{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:L627Q6HFIYJUHIXDHZCSPP33BC","short_pith_number":"pith:L627Q6HF","canonical_record":{"source":{"id":"1304.3217","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-04-11T07:00:18Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"2000e4d958adad4598325894fc8abe51d9cc4b1ec9833f505636adbe3ba40300","abstract_canon_sha256":"7e38b82cc3cddfef3ba400d8f5a06ac61f2f66a886f3172b4db92909f553b378"},"schema_version":"1.0"},"canonical_sha256":"5fb5f878e5461343a2e33e4527bf7b089f7a0fdde960023eb57a9b301e58f8c0","source":{"kind":"arxiv","id":"1304.3217","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1304.3217","created_at":"2026-05-18T01:20:03Z"},{"alias_kind":"arxiv_version","alias_value":"1304.3217v2","created_at":"2026-05-18T01:20:03Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1304.3217","created_at":"2026-05-18T01:20:03Z"},{"alias_kind":"pith_short_12","alias_value":"L627Q6HFIYJU","created_at":"2026-05-18T12:27:51Z"},{"alias_kind":"pith_short_16","alias_value":"L627Q6HFIYJUHIXD","created_at":"2026-05-18T12:27:51Z"},{"alias_kind":"pith_short_8","alias_value":"L627Q6HF","created_at":"2026-05-18T12:27:51Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:L627Q6HFIYJUHIXDHZCSPP33BC","target":"record","payload":{"canonical_record":{"source":{"id":"1304.3217","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-04-11T07:00:18Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"2000e4d958adad4598325894fc8abe51d9cc4b1ec9833f505636adbe3ba40300","abstract_canon_sha256":"7e38b82cc3cddfef3ba400d8f5a06ac61f2f66a886f3172b4db92909f553b378"},"schema_version":"1.0"},"canonical_sha256":"5fb5f878e5461343a2e33e4527bf7b089f7a0fdde960023eb57a9b301e58f8c0","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:20:03.991622Z","signature_b64":"giL7idrgGYPRc9e3Vqks023atKHtDj90b4npHhiKk2vtg0qrikzJNcFEonO1+6XkL8Csws57/SLIDmAH/kHSBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5fb5f878e5461343a2e33e4527bf7b089f7a0fdde960023eb57a9b301e58f8c0","last_reissued_at":"2026-05-18T01:20:03.991044Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:20:03.991044Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1304.3217","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":"2026-05-18T01:20:03Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"seXOqsh3d0H6biXhAH6v6Sa08BdhWWVHAT0Dp7gNFBD2qvRefD5UyVt7xYz280V+9Gueo3WPyb/lGRctwMvACw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T17:00:13.513302Z"},"content_sha256":"8230a2fb96807265dd8eb70433a33d234c5253b106e9dd5b5395fcc6415e39db","schema_version":"1.0","event_id":"sha256:8230a2fb96807265dd8eb70433a33d234c5253b106e9dd5b5395fcc6415e39db"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:L627Q6HFIYJUHIXDHZCSPP33BC","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Mapping UHECRs deflections through the turbulent galactic magnetic field with the latest RM data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"F. R. Urban, M. S. Pshirkov, P. G. Tinyakov","submitted_at":"2013-04-11T07:00:18Z","abstract_excerpt":"We study the influence of the random part of the Galactic magnetic field on the propagation of ultra high-energy cosmic rays. Within very mild approximations about the properties of the electron density fluctuations in the Galaxy we are able to derive a clear and direct relation between the observed variance of rotation measures and the predicted cosmic ray deflections. Remarkably, this is obtained bypassing entirely the detailed knowledge of the magnetic properties of the turbulent plasma. Depending on the parameters of the electron density spectrum, we can either directly estimate the expect"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1304.3217","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"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":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:20:03Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"wQqZb+eldhLsteyYkIjp00UcxoRQCj9+nMYhTz66UrXESx+KI/qB10cXQ60RdsVcoirjCLi5LAr1/yGMSzsfDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T17:00:13.514076Z"},"content_sha256":"c998fff4a98b43bb063816dbbc8f4c26bd68f100abd7384b3e6eeb627d3f8f4f","schema_version":"1.0","event_id":"sha256:c998fff4a98b43bb063816dbbc8f4c26bd68f100abd7384b3e6eeb627d3f8f4f"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/L627Q6HFIYJUHIXDHZCSPP33BC/bundle.json","state_url":"https://pith.science