWkiklBCg==","signature_status":"signed_v1","signed_at":"2026-05-25T02:01:19.379574Z","signed_message":"canonical_sha256_bytes"},"source_id":"2604.11106","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:0e756f4ec43cc3a821f600d7c0b37f6b4a68f0e6950a7659e95a95f1b511bed9","sha256:c225c6ebc2823405ff906699410fc91661aa650af45f095e54017619c34ffec0"],"state_sha256":"9e4a26baf13b43ebf430eeb8680bb1ff207c20b8f318166debb19c3b5627a9c2"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"SB+7AYr/1WKEquXjeILoIBiCjK236g9AanTdDqt8/LE2P1Yx2iEldQCrS2UD0DkkILVodKuk58jH+fUUYf/aCQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-10T08:07:09.064197Z","bundle_sha256":"7baad5c9dc44a1b9d895e0601200f18742e021a3ecf78221047aaa750b5ac64d"}}