{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2026:4NJO3H2RHKMYMSIZ3RA7TICSQI","short_pith_number":"pith:4NJO3H2R","canonical_record":{"source":{"id":"2605.14077","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-05-13T20:00:38Z","cross_cats_sorted":["astro-ph.EP","astro-ph.SR"],"title_canon_sha256":"05422384fdc671a3245edaa0c3f697faeb8c2b79ccfb3e0a97f239cf84c9b8a4","abstract_canon_sha256":"bd6930f4c468d2f7adf8ffcf8d8ac5132cde4db1f2808d5230badfe215fd69fb"},"schema_version":"1.0"},"canonical_sha256":"e352ed9f513a99864919dc41f9a0528213fb85198318ad1552ea0d556e2cb02d","source":{"kind":"arxiv","id":"2605.14077","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2605.14077","created_at":"2026-05-17T23:39:12Z"},{"alias_kind":"arxiv_version","alias_value":"2605.14077v1","created_at":"2026-05-17T23:39:12Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.14077","created_at":"2026-05-17T23:39:12Z"},{"alias_kind":"pith_short_12","alias_value":"4NJO3H2RHKMY","created_at":"2026-05-18T12:33:37Z"},{"alias_kind":"pith_short_16","alias_value":"4NJO3H2RHKMYMSIZ","created_at":"2026-05-18T12:33:37Z"},{"alias_kind":"pith_short_8","alias_value":"4NJO3H2R","created_at":"2026-05-18T12:33:37Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2026:4NJO3H2RHKMYMSIZ3RA7TICSQI","target":"record","payload":{"canonical_record":{"source":{"id":"2605.14077","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-05-13T20:00:38Z","cross_cats_sorted":["astro-ph.EP","astro-ph.SR"],"title_canon_sha256":"05422384fdc671a3245edaa0c3f697faeb8c2b79ccfb3e0a97f239cf84c9b8a4","abstract_canon_sha256":"bd6930f4c468d2f7adf8ffcf8d8ac5132cde4db1f2808d5230badfe215fd69fb"},"schema_version":"1.0"},"canonical_sha256":"e352ed9f513a99864919dc41f9a0528213fb85198318ad1552ea0d556e2cb02d","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:39:12.354043Z","signature_b64":"K+TMefaJHf/55rG+Lncu6nKA2Hx1qdfm4bOx14jcKNgM4FUhMhDbFMZqInH0N+UWcRDZr+SZGOgM6PEUil9IAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e352ed9f513a99864919dc41f9a0528213fb85198318ad1552ea0d556e2cb02d","last_reissued_at":"2026-05-17T23:39:12.353455Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:39:12.353455Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"2605.14077","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":"2026-05-17T23:39:12Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Mxc7cyqYz9gYV4rP3Bid/dpheIupo69cfnoETcXvYvD0WTzJEVDC9DvSPh4iwbXMLASCHKBuFcr3RjittN9dCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T07:34:39.249024Z"},"content_sha256":"ff2aa900deb57804268dfa8ddb033207fd6e8e9c7efd92acbf66742239195ab4","schema_version":"1.0","event_id":"sha256:ff2aa900deb57804268dfa8ddb033207fd6e8e9c7efd92acbf66742239195ab4"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2026:4NJO3H2RHKMYMSIZ3RA7TICSQI","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Planets in Pulsar Winds","license":"http://creativecommons.org/licenses/by/4.0/","headline":"A planet orbiting the pulsar PSR J0636+5129 could be detected through radio emission produced by its interaction with the pulsar wind.","cross_cats":["astro-ph.EP","astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"J. Varela, M. Falanga, M. \\v{C}emelji\\'c, M. Velli, P. Marmat, S. Andr\\'es Joya M\\'endez, T. Kaister","submitted_at":"2026-05-13T20:00:38Z","abstract_excerpt":"Planets around pulsars were the first discovered exoplanets, found thanks to the extremely precise pulsar timing. Here we suggest that they could also be found through the radio emission generated by the pulsar-planet magnetospheric interaction. We present the results of special relativistic numerical simulations of planets in a pulsar wind of velocity $v=0.985~c$, corresponding to a Lorentz factor $\\gamma=5.795$. Planets, modeled as a perfectly conducting solid surface in an external magnetic field originating from the pulsar, produce radio emission in the extended magnetic structure on the p"},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"We find that the planet around a known pulsar, PSR J0636+5129 b, could be detected via its radio emission.