{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2026:K6JASXGVW2NJCF4VUU6H675U33","short_pith_number":"pith:K6JASXGV","canonical_record":{"source":{"id":"2605.16498","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2026-05-15T18:00:06Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"323f79640f770606c8de0963753523403f9ba74044e5815a1285dc3a02c1492a","abstract_canon_sha256":"4d88cda7f521938a011daeb55930024704862d6985929e55026ea2dca6bcbf03"},"schema_version":"1.0"},"canonical_sha256":"5792095cd5b69a911795a53c7f7fb4decccd53ec5faf10a3af768c513f2af5a4","source":{"kind":"arxiv","id":"2605.16498","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2605.16498","created_at":"2026-05-20T00:02:25Z"},{"alias_kind":"arxiv_version","alias_value":"2605.16498v1","created_at":"2026-05-20T00:02:25Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.16498","created_at":"2026-05-20T00:02:25Z"},{"alias_kind":"pith_short_12","alias_value":"K6JASXGVW2NJ","created_at":"2026-05-20T00:02:25Z"},{"alias_kind":"pith_short_16","alias_value":"K6JASXGVW2NJCF4V","created_at":"2026-05-20T00:02:25Z"},{"alias_kind":"pith_short_8","alias_value":"K6JASXGV","created_at":"2026-05-20T00:02:25Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2026:K6JASXGVW2NJCF4VUU6H675U33","target":"record","payload":{"canonical_record":{"source":{"id":"2605.16498","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2026-05-15T18:00:06Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"323f79640f770606c8de0963753523403f9ba74044e5815a1285dc3a02c1492a","abstract_canon_sha256":"4d88cda7f521938a011daeb55930024704862d6985929e55026ea2dca6bcbf03"},"schema_version":"1.0"},"canonical_sha256":"5792095cd5b69a911795a53c7f7fb4decccd53ec5faf10a3af768c513f2af5a4","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-20T00:02:25.750455Z","signature_b64":"RdUzBN5m/9VNgOr8ASOOAuWMd80tG6sRfkCXAp6orq/kPrgC6Zw0iD1yIUhypzSuvdADBnXr31PgnfUOC6ScBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5792095cd5b69a911795a53c7f7fb4decccd53ec5faf10a3af768c513f2af5a4","last_reissued_at":"2026-05-20T00:02:25.749607Z","signature_status":"signed_v1","first_computed_at":"2026-05-20T00:02:25.749607Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"2605.16498","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":"2026-05-20T00:02:25Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"PenR9N6Pu3iMv5OLvyXurlahy+EnXEHXxnfiiL61vRx3bz19kcFaA6yeYMeBGuuDJZ/TRctPxuHnAzUWDgCoDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-20T15:18:27.746747Z"},"content_sha256":"ef03d146b071ad3a017db602f4b4298336ea5dc3b30f521d394c007bd2ae4492","schema_version":"1.0","event_id":"sha256:ef03d146b071ad3a017db602f4b4298336ea5dc3b30f521d394c007bd2ae4492"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2026:K6JASXGVW2NJCF4VUU6H675U33","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Searching for the Third Wheel: High-Contrast Imaging Constraints on Tertiaries to Black Hole and Neutron Star Binaries","license":"http://creativecommons.org/licenses/by/4.0/","headline":"Deep imaging rules out main-sequence and hot white-dwarf tertiaries to black hole and neutron star binaries at large separations.","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Aniket Sanghi, Kareem El-Badry, Pranav Nagarajan","submitted_at":"2026-05-15T18:00:06Z","abstract_excerpt":"Hierarchical triple evolution provides a promising alternative to isolated binary formation models for black holes (BHs) and neutron stars (NSs) with low-mass stellar companions. To search for tertiaries, we perform deep, adaptive optics-assisted, near-infrared imaging of five quiescent BH low-mass X-ray binaries (LMXBs), Gaia BH1, and twelve Gaia NSs. We detect several faint stars previously unresolved in survey imaging, but none are close enough to robustly rule out a chance alignment. To achieve high contrast sensitivity at close separations, we use the reference star differential imaging s"},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"We rule out plausible MS tertiaries and young, hot WD tertiaries at projected separations ≳500 au for the Gaia compact object binaries and ≳2000 au for the more distant BH LMXBs.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"That the injection-recovery tests and contrast curves accurately capture the true sensitivity to bound companions rather than being dominated by residual speckles or unaccounted systematics at the smallest separations.