{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2006:KAESZDFLZUW5NSRZH4LAP2H7X7","short_pith_number":"pith:KAESZDFL","canonical_record":{"source":{"id":"astro-ph/0605327","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-05-12T18:59:22Z","cross_cats_sorted":[],"title_canon_sha256":"ead6873c149bec78f85d3c47cd055611800ba38317bf9cb4902c2fa2d10035ae","abstract_canon_sha256":"daa7e3dfb6af5ea66c34589f0c10d909c91d5b15589204c4151282d730fa149d"},"schema_version":"1.0"},"canonical_sha256":"50092c8cabcd2dd6ca393f1607e8ffbfedac5a8d006d3086fec436a296af6370","source":{"kind":"arxiv","id":"astro-ph/0605327","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0605327","created_at":"2026-05-18T04:22:20Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0605327v2","created_at":"2026-05-18T04:22:20Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0605327","created_at":"2026-05-18T04:22:20Z"},{"alias_kind":"pith_short_12","alias_value":"KAESZDFLZUW5","created_at":"2026-05-18T12:25:54Z"},{"alias_kind":"pith_short_16","alias_value":"KAESZDFLZUW5NSRZ","created_at":"2026-05-18T12:25:54Z"},{"alias_kind":"pith_short_8","alias_value":"KAESZDFL","created_at":"2026-05-18T12:25:54Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2006:KAESZDFLZUW5NSRZH4LAP2H7X7","target":"record","payload":{"canonical_record":{"source":{"id":"astro-ph/0605327","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-05-12T18:59:22Z","cross_cats_sorted":[],"title_canon_sha256":"ead6873c149bec78f85d3c47cd055611800ba38317bf9cb4902c2fa2d10035ae","abstract_canon_sha256":"daa7e3dfb6af5ea66c34589f0c10d909c91d5b15589204c4151282d730fa149d"},"schema_version":"1.0"},"canonical_sha256":"50092c8cabcd2dd6ca393f1607e8ffbfedac5a8d006d3086fec436a296af6370","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:22:20.493991Z","signature_b64":"FP+v4LOZncbV0x8ThXYj1kSgnGi1rpB1GXVH0B9FWJEInQW4r/QhXJe6pl6z/wX++UG43lB+W4egjtB7Z4jWCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"50092c8cabcd2dd6ca393f1607e8ffbfedac5a8d006d3086fec436a296af6370","last_reissued_at":"2026-05-18T04:22:20.493324Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:22:20.493324Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"astro-ph/0605327","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":"2026-05-18T04:22:20Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"l4QdoCNwWJ9R1aOIH6wobJ7S/WqM3eX0I60MY+RGPWdKEeJEJ0eANYiqFy224o2cWgHOu/RJjmeyRNUfOwjIBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T01:11:47.099512Z"},"content_sha256":"ce89e93caaa4331544662d7fa69d0242f29560f1d3ce7f5e5329518372bf06dc","schema_version":"1.0","event_id":"sha256:ce89e93caaa4331544662d7fa69d0242f29560f1d3ce7f5e5329518372bf06dc"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2006:KAESZDFLZUW5NSRZH4LAP2H7X7","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Cosmogenic Neutrinos from the propagation of Ultra High Energy Nuclei","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. V. Olinto, D. Allard, E. Parizot, F. W. Stecker, M. A. Malkan, M. Ave, N. Busca, T. Yamamoto","submitted_at":"2006-05-12T18:59:22Z","abstract_excerpt":"We calculate the flux of neutrinos generated by the propagation of ultra-high energy nuclei over cosmological distances. The propagation takes into account the interactions with cosmic background radiations including the CMB and the most recent estimates of higher energy (infra-red, optical, and ultra violet) backgrounds. We assume that the composition of ultra-high energy cosmic rays (UHECRs) at the source is the same as the observed one at low energies. This assumption fits well the present data at the highest energies. We compare the cosmogenic neutrino flux from mixed composition sources t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0605327","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":"2026-05-18T04:22:20Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"QRl+qheQHYlN9nM0h7cwZbZL5jE9q0UEdjaftSNnSZZc0nxVEDtnVyO8YvrvjskcV8g+lD+KXGkfifZM3evECA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T01:11:47.100117Z"},"content_sha256":"bd7cf760c68290ba66935c695260465d038f039f5148d1d8ffe35578c2677520","schema_version":"1.0","event_id":"sha256:bd7cf760c68290ba66935c695260465d038f039f5148d1d8ffe35578c2677520"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/KAESZDFLZUW5NSRZH4LAP2H7X7/bundle.json","state_url":"https://pith.science/pith