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"The planet is modeled as a perfectly conducting solid surface interacting with the pulsar's external magnetic field, producing radio emission specifically in the extended nightside magnetic structure that is observable without dominant interference.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"Special relativistic simulations predict detectable radio emission from nightside magnetic structures around planets in pulsar winds, including for the known planet PSR J0636+5129 b.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"A planet orbiting the pulsar PSR J0636+5129 could be detected through radio emission produced by its interaction with the pulsar wind.","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"e3908a1de852bbb28c9b7eecffb9d7acada58f3f54dfa9aaeab6209cff47ed5a"},"source":{"id":"2605.14077","kind":"arxiv","version":1},"verdict":{"id":"6c7882aa-7ccd-4307-b88a-5f6eaccf61dd","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-15T02:12:27.528390Z","strongest_claim":"We find that the planet around a known pulsar, PSR J0636+5129 b, could be detected via its radio emission.","one_line_summary":"Special relativistic simulations predict detectable radio emission from nightside magnetic structures around planets in pulsar winds, including for the known planet PSR J0636+5129 b.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"The planet is modeled as a perfectly conducting solid surface interacting with the pulsar's external magnetic field, producing radio emission specifically in the extended nightside magnetic structure that is observable without dominant interference.","pith_extraction_headline":"A planet orbiting the pulsar PSR J0636+5129 could be detected through radio emission produced by its interaction with the pulsar wind."},"references":{"count":20,"sample":[{"doi":"10.1038/nature10793","year":2012,"title":"Aharonian, F. A., Bogovalov, S. V ., & Khangulyan, D. 2012, Nature, 482, 507, doi: 10.1038/nature10793","work_id":"73b8d6d2-5d5d-4025-beeb-bd71f86c39b1","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"10.1051/eas:2006008","year":2006,"title":"2006, http://dx.doi.org/10.1051/eas:2006008, 464, doi: 10.1051/eas:2006008","work_id":"0dfef681-5e0c-4849-8504-084eedeb0ef1","ref_index":2,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"10.3847/2041-8213/ab8121","year":2020,"title":"Behrens, E. A. e. a. 2020, The Astrophysical Journal Letters, 893, L8, doi: 10.3847/2041-8213/ab8121","work_id":"3b5a9f93-cdd2-4cf9-9fb3-b584f5b15421","ref_index":3,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"10.1006/jcph.2001.6961","year":2002,"title":"2002, Journal of Computational Physics, 175, 645, doi: 10.1006/jcph.2001.6961","work_id":"4b0557bd-3a02-4d21-82fd-43f8e192e2ec","ref_index":4,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"10.1038/282383a0","year":1979,"title":"1979, Nature, 282, 383, doi: 10.1038/282383a0","work_id":"aead5502-0ef9-43f0-87e6-3ba368799993","ref_index":5,"cited_arxiv_id":"","is_internal_anchor":false}],"resolved_work":20,"snapshot_sha256":"b9c84908967866856259bbda8ccf27a3e5dba65d9fc8b182a0427e9ce9888802","internal_anchors":0},"formal_canon":{"evidence_count":2,"snapshot_sha256":"646f6d97be2deb7e2185cafd4a359ce2952b7d46a5b5d0e9c0416728628eca39"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"verdict_id":"6c7882aa-7ccd-4307-b88a-5f6eaccf61dd"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-17T23:39:12Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"FnYAN3R5FuvWJs2NynKff38mT7Tn0PxsVVJRIQSEf+61Yf54xNocr/Hk2ZXq6oOH/2VgEfHVg18wPhdhc8PvCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T07:34:39.249799Z"},"content_sha256":"d7c8499fabf4d5dd1ae87b1d6f951c8677fe774fbd2d014d73833f70cddd66ed","schema_version":"1.0","event_id":"sha256:d7c8499fabf4d5dd1ae87b1d6f951c8677fe774fbd2d014d73833f70cddd66ed"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/4NJO3H2RHKMYMSIZ3RA7TICSQI/bundle.json","state_url":"https://pith.science/pith/4NJO3H2RHKMYMSIZ3RA7TICSQI/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/4NJO3H2RHKMYMSIZ3RA7TICSQI/