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"High-contrast imaging of 18 compact-object binaries yields no robust tertiary detections and rules out main-sequence tertiaries at projected separations greater than 500 au for Gaia systems and 2000 au for BH LMXBs.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"Deep imaging rules out main-sequence and hot white-dwarf tertiaries to black hole and neutron star binaries at large separations.","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"69cb4a013d9fcb1671dc6192633a215076647d6eea5a7c0b0e37dfe7609f48d6"},"source":{"id":"2605.16498","kind":"arxiv","version":1},"verdict":{"id":"2dcc6902-c265-4578-bf59-bfeb8b9f9ce0","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-19T21:52:50.180936Z","strongest_claim":"We rule out plausible MS tertiaries and young, hot WD tertiaries at projected separations ≳500 au for the Gaia compact object binaries and ≳2000 au for the more distant BH LMXBs.","one_line_summary":"High-contrast imaging of 18 compact-object binaries yields no robust tertiary detections and rules out main-sequence tertiaries at projected separations greater than 500 au for Gaia systems and 2000 au for BH LMXBs.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"That the injection-recovery tests and contrast curves accurately capture the true sensitivity to bound companions rather than being dominated by residual speckles or unaccounted systematics at the smallest separations.","pith_extraction_headline":"Deep imaging rules out main-sequence and hot white-dwarf tertiaries to black hole and neutron star binaries at large separations."},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2605.16498/integrity.json","findings":[],"available":true,"detectors_run":[{"name":"doi_compliance","ran_at":"2026-05-19T22:01:30.018305Z","status":"completed","version":"1.0.0","findings_count":0},{"name":"doi_title_agreement","ran_at":"2026-05-19T22:01:23.157195Z","status":"completed","version":"1.0.0","findings_count":0},{"name":"ai_meta_artifact","ran_at":"2026-05-19T19:33:23.099446Z","status":"skipped","version":"1.0.0","findings_count":0},{"name":"claim_evidence","ran_at":"2026-05-19T19:21:57.008458Z","status":"completed","version":"1.0.0","findings_count":0}],"snapshot_sha256":"00ec589b17ea2f4a43db83c53d6995f841295d56a47c6e9b74f1cbd14c37119f"},"references":{"count":81,"sample":[{"doi":"10.1007/s00159-010-0033-1","year":2010,"title":"G., C \\'o rsico , A","work_id":"72daf4bd-03f3-4003-8cd1-71b439f578b9","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"10.1093/mnras/stz2335","year":2019,"title":"Atri, P., Miller-Jones, J. C. A., Bahramian, A., et al. 2019, Monthly Notices of the Royal Astronomical Society, 489, 3116, doi: 10.1093/mnras/stz2335","work_id":"9313fb44-37e5-4a4c-95c8-6c6fd35ba5bb","ref_index":2,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"10.1093/mnrasl/slaa010","year":2020,"title":"Atri, P., Miller-Jones, J. C. A., Bahramian, A., et al. 2020, Modern Notices of the Royal Astronomical Society, 493, L81, doi: 10.1093/mnrasl/slaa010","work_id":"2298982b-ba5a-40ff-8f46-3bdcbac41830","ref_index":3,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"10.1007/978-981-16-4544-0","year":2023,"title":"doi:10.1007/978-981-16-4544-0\\_151-1","work_id":"63f67c3b-d368-447b-acfd-b25c94055b58","ref_index":4,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"10.3847/1538-3881/abd806","year":null,"title":"Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3","work_id":"11e3916b-515c-4528-8feb-7528b967b896","ref_index":6,"cited_arxiv_id":"2012.05220","is_internal_anchor":true}],"resolved_work":81,"snapshot_sha256":"3fa7a28a2c586de5332d88db1bd6d4783dfca5ec73f13c4a560471a1cdc0b8b3","internal_anchors":6},"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":"2dcc6902-c265-4578-bf59-bfeb8b9f9ce0"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-20T00:02:25Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"kCI101jQ5gx92gI0+Yugs0FQg/mLFx1FsVQHzlzfYqX4esUydiDqK2q002neGNY2wVqGdSMwMOGIVW9tg8wxBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-20T15:18:27.747482Z"},"content_sha256":"f1b95dd161b3978d911584ed4f684998f5967e1e9f0784552c83bba74e143e98","schema_version":"1.0","event_id":"sha256:f1b95dd161b3978d911584ed4f684998f5967e1e9f0784552c83bba74e143e98"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/K6JASXGVW2NJCF4VUU6H675U33/bundle.json","state_url":"https://pith.science/pith/K6JASXGVW2NJCF4VUU6H675U33/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/K6JASXGVW2NJCF4VUU6H675U33/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