{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2026:NFTHIGJ2KY4EIDM5WWI23CPPPO","short_pith_number":"pith:NFTHIGJ2","canonical_record":{"source":{"id":"2605.13298","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-05-13T10:12:06Z","cross_cats_sorted":[],"title_canon_sha256":"94bc6c33096b53d7522b7ed9966cf09385b90c120e307679ec367fccf2fbc304","abstract_canon_sha256":"b06f2570b8ac42355a8b2ac3844ec4119893fa5fb7306545444f8a63b2f7a814"},"schema_version":"1.0"},"canonical_sha256":"696674193a5638440d9db591ad89ef7ba7761d4be8af97c72beddee0de7f021f","source":{"kind":"arxiv","id":"2605.13298","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2605.13298","created_at":"2026-05-18T02:44:49Z"},{"alias_kind":"arxiv_version","alias_value":"2605.13298v1","created_at":"2026-05-18T02:44:49Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.13298","created_at":"2026-05-18T02:44:49Z"},{"alias_kind":"pith_short_12","alias_value":"NFTHIGJ2KY4E","created_at":"2026-05-18T12:33:37Z"},{"alias_kind":"pith_short_16","alias_value":"NFTHIGJ2KY4EIDM5","created_at":"2026-05-18T12:33:37Z"},{"alias_kind":"pith_short_8","alias_value":"NFTHIGJ2","created_at":"2026-05-18T12:33:37Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2026:NFTHIGJ2KY4EIDM5WWI23CPPPO","target":"record","payload":{"canonical_record":{"source":{"id":"2605.13298","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-05-13T10:12:06Z","cross_cats_sorted":[],"title_canon_sha256":"94bc6c33096b53d7522b7ed9966cf09385b90c120e307679ec367fccf2fbc304","abstract_canon_sha256":"b06f2570b8ac42355a8b2ac3844ec4119893fa5fb7306545444f8a63b2f7a814"},"schema_version":"1.0"},"canonical_sha256":"696674193a5638440d9db591ad89ef7ba7761d4be8af97c72beddee0de7f021f","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:44:49.066880Z","signature_b64":"fNl2p8QwWVx1SVShRhyzdJ8oCyHDYPu1gsFXGSc8HAbrLgHlFi4PzPw9J7/J7v/Mr2AcZXm51RzyTEBML2mdCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"696674193a5638440d9db591ad89ef7ba7761d4be8af97c72beddee0de7f021f","last_reissued_at":"2026-05-18T02:44:49.066452Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:44:49.066452Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"2605.13298","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":"2026-05-18T02:44:49Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"HepwOxbd6xHRhsSsg69caNnAtseJMTsn1KbRwY0Ygxy3WoPYDSKU/ekfYU0INvbX8wTULl966bmykU/yNFULBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-08T19:06:22.095243Z"},"content_sha256":"f1a9dcde300a22db061f27413c55f424daf363744dbff1e27f828f9874c65d55","schema_version":"1.0","event_id":"sha256:f1a9dcde300a22db061f27413c55f424daf363744dbff1e27f828f9874c65d55"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2026:NFTHIGJ2KY4EIDM5WWI23CPPPO","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Probing nonlinear structure formation beyond $\\Lambda$CDM with the LSS bootstrap: a joint power spectrum and bispectrum analysis","license":"http://creativecommons.org/licenses/by/4.0/","headline":"The LSS bootstrap yields first MCMC constraints on deviations from ΛCDM using power spectrum and bispectrum.","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Giorgia Biselli, Guido D'Amico, Marco Marinucci, Massimo Pietroni","submitted_at":"2026-05-13T10:12:06Z","abstract_excerpt":"We present the first MCMC-derived constraints on the parameters of the Large Scale Structure (LSS) bootstrap, a model-independent framework that captures deviations from $\\Lambda$CDM using symmetry arguments alone. Focusing on modifications to the linear growth rate and to the quadratic perturbation-theory kernel -- quantified by the fractional parameters $\\varepsilon_f$ and $\\varepsilon_{d_{\\gamma}}$, respectively -- we carry out a joint analysis of the one-loop galaxy power spectrum and the tree-level bispectrum multipoles within the EFTofLSS, employing the \\texttt{PyBird} code extended to i"},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"We present the first MCMC-derived constraints on the parameters of the Large Scale Structure (LSS) bootstrap... For BOSS, combining the power spectrum with the bispectrum monopole yields ∼7% constraints on ε_f and ∼57% constraints on ε_{d_γ}.