{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2019:PWJQABQMB2FGDTTI2TOMQJJ4VH","short_pith_number":"pith:PWJQABQM","canonical_record":{"source":{"id":"1902.07727","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-02-20T19:00:14Z","cross_cats_sorted":[],"title_canon_sha256":"d0371635b2e449acfc7767df907f850987f7f6b89a17ef8d2f3b03a0e0f052a8","abstract_canon_sha256":"f5e94ae3b6470b97e0411b433b79564e095ae6b9b34ab2a71ab346dce5112c84"},"schema_version":"1.0"},"canonical_sha256":"7d9300060c0e8a61ce68d4dcc8253ca9c1d90db8f938963c6ff2a62c13aa6016","source":{"kind":"arxiv","id":"1902.07727","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1902.07727","created_at":"2026-05-17T23:52:01Z"},{"alias_kind":"arxiv_version","alias_value":"1902.07727v1","created_at":"2026-05-17T23:52:01Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1902.07727","created_at":"2026-05-17T23:52:01Z"},{"alias_kind":"pith_short_12","alias_value":"PWJQABQMB2FG","created_at":"2026-05-18T12:33:24Z"},{"alias_kind":"pith_short_16","alias_value":"PWJQABQMB2FGDTTI","created_at":"2026-05-18T12:33:24Z"},{"alias_kind":"pith_short_8","alias_value":"PWJQABQM","created_at":"2026-05-18T12:33:24Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2019:PWJQABQMB2FGDTTI2TOMQJJ4VH","target":"record","payload":{"canonical_record":{"source":{"id":"1902.07727","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-02-20T19:00:14Z","cross_cats_sorted":[],"title_canon_sha256":"d0371635b2e449acfc7767df907f850987f7f6b89a17ef8d2f3b03a0e0f052a8","abstract_canon_sha256":"f5e94ae3b6470b97e0411b433b79564e095ae6b9b34ab2a71ab346dce5112c84"},"schema_version":"1.0"},"canonical_sha256":"7d9300060c0e8a61ce68d4dcc8253ca9c1d90db8f938963c6ff2a62c13aa6016","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:52:01.090979Z","signature_b64":"fLMT7kh7wEldEXoTS8Ao/u5y+zsIJF7svj2Yn8vXB2+6t0uCFKqC3wB2QvCpTaUld7bKtYsP8a1pcrH8fqFLAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7d9300060c0e8a61ce68d4dcc8253ca9c1d90db8f938963c6ff2a62c13aa6016","last_reissued_at":"2026-05-17T23:52:01.090496Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:52:01.090496Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1902.07727","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":"2026-05-17T23:52:01Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"utbNHvvdrvQViZLz7VYfeu024tHmdC2CUHacEl3aS7utJZO8KI0p1uXzrD6rJluSUobZgPdW4HZMc5dBxPWVCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T03:52:42.268514Z"},"content_sha256":"0ad54b68458ce0d36d5baec7d4a3cb6eb080cb5ae5a8092ddb1c0c7388d196b3","schema_version":"1.0","event_id":"sha256:0ad54b68458ce0d36d5baec7d4a3cb6eb080cb5ae5a8092ddb1c0c7388d196b3"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2019:PWJQABQMB2FGDTTI2TOMQJJ4VH","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Prevalence of radio jets associated with galactic outflows and feedback from quasars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. C. Edge, A. P. Thomson, C. Circosta, C. M. Harrison, D. M. Alexander, G. B. Lansbury, J. R. Mullaney, M. E. Jarvis, S. J. Molyneux, V. Mainieri","submitted_at":"2019-02-20T19:00:14Z","abstract_excerpt":"We present 1-7 GHz high-resolution radio imaging (VLA and e-MERLIN) and spatially-resolved ionized gas kinematics for ten z<0.2 type~2 `obscured' quasars (log [L(AGN)/(erg/s)]>~45) with moderate radio luminosities (log [L(1.4GHz)/(W/Hz)]=23.3-24.4). These targets were selected to have known ionized outflows based on broad [OIII] emission-line components (FWHM~800-1800 km/s). Although `radio-quiet' and not `radio AGN' by many traditional criteria, we show that for nine of the targets, star formation likely accounts for <~10 per cent of the radio emission. We find that ~80-90 per cent of these n"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1902.07727","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":"2026-05-17T23:52:01Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"z3QQ98XnuUc0eTNuBO+xKrjcWt8hEQJkgyOumDM9owEwyCSwbY5RN3gOohxkWDVpqo2HNE34m8U8Ddvv14gIAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T03:52:42.269409Z"},"content_sha256":"a6379fb90ff868e3c614116803d43e3cdb07ed2b8dae2ef256e660883c59b396","schema_version":"1.0","event_id":"sha256:a6379fb90ff868e3c614116803d43e3cdb07ed2b8dae2ef256e660883c59b396"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/PWJQABQMB2FGDTTI2TOMQJJ4VH/bundle.json","state_url":"https://pith.science/pith/PWJQABQMB2FGDTTI2TOMQJJ4VH/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/PWJQABQMB2FGDTTI2TOMQJJ4VH/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":"2026-05-27T03:52:42Z","links":{"resolver":"https://pith.science/pith/PWJQABQMB2FGDTTI2TOMQJJ4VH","bundle":"https://pith.science/pith/PWJQABQMB2FGDTTI2TOMQJJ4VH/bundle.json","state":"https://pith.science/pith/PWJQABQMB2FGDTTI2TOMQJJ4VH/state.json","well_known_bundle":"https://pith.science/.well-known/pith/PWJQABQMB2FGDTTI2TOMQJJ4VH/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2019:PWJQABQMB2FGDTTI2TOMQJJ4VH","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":"f5e94ae3b6470b97e0411b433b79564e095ae6b9b34ab2a71ab346dce5112c84","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-02-20T19:00:14Z","title_canon_sha256":"d0371635b2e449acfc7767df907f850987f7f6b89a17ef8d2f3b03a0e0f052a8"},"schema_version":"1.0","source":{"id":"1902.07727","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1902.07727","created_at":"2026-05-17T23:52:01Z"},{"alias_kind":"arxiv_version","alias_value":"1902.07727v1","created_at":"2026-05-17T23:52:01Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1902.07727","created_at":"2026-05-17T23:52:01Z"},{"alias_kind":"pith_short_12","alias_value":"PWJQABQMB2FG","created_at":"2026-05-18T12:33:24Z"},{"alias_kind":"pith_short_16","alias_value":"PWJQABQMB2FGDTTI","created_at":"2026-05-18T12:33:24Z"},{"alias_kind":"pith_short_8","alias_value":"PWJQABQM","created_at":"2026-05-18T12:33:24Z"}],"graph_snapshots":[{"event_id":"sha256:a6379fb90ff868e3c614116803d43e3cdb07ed2b8dae2ef256e660883c59b396","target":"graph","created_at":"2026-05-17T23:52:01Z","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 1-7 GHz high-resolution radio imaging (VLA and e-MERLIN) and spatially-resolved ionized gas kinematics for ten z<0.2 type~2 `obscured' quasars (log [L(AGN)/(erg/s)]>~45) with moderate radio luminosities (log [L(1.4GHz)/(W/Hz)]=23.3-24.4). These targets were selected to have known ionized outflows based on broad [OIII] emission-line components (FWHM~800-1800 km/s). Although `radio-quiet' and not `radio AGN' by many traditional criteria, we show that for nine of the targets, star formation likely accounts for <~10 per cent of the radio emission. We find that ~80-90 per cent of these n","authors_text":"A. C. Edge, A. P. Thomson, C. Circosta, C. M. Harrison, D. M. Alexander, G. B. Lansbury, J. R. Mullaney, M. E. Jarvis, S. J. Molyneux, V. Mainieri","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-02-20T19:00:14Z","title":"Prevalence of radio jets associated with galactic outflows and feedback from quasars"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1902.07727","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":"sha256:0ad54b68458ce0d36d5baec7d4a3cb6eb080cb5ae5a8092ddb1c0c7388d196b3","target":"record","created_at":"2026-05-17T23:52:01Z","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":"f5e94ae3b6470b97e0411b433b79564e095ae6b9b34ab2a71ab346dce5112c84","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-02-20T19:00:14Z","title_canon_sha256":"d0371635b2e449acfc7767df907f850987f7f6b89a17ef8d2f3b03a0e0f052a8"},"schema_version":"1.0","source":{"id":"1902.07727","kind":"arxiv","version":1}},"canonical_sha256":"7d9300060c0e8a61ce68d4dcc8253ca9c1d90db8f938963c6ff2a62c13aa6016","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"7d9300060c0e8a61ce68d4dcc8253ca9c1d90db8f938963c6ff2a62c13aa6016","first_computed_at":"2026-05-17T23:52:01.090496Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-17T23:52:01.090496Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"fLMT7kh7wEldEXoTS8Ao/u5y+zsIJF7svj2Yn8vXB2+6t0uCFKqC3wB2QvCpTaUld7bKtYsP8a1pcrH8fqFLAQ==","signature_status":"signed_v1","signed_at":"2026-05-17T23:52:01.090979Z","signed_message":"canonical_sha256_bytes"},"source_id":"1902.07727","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:0ad54b68458ce0d36d5baec7d4a3cb6eb080cb5ae5a8092ddb1c0c7388d196b3","sha256:a6379fb90ff868e3c614116803d43e3cdb07ed2b8dae2ef256e660883c59b396"],"state_sha256":"907aebd23ec3a2aa0b2bbac0d02a2a74a759522b7476f41c890f812405c1b5fc"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"znhu0kTkFyLuLve32uEFMRC2UkWw2xMfC5uF5C50uS0nrSJdASlGbnd0Y0lF7DNhBtPqFD53qlyvJLSuiglOAQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-27T03:52:42.272728Z","bundle_sha256":"a492427d21ec69f310e6a2c13ed6399956284911d04bd591747b466ee0262726"}}