/KAESZDFLZUW5NSRZH4LAP2H7X7/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/KAESZDFLZUW5NSRZH4LAP2H7X7/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":"2026-05-26T01:11:47Z","links":{"resolver":"https://pith.science/pith/KAESZDFLZUW5NSRZH4LAP2H7X7","bundle":"https://pith.science/pith/KAESZDFLZUW5NSRZH4LAP2H7X7/bundle.json","state":"https://pith.science/pith/KAESZDFLZUW5NSRZH4LAP2H7X7/state.json","well_known_bundle":"https://pith.science/.well-known/pith/KAESZDFLZUW5NSRZH4LAP2H7X7/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2006:KAESZDFLZUW5NSRZH4LAP2H7X7","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":"daa7e3dfb6af5ea66c34589f0c10d909c91d5b15589204c4151282d730fa149d","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2006-05-12T18:59:22Z","title_canon_sha256":"ead6873c149bec78f85d3c47cd055611800ba38317bf9cb4902c2fa2d10035ae"},"schema_version":"1.0","source":{"id":"astro-ph/0605327","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0605327","created_at":"2026-05-18T04:22:20Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0605327v2","created_at":"2026-05-18T04:22:20Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0605327","created_at":"2026-05-18T04:22:20Z"},{"alias_kind":"pith_short_12","alias_value":"KAESZDFLZUW5","created_at":"2026-05-18T12:25:54Z"},{"alias_kind":"pith_short_16","alias_value":"KAESZDFLZUW5NSRZ","created_at":"2026-05-18T12:25:54Z"},{"alias_kind":"pith_short_8","alias_value":"KAESZDFL","created_at":"2026-05-18T12:25:54Z"}],"graph_snapshots":[{"event_id":"sha256:bd7cf760c68290ba66935c695260465d038f039f5148d1d8ffe35578c2677520","target":"graph","created_at":"2026-05-18T04:22:20Z","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 calculate the flux of neutrinos generated by the propagation of ultra-high energy nuclei over cosmological distances. The propagation takes into account the interactions with cosmic background radiations including the CMB and the most recent estimates of higher energy (infra-red, optical, and ultra violet) backgrounds. We assume that the composition of ultra-high energy cosmic rays (UHECRs) at the source is the same as the observed one at low energies. This assumption fits well the present data at the highest energies. We compare the cosmogenic neutrino flux from mixed composition sources t","authors_text":"A. V. Olinto, D. Allard, E. Parizot, F. W. Stecker, M. A. Malkan, M. Ave, N. Busca, T. Yamamoto","cross_cats":[],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"2006-05-12T18:59:22Z","title":"Cosmogenic Neutrinos from the propagation of Ultra High Energy Nuclei"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0605327","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:ce89e93caaa4331544662d7fa69d0242f29560f1d3ce7f5e5329518372bf06dc","target":"record","created_at":"2026-05-18T04:22:20Z","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":"daa7e3dfb6af5ea66c34589f0c10d909c91d5b15589204c4151282d730fa149d","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2006-05-12T18:59:22Z","title_canon_sha256":"ead6873c149bec78f85d3c47cd055611800ba38317bf9cb4902c2fa2d10035ae"},"schema_version":"1.0","source":{"id":"astro-ph/0605327","kind":"arxiv","version":2}},"canonical_sha256":"50092c8cabcd2dd6ca393f1607e8ffbfedac5a8d006d3086fec436a296af6370","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"50092c8cabcd2dd6ca393f1607e8ffbfedac5a8d006d3086fec436a296af6370","first_computed_at":"2026-05-18T04:22:20.493324Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T04:22:20.493324Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"FP+v4LOZncbV0x8ThXYj1kSgnGi1rpB1GXVH0B9FWJEInQW4r/QhXJe6pl6z/wX++UG43lB+W4egjtB7Z4jWCA==","signature_status":"signed_v1","signed_at":"2026-05-18T04:22:20.493991Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/0605327","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:ce89e93caaa4331544662d7fa69d0242f29560f1d3ce7f5e5329518372bf06dc","sha256:bd7cf760c68290ba66935c695260465d038f039f5148d1d8ffe35578c2677520"],"state_sha256":"8ffb3ced4736398f287a92477f3e449304bd12b3b00a9ef19018657501d7f417"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"qKV9kdTzfe+6V+4Z3LVPeef8dsRMGIMJjcePmJWEQRz+Bz+HwCJC0Jwvq3GU41DjcBQilKUYPnkVFWCWpriZDg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T01:11:47.103434Z","bundle_sha256":"ca88d6605392eed81213326f3841986a4103c5e35e225eb6e2be90032a5162c2"}}