/pith/L627Q6HFIYJUHIXDHZCSPP33BC/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/L627Q6HFIYJUHIXDHZCSPP33BC/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":"2026-05-31T17:00:13Z","links":{"resolver":"https://pith.science/pith/L627Q6HFIYJUHIXDHZCSPP33BC","bundle":"https://pith.science/pith/L627Q6HFIYJUHIXDHZCSPP33BC/bundle.json","state":"https://pith.science/pith/L627Q6HFIYJUHIXDHZCSPP33BC/state.json","well_known_bundle":"https://pith.science/.well-known/pith/L627Q6HFIYJUHIXDHZCSPP33BC/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:L627Q6HFIYJUHIXDHZCSPP33BC","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":"7e38b82cc3cddfef3ba400d8f5a06ac61f2f66a886f3172b4db92909f553b378","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-04-11T07:00:18Z","title_canon_sha256":"2000e4d958adad4598325894fc8abe51d9cc4b1ec9833f505636adbe3ba40300"},"schema_version":"1.0","source":{"id":"1304.3217","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1304.3217","created_at":"2026-05-18T01:20:03Z"},{"alias_kind":"arxiv_version","alias_value":"1304.3217v2","created_at":"2026-05-18T01:20:03Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1304.3217","created_at":"2026-05-18T01:20:03Z"},{"alias_kind":"pith_short_12","alias_value":"L627Q6HFIYJU","created_at":"2026-05-18T12:27:51Z"},{"alias_kind":"pith_short_16","alias_value":"L627Q6HFIYJUHIXD","created_at":"2026-05-18T12:27:51Z"},{"alias_kind":"pith_short_8","alias_value":"L627Q6HF","created_at":"2026-05-18T12:27:51Z"}],"graph_snapshots":[{"event_id":"sha256:c998fff4a98b43bb063816dbbc8f4c26bd68f100abd7384b3e6eeb627d3f8f4f","target":"graph","created_at":"2026-05-18T01:20:03Z","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":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We study the influence of the random part of the Galactic magnetic field on the propagation of ultra high-energy cosmic rays. Within very mild approximations about the properties of the electron density fluctuations in the Galaxy we are able to derive a clear and direct relation between the observed variance of rotation measures and the predicted cosmic ray deflections. Remarkably, this is obtained bypassing entirely the detailed knowledge of the magnetic properties of the turbulent plasma. Depending on the parameters of the electron density spectrum, we can either directly estimate the expect","authors_text":"F. R. Urban, M. S. Pshirkov, P. G. Tinyakov","cross_cats":["astro-ph.HE"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-04-11T07:00:18Z","title":"Mapping UHECRs deflections through the turbulent galactic magnetic field with the latest RM data"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1304.3217","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:8230a2fb96807265dd8eb70433a33d234c5253b106e9dd5b5395fcc6415e39db","target":"record","created_at":"2026-05-18T01:20:03Z","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":"7e38b82cc3cddfef3ba400d8f5a06ac61f2f66a886f3172b4db92909f553b378","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-04-11T07:00:18Z","title_canon_sha256":"2000e4d958adad4598325894fc8abe51d9cc4b1ec9833f505636adbe3ba40300"},"schema_version":"1.0","source":{"id":"1304.3217","kind":"arxiv","version":2}},"canonical_sha256":"5fb5f878e5461343a2e33e4527bf7b089f7a0fdde960023eb57a9b301e58f8c0","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"5fb5f878e5461343a2e33e4527bf7b089f7a0fdde960023eb57a9b301e58f8c0","first_computed_at":"2026-05-18T01:20:03.991044Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:20:03.991044Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"giL7idrgGYPRc9e3Vqks023atKHtDj90b4npHhiKk2vtg0qrikzJNcFEonO1+6XkL8Csws57/SLIDmAH/kHSBQ==","signature_status":"signed_v1","signed_at":"2026-05-18T01:20:03.991622Z","signed_message":"canonical_sha256_bytes"},"source_id":"1304.3217","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:8230a2fb96807265dd8eb70433a33d234c5253b106e9dd5b5395fcc6415e39db","sha256:c998fff4a98b43bb063816dbbc8f4c26bd68f100abd7384b3e6eeb627d3f8f4f"],"state_sha256":"273df95b347e7223ebcf00d2e6bb37467dcc8e226c1a3dc2b18c3a1b4922f545"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"AbrwnlZdGZgH1T5q7Pq3VtzWPJf3hixDo4vlsCLRNA+bfZ7opwDq+98SU7fqlfhca7KYuaWJ5Ty3XPOpbAVADA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-31T17:00:13.517932Z","bundle_sha256":"5a693ee1765aaf3059b46733b2e4b047fc66b74dd9bca6e502d375cd77208402"}}