{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:XP2FDEN6HMLUSU3VMUBFFRUUO2","short_pith_number":"pith:XP2FDEN6","schema_version":"1.0","canonical_sha256":"bbf45191be3b17495375650252c694769c88e00f23f36af1c0fc53de9b267811","source":{"kind":"arxiv","id":"1309.7486","version":3},"attestation_state":"computed","paper":{"title":"ALMA observations of feeding and feedback in nearby Seyfert galaxies: an AGN-driven outflow in NGC 1433","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Eckart (Koeln), A.J. Baker (Rutgers), Bologna), E. Schinnerer (MPIA-Heidelberg), F. Boone (Toulouse), F. Combes (LERMA, I. Marquez (IAA-Granada), L.J. Tacconi (MPE-Garching), L. K. Hunt (INAF-Arcetri), M. Krips (IRAM-Grenoble), Obs-Paris), R. Neri (IRAM-Grenoble), S. Garcia-Burillo (Obs-Madrid), V. Casasola (INAF","submitted_at":"2013-09-28T18:08:55Z","abstract_excerpt":"We report ALMA observations of CO(3-2) emission in the Seyfert 2 double-barred galaxy NGC1433, at the unprecedented spatial resolution of 0.5\"=24 pc. Our aim is to probe AGN feeding and feedback phenomena through the morphology and dynamics of the gas inside the central kpc. The CO map, which covers the whole nuclear region (nuclear bar and ring), reveals a nuclear gaseous spiral structure, inside the nuclear ring encircling the nuclear stellar bar.\n  This gaseous spiral is well correlated with the dusty spiral seen in Hubble Space Telescope images. The nuclear spiral winds up in a pseudo-ring"},"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":"1309.7486","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-09-28T18:08:55Z","cross_cats_sorted":[],"title_canon_sha256":"e556798338384dfe4ac2cd7091852197a362ed7a6a7e81b76bec3ddd0ed199e6","abstract_canon_sha256":"69d228bdcff54751ed76f0ef963f1fa7ed2125b5bd427b7b3be22ededcdcae6d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:25.023979Z","signature_b64":"9qNODZpzY6N7/hwxJZ6jTWxmon8mgE+5bvVHGGjA7VbOUhTSz00AXUaR+X9+xxQXiEihURyHfEoLU3LZtZwQCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bbf45191be3b17495375650252c694769c88e00f23f36af1c0fc53de9b267811","last_reissued_at":"2026-05-18T01:47:25.023187Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:25.023187Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"ALMA observations of feeding and feedback in nearby Seyfert galaxies: an AGN-driven outflow in NGC 1433","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Eckart (Koeln), A.J. Baker (Rutgers), Bologna), E. Schinnerer (MPIA-Heidelberg), F. Boone (Toulouse), F. Combes (LERMA, I. Marquez (IAA-Granada), L.J. Tacconi (MPE-Garching), L. K. Hunt (INAF-Arcetri), M. Krips (IRAM-Grenoble), Obs-Paris), R. Neri (IRAM-Grenoble), S. Garcia-Burillo (Obs-Madrid), V. Casasola (INAF","submitted_at":"2013-09-28T18:08:55Z","abstract_excerpt":"We report ALMA observations of CO(3-2) emission in the Seyfert 2 double-barred galaxy NGC1433, at the unprecedented spatial resolution of 0.5\"=24 pc. Our aim is to probe AGN feeding and feedback phenomena through the morphology and dynamics of the gas inside the central kpc. The CO map, which covers the whole nuclear region (nuclear bar and ring), reveals a nuclear gaseous spiral structure, inside the nuclear ring encircling the nuclear stellar bar.\n  This gaseous spiral is well correlated with the dusty spiral seen in Hubble Space Telescope images. The nuclear spiral winds up in a pseudo-ring"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1309.7486","kind":"arxiv","version":3},"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":"1309.7486","created_at":"2026-05-18T01:47:25.023297+00:00"},{"alias_kind":"arxiv_version","alias_value":"1309.7486v3","created_at":"2026-05-18T01:47:25.023297+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1309.7486","created_at":"2026-05-18T01:47:25.023297+00:00"},{"alias_kind":"pith_short_12","alias_value":"XP2FDEN6HMLU","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_16","alias_value":"XP2FDEN6HMLUSU3V","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_8","alias_value":"XP2FDEN6","created_at":"2026-05-18T12:28:06.772260+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XP2FDEN6HMLUSU3VMUBFFRUUO2","json":"https://pith.science/pith/XP2FDEN6HMLUSU3VMUBFFRUUO2.json","graph_json":"https://pith.science/api/pith-number/XP2FDEN6HMLUSU3VMUBFFRUUO2/graph.json","events_json":"https://pith.science/api/pith-number/XP2FDEN6HMLUSU3VMUBFFRUUO2/events.json","paper":"https://pith.science/paper/XP2FDEN6"},"agent_actions":{"view_html":"https://pith.science/pith/XP2FDEN6HMLUSU3VMUBFFRUUO2","download_json":"https://pith.science/pith/XP2FDEN6HMLUSU3VMUBFFRUUO2.json","view_paper":"https://pith.science/paper/XP2FDEN6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1309.7486&json=true","fetch_graph":"https://pith.science/api/pith-number/XP2FDEN6HMLUSU3VMUBFFRUUO2/graph.json","fetch_events":"https://pith.science/api/pith-number/XP2FDEN6HMLUSU3VMUBFFRUUO2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XP2FDEN6HMLUSU3VMUBFFRUUO2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XP2FDEN6HMLUSU3VMUBFFRUUO2/action/storage_attestation","attest_author":"https://pith.science/pith/XP2FDEN6HMLUSU3VMUBFFRUUO2/action/author_attestation","sign_citation":"https://pith.science/pith/XP2FDEN6HMLUSU3VMUBFFRUUO2/action/citation_signature","submit_replication":"https://pith.science/pith/XP2FDEN6HMLUSU3VMUBFFRUUO2/action/replication_record"}},"created_at":"2026-05-18T01:47:25.023297+00:00","updated_at":"2026-05-18T01:47:25.023297+00:00"}