{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:MQLDU7N5TAPKQNKFPA3I7LLSC7","short_pith_number":"pith:MQLDU7N5","schema_version":"1.0","canonical_sha256":"64163a7dbd981ea8354578368fad7217ed3d12a4ee1cf6b4101156bbb02afe1c","source":{"kind":"arxiv","id":"1210.8039","version":1},"attestation_state":"computed","paper":{"title":"Fueling the central engine of radio galaxies. II. The footprints of AGN feedback on the ISM of 3C 236","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Fuente, A. Labiano, A. Usero, F. Combes, G. Tremblay, R. Morganti, R. Neri, R. Soria-Ruiz, S. Garcia-Burillo, T. Oosterloo","submitted_at":"2012-10-30T15:03:13Z","abstract_excerpt":"Aims: We study the emission of molecular gas in 3C236, a FR II radio source at z~0.1, and search for the footprints of AGN feedback. 3C236 shows signs of a reactivation of its AGN triggered by a recent minor merger episode. Observations have also previously identified an extreme HI outflow in this source. Methods: The IRAM PdBI has been used to study the distribution and kinematics of molecular gas in 3C236 by imaging with high spatial resolution the emission of the 12CO(2-1) line in the nucleus of the galaxy. We have searched for outflow signatures in the CO map. We have also derived the SFR "},"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":"1210.8039","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-10-30T15:03:13Z","cross_cats_sorted":[],"title_canon_sha256":"56b73378a3595fbeb8f4d230909bba552469a31ee49e44e665bd2a1c42a597d3","abstract_canon_sha256":"0cad0f8b1f99b7857c053dba52a8a126fae43c8b9cef2346178a1390a4f3aa15"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:53:35.548901Z","signature_b64":"UAyjnvGXmjX0l2e/ohNvKSe6QjNlP9jKgYMUvFglLmeakFW8zQvB00kp6Z/03g/G5npIMijQ9AA3E2q2yDphDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"64163a7dbd981ea8354578368fad7217ed3d12a4ee1cf6b4101156bbb02afe1c","last_reissued_at":"2026-05-18T01:53:35.548325Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:53:35.548325Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fueling the central engine of radio galaxies. II. The footprints of AGN feedback on the ISM of 3C 236","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Fuente, A. Labiano, A. Usero, F. Combes, G. Tremblay, R. Morganti, R. Neri, R. Soria-Ruiz, S. Garcia-Burillo, T. Oosterloo","submitted_at":"2012-10-30T15:03:13Z","abstract_excerpt":"Aims: We study the emission of molecular gas in 3C236, a FR II radio source at z~0.1, and search for the footprints of AGN feedback. 3C236 shows signs of a reactivation of its AGN triggered by a recent minor merger episode. Observations have also previously identified an extreme HI outflow in this source. Methods: The IRAM PdBI has been used to study the distribution and kinematics of molecular gas in 3C236 by imaging with high spatial resolution the emission of the 12CO(2-1) line in the nucleus of the galaxy. We have searched for outflow signatures in the CO map. We have also derived the SFR "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.8039","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":"1210.8039","created_at":"2026-05-18T01:53:35.548446+00:00"},{"alias_kind":"arxiv_version","alias_value":"1210.8039v1","created_at":"2026-05-18T01:53:35.548446+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.8039","created_at":"2026-05-18T01:53:35.548446+00:00"},{"alias_kind":"pith_short_12","alias_value":"MQLDU7N5TAPK","created_at":"2026-05-18T12:27:14.488303+00:00"},{"alias_kind":"pith_short_16","alias_value":"MQLDU7N5TAPKQNKF","created_at":"2026-05-18T12:27:14.488303+00:00"},{"alias_kind":"pith_short_8","alias_value":"MQLDU7N5","created_at":"2026-05-18T12:27:14.488303+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/MQLDU7N5TAPKQNKFPA3I7LLSC7","json":"https://pith.science/pith/MQLDU7N5TAPKQNKFPA3I7LLSC7.json","graph_json":"https://pith.science/api/pith-number/MQLDU7N5TAPKQNKFPA3I7LLSC7/graph.json","events_json":"https://pith.science/api/pith-number/MQLDU7N5TAPKQNKFPA3I7LLSC7/events.json","paper":"https://pith.science/paper/MQLDU7N5"},"agent_actions":{"view_html":"https://pith.science/pith/MQLDU7N5TAPKQNKFPA3I7LLSC7","download_json":"https://pith.science/pith/MQLDU7N5TAPKQNKFPA3I7LLSC7.json","view_paper":"https://pith.science/paper/MQLDU7N5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1210.8039&json=true","fetch_graph":"https://pith.science/api/pith-number/MQLDU7N5TAPKQNKFPA3I7LLSC7/graph.json","fetch_events":"https://pith.science/api/pith-number/MQLDU7N5TAPKQNKFPA3I7LLSC7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MQLDU7N5TAPKQNKFPA3I7LLSC7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MQLDU7N5TAPKQNKFPA3I7LLSC7/action/storage_attestation","attest_author":"https://pith.science/pith/MQLDU7N5TAPKQNKFPA3I7LLSC7/action/author_attestation","sign_citation":"https://pith.science/pith/MQLDU7N5TAPKQNKFPA3I7LLSC7/action/citation_signature","submit_replication":"https://pith.science/pith/MQLDU7N5TAPKQNKFPA3I7LLSC7/action/replication_record"}},"created_at":"2026-05-18T01:53:35.548446+00:00","updated_at":"2026-05-18T01:53:35.548446+00:00"}