{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2006:TFQI5USQCQJ55LW3FEGIZIFBLI","short_pith_number":"pith:TFQI5USQ","canonical_record":{"source":{"id":"astro-ph/0608577","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-08-28T16:45:53Z","cross_cats_sorted":[],"title_canon_sha256":"6a59019e0da99719b0bc1870d592e964f222d60d8a7aff8556dadf76aab6ef95","abstract_canon_sha256":"e0cf2107eac62cca9735ab28a60480e5d7eadcfc089d197f7cb34ca44511f204"},"schema_version":"1.0"},"canonical_sha256":"99608ed2501413deaedb290c8ca0a15a088d64ec2c922712c21a357c508f01d4","source":{"kind":"arxiv","id":"astro-ph/0608577","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0608577","created_at":"2026-07-04T14:55:51Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0608577v1","created_at":"2026-07-04T14:55:51Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0608577","created_at":"2026-07-04T14:55:51Z"},{"alias_kind":"pith_short_12","alias_value":"TFQI5USQCQJ5","created_at":"2026-07-04T14:55:51Z"},{"alias_kind":"pith_short_16","alias_value":"TFQI5USQCQJ55LW3","created_at":"2026-07-04T14:55:51Z"},{"alias_kind":"pith_short_8","alias_value":"TFQI5USQ","created_at":"2026-07-04T14:55:51Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2006:TFQI5USQCQJ55LW3FEGIZIFBLI","target":"record","payload":{"canonical_record":{"source":{"id":"astro-ph/0608577","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-08-28T16:45:53Z","cross_cats_sorted":[],"title_canon_sha256":"6a59019e0da99719b0bc1870d592e964f222d60d8a7aff8556dadf76aab6ef95","abstract_canon_sha256":"e0cf2107eac62cca9735ab28a60480e5d7eadcfc089d197f7cb34ca44511f204"},"schema_version":"1.0"},"canonical_sha256":"99608ed2501413deaedb290c8ca0a15a088d64ec2c922712c21a357c508f01d4","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T14:55:51.260972Z","signature_b64":"OfL5fJfQVDJztxo5cEXlnXxkfGCIKw40mMqwC5igZIP/HSDtW7vpavpG+mKxPUeltUlINHi6iXGtjKJtH8//Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"99608ed2501413deaedb290c8ca0a15a088d64ec2c922712c21a357c508f01d4","last_reissued_at":"2026-07-04T14:55:51.260544Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T14:55:51.260544Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"astro-ph/0608577","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":"2026-07-04T14:55:51Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"GVCuNr/+cMM+Wa43W9SfR1Hmt++yyivfUxBap5klfA+qccybdFQ53S1PLrfiG+yRL9J3vj0dQ9vWu/XhleuLDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-19T00:27:57.932196Z"},"content_sha256":"9624820d7086c62e616bac8a228b651596c7db07584b13efe26025b7aacce450","schema_version":"1.0","event_id":"sha256:9624820d7086c62e616bac8a228b651596c7db07584b13efe26025b7aacce450"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2006:TFQI5USQCQJ55LW3FEGIZIFBLI","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A Search for Molecular Gas in Low Luminosity Radio Galaxies","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"F.M. Montenegro-Montes, H.R. de Ruiter, I. Prandoni, P. Parma, R.A. Laing, T.L. Wilson","submitted_at":"2006-08-28T16:45:53Z","abstract_excerpt":"We discuss CO spectral line data of a volume-limited sample of 23 nearby (z<0.03) low luminosity radi galaxies, selected from the B2 catalogue. Most of such objects (16/23) have HST imaging. Our aim is to establish the distribution of molecular gas masses in low luminosity radio galaxies, in comparison with other radio source samples, confirm the suggestion that the CO is in ordered rotation, determine its relation to the dust disks observed in these objects with HST and establish targets for future interferometric imaging."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0608577","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0608577/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":"2026-07-04T14:55:51Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Sn4fSusuy7TmL6d2Sl/I4oYox7PKWSTenYNJvLREJUoGD45YWqxiqyBNNy5Bd26+YTLScdwckpQZ0/4H52EqDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-19T00:27:57.932745Z"},"content_sha256":"86787750342c86f89306fbaf247140c3d946f62ead11cca327033d8ce5bff3ce","schema_version":"1.0","event_id":"sha256:86787750342c86f89306fbaf247140c3d946f62ead11cca327033d8ce5bff3ce"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/TFQI5USQCQJ55LW3FEGIZIFBLI/bundle.json","state_url":"https://pith.science/pith/TFQI5USQCQJ55LW3FEGIZIFBLI/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/TFQI5USQCQJ55LW3FEGIZIFBLI/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":"2026-08-19T00:27:57Z","links":{"resolver":"https://pith.science/pith/TFQI5USQCQJ55LW3FEGIZIFBLI","bundle":"https://pith.science/pith/TFQI5USQCQJ55LW3FEGIZIFBLI/bundle.json","state":"https://pith.science/pith/TFQI5USQCQJ55LW3FEGIZIFBLI/state.json","well_known_bundle":"https://pith.science/.well-known/pith/TFQI5USQCQJ55LW3FEGIZIFBLI/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2006:TFQI5USQCQJ55LW3FEGIZIFBLI","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":"e0cf2107eac62cca9735ab28a60480e5d7eadcfc089d197f7cb34ca44511f204","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2006-08-28T16:45:53Z","title_canon_sha256":"6a59019e0da99719b0bc1870d592e964f222d60d8a7aff8556dadf76aab6ef95"},"schema_version":"1.0","source":{"id":"astro-ph/0608577","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0608577","created_at":"2026-07-04T14:55:51Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0608577v1","created_at":"2026-07-04T14:55:51Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0608577","created_at":"2026-07-04T14:55:51Z"},{"alias_kind":"pith_short_12","alias_value":"TFQI5USQCQJ5","created_at":"2026-07-04T14:55:51Z"},{"alias_kind":"pith_short_16","alias_value":"TFQI5USQCQJ55LW3","created_at":"2026-07-04T14:55:51Z"},{"alias_kind":"pith_short_8","alias_value":"TFQI5USQ","created_at":"2026-07-04T14:55:51Z"}],"graph_snapshots":[{"event_id":"sha256:86787750342c86f89306fbaf247140c3d946f62ead11cca327033d8ce5bff3ce","target":"graph","created_at":"2026-07-04T14:55:51Z","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/0608577/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"We discuss CO spectral line data of a volume-limited sample of 23 nearby (z<0.03) low luminosity radi galaxies, selected from the B2 catalogue. Most of such objects (16/23) have HST imaging. Our aim is to establish the distribution of molecular gas masses in low luminosity radio galaxies, in comparison with other radio source samples, confirm the suggestion that the CO is in ordered rotation, determine its relation to the dust disks observed in these objects with HST and establish targets for future interferometric imaging.","authors_text":"F.M. Montenegro-Montes, H.R. de Ruiter, I. Prandoni, P. Parma, R.A. Laing, T.L. Wilson","cross_cats":[],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"2006-08-28T16:45:53Z","title":"A Search for Molecular Gas in Low Luminosity Radio Galaxies"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0608577","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":"sha256:9624820d7086c62e616bac8a228b651596c7db07584b13efe26025b7aacce450","target":"record","created_at":"2026-07-04T14:55:51Z","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":"e0cf2107eac62cca9735ab28a60480e5d7eadcfc089d197f7cb34ca44511f204","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2006-08-28T16:45:53Z","title_canon_sha256":"6a59019e0da99719b0bc1870d592e964f222d60d8a7aff8556dadf76aab6ef95"},"schema_version":"1.0","source":{"id":"astro-ph/0608577","kind":"arxiv","version":1}},"canonical_sha256":"99608ed2501413deaedb290c8ca0a15a088d64ec2c922712c21a357c508f01d4","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"99608ed2501413deaedb290c8ca0a15a088d64ec2c922712c21a357c508f01d4","first_computed_at":"2026-07-04T14:55:51.260544Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-04T14:55:51.260544Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"OfL5fJfQVDJztxo5cEXlnXxkfGCIKw40mMqwC5igZIP/HSDtW7vpavpG+mKxPUeltUlINHi6iXGtjKJtH8//Cg==","signature_status":"signed_v1","signed_at":"2026-07-04T14:55:51.260972Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/0608577","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:9624820d7086c62e616bac8a228b651596c7db07584b13efe26025b7aacce450","sha256:86787750342c86f89306fbaf247140c3d946f62ead11cca327033d8ce5bff3ce"],"state_sha256":"8d99b0598d745e91540d58f75f0714937a0d189f6e8258943a12238cce606bb0"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"EoSAz7KeykbpIaXgTVtA9FWgVKs1v7/UzIq6FrnGN+aWqDdoAuJLaccHrI3631Q+/BYXZUUSgUNrBnTf5F2vCQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-19T00:27:57.937958Z","bundle_sha256":"37ecadec3107bf8690392edf1342099798430afa52004e4d748247012f1fd91a"}}