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":"2026-05-25T07:34:39Z","links":{"resolver":"https://pith.science/pith/4NJO3H2RHKMYMSIZ3RA7TICSQI","bundle":"https://pith.science/pith/4NJO3H2RHKMYMSIZ3RA7TICSQI/bundle.json","state":"https://pith.science/pith/4NJO3H2RHKMYMSIZ3RA7TICSQI/state.json","well_known_bundle":"https://pith.science/.well-known/pith/4NJO3H2RHKMYMSIZ3RA7TICSQI/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2026:4NJO3H2RHKMYMSIZ3RA7TICSQI","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":"bd6930f4c468d2f7adf8ffcf8d8ac5132cde4db1f2808d5230badfe215fd69fb","cross_cats_sorted":["astro-ph.EP","astro-ph.SR"],"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-05-13T20:00:38Z","title_canon_sha256":"05422384fdc671a3245edaa0c3f697faeb8c2b79ccfb3e0a97f239cf84c9b8a4"},"schema_version":"1.0","source":{"id":"2605.14077","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2605.14077","created_at":"2026-05-17T23:39:12Z"},{"alias_kind":"arxiv_version","alias_value":"2605.14077v1","created_at":"2026-05-17T23:39:12Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.14077","created_at":"2026-05-17T23:39:12Z"},{"alias_kind":"pith_short_12","alias_value":"4NJO3H2RHKMY","created_at":"2026-05-18T12:33:37Z"},{"alias_kind":"pith_short_16","alias_value":"4NJO3H2RHKMYMSIZ","created_at":"2026-05-18T12:33:37Z"},{"alias_kind":"pith_short_8","alias_value":"4NJO3H2R","created_at":"2026-05-18T12:33:37Z"}],"graph_snapshots":[{"event_id":"sha256:d7c8499fabf4d5dd1ae87b1d6f951c8677fe774fbd2d014d73833f70cddd66ed","target":"graph","created_at":"2026-05-17T23:39:12Z","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 find that the planet around a known pulsar, PSR J0636+5129 b, could be detected via its radio emission."},{"attestation":"unclaimed","claim_id":"C2","kind":"weakest_assumption","source":"verdict.weakest_assumption","status":"machine_extracted","text":"The planet is modeled as a perfectly conducting solid surface interacting with the pulsar's external magnetic field, producing radio emission specifically in the extended nightside magnetic structure that is observable without dominant interference."},{"attestation":"unclaimed","claim_id":"C3","kind":"one_line_summary","source":"verdict.one_line_summary","status":"machine_extracted","text":"Special relativistic simulations predict detectable radio emission from nightside magnetic structures around planets in pulsar winds, including for the known planet PSR J0636+5129 b."},{"attestation":"unclaimed","claim_id":"C4","kind":"headline","source":"verdict.pith_extraction.headline","status":"machine_extracted","text":"A planet orbiting the pulsar PSR J0636+5129 could be detected through radio emission produced by its interaction with the pulsar wind."}],"snapshot_sha256":"e3908a1de852bbb28c9b7eecffb9d7acada58f3f54dfa9aaeab6209cff47ed5a"},"formal_canon":{"evidence_count":2,"snapshot_sha256":"646f6d97be2deb7e2185cafd4a359ce2952b7d46a5b5d0e9c0416728628eca39"},"paper":{"abstract_excerpt":"Planets around pulsars were the first discovered exoplanets, found thanks to the extremely precise pulsar timing. Here we suggest that they could also be found through the radio emission generated by the pulsar-planet magnetospheric interaction. We present the results of special relativistic numerical simulations of planets in a pulsar wind of velocity $v=0.985~c$, corresponding to a Lorentz factor $\\gamma=5.795$. Planets, modeled as a perfectly conducting solid surface in an external magnetic field originating from the pulsar, produce radio emission in the extended magnetic structure on the p","authors_text":"J. Varela, M. Falanga, M. \\v{C}emelji\\'c, M. Velli, P. Marmat, S. Andr\\'es Joya M\\'endez, T. Kaister","cross_cats":["astro-ph.EP","astro-ph.SR"],"headline":"A planet orbiting the pulsar PSR J0636+5129 could be detected through radio emission produced by its interaction with the pulsar wind.","license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-05-13T20:00:38Z","title":"Planets in Pulsar