{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2001:THOT626Z64K4OK64ZCL2FMCEIW","short_pith_number":"pith:THOT626Z","canonical_record":{"source":{"id":"astro-ph/0102154","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-02-08T23:40:40Z","cross_cats_sorted":[],"title_canon_sha256":"d573fa0b00c8346f3cc055ebe2b1c50f2757f2e9f92eb65207406b693415a2aa","abstract_canon_sha256":"a8f240c6e41d05b9d4bd9777798f3bf15b4d4d77d48e0039f74afc83acecb0c3"},"schema_version":"1.0"},"canonical_sha256":"99dd3f6bd9f715c72bdcc897a2b04445928d42d1cdc1a845a50af47228e5eefe","source":{"kind":"arxiv","id":"astro-ph/0102154","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0102154","created_at":"2026-07-04T15:51:10Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0102154v2","created_at":"2026-07-04T15:51:10Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0102154","created_at":"2026-07-04T15:51:10Z"},{"alias_kind":"pith_short_12","alias_value":"THOT626Z64K4","created_at":"2026-07-04T15:51:10Z"},{"alias_kind":"pith_short_16","alias_value":"THOT626Z64K4OK64","created_at":"2026-07-04T15:51:10Z"},{"alias_kind":"pith_short_8","alias_value":"THOT626Z","created_at":"2026-07-04T15:51:10Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2001:THOT626Z64K4OK64ZCL2FMCEIW","target":"record","payload":{"canonical_record":{"source":{"id":"astro-ph/0102154","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-02-08T23:40:40Z","cross_cats_sorted":[],"title_canon_sha256":"d573fa0b00c8346f3cc055ebe2b1c50f2757f2e9f92eb65207406b693415a2aa","abstract_canon_sha256":"a8f240c6e41d05b9d4bd9777798f3bf15b4d4d77d48e0039f74afc83acecb0c3"},"schema_version":"1.0"},"canonical_sha256":"99dd3f6bd9f715c72bdcc897a2b04445928d42d1cdc1a845a50af47228e5eefe","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:51:10.807951Z","signature_b64":"6TQiW/4Ti7F42Hm7aSqRw7VoQ1Xgm6WBAtVFVu/Y7M2tD2ApPqyNlG4SkeBfnaqXEPWCVKTE3xDBi9yBKiuNAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"99dd3f6bd9f715c72bdcc897a2b04445928d42d1cdc1a845a50af47228e5eefe","last_reissued_at":"2026-07-04T15:51:10.807569Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:51:10.807569Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"astro-ph/0102154","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":"2026-07-04T15:51:10Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"dlPsX1CdloPE+H7yD5L8nMWLq567megsQHKEXRhrKsdyVm5ju/LIAXeFoRMAOB+tPa2BFlzsKOwTpW1zmokxBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-13T02:08:32.494220Z"},"content_sha256":"d31ec729b9d25cfe5fe6c237893fb346cf7e38b92154147141c84f206692531e","schema_version":"1.0","event_id":"sha256:d31ec729b9d25cfe5fe6c237893fb346cf7e38b92154147141c84f206692531e"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2001:THOT626Z64K4OK64ZCL2FMCEIW","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Radio Properties of Infrared Selected Galaxies in the IRAS 2 Jy Sample","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"J. J. Condon (NRAO), Min S. Yun, Naveen A. Reddy","submitted_at":"2001-02-08T23:40:40Z","abstract_excerpt":"The radio counterparts to the IRAS Redshift Survey galaxies are identified in the NRAO VLA Sky Survey (NVSS) catalog. Our new catalog of the infrared flux-limited (S60 >= 2 Jy) complete sample of 1809 galaxies lists accurate radio positions, redshifts, and 1.4 GHz radio and IRAS fluxes. This sample is six times larger in size and five times deeper in redshift coverage (to z ~ 0.15) compared with those used in earlier studies of the radio and far-infrared (FIR) properties of galaxies in the local volume. The well known radio-FIR correlation is obeyed by the overwhelming majority (>98%) of the i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0102154","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0102154/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2026-07-04T15:51:10Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ZPgpftmyN5volKf/L1jrMaZoo0m/2yH9wF/z681TkyvxMS7954KXiMNVTTTVm6wAPTumhnncxDRvx7qSXxMvCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-13T02:08:32.494638Z"},"content_sha256":"072032254dcb172a4b70966e52b5a5977e44b6525bac6ba98956b0829b47e2c1","schema_version":"1.0","event_id":"sha256:072032254dcb172a4b70966e52b5a5977e44b6525bac6ba98956b0829b47e2c1"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/THOT626Z64K4OK64ZCL2FMCEIW/bundle.json","state_url":"https://pith.science/pith/THOT626Z64K4OK64ZCL2FMCEIW/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/THOT626Z64K4OK64ZCL2FMCEIW/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":"2026-07-13T02:08:32Z","links":{"resolver":"https://pith.science/pith/THOT626Z64K4OK64ZCL2FMCEIW","bundle":"https://pith.science/pith/THOT626Z64K4OK64ZCL2FMCEIW/bundle.json","state":"https://pith.science/pith/THOT626Z64K4OK64ZCL2FMCEIW/state.json","well_known_bundle":"https://pith.science/.well-known/pith/THOT626Z64K4OK64ZCL2FMCEIW/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2001:THOT626Z64K4OK64ZCL2FMCEIW","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":"a8f240c6e41d05b9d4bd9777798f3bf15b4d4d77d48e0039f74afc83acecb0c3","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2001-02-08T23:40:40Z","title_canon_sha256":"d573fa0b00c8346f3cc055ebe2b1c50f2757f2e9f92eb65207406b693415a2aa"},"schema_version":"1.0","source":{"id":"astro-ph/0102154","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0102154","created_at":"2026-07-04T15:51:10Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0102154v2","created_at":"2026-07-04T15:51:10Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0102154","created_at":"2026-07-04T15:51:10Z"},{"alias_kind":"pith_short_12","alias_value":"THOT626Z64K4","created_at":"2026-07-04T15:51:10Z"},{"alias_kind":"pith_short_16","alias_value":"THOT626Z64K4OK64","created_at":"2026-07-04T15:51:10Z"},{"alias_kind":"pith_short_8","alias_value":"THOT626Z","created_at":"2026-07-04T15:51:10Z"}],"graph_snapshots":[{"event_id":"sha256:072032254dcb172a4b70966e52b5a5977e44b6525bac6ba98956b0829b47e2c1","target":"graph","created_at":"2026-07-04T15:51:10Z","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"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/astro-ph/0102154/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"The radio counterparts to the IRAS Redshift Survey galaxies are identified in the NRAO VLA Sky Survey (NVSS) catalog. Our new catalog of the infrared flux-limited (S60 >= 2 Jy) complete sample of 1809 galaxies lists accurate radio positions, redshifts, and 1.4 GHz radio and IRAS fluxes. This sample is six times larger in size and five times deeper in redshift coverage (to z ~ 0.15) compared with those used in earlier studies of the radio and far-infrared (FIR) properties of galaxies in the local volume. The well known radio-FIR correlation is obeyed by the overwhelming majority (>98%) of the i","authors_text":"J. J. Condon (NRAO), Min S. Yun, Naveen A. Reddy","cross_cats":[],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"2001-02-08T23:40:40Z","title":"Radio Properties of Infrared Selected Galaxies in the IRAS 2 Jy Sample"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0102154","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:d31ec729b9d25cfe5fe6c237893fb346cf7e38b92154147141c84f206692531e","target":"record","created_at":"2026-07-04T15:51:10Z","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":"a8f240c6e41d05b9d4bd9777798f3bf15b4d4d77d48e0039f74afc83acecb0c3","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2001-02-08T23:40:40Z","title_canon_sha256":"d573fa0b00c8346f3cc055ebe2b1c50f2757f2e9f92eb65207406b693415a2aa"},"schema_version":"1.0","source":{"id":"astro-ph/0102154","kind":"arxiv","version":2}},"canonical_sha256":"99dd3f6bd9f715c72bdcc897a2b04445928d42d1cdc1a845a50af47228e5eefe","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"99dd3f6bd9f715c72bdcc897a2b04445928d42d1cdc1a845a50af47228e5eefe","first_computed_at":"2026-07-04T15:51:10.807569Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-04T15:51:10.807569Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"6TQiW/4Ti7F42Hm7aSqRw7VoQ1Xgm6WBAtVFVu/Y7M2tD2ApPqyNlG4SkeBfnaqXEPWCVKTE3xDBi9yBKiuNAQ==","signature_status":"signed_v1","signed_at":"2026-07-04T15:51:10.807951Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/0102154","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:d31ec729b9d25cfe5fe6c237893fb346cf7e38b92154147141c84f206692531e","sha256:072032254dcb172a4b70966e52b5a5977e44b6525bac6ba98956b0829b47e2c1"],"state_sha256":"c872f6d78408009c208f4ebeaf05ad3c5ba9ce0551bc98eadcb419dde2d340d1"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"5AVKeIpsIpmKvUtdoCe85dfz+t5znqJyGQMY3bio7Xjb1Fz8zPAyVTIr1GrIkLgHH28y8hoY2LueKDJKqXxHDw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-07-13T02:08:32.497757Z","bundle_sha256":"2b41d7d76b830c7d9e9b4dacdfd8601262c5f106344524f4c1589657236ffbe7"}}