":"2026-05-20T15:18:27Z","links":{"resolver":"https://pith.science/pith/K6JASXGVW2NJCF4VUU6H675U33","bundle":"https://pith.science/pith/K6JASXGVW2NJCF4VUU6H675U33/bundle.json","state":"https://pith.science/pith/K6JASXGVW2NJCF4VUU6H675U33/state.json","well_known_bundle":"https://pith.science/.well-known/pith/K6JASXGVW2NJCF4VUU6H675U33/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2026:K6JASXGVW2NJCF4VUU6H675U33","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":"4d88cda7f521938a011daeb55930024704862d6985929e55026ea2dca6bcbf03","cross_cats_sorted":["astro-ph.HE"],"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2026-05-15T18:00:06Z","title_canon_sha256":"323f79640f770606c8de0963753523403f9ba74044e5815a1285dc3a02c1492a"},"schema_version":"1.0","source":{"id":"2605.16498","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2605.16498","created_at":"2026-05-20T00:02:25Z"},{"alias_kind":"arxiv_version","alias_value":"2605.16498v1","created_at":"2026-05-20T00:02:25Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.16498","created_at":"2026-05-20T00:02:25Z"},{"alias_kind":"pith_short_12","alias_value":"K6JASXGVW2NJ","created_at":"2026-05-20T00:02:25Z"},{"alias_kind":"pith_short_16","alias_value":"K6JASXGVW2NJCF4V","created_at":"2026-05-20T00:02:25Z"},{"alias_kind":"pith_short_8","alias_value":"K6JASXGV","created_at":"2026-05-20T00:02:25Z"}],"graph_snapshots":[{"event_id":"sha256:f1b95dd161b3978d911584ed4f684998f5967e1e9f0784552c83bba74e143e98","target":"graph","created_at":"2026-05-20T00:02:25Z","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 rule out plausible MS tertiaries and young, hot WD tertiaries at projected separations ≳500 au for the Gaia compact object binaries and ≳2000 au for the more distant BH LMXBs."},{"attestation":"unclaimed","claim_id":"C2","kind":"weakest_assumption","source":"verdict.weakest_assumption","status":"machine_extracted","text":"That the injection-recovery tests and contrast curves accurately capture the true sensitivity to bound companions rather than being dominated by residual speckles or unaccounted systematics at the smallest separations."},{"attestation":"unclaimed","claim_id":"C3","kind":"one_line_summary","source":"verdict.one_line_summary","status":"machine_extracted","text":"High-contrast imaging of 18 compact-object binaries yields no robust tertiary detections and rules out main-sequence tertiaries at projected separations greater than 500 au for Gaia systems and 2000 au for BH LMXBs."},{"attestation":"unclaimed","claim_id":"C4","kind":"headline","source":"verdict.pith_extraction.headline","status":"machine_extracted","text":"Deep imaging rules out main-sequence and hot white-dwarf tertiaries to black hole and neutron star binaries at large separations."}],"snapshot_sha256":"69cb4a013d9fcb1671dc6192633a215076647d6eea5a7c0b0e37dfe7609f48d6"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"integrity":{"available":true,"clean":true,"detectors_run":[{"findings_count":0,"name":"doi_compliance","ran_at":"2026-05-19T22:01:30.018305Z","status":"completed","version":"1.0.0"},{"findings_count":0,"name":"doi_title_agreement","ran_at":"2026-05-19T22:01:23.157195Z","status":"completed","version":"1.0.0"},{"findings_count":0,"name":"ai_meta_artifact","ran_at":"2026-05-19T19:33:23.099446Z","status":"skipped","version":"1.0.0"},{"findings_count":0,"name":"claim_evidence","ran_at":"2026-05-19T19:21:57.008458Z","status":"completed","version":"1.0.0"}],"endpoint":"/pith/2605.16498/integrity.json","findings":[],"snapshot_sha256":"00ec589b17ea2f4a43db83c53d6995f841295d56a47c6e9b74f1cbd14c37119f","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"Hierarchical triple evolution provides a promising alternative to isolated binary formation models for black holes (BHs) and neutron stars (NSs) with low-mass stellar companions. To search for tertiaries, we perform deep, adaptive optics-assisted, near-infrared imaging of five quiescent BH low-mass X-ray binaries (LMXBs), Gaia BH1, and twelve Gaia NSs. We detect several faint stars previously unresolved in survey imaging, but none are close enough to robustly rule out a chance alignment. To achieve high contrast sensitivity at close separations, we use the reference star differential imaging s","authors_text":"Aniket Sanghi, Kareem El-Badry, Pranav Nagarajan","cross_cats":["astro-ph.HE"],"headline":"Deep imaging rules out main-sequence and hot white-dwarf tertiaries to black hole and neutron star binaries at large separations.","license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2026-05-15T18:00:06Z","title":"Searching for the Third Wheel: High-Contrast Imaging Constraints on Tertiaries to Black Hole and Neutron Star Binaries"},"references":{"count":81,"internal_anchors":6,"resolved_work":81,"sample":[{"cited_arxiv_id":"","doi":"10.1007/s00159-010-0033-1","is_internal_anchor":false,"ref_index":1,"title":"G., C \\'o rsico , A","work_id":"72daf4bd-03f3-4003-8cd1-71b439f578b9","year":2010},{"cited_arxiv_id":"","doi":"10.1093/mnras/stz2335","is_internal_anchor":false,"ref_index":2,"title":"Atri, P., Miller-Jones, J. C. A., Bahramian, A., et al. 2019, Monthly Notices of the Royal Astronomical Society, 489, 3116, doi: 10.1093/mnras/stz2335","work_id":"9313fb44-37e5-4a4c-95c8-6c6fd35ba5bb","year":2019},{"cited_arxiv_id":"","doi":"10.1093/mnrasl/slaa010","is_internal_anchor":false,"ref_index":3,"title":"Atri, P., Miller-Jones, J. C. A., Bahramian, A., et al. 2020, Modern Notices of the Royal Astronomical Society, 493, L81, doi: 10.1093/mnrasl/slaa010","work_id":"2298982b-ba5a-40ff-8f46-3bdcbac41830","year":2020},{"cited_arxiv_id":"","doi":"10.1007/978-981-16-4544-0","is_internal_anchor":false,"ref_index":4,"title":"doi:10.1007/978-981-16-4544-0\\_151-1","work_id":"63f67c3b-d368-447b-acfd-b25c94055b58","year":2023},{"cited_arxiv_id":"2012.05220","doi":"10.3847/1538-3881/abd806","is_internal_anchor":true,"ref_index":6,"title":"Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3","work_id":"11e3916b-515c-4528-8feb-7528b967b896","year":null}],"snapshot_sha256":"3fa7a28a2c586de5332d88db1bd6d4783dfca5ec73f13c4a560471a1cdc0b8b3"},"source":{"id":"2605.16498","kind":"arxiv","version":1},"verdict":{"created_at":"2026-05-19T21:52:50.180936Z","id":"2dcc6902-c265-4578-bf59-bfeb8b9f9ce0","model_set":{"reader":"grok-4.3"},"one_line_summary":"High-contrast imaging of 18 compact-object binaries yields no robust tertiary detections and rules out main-sequence tertiaries at projected separations greater than 500 au for Gaia systems and 2000 au for BH LMXBs.","pipeline_version":"pith-pipeline@v0.9.0","pith_extraction_headline":"Deep imaging rules out main-sequence and hot white-dwarf tertiaries to black hole and neutron star binaries at large separations.","strongest_claim":"We rule out plausible MS tertiaries and young, hot WD tertiaries at projected separations ≳500 au for the Gaia compact object binaries and ≳2000 au for the more distant BH LMXBs.","weakest_assumption":"That the injection-recovery tests and contrast curves accurately capture the true sensitivity to bound companions rather than being dominated by residual speckles or unaccounted systematics at the smallest separations."}},"verdict_id":"2dcc6902-c265-4578-bf59-bfeb8b9f9ce0"}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:ef03d146b071ad3a017db602f4b4298336ea5dc3b30f521d394c007bd2ae4492","target":"record","created_at":"2026-05-20T00:02:25Z","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":"4d88cda7f521938a011daeb55930024704862d6985929e55026ea2dca6bcbf03","cross_cats_sorted":["astro-ph.HE"],"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2026-05-15T18:00:06Z","title_canon_sha256":"323f79640f770606c8de0963753523403f9ba74044e5815a1285dc3a02c1492a"},"schema_version":"1.0","source":{"id":"2605.16498","kind":"arxiv","version":1}},"canonical_sha256":"5792095cd5b69a911795a53c7f7fb4decccd53ec5faf10a3af768c513f2af5a4","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"5792095cd5b69a911795a53c7f7fb4decccd53ec5faf10a3af768c513f2af5a4","first_computed_at":"2026-05-20T00:02:25.749607Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-20T00:02:25.749607Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"RdUzBN5m/9VNgOr8ASOOAuWMd80tG6sRfkCXAp6orq/kPrgC6Zw0iD1yIUhypzSuvdADBnXr31PgnfUOC6ScBw==","signature_status":"signed_v1","signed_at":"2026-05-20T00:02:25.750455Z","signed_message":"canonical_sha256_bytes"},"source_id":"2605.16498","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:ef03d146b071ad3a017db602f4b4298336ea5dc3b30f521d394c007bd2ae4492","sha256:f1b95dd161b3978d911584ed4f684998f5967e1e9f0784552c83bba74e143e98"],"state_sha256":"11afee44328bdaa46fa88451f72b1db352d87dbddff986ad55f9d7c7f5d13e54"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"gHYnEvsvDEM/nhYtnV91RJ1RBNRo8pBE4BPb5VCAOQSZKtWgU2B+Zjw0jjilmL9HiadYlaskDUVU+X6BWV8XBA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-20T15:18:27.750296Z","bundle_sha256":"63711d1681e7db0849acffd6afb5f5987f1011dea392e7b60bc76978d0c66cd9"}}