Winds"},"references":{"count":20,"internal_anchors":0,"resolved_work":20,"sample":[{"cited_arxiv_id":"","doi":"10.1038/nature10793","is_internal_anchor":false,"ref_index":1,"title":"Aharonian, F. A., Bogovalov, S. V ., & Khangulyan, D. 2012, Nature, 482, 507, doi: 10.1038/nature10793","work_id":"73b8d6d2-5d5d-4025-beeb-bd71f86c39b1","year":2012},{"cited_arxiv_id":"","doi":"10.1051/eas:2006008","is_internal_anchor":false,"ref_index":2,"title":"2006, http://dx.doi.org/10.1051/eas:2006008, 464, doi: 10.1051/eas:2006008","work_id":"0dfef681-5e0c-4849-8504-084eedeb0ef1","year":2006},{"cited_arxiv_id":"","doi":"10.3847/2041-8213/ab8121","is_internal_anchor":false,"ref_index":3,"title":"Behrens, E. A. e. a. 2020, The Astrophysical Journal Letters, 893, L8, doi: 10.3847/2041-8213/ab8121","work_id":"3b5a9f93-cdd2-4cf9-9fb3-b584f5b15421","year":2020},{"cited_arxiv_id":"","doi":"10.1006/jcph.2001.6961","is_internal_anchor":false,"ref_index":4,"title":"2002, Journal of Computational Physics, 175, 645, doi: 10.1006/jcph.2001.6961","work_id":"4b0557bd-3a02-4d21-82fd-43f8e192e2ec","year":2002},{"cited_arxiv_id":"","doi":"10.1038/282383a0","is_internal_anchor":false,"ref_index":5,"title":"1979, Nature, 282, 383, doi: 10.1038/282383a0","work_id":"aead5502-0ef9-43f0-87e6-3ba368799993","year":1979}],"snapshot_sha256":"b9c84908967866856259bbda8ccf27a3e5dba65d9fc8b182a0427e9ce9888802"},"source":{"id":"2605.14077","kind":"arxiv","version":1},"verdict":{"created_at":"2026-05-15T02:12:27.528390Z","id":"6c7882aa-7ccd-4307-b88a-5f6eaccf61dd","model_set":{"reader":"grok-4.3"},"one_line_summary":"Special relativistic simulations predict detectable radio emission from nightside magnetic structures around planets in pulsar winds, including for the known planet PSR J0636+5129 b.","pipeline_version":"pith-pipeline@v0.9.0","pith_extraction_headline":"A planet orbiting the pulsar PSR J0636+5129 could be detected through radio emission produced by its interaction with the pulsar wind.","strongest_claim":"We find that the planet around a known pulsar, PSR J0636+5129 b, could be detected via its radio emission.","weakest_assumption":"The planet is modeled as a perfectly conducting solid surface interacting with the pulsar's external magnetic field, producing radio emission specifically in the extended nightside magnetic structure that is observable without dominant interference."}},"verdict_id":"6c7882aa-7ccd-4307-b88a-5f6eaccf61dd"}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:ff2aa900deb57804268dfa8ddb033207fd6e8e9c7efd92acbf66742239195ab4","target":"record","created_at":"2026-05-17T23:39:12Z","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":"bd6930f4c468d2f7adf8ffcf8d8ac5132cde4db1f2808d5230badfe215fd69fb","cross_cats_sorted":["astro-ph.EP","astro-ph.SR"],"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-05-13T20:00:38Z","title_canon_sha256":"05422384fdc671a3245edaa0c3f697faeb8c2b79ccfb3e0a97f239cf84c9b8a4"},"schema_version":"1.0","source":{"id":"2605.14077","kind":"arxiv","version":1}},"canonical_sha256":"e352ed9f513a99864919dc41f9a0528213fb85198318ad1552ea0d556e2cb02d","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"e352ed9f513a99864919dc41f9a0528213fb85198318ad1552ea0d556e2cb02d","first_computed_at":"2026-05-17T23:39:12.353455Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-17T23:39:12.353455Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"K+TMefaJHf/55rG+Lncu6nKA2Hx1qdfm4bOx14jcKNgM4FUhMhDbFMZqInH0N+UWcRDZr+SZGOgM6PEUil9IAw==","signature_status":"signed_v1","signed_at":"2026-05-17T23:39:12.354043Z","signed_message":"canonical_sha256_bytes"},"source_id":"2605.14077","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:ff2aa900deb57804268dfa8ddb033207fd6e8e9c7efd92acbf66742239195ab4","sha256:d7c8499fabf4d5dd1ae87b1d6f951c8677fe774fbd2d014d73833f70cddd66ed"],"state_sha256":"fc86513f1ce48761837a76ee7ad0eae2045f91c8658533697dcefe83755b8523"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"dZ790ePJU8wTXrCgNB0ssyfie1S83MhPLXegM26eTXtLpM8zUYGELFi58EvccW8N+X5FDqDKyurghcOZJICOBA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T07:34:39.253091Z","bundle_sha256":"3322349815e79322ff67a1487b850bed63e62f17115e1525c929076a6bef396a"}}