{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:JDIEOAAYJSRDEKNFOKJHR5SVMW","short_pith_number":"pith:JDIEOAAY","schema_version":"1.0","canonical_sha256":"48d04700184ca23229a5729278f65565af3085cd01d50e3bc6e0c0e111495132","source":{"kind":"arxiv","id":"1902.06790","version":2},"attestation_state":"computed","paper":{"title":"Gemini NIFS survey of feeding and feedback in nearbyActive Galaxies - III. Ionized versus warm molecular gasmasses and distributions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Astor J. Schonell Jr., Luis G. Dahmer-Hahn, Marina Bianchin, Marlon R. Diniz, Natacha Z. Dametto, Rogemar A. Riffel, Rog\\'erio Riffel, Thaisa Storchi-Bergmann","submitted_at":"2019-02-18T20:38:51Z","abstract_excerpt":"We have used the Gemini Near-Infrared Integral Field Spectrograph (NIFS) in the J and K bands to map the distribution, excitation and kinematics of the ionized HII and warm molecular gas H$_2$, in the inner few 100 pc of 6 nearby active galaxies: NGC 788, Mrk 607, NGC 3227, NGC 3516, NGC 5506, NGC 5899. {For most galaxies, this is the first time that such maps have been obtained}. The ionized and H$_2$ gas show distinct kinematics: while the H$_2$ gas is mostly rotating in the galaxy plane with low velocity dispersion ($\\sigma$), the ionized gas usually shows signatures of outflows associated "},"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":"1902.06790","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-02-18T20:38:51Z","cross_cats_sorted":[],"title_canon_sha256":"d50e3ae36cba17724f26734aa009fb4cca110dac6aa0a90974c7a1cf847b3cdb","abstract_canon_sha256":"624b22119aa6d16a5160e648a0ea5358dbebd806603450eae64fbd6b70a490e4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:50:19.252662Z","signature_b64":"bujdyMVQXKsV0R53XcQ+3WWJcdQ2Jz1wT1LpR1er/WLm5AIqbTKLYQBu/SHZkkgIhkZEL775yBam3HlZk9SnAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"48d04700184ca23229a5729278f65565af3085cd01d50e3bc6e0c0e111495132","last_reissued_at":"2026-05-17T23:50:19.252002Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:50:19.252002Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gemini NIFS survey of feeding and feedback in nearbyActive Galaxies - III. Ionized versus warm molecular gasmasses and distributions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Astor J. Schonell Jr., Luis G. Dahmer-Hahn, Marina Bianchin, Marlon R. Diniz, Natacha Z. Dametto, Rogemar A. Riffel, Rog\\'erio Riffel, Thaisa Storchi-Bergmann","submitted_at":"2019-02-18T20:38:51Z","abstract_excerpt":"We have used the Gemini Near-Infrared Integral Field Spectrograph (NIFS) in the J and K bands to map the distribution, excitation and kinematics of the ionized HII and warm molecular gas H$_2$, in the inner few 100 pc of 6 nearby active galaxies: NGC 788, Mrk 607, NGC 3227, NGC 3516, NGC 5506, NGC 5899. {For most galaxies, this is the first time that such maps have been obtained}. The ionized and H$_2$ gas show distinct kinematics: while the H$_2$ gas is mostly rotating in the galaxy plane with low velocity dispersion ($\\sigma$), the ionized gas usually shows signatures of outflows associated "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1902.06790","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":""},"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":"1902.06790","created_at":"2026-05-17T23:50:19.252109+00:00"},{"alias_kind":"arxiv_version","alias_value":"1902.06790v2","created_at":"2026-05-17T23:50:19.252109+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1902.06790","created_at":"2026-05-17T23:50:19.252109+00:00"},{"alias_kind":"pith_short_12","alias_value":"JDIEOAAYJSRD","created_at":"2026-05-18T12:33:18.533446+00:00"},{"alias_kind":"pith_short_16","alias_value":"JDIEOAAYJSRDEKNF","created_at":"2026-05-18T12:33:18.533446+00:00"},{"alias_kind":"pith_short_8","alias_value":"JDIEOAAY","created_at":"2026-05-18T12:33:18.533446+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/JDIEOAAYJSRDEKNFOKJHR5SVMW","json":"https://pith.science/pith/JDIEOAAYJSRDEKNFOKJHR5SVMW.json","graph_json":"https://pith.science/api/pith-number/JDIEOAAYJSRDEKNFOKJHR5SVMW/graph.json","events_json":"https://pith.science/api/pith-number/JDIEOAAYJSRDEKNFOKJHR5SVMW/events.json","paper":"https://pith.science/paper/JDIEOAAY"},"agent_actions":{"view_html":"https://pith.science/pith/JDIEOAAYJSRDEKNFOKJHR5SVMW","download_json":"https://pith.science/pith/JDIEOAAYJSRDEKNFOKJHR5SVMW.json","view_paper":"https://pith.science/paper/JDIEOAAY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1902.06790&json=true","fetch_graph":"https://pith.science/api/pith-number/JDIEOAAYJSRDEKNFOKJHR5SVMW/graph.json","fetch_events":"https://pith.science/api/pith-number/JDIEOAAYJSRDEKNFOKJHR5SVMW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JDIEOAAYJSRDEKNFOKJHR5SVMW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JDIEOAAYJSRDEKNFOKJHR5SVMW/action/storage_attestation","attest_author":"https://pith.science/pith/JDIEOAAYJSRDEKNFOKJHR5SVMW/action/author_attestation","sign_citation":"https://pith.science/pith/JDIEOAAYJSRDEKNFOKJHR5SVMW/action/citation_signature","submit_replication":"https://pith.science/pith/JDIEOAAYJSRDEKNFOKJHR5SVMW/action/replication_record"}},"created_at":"2026-05-17T23:50:19.252109+00:00","updated_at":"2026-05-17T23:50:19.252109+00:00"}