{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2012:PHIMH5AJVZAUGCFFRTAUCC3FQY","short_pith_number":"pith:PHIMH5AJ","canonical_record":{"source":{"id":"1211.2688","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-11-12T16:39:35Z","cross_cats_sorted":[],"title_canon_sha256":"a4031870fd05a6548b9fb3acbfdcd42e621bd4f2482792e7eed4652992ff46d8","abstract_canon_sha256":"f97d56c595b1b9df60f63610fdb765c7b501882821735e7ab93a277f2523beec"},"schema_version":"1.0"},"canonical_sha256":"79d0c3f409ae414308a58cc1410b65862007214e115c9818b32f3109fe62640f","source":{"kind":"arxiv","id":"1211.2688","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1211.2688","created_at":"2026-05-18T00:48:21Z"},{"alias_kind":"arxiv_version","alias_value":"1211.2688v1","created_at":"2026-05-18T00:48:21Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1211.2688","created_at":"2026-05-18T00:48:21Z"},{"alias_kind":"pith_short_12","alias_value":"PHIMH5AJVZAU","created_at":"2026-05-18T12:27:18Z"},{"alias_kind":"pith_short_16","alias_value":"PHIMH5AJVZAUGCFF","created_at":"2026-05-18T12:27:18Z"},{"alias_kind":"pith_short_8","alias_value":"PHIMH5AJ","created_at":"2026-05-18T12:27:18Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2012:PHIMH5AJVZAUGCFFRTAUCC3FQY","target":"record","payload":{"canonical_record":{"source":{"id":"1211.2688","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-11-12T16:39:35Z","cross_cats_sorted":[],"title_canon_sha256":"a4031870fd05a6548b9fb3acbfdcd42e621bd4f2482792e7eed4652992ff46d8","abstract_canon_sha256":"f97d56c595b1b9df60f63610fdb765c7b501882821735e7ab93a277f2523beec"},"schema_version":"1.0"},"canonical_sha256":"79d0c3f409ae414308a58cc1410b65862007214e115c9818b32f3109fe62640f","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:48:21.191941Z","signature_b64":"kvFAGHWtQ1tC678rWEkF/nNTtbJkI+mAnDCubLbLzn7w0O9CmbEITZvNciZA+xjjpR2v+g72KrRqoSkPyEzOCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"79d0c3f409ae414308a58cc1410b65862007214e115c9818b32f3109fe62640f","last_reissued_at":"2026-05-18T00:48:21.191287Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:48:21.191287Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1211.2688","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":"2026-05-18T00:48:21Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"24gU+ADKvpGkGD/sg/Jv9zMwA0mfu75x1MV/mwgcKuufhwCXjA9XP/LcIDcbwZRliw5f8DV/zEnGWTmPkXWABA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-23T01:30:06.607489Z"},"content_sha256":"117e2f9f143cf0ec93ec6dfb6029f71f627390a02d37a8e814e75c84602aca3c","schema_version":"1.0","event_id":"sha256:117e2f9f143cf0ec93ec6dfb6029f71f627390a02d37a8e814e75c84602aca3c"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2012:PHIMH5AJVZAUGCFFRTAUCC3FQY","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"On the AGN radio luminosity distribution and the black hole fundamental plane","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) OARoma-INAF), A. Bonchi (1), A. Bongiorno (2), F. Fiore (2) ((1) Universita` Roma Tre, F. La Franca (1), G. Melini (1)","submitted_at":"2012-11-12T16:39:35Z","abstract_excerpt":"We have studied the dependence of the AGN nuclear radio (1.4 GHz) luminosity on both the AGN 2-10 keV X-ray and the host-galaxy K-band luminosity. A complete sample of 1268 X-ray selected AGN (both type 1 and type 2) has been used, which is the largest catalogue of AGN belonging to statistically well defined samples where radio, X and K band information exists. At variance with previous studies, radio upper limits have been statistically taken into account using a Bayesian Maximum Likelihood fitting method. It resulted that a good fit is obtained assuming a plane in the 3D L_R-L_X-L_K space, n"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1211.2688","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":"2026-05-18T00:48:21Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"DsmrWyoeKDv/GE6Qud7PHdDBRmHEjgSZi0XuU2buCVgubSkuleSPgsjjbL38ZCbKe3iYiDfHyX1Ci+Zpt23EDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-23T01:30:06.608141Z"},"content_sha256":"6b62b3df90e9e1c6b4a4fd9dbb6d17bcd52c71348fc88cb68f14feeca0be27ff","schema_version":"1.0","event_id":"sha256:6b62b3df90e9e1c6b4a4fd9dbb6d17bcd52c71348fc88cb68f14feeca0be27ff"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/PHIMH5AJVZAUGCFFRTAUCC3FQY/bundle.json","state_url":"https://pith.science