{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:I5Y54YF24CFFYTIG6YNH2UQ3AM","short_pith_number":"pith:I5Y54YF2","schema_version":"1.0","canonical_sha256":"4771de60bae08a5c4d06f61a7d521b030f04d1415ef8bb2d41c9b0ac87fc22e2","source":{"kind":"arxiv","id":"1907.00982","version":1},"attestation_state":"computed","paper":{"title":"Positive and negative feedback of AGN outflows in NGC 5728","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aeree Chung, Daeun Kang, Hyun-Jin Bae, Jaejin Shin, Jong-Hak Woo, Junhyun Baek, Kyuhyoun Cho","submitted_at":"2019-07-01T18:00:02Z","abstract_excerpt":"We present a spatially-resolved analysis of ionized and molecular gas in a nearby Seyfert 2 galaxy NGC 5728, using the VLT/MUSE and ALMA data. We find ionized gas outflows out to ~kpc scales, which encounter the star formation ring at 1 kpc radius. The star formation rate of the encountering region is significantly high (~1.8 M$_{\\rm sol}/yr/kpc^2$) compared to other regions in the ring. In contrast, the CO (2-1) emission is significantly weaker by a factor of ~3.5, indicating very high star formation efficiency. These results support the positive feedback scenario that the AGN-driven outflows"},"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":"1907.00982","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-07-01T18:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"9ad9f8121b8d424d7b8c0de9d08d0bf03c22d2a6796d26f9d1e3f4fe3b2f9aeb","abstract_canon_sha256":"29c8a99317ee4134ab41300556d8fa14b29b37e2a44494930a5371144d9498b0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:01:57.365734Z","signature_b64":"v9vW3BIgvT9e5fVYcI6BQa6D6CJibA3f6ZJIw4e8z6nCf+vAqpQ2eQuqYIg86fvICBbSWCb0Wy1FkwGr84bTBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4771de60bae08a5c4d06f61a7d521b030f04d1415ef8bb2d41c9b0ac87fc22e2","last_reissued_at":"2026-07-05T00:01:57.365234Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:01:57.365234Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Positive and negative feedback of AGN outflows in NGC 5728","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aeree Chung, Daeun Kang, Hyun-Jin Bae, Jaejin Shin, Jong-Hak Woo, Junhyun Baek, Kyuhyoun Cho","submitted_at":"2019-07-01T18:00:02Z","abstract_excerpt":"We present a spatially-resolved analysis of ionized and molecular gas in a nearby Seyfert 2 galaxy NGC 5728, using the VLT/MUSE and ALMA data. We find ionized gas outflows out to ~kpc scales, which encounter the star formation ring at 1 kpc radius. The star formation rate of the encountering region is significantly high (~1.8 M$_{\\rm sol}/yr/kpc^2$) compared to other regions in the ring. In contrast, the CO (2-1) emission is significantly weaker by a factor of ~3.5, indicating very high star formation efficiency. These results support the positive feedback scenario that the AGN-driven outflows"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1907.00982","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/1907.00982/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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1907.00982","created_at":"2026-07-05T00:01:57.365292+00:00"},{"alias_kind":"arxiv_version","alias_value":"1907.00982v1","created_at":"2026-07-05T00:01:57.365292+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1907.00982","created_at":"2026-07-05T00:01:57.365292+00:00"},{"alias_kind":"pith_short_12","alias_value":"I5Y54YF24CFF","created_at":"2026-07-05T00:01:57.365292+00:00"},{"alias_kind":"pith_short_16","alias_value":"I5Y54YF24CFFYTIG","created_at":"2026-07-05T00:01:57.365292+00:00"},{"alias_kind":"pith_short_8","alias_value":"I5Y54YF2","created_at":"2026-07-05T00:01:57.365292+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/I5Y54YF24CFFYTIG6YNH2UQ3AM","json":"https://pith.science/pith/I5Y54YF24CFFYTIG6YNH2UQ3AM.json","graph_json":"https://pith.science/api/pith-number/I5Y54YF24CFFYTIG6YNH2UQ3AM/graph.json","events_json":"https://pith.science/api/pith-number/I5Y54YF24CFFYTIG6YNH2UQ3AM/events.json","paper":"https://pith.science/paper/I5Y54YF2"},"agent_actions":{"view_html":"https://pith.science/pith/I5Y54YF24CFFYTIG6YNH2UQ3AM","download_json":"https://pith.science/pith/I5Y54YF24CFFYTIG6YNH2UQ3AM.json","view_paper":"https://pith.science/paper/I5Y54YF2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1907.00982&json=true","fetch_graph":"https://pith.science/api/pith-number/I5Y54YF24CFFYTIG6YNH2UQ3AM/graph.json","fetch_events":"https://pith.science/api/pith-number/I5Y54YF24CFFYTIG6YNH2UQ3AM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I5Y54YF24CFFYTIG6YNH2UQ3AM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I5Y54YF24CFFYTIG6YNH2UQ3AM/action/storage_attestation","attest_author":"https://pith.science/pith/I5Y54YF24CFFYTIG6YNH2UQ3AM/action/author_attestation","sign_citation":"https://pith.science/pith/I5Y54YF24CFFYTIG6YNH2UQ3AM/action/citation_signature","submit_replication":"https://pith.science/pith/I5Y54YF24CFFYTIG6YNH2UQ3AM/action/replication_record"}},"created_at":"2026-07-05T00:01:57.365292+00:00","updated_at":"2026-07-05T00:01:57.365292+00:00"}