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"The LSS bootstrap parametrization, based on symmetry arguments alone, correctly captures all relevant deviations from ΛCDM in the linear growth rate and quadratic perturbation-theory kernel for the scales probed by BOSS and PT Challenge data.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"First MCMC constraints on LSS bootstrap parameters yield ~7% precision on linear growth modifications and ~57% on quadratic kernel modifications from BOSS data, improving to 1% and 25% with larger simulations.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"The LSS bootstrap yields first MCMC constraints on deviations from ΛCDM using power spectrum and bispectrum.","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"1f00f1b131e31d8408ef4a58fc2d8075dc351f16c30bf280fa7888306d5bccb5"},"source":{"id":"2605.13298","kind":"arxiv","version":1},"verdict":{"id":"0ed59910-a490-4b1c-888e-d8775288dad2","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-14T17:33:25.853949Z","strongest_claim":"We present the first MCMC-derived constraints on the parameters of the Large Scale Structure (LSS) bootstrap... For BOSS, combining the power spectrum with the bispectrum monopole yields ∼7% constraints on ε_f and ∼57% constraints on ε_{d_γ}.","one_line_summary":"First MCMC constraints on LSS bootstrap parameters yield ~7% precision on linear growth modifications and ~57% on quadratic kernel modifications from BOSS data, improving to 1% and 25% with larger simulations.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"The LSS bootstrap parametrization, based on symmetry arguments alone, correctly captures all relevant deviations from ΛCDM in the linear growth rate and quadratic perturbation-theory kernel for the scales probed by BOSS and PT Challenge data.","pith_extraction_headline":"The LSS bootstrap yields first MCMC constraints on deviations from ΛCDM using power spectrum and bispectrum."},"references":{"count":72,"sample":[{"doi":"","year":2048,"title":"(see also [13]), which provided the initial Fisher-matrix forecasts for these parameters for a Euclid-like survey. Here, we perform a state-of-the-art combined analysis of the one-loop galaxy power sp","work_id":"f3159602-e0f9-481a-a887-b4f2655fc8a9","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":null,"title":"we leave it free (only for the BOSS analysis)","work_id":"e2d6b48b-2966-4e1f-a0de-b4b354ec347b","ref_index":2,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":null,"title":"we fixln (1010As) = 3.0448, thePlanckbest-fit value [39], for the BOSS analysis, and to the true value used in the simulations for the PT Challenge","work_id":"34e70151-9fe2-4d26-bf53-5bf8d1f0fa71","ref_index":3,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2048,"title":"we instead adopt a Gaussian prior onAs with a width equal to3σof thePlanckuncertainty [ 39], following refs. [40, 41]. Given thatPlanck’s uncertainty onAs is extremely small, fixingAs or applying a3σG","work_id":"99b7eb15-1e65-4a53-84be-4d0be65f4296","ref_index":4,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2025,"title":"Y. Mellieret al.(Euclid), Euclid. I. Overview of the Euclid mission, Astron. Astrophys.697, A1 (2025), arXiv:2405.13491 [astro-ph.CO]","work_id":"15ed38b8-e601-4fbb-b3c5-a0d8b595c401","ref_index":5,"cited_arxiv_id":"","is_internal_anchor":false}],"resolved_work":72,"snapshot_sha256":"13f8acc33674def4370f52b7f0ed5acb7928f2a8f5e16e71228b4ef7091654e0","internal_anchors":22},"formal_canon":{"evidence_count":2,"snapshot_sha256":"8aefcfd0463bfcb4dbfe4ef987e281b3b9b4298e1166d8fa59d052e86b9f62e1"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"verdict_id":"0ed59910-a490-4b1c-888e-d8775288dad2"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:44:49Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"d7R0kOHuRZKi/eYrygFD78lT/TAl/G8l940rQoAEWe2piT6m+/VnH+XEA4xALchTThKhcQ6sVTtZYVjLoMxUAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-08T19:06:22.096425Z"},"content_sha256":"8406a677d393bdb978e6ba3c0c4353cce8bedb6d25da13cb6e813aec854b7141","schema_version":"1.0","event_id":"sha256:8406a677d393bdb978e6ba3c0c4353cce8bedb6d25da13cb6e813aec854b7141"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/NFTHIGJ2KY4EIDM5WWI23CPPPO/bundle.json","state_url":"https://pith.science/pith/NFTHIGJ2KY4EIDM5WWI23CPPPO/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/NFTHIGJ2KY4EIDM5WWI23CPPPO/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":"2026-06-08T19:06:22Z","links":{"resolver":"https://pith.science/pith/NFTHIGJ2KY4EIDM5WWI23CPPPO","bundle":"https://pith.science/pith/NFTHIGJ2KY4EIDM5WWI23CPPPO/bundle.json","state":"https://pith.science/pith/NFTHIGJ2KY4EIDM5WWI23CPPPO/state.json","well_known_bundle":"https://pith.science/.well-known/pith/NFTHIGJ2KY4EIDM5WWI23CPPPO/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2026:NFTHIGJ2KY4EIDM5WWI23CPPPO","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":"b06f2570b8ac42355a8b2ac3844ec4119893fa5fb7306545444f8a63b2f7a814","cross_cats_sorted":[],"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-05-13T10:12:06Z","title_canon_sha256":"94bc6c33096b53d7522b7ed9966cf09385b90c120e307679ec367fccf2fbc304"},"schema_version":"1.0","source":{"id":"2605.13298","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2605.13298","created_at":"2026-05-18T02:44:49Z"},{"alias_kind":"arxiv_version","alias_value":"2605.13298v1","created_at":"2026-05-18T02:44:49Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.13298","created_at":"2026-05-18T02:44:49Z"},{"alias_kind":"pith_short_12","alias_value":"NFTHIGJ2KY4E","created_at":"2026-05-18T12:33:37Z"},{"alias_kind":"pith_short_16","alias_value":"NFTHIGJ2KY4EIDM5","created_at":"2026-05-18T12:33:37Z"},{"alias_kind":"pith_short_8","alias_value":"NFTHIGJ2","created_at":"2026-05-18T12:33:37Z"}],"graph_snapshots":[{"event_id":"sha256:8406a677d393bdb978e6ba3c0c4353cce8bedb6d25da13cb6e813aec854b7141","target":"graph","created_at":"2026-05-18T02:44:49Z","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":"We present the first MCMC-derived constraints on the parameters of the Large Scale Structure (LSS) bootstrap... For BOSS, combining the power spectrum with the bispectrum monopole yields ∼7% constraints on ε_f and ∼57% constraints on ε_{d_γ}."},{"attestation":"unclaimed","claim_id":"C2","kind":"weakest_assumption","source":"verdict.weakest_assumption","status":"machine_extracted","text":"The LSS bootstrap parametrization, based on symmetry arguments alone, correctly captures all relevant deviations from ΛCDM in the linear growth rate and quadratic perturbation-theory kernel for the scales probed by BOSS and PT Challenge data."},{"attestation":"unclaimed","claim_id":"C3","kind":"one_line_summary","source":"verdict.one_line_summary","status":"machine_extracted","text":"First MCMC constraints on LSS bootstrap parameters yield ~7% precision on linear growth modifications and ~57% on quadratic kernel modifications from BOSS data, improving to 1% and 25% with larger simulations."},{"attestation":"unclaimed","claim_id":"C4","kind":"headline","source":"verdict.pith_extraction.headline","status":"machine_extracted","text":"The LSS bootstrap yields first MCMC constraints on deviations from ΛCDM using power spectrum and bispectrum."}],"snapshot_sha256":"1f00f1b131e31d8408ef4a58fc2d8075dc351f16c30bf280fa7888306d5bccb5"},"formal_canon":{"evidence_count":2,"snapshot_sha256":"8aefcfd0463bfcb4dbfe4ef987e281b3b9b4298e1166d8fa59d052e86b9f62e1"},"paper":{"abstract_excerpt":"We present the first MCMC-derived constraints on the parameters of the Large Scale Structure (LSS) bootstrap, a model-independent framework that captures deviations from $\\Lambda$CDM using symmetry arguments alone. Focusing on modifications to the linear growth rate and to the quadratic perturbation-theory kernel -- quantified by the fractional parameters $\\varepsilon_f$ and $\\varepsilon_{d_{\\gamma}}$, respectively -- we carry out a joint analysis of the one-loop galaxy power spectrum and the tree-level bispectrum multipoles within the EFTofLSS, employing the \\texttt{PyBird} code extended to i","authors_text":"Giorgia Biselli, Guido D'Amico, Marco Marinucci, Massimo Pietroni","cross_cats":[],"headline":"The LSS bootstrap yields first MCMC constraints on deviations from ΛCDM using power spectrum and bispectrum.","license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-05-13T10:12:06Z","title":"Probing nonlinear structure formation beyond $\\Lambda$CDM with the LSS bootstrap: a joint power spectrum and bispectrum analysis"},"references":{"count":72,"internal_anchors":22,"resolved_work":72,"sample":[{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":1,"title":"(see