{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:MUTENGHDGN655QBMH53KXWA7JB","short_pith_number":"pith:MUTENGHD","schema_version":"1.0","canonical_sha256":"65264698e3337ddec02c3f76abd81f48710d51b230f15b74752c99c087b646c5","source":{"kind":"arxiv","id":"2505.08867","version":2},"attestation_state":"computed","paper":{"title":"GA-NIFS: Mapping $z\\simeq3.5$ AGN-driven ionized outflows in the COSMOS field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. J. Bunker, B. Rodr\\'iguez Del Pino, C. Circosta, C. J. Willott, C. Vignali, E. Bertola, E. Parlanti, G. Cresci, G. Tozzi, G. Venturi, H. \\\"Ubler, I. Lamperti, J. Scholtz, M. A. Marshall, M. Perna, R. Maiolino, S. Arribas, S. Carniani, S. Charlot, T. B\\\"oker","submitted_at":"2025-05-13T18:00:02Z","abstract_excerpt":"Active galactic nuclei (AGNi) are a key ingredient in galaxy evolution and possibly shape galaxy growth through the generation of powerful outflows. Little is known regarding AGN-driven ionized outflows in moderate-luminosity AGNi (logLbol[erg/s]<47) beyond cosmic noon (z>3). We present the first systematic analysis of the ionized outflow properties of a sample of X-ray-selected AGNi (logLx[erg/s]>44) from the COSMOS-Legacy field at z~3.5 and with logLbol[erg/s]=45.2-46.7, by using JWST NIRSpec/IFU spectroscopic observations as part of the GA-NIFS program. We spectrally isolated and spatially "},"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":"2505.08867","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-05-13T18:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"af65d0f5919772630cb7851066602d712d37cad35cbd8c93ada2f7f7e743b213","abstract_canon_sha256":"0c1d0b5eb2e1ccd264c1dd324d6b98a35f3facfbba7fa347940cd5511e38dcb5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:33:51.009655Z","signature_b64":"7vXnRlSDNLnOU4qdZ20s8I6XcC2Bm9QPsC2PsnhixTc7U/E9AX4UestJL0By29YhnUQY21sfmtFXcmz5D2h/BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"65264698e3337ddec02c3f76abd81f48710d51b230f15b74752c99c087b646c5","last_reissued_at":"2026-07-05T11:33:51.009132Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:33:51.009132Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"GA-NIFS: Mapping $z\\simeq3.5$ AGN-driven ionized outflows in the COSMOS field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. J. Bunker, B. Rodr\\'iguez Del Pino, C. Circosta, C. J. Willott, C. Vignali, E. Bertola, E. Parlanti, G. Cresci, G. Tozzi, G. Venturi, H. \\\"Ubler, I. Lamperti, J. Scholtz, M. A. Marshall, M. Perna, R. Maiolino, S. Arribas, S. Carniani, S. Charlot, T. B\\\"oker","submitted_at":"2025-05-13T18:00:02Z","abstract_excerpt":"Active galactic nuclei (AGNi) are a key ingredient in galaxy evolution and possibly shape galaxy growth through the generation of powerful outflows. Little is known regarding AGN-driven ionized outflows in moderate-luminosity AGNi (logLbol[erg/s]<47) beyond cosmic noon (z>3). We present the first systematic analysis of the ionized outflow properties of a sample of X-ray-selected AGNi (logLx[erg/s]>44) from the COSMOS-Legacy field at z~3.5 and with logLbol[erg/s]=45.2-46.7, by using JWST NIRSpec/IFU spectroscopic observations as part of the GA-NIFS program. We spectrally isolated and spatially "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2505.08867","kind":"arxiv","version":2},"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/2505.08867/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":"2505.08867","created_at":"2026-07-05T11:33:51.009192+00:00"},{"alias_kind":"arxiv_version","alias_value":"2505.08867v2","created_at":"2026-07-05T11:33:51.009192+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2505.08867","created_at":"2026-07-05T11:33:51.009192+00:00"},{"alias_kind":"pith_short_12","alias_value":"MUTENGHDGN65","created_at":"2026-07-05T11:33:51.009192+00:00"},{"alias_kind":"pith_short_16","alias_value":"MUTENGHDGN655QBM","created_at":"2026-07-05T11:33:51.009192+00:00"},{"alias_kind":"pith_short_8","alias_value":"MUTENGHD","created_at":"2026-07-05T11:33:51.009192+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.07064","citing_title":"GA-NIFS: an extended [OIII] halo around the sub-Eddington quasar J1342+0928 at z=7.54","ref_index":20,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MUTENGHDGN655QBMH53KXWA7JB","json":"https://pith.science/pith/MUTENGHDGN655QBMH53KXWA7JB.json","graph_json":"https://pith.science/api/pith-number/MUTENGHDGN655QBMH53KXWA7JB/graph.json","events_json":"https://pith.science/api/pith-number/MUTENGHDGN655QBMH53KXWA7JB/events.json","paper":"https://pith.science/paper/MUTENGHD"},"agent_actions":{"view_html":"https://pith.science/pith/MUTENGHDGN655QBMH53KXWA7JB","download_json":"https://pith.science/pith/MUTENGHDGN655QBMH53KXWA7JB.json","view_paper":"https://pith.science/paper/MUTENGHD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2505.08867&json=true","fetch_graph":"https://pith.science/api/pith-number/MUTENGHDGN655QBMH53KXWA7JB/graph.json","fetch_events":"https://pith.science/api/pith-number/MUTENGHDGN655QBMH53KXWA7JB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MUTENGHDGN655QBMH53KXWA7JB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MUTENGHDGN655QBMH53KXWA7JB/action/storage_attestation","attest_author":"https://pith.science/pith/MUTENGHDGN655QBMH53KXWA7JB/action/author_attestation","sign_citation":"https://pith.science/pith/MUTENGHDGN655QBMH53KXWA7JB/action/citation_signature","submit_replication":"https://pith.science/pith/MUTENGHDGN655QBMH53KXWA7JB/action/replication_record"}},"created_at":"2026-07-05T11:33:51.009192+00:00","updated_at":"2026-07-05T11:33:51.009192+00:00"}