{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:QQYGGRB2P2P5AI3HIGQOGJYZZF","short_pith_number":"pith:QQYGGRB2","schema_version":"1.0","canonical_sha256":"843063443a7e9fd0236741a0e32719c940f2850ee1e1fa2700fbbc331ac81509","source":{"kind":"arxiv","id":"1610.01167","version":1},"attestation_state":"computed","paper":{"title":"Radio Properties of the BAT AGN: the FIR-Radio Relation, the Fundamental Plane, and the Main Sequence of Star Formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Krista Lynne Smith, Neal Miller, Richard F. Mushotzky, Stuart Vogel, Thomas T. Shimizu","submitted_at":"2016-10-04T20:00:18Z","abstract_excerpt":"We have conducted 22 GHz 1\" JVLA imaging of 70 radio-quiet AGN from the Swift-BAT survey. We find radio cores in all but three objects. The radio morphologies of the sample fall into three groups: compact and core-dominated, extended, and jet-like. We spatially decompose each image into core flux and extended flux, and compare the extended radio emission to that predicted from previous Herschel observations using the canonical FIR-radio relation. After removing the AGN contribution to the FIR and radio flux densities, we find that the relation holds remarkably well despite the potentially diff"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1610.01167","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-10-04T20:00:18Z","cross_cats_sorted":[],"title_canon_sha256":"7322f1c4a792973a99ffa04f877ec0d802f935e90ccb20fe72c839a4fb40b019","abstract_canon_sha256":"852e247d61ad884ec0bbe3503ed5550c95a37c2dc630977b11ee953117d0cfac"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:55:07.428666Z","signature_b64":"vb3DQXTqHaqmRL5zCKPwlIudfQHsCZd3JIpQ95sW2gzGkKmrIoM3fTmNWwL2E90eBIlFjmLjMJV4wKThKpiLAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"843063443a7e9fd0236741a0e32719c940f2850ee1e1fa2700fbbc331ac81509","last_reissued_at":"2026-05-18T00:55:07.427958Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:55:07.427958Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Radio Properties of the BAT AGN: the FIR-Radio Relation, the Fundamental Plane, and the Main Sequence of Star Formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Krista Lynne Smith, Neal Miller, Richard F. Mushotzky, Stuart Vogel, Thomas T. Shimizu","submitted_at":"2016-10-04T20:00:18Z","abstract_excerpt":"We have conducted 22 GHz 1\" JVLA imaging of 70 radio-quiet AGN from the Swift-BAT survey. We find radio cores in all but three objects. The radio morphologies of the sample fall into three groups: compact and core-dominated, extended, and jet-like. We spatially decompose each image into core flux and extended flux, and compare the extended radio emission to that predicted from previous Herschel observations using the canonical FIR-radio relation. After removing the AGN contribution to the FIR and radio flux densities, we find that the relation holds remarkably well despite the potentially diff"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.01167","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1610.01167","created_at":"2026-05-18T00:55:07.428067+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.01167v1","created_at":"2026-05-18T00:55:07.428067+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.01167","created_at":"2026-05-18T00:55:07.428067+00:00"},{"alias_kind":"pith_short_12","alias_value":"QQYGGRB2P2P5","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_16","alias_value":"QQYGGRB2P2P5AI3H","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_8","alias_value":"QQYGGRB2","created_at":"2026-05-18T12:30:41.710351+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.17993","citing_title":"Nuclear Activity and Host Galaxy Properties of Low-Luminosity AGN Identified from VLA Observations","ref_index":13,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QQYGGRB2P2P5AI3HIGQOGJYZZF","json":"https://pith.science/pith/QQYGGRB2P2P5AI3HIGQOGJYZZF.json","graph_json":"https://pith.science/api/pith-number/QQYGGRB2P2P5AI3HIGQOGJYZZF/graph.json","events_json":"https://pith.science/api/pith-number/QQYGGRB2P2P5AI3HIGQOGJYZZF/events.json","paper":"https://pith.science/paper/QQYGGRB2"},"agent_actions":{"view_html":"https://pith.science/pith/QQYGGRB2P2P5AI3HIGQOGJYZZF","download_json":"https://pith.science/pith/QQYGGRB2P2P5AI3HIGQOGJYZZF.json","view_paper":"https://pith.science/paper/QQYGGRB2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.01167&json=true","fetch_graph":"https://pith.science/api/pith-number/QQYGGRB2P2P5AI3HIGQOGJYZZF/graph.json","fetch_events":"https://pith.science/api/pith-number/QQYGGRB2P2P5AI3HIGQOGJYZZF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QQYGGRB2P2P5AI3HIGQOGJYZZF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QQYGGRB2P2P5AI3HIGQOGJYZZF/action/storage_attestation","attest_author":"https://pith.science/pith/QQYGGRB2P2P5AI3HIGQOGJYZZF/action/author_attestation","sign_citation":"https://pith.science/pith/QQYGGRB2P2P5AI3HIGQOGJYZZF/action/citation_signature","submit_replication":"https://pith.science/pith/QQYGGRB2P2P5AI3HIGQOGJYZZF/action/replication_record"}},"created_at":"2026-05-18T00:55:07.428067+00:00","updated_at":"2026-05-18T00:55:07.428067+00:00"}