also [13]), which provided the initial Fisher-matrix forecasts for these parameters for a Euclid-like survey. Here, we perform a state-of-the-art combined analysis of the one-loop galaxy power sp","work_id":"f3159602-e0f9-481a-a887-b4f2655fc8a9","year":2048},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":2,"title":"we leave it free (only for the BOSS analysis)","work_id":"e2d6b48b-2966-4e1f-a0de-b4b354ec347b","year":null},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":3,"title":"we fixln (1010As) = 3.0448, thePlanckbest-fit value [39], for the BOSS analysis, and to the true value used in the simulations for the PT Challenge","work_id":"34e70151-9fe2-4d26-bf53-5bf8d1f0fa71","year":null},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":4,"title":"we instead adopt a Gaussian prior onAs with a width equal to3σof thePlanckuncertainty [ 39], following refs. [40, 41]. Given thatPlanck’s uncertainty onAs is extremely small, fixingAs or applying a3σG","work_id":"99b7eb15-1e65-4a53-84be-4d0be65f4296","year":2048},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":5,"title":"Y. Mellieret al.(Euclid), Euclid. I. Overview of the Euclid mission, Astron. Astrophys.697, A1 (2025), arXiv:2405.13491 [astro-ph.CO]","work_id":"15ed38b8-e601-4fbb-b3c5-a0d8b595c401","year":2025}],"snapshot_sha256":"13f8acc33674def4370f52b7f0ed5acb7928f2a8f5e16e71228b4ef7091654e0"},"source":{"id":"2605.13298","kind":"arxiv","version":1},"verdict":{"created_at":"2026-05-14T17:33:25.853949Z","id":"0ed59910-a490-4b1c-888e-d8775288dad2","model_set":{"reader":"grok-4.3"},"one_line_summary":"First MCMC constraints on LSS bootstrap parameters yield ~7% precision on linear growth modifications and ~57% on quadratic kernel modifications from BOSS data, improving to 1% and 25% with larger simulations.","pipeline_version":"pith-pipeline@v0.9.0","pith_extraction_headline":"The LSS bootstrap yields first MCMC constraints on deviations from ΛCDM using power spectrum and bispectrum.","strongest_claim":"We present the first MCMC-derived constraints on the parameters of the Large Scale Structure (LSS) bootstrap... For BOSS, combining the power spectrum with the bispectrum monopole yields ∼7% constraints on ε_f and ∼57% constraints on ε_{d_γ}.","weakest_assumption":"The LSS bootstrap parametrization, based on symmetry arguments alone, correctly captures all relevant deviations from ΛCDM in the linear growth rate and quadratic perturbation-theory kernel for the scales probed by BOSS and PT Challenge data."}},"verdict_id":"0ed59910-a490-4b1c-888e-d8775288dad2"}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:f1a9dcde300a22db061f27413c55f424daf363744dbff1e27f828f9874c65d55","target":"record","created_at":"2026-05-18T02:44:49Z","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":"b06f2570b8ac42355a8b2ac3844ec4119893fa5fb7306545444f8a63b2f7a814","cross_cats_sorted":[],"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-05-13T10:12:06Z","title_canon_sha256":"94bc6c33096b53d7522b7ed9966cf09385b90c120e307679ec367fccf2fbc304"},"schema_version":"1.0","source":{"id":"2605.13298","kind":"arxiv","version":1}},"canonical_sha256":"696674193a5638440d9db591ad89ef7ba7761d4be8af97c72beddee0de7f021f","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"696674193a5638440d9db591ad89ef7ba7761d4be8af97c72beddee0de7f021f","first_computed_at":"2026-05-18T02:44:49.066452Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:44:49.066452Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"fNl2p8QwWVx1SVShRhyzdJ8oCyHDYPu1gsFXGSc8HAbrLgHlFi4PzPw9J7/J7v/Mr2AcZXm51RzyTEBML2mdCQ==","signature_status":"signed_v1","signed_at":"2026-05-18T02:44:49.066880Z","signed_message":"canonical_sha256_bytes"},"source_id":"2605.13298","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:f1a9dcde300a22db061f27413c55f424daf363744dbff1e27f828f9874c65d55","sha256:8406a677d393bdb978e6ba3c0c4353cce8bedb6d25da13cb6e813aec854b7141"],"state_sha256":"3be6c8fe9e84ef3e852fc7be712eb6469992bda9c286fae05a8e8de570d659aa"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"mUK+J4KbRIxSyBWvxDFzyy4gRaeqtRaymztL5W7r9YltXVkX3h4lk7bv4cjRfQ9YQoSi5bwmiz5qOE/8hs1xAA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-08T19:06:22.101781Z","bundle_sha256":"44663293763634640b12bd56972f1d3159cac8407d186281eee30276d423f0f1"}}