{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:566LZFRCRKM7DZUKUGXTVOCN5Y","short_pith_number":"pith:566LZFRC","schema_version":"1.0","canonical_sha256":"efbcbc96228a99f1e68aa1af3ab84dee38220fa1bb2fae51a21513440c38c260","source":{"kind":"arxiv","id":"1409.1580","version":1},"attestation_state":"computed","paper":{"title":"A Census of Gas Outflows in Type 2 Active Galactic Nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Hyun-Jin Bae, Jong-Hak Woo","submitted_at":"2014-09-04T20:00:13Z","abstract_excerpt":"We perform a census of ionized gas outflows using a sample of ~23,000 type 2 active galactic nuclei (AGNs) out to z~0.1. By measuring the velocity offset of narrow emission lines, i.e., [O III] {\\lambda}5007 and H{\\alpha}, with respect to the systemic velocity measured from the stellar absorption lines, we find that 47% of AGNs display an [O III] line-of-sight velocity offset $\\geq$ 20 km/s. The fraction of the [O III] velocity offset in type 2 AGNs is comparable to that in type 1 AGNs after considering the projection effect. AGNs with a large [O III] velocity offset preferentially have a high"},"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":"1409.1580","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-09-04T20:00:13Z","cross_cats_sorted":[],"title_canon_sha256":"9f71b525feaffba139ac42a223ff23219009e6dda837cd504b70d62f683cd8db","abstract_canon_sha256":"6ef904dbfb4345bdf6fb2eee651dd67d6d09a6eea05a0c35c63c1dd562fa5f06"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:40:17.770895Z","signature_b64":"lq4aAYc34CU4o35NXi5yb7l1YggVDq1Rx2neeJc1scnEggs5mtZDt6mW267/CGd1rtdLSaExzl95PB/v7fCeAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"efbcbc96228a99f1e68aa1af3ab84dee38220fa1bb2fae51a21513440c38c260","last_reissued_at":"2026-05-18T02:40:17.770236Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:40:17.770236Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Census of Gas Outflows in Type 2 Active Galactic Nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Hyun-Jin Bae, Jong-Hak Woo","submitted_at":"2014-09-04T20:00:13Z","abstract_excerpt":"We perform a census of ionized gas outflows using a sample of ~23,000 type 2 active galactic nuclei (AGNs) out to z~0.1. By measuring the velocity offset of narrow emission lines, i.e., [O III] {\\lambda}5007 and H{\\alpha}, with respect to the systemic velocity measured from the stellar absorption lines, we find that 47% of AGNs display an [O III] line-of-sight velocity offset $\\geq$ 20 km/s. The fraction of the [O III] velocity offset in type 2 AGNs is comparable to that in type 1 AGNs after considering the projection effect. AGNs with a large [O III] velocity offset preferentially have a high"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1409.1580","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":"1409.1580","created_at":"2026-05-18T02:40:17.770309+00:00"},{"alias_kind":"arxiv_version","alias_value":"1409.1580v1","created_at":"2026-05-18T02:40:17.770309+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1409.1580","created_at":"2026-05-18T02:40:17.770309+00:00"},{"alias_kind":"pith_short_12","alias_value":"566LZFRCRKM7","created_at":"2026-05-18T12:28:14.216126+00:00"},{"alias_kind":"pith_short_16","alias_value":"566LZFRCRKM7DZUK","created_at":"2026-05-18T12:28:14.216126+00:00"},{"alias_kind":"pith_short_8","alias_value":"566LZFRC","created_at":"2026-05-18T12:28:14.216126+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.00105","citing_title":"AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN","ref_index":34,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/566LZFRCRKM7DZUKUGXTVOCN5Y","json":"https://pith.science/pith/566LZFRCRKM7DZUKUGXTVOCN5Y.json","graph_json":"https://pith.science/api/pith-number/566LZFRCRKM7DZUKUGXTVOCN5Y/graph.json","events_json":"https://pith.science/api/pith-number/566LZFRCRKM7DZUKUGXTVOCN5Y/events.json","paper":"https://pith.science/paper/566LZFRC"},"agent_actions":{"view_html":"https://pith.science/pith/566LZFRCRKM7DZUKUGXTVOCN5Y","download_json":"https://pith.science/pith/566LZFRCRKM7DZUKUGXTVOCN5Y.json","view_paper":"https://pith.science/paper/566LZFRC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1409.1580&json=true","fetch_graph":"https://pith.science/api/pith-number/566LZFRCRKM7DZUKUGXTVOCN5Y/graph.json","fetch_events":"https://pith.science/api/pith-number/566LZFRCRKM7DZUKUGXTVOCN5Y/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/566LZFRCRKM7DZUKUGXTVOCN5Y/action/timestamp_anchor","attest_storage":"https://pith.science/pith/566LZFRCRKM7DZUKUGXTVOCN5Y/action/storage_attestation","attest_author":"https://pith.science/pith/566LZFRCRKM7DZUKUGXTVOCN5Y/action/author_attestation","sign_citation":"https://pith.science/pith/566LZFRCRKM7DZUKUGXTVOCN5Y/action/citation_signature","submit_replication":"https://pith.science/pith/566LZFRCRKM7DZUKUGXTVOCN5Y/action/replication_record"}},"created_at":"2026-05-18T02:40:17.770309+00:00","updated_at":"2026-05-18T02:40:17.770309+00:00"}