{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:GW5BJ7RTT6ZKYOT5AWMXAPVWZV","short_pith_number":"pith:GW5BJ7RT","canonical_record":{"source":{"id":"1008.2719","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-08-16T17:41:15Z","cross_cats_sorted":[],"title_canon_sha256":"908e2375ce3bb24628f0be0cbd35f25d30f034c0bef961f3199bd7e323ffb6b9","abstract_canon_sha256":"258952369ceed24cedd8490ba014e1ff810d0fff67076a1636623eec2c2cd8dc"},"schema_version":"1.0"},"canonical_sha256":"35ba14fe339fb2ac3a7d0599703eb6cd53f479873076b210ea82198acd9f0b37","source":{"kind":"arxiv","id":"1008.2719","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1008.2719","created_at":"2026-05-18T02:05:47Z"},{"alias_kind":"arxiv_version","alias_value":"1008.2719v1","created_at":"2026-05-18T02:05:47Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1008.2719","created_at":"2026-05-18T02:05:47Z"},{"alias_kind":"pith_short_12","alias_value":"GW5BJ7RTT6ZK","created_at":"2026-05-18T12:26:07Z"},{"alias_kind":"pith_short_16","alias_value":"GW5BJ7RTT6ZKYOT5","created_at":"2026-05-18T12:26:07Z"},{"alias_kind":"pith_short_8","alias_value":"GW5BJ7RT","created_at":"2026-05-18T12:26:07Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:GW5BJ7RTT6ZKYOT5AWMXAPVWZV","target":"record","payload":{"canonical_record":{"source":{"id":"1008.2719","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-08-16T17:41:15Z","cross_cats_sorted":[],"title_canon_sha256":"908e2375ce3bb24628f0be0cbd35f25d30f034c0bef961f3199bd7e323ffb6b9","abstract_canon_sha256":"258952369ceed24cedd8490ba014e1ff810d0fff67076a1636623eec2c2cd8dc"},"schema_version":"1.0"},"canonical_sha256":"35ba14fe339fb2ac3a7d0599703eb6cd53f479873076b210ea82198acd9f0b37","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:47.890860Z","signature_b64":"tYICO0UrZQUAdIL/E1bqU+LEPQyKAptYTgzW/Ouw9NM4a/h6fv8pQDXN+aQgaRXBJH8tCIL+oJYhcmR64oa/Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"35ba14fe339fb2ac3a7d0599703eb6cd53f479873076b210ea82198acd9f0b37","last_reissued_at":"2026-05-18T02:05:47.890126Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:47.890126Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1008.2719","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":"2026-05-18T02:05:47Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"sGLSjUgZufU0af2peFwMw4P9l0do4d8rgx40oLcSgiXlmDNRMoxYMEjm6I6j0XVDHrvvGjM94hdGCgoLE0zsCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T06:23:21.003547Z"},"content_sha256":"21353781e1f5bf6c914d4126aec1499dbcd157f99771285ee2ae5160c647989e","schema_version":"1.0","event_id":"sha256:21353781e1f5bf6c914d4126aec1499dbcd157f99771285ee2ae5160c647989e"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:GW5BJ7RTT6ZKYOT5AWMXAPVWZV","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The origin of the infrared emission in radio galaxies. III. Analysis of 3CRR objects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Robinson (RIT), C. Tadhunter (Univ of Sheffield), D. Axon (RIT, D. Dicken (RIT), P. Kharb (RIT), R. Morganti (ASTRON), Univ of Sussex)","submitted_at":"2010-08-16T17:41:15Z","abstract_excerpt":"We present Spitzer photometric data for a complete sample of 19 low redshift (z<0.1) 3CRR radio galaxies as part of our efforts to understand the origin of the prodigious mid- to far-infrared (MFIR) emission from radio-loud AGN. Our results show a correlation between AGN power (indicated by [OIII] 5007 emission line luminosity) and 24 micron luminosity. This result is consistent with the 24 micron thermal emission originating from warm dust heated directly by AGN illumination. Applying the same correlation test for 70 micron luminosity against [OIII] luminosity we find this relation to suffer "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1008.2719","kind":"arxiv","version":1},"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":"2026-05-18T02:05:47Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"10NJ5vWNDkU426pUTJNfdgTYHwcdyfQDu3sGidrSItcbPsSNUIEeRudEIVRlyHqxc9aLXnEx5gR5NGyy5v0QDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T06:23:21.003893Z"},"content_sha256":"f8e1dbcb617031af4c3c1e7fdce1923b88f60992e8b127212ba4d424c35479d1","schema_version":"1.0","event_id":"sha256:f8e1dbcb617031af4c3c1e7fdce1923b88f60992e8b127212ba4d424c35479d1"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/GW5BJ7RTT6ZKYOT5AWMXAPVWZV/bundle.json","state_url":"https://pith.science/pith/GW5BJ7RTT6ZKYOT5AWMXAPVWZV/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/GW5BJ7RTT6ZKYOT5AWMXAPVWZV/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":"2026-05-28T06:23:21Z","links":{"resolver":"https://pith.science/pith/GW5BJ7RTT6ZKYOT5AWMXAPVWZV","bundle":"https://pith.science/pith/GW5BJ7RTT6ZKYOT5AWMXAPVWZV/bundle.json","state":"https://pith.science/pith/GW5BJ7RTT6ZKYOT5AWMXAPVWZV/state.json","well_known_bundle":"https://pith.science/.well-known/pith/GW5BJ7RTT6ZKYOT5AWMXAPVWZV/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:GW5BJ7RTT6ZKYOT5AWMXAPVWZV","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":"258952369ceed24cedd8490ba014e1ff810d0fff67076a1636623eec2c2cd8dc","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-08-16T17:41:15Z","title_canon_sha256":"908e2375ce3bb24628f0be0cbd35f25d30f034c0bef961f3199bd7e323ffb6b9"},"schema_version":"1.0","source":{"id":"1008.2719","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1008.2719","created_at":"2026-05-18T02:05:47Z"},{"alias_kind":"arxiv_version","alias_value":"1008.2719v1","created_at":"2026-05-18T02:05:47Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1008.2719","created_at":"2026-05-18T02:05:47Z"},{"alias_kind":"pith_short_12","alias_value":"GW5BJ7RTT6ZK","created_at":"2026-05-18T12:26:07Z"},{"alias_kind":"pith_short_16","alias_value":"GW5BJ7RTT6ZKYOT5","created_at":"2026-05-18T12:26:07Z"},{"alias_kind":"pith_short_8","alias_value":"GW5BJ7RT","created_at":"2026-05-18T12:26:07Z"}],"graph_snapshots":[{"event_id":"sha256:f8e1dbcb617031af4c3c1e7fdce1923b88f60992e8b127212ba4d424c35479d1","target":"graph","created_at":"2026-05-18T02:05:47Z","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 present Spitzer photometric data for a complete sample of 19 low redshift (z<0.1) 3CRR radio galaxies as part of our efforts to understand the origin of the prodigious mid- to far-infrared (MFIR) emission from radio-loud AGN. Our results show a correlation between AGN power (indicated by [OIII] 5007 emission line luminosity) and 24 micron luminosity. This result is consistent with the 24 micron thermal emission originating from warm dust heated directly by AGN illumination. Applying the same correlation test for 70 micron luminosity against [OIII] luminosity we find this relation to suffer ","authors_text":"A. Robinson (RIT), C. Tadhunter (Univ of Sheffield), D. Axon (RIT, D. Dicken (RIT), P. Kharb (RIT), R. Morganti (ASTRON), Univ of Sussex)","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-08-16T17:41:15Z","title":"The origin of the infrared emission in radio galaxies. III. Analysis of 3CRR objects"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1008.2719","kind":"arxiv","version":1},"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":"sha256:21353781e1f5bf6c914d4126aec1499dbcd157f99771285ee2ae5160c647989e","target":"record","created_at":"2026-05-18T02:05:47Z","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":"258952369ceed24cedd8490ba014e1ff810d0fff67076a1636623eec2c2cd8dc","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-08-16T17:41:15Z","title_canon_sha256":"908e2375ce3bb24628f0be0cbd35f25d30f034c0bef961f3199bd7e323ffb6b9"},"schema_version":"1.0","source":{"id":"1008.2719","kind":"arxiv","version":1}},"canonical_sha256":"35ba14fe339fb2ac3a7d0599703eb6cd53f479873076b210ea82198acd9f0b37","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"35ba14fe339fb2ac3a7d0599703eb6cd53f479873076b210ea82198acd9f0b37","first_computed_at":"2026-05-18T02:05:47.890126Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:05:47.890126Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"tYICO0UrZQUAdIL/E1bqU+LEPQyKAptYTgzW/Ouw9NM4a/h6fv8pQDXN+aQgaRXBJH8tCIL+oJYhcmR64oa/Aw==","signature_status":"signed_v1","signed_at":"2026-05-18T02:05:47.890860Z","signed_message":"canonical_sha256_bytes"},"source_id":"1008.2719","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:21353781e1f5bf6c914d4126aec1499dbcd157f99771285ee2ae5160c647989e","sha256:f8e1dbcb617031af4c3c1e7fdce1923b88f60992e8b127212ba4d424c35479d1"],"state_sha256":"94f122946fdcda47a96c657099bfbe48a80f63cf407ecec6a2c8e39b85810cf3"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"1vsrpWWuCMKe19EAzXa9prnEPvO+03T+/czhvd+50xjgQIDT6AE85pdZGQMGIVVk7PyQvUcwd9n6+YzOEeKsBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-28T06:23:21.005876Z","bundle_sha256":"1c22a9b2c9d259658977bcbdc4d2b1b30a62871b197156e360ab3ea3cfaa626d"}}