{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:IEMXHHYIPP6WGBIUPD2BIYEWN6","short_pith_number":"pith:IEMXHHYI","schema_version":"1.0","canonical_sha256":"4119739f087bfd63051478f41460966fbbaad93c35df5cbca681db485910f143","source":{"kind":"arxiv","id":"1201.1503","version":1},"attestation_state":"computed","paper":{"title":"Strong molecular hydrogen emission and kinematics of the multiphase gas in radio galaxies with fast jet-driven outflows","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Aaron Evans, Bjorn Emonts, Clive Tadhunter, Dan Evans, Patrick Ogle, Philip Appleton, Pierre Guillard, Raffaella Morganti, Tom Oosterloo","submitted_at":"2012-01-06T21:00:23Z","abstract_excerpt":"Observations of ionized and neutral gas outflows in radio-galaxies (RGs) suggest that AGN radio jet feedback has a galaxy-scale impact on the host ISM, but it is still unclear how the molecular gas is affected. We present deep Spitzer IRS spectroscopy of 8 RGs that show fast HI outflows. All of these HI-outflow RGs have bright H2 mid-IR lines that cannot be accounted for by UV or X-ray heating. This suggests that the radio jet, which drives the HI outflow, is also responsible for the shock-excitation of the warm H2 gas. In addition, the warm H2 gas does not share the kinematics of the ionized/"},"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":"1201.1503","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-01-06T21:00:23Z","cross_cats_sorted":[],"title_canon_sha256":"aeb8a7fe16f5dbc40d52883cf83e595f657e6fb2123795b8a9926a57b540d892","abstract_canon_sha256":"931b5b396a5b93d13ad13b1b1ad4b28fbf5d5d20f8952e067864c62cf5bd9be2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:54.703268Z","signature_b64":"ZOiwnBWudx3XcJkFZEM6y3ZKhaf5mt8FcIiDLzbHl0GjNMHEXR1o/8J19lld+VdNTU0TzRl+rk9yH/PyjEVhCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4119739f087bfd63051478f41460966fbbaad93c35df5cbca681db485910f143","last_reissued_at":"2026-05-18T01:58:54.702490Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:54.702490Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Strong molecular hydrogen emission and kinematics of the multiphase gas in radio galaxies with fast jet-driven outflows","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Aaron Evans, Bjorn Emonts, Clive Tadhunter, Dan Evans, Patrick Ogle, Philip Appleton