/pith/PHIMH5AJVZAUGCFFRTAUCC3FQY/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/PHIMH5AJVZAUGCFFRTAUCC3FQY/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":"2026-05-23T01:30:06Z","links":{"resolver":"https://pith.science/pith/PHIMH5AJVZAUGCFFRTAUCC3FQY","bundle":"https://pith.science/pith/PHIMH5AJVZAUGCFFRTAUCC3FQY/bundle.json","state":"https://pith.science/pith/PHIMH5AJVZAUGCFFRTAUCC3FQY/state.json","well_known_bundle":"https://pith.science/.well-known/pith/PHIMH5AJVZAUGCFFRTAUCC3FQY/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2012:PHIMH5AJVZAUGCFFRTAUCC3FQY","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":"f97d56c595b1b9df60f63610fdb765c7b501882821735e7ab93a277f2523beec","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-11-12T16:39:35Z","title_canon_sha256":"a4031870fd05a6548b9fb3acbfdcd42e621bd4f2482792e7eed4652992ff46d8"},"schema_version":"1.0","source":{"id":"1211.2688","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1211.2688","created_at":"2026-05-18T00:48:21Z"},{"alias_kind":"arxiv_version","alias_value":"1211.2688v1","created_at":"2026-05-18T00:48:21Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1211.2688","created_at":"2026-05-18T00:48:21Z"},{"alias_kind":"pith_short_12","alias_value":"PHIMH5AJVZAU","created_at":"2026-05-18T12:27:18Z"},{"alias_kind":"pith_short_16","alias_value":"PHIMH5AJVZAUGCFF","created_at":"2026-05-18T12:27:18Z"},{"alias_kind":"pith_short_8","alias_value":"PHIMH5AJ","created_at":"2026-05-18T12:27:18Z"}],"graph_snapshots":[{"event_id":"sha256:6b62b3df90e9e1c6b4a4fd9dbb6d17bcd52c71348fc88cb68f14feeca0be27ff","target":"graph","created_at":"2026-05-18T00:48:21Z","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 have studied the dependence of the AGN nuclear radio (1.4 GHz) luminosity on both the AGN 2-10 keV X-ray and the host-galaxy K-band luminosity. A complete sample of 1268 X-ray selected AGN (both type 1 and type 2) has been used, which is the largest catalogue of AGN belonging to statistically well defined samples where radio, X and K band information exists. At variance with previous studies, radio upper limits have been statistically taken into account using a Bayesian Maximum Likelihood fitting method. It resulted that a good fit is obtained assuming a plane in the 3D L_R-L_X-L_K space, n","authors_text":"(2) OARoma-INAF), A. Bonchi (1), A. Bongiorno (2), F. Fiore (2) ((1) Universita` Roma Tre, F. La Franca (1), G. Melini (1)","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-11-12T16:39:35Z","title":"On the AGN radio luminosity distribution and the black hole fundamental plane"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1211.2688","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":"sha256:117e2f9f143cf0ec93ec6dfb6029f71f627390a02d37a8e814e75c84602aca3c","target":"record","created_at":"2026-05-18T00:48:21Z","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":"f97d56c595b1b9df60f63610fdb765c7b501882821735e7ab93a277f2523beec","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-11-12T16:39:35Z","title_canon_sha256":"a4031870fd05a6548b9fb3acbfdcd42e621bd4f2482792e7eed4652992ff46d8"},"schema_version":"1.0","source":{"id":"1211.2688","kind":"arxiv","version":1}},"canonical_sha256":"79d0c3f409ae414308a58cc1410b65862007214e115c9818b32f3109fe62640f","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"79d0c3f409ae414308a58cc1410b65862007214e115c9818b32f3109fe62640f","first_computed_at":"2026-05-18T00:48:21.191287Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:48:21.191287Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"kvFAGHWtQ1tC678rWEkF/nNTtbJkI+mAnDCubLbLzn7w0O9CmbEITZvNciZA+xjjpR2v+g72KrRqoSkPyEzOCg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:48:21.191941Z","signed_message":"canonical_sha256_bytes"},"source_id":"1211.2688","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:117e2f9f143cf0ec93ec6dfb6029f71f627390a02d37a8e814e75c84602aca3c","sha256:6b62b3df90e9e1c6b4a4fd9dbb6d17bcd52c71348fc88cb68f14feeca0be27ff"],"state_sha256":"725640dc535581b320d859d9d9c7c1d88086ca6669e0bba8000a442267ff0d44"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"qEs6i/QeSb3e7QjiajmlvQ2myu8Poyg/984t7lWB7U4UO5cO0iHNaGF1NaQn97oKa5x/CC/DRN+LXRPaWBwLCg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-23T01:30:06.610782Z","bundle_sha256":"f755d46cfbd5c92811dd82dce035abdda93a91cd28fc5200858f31743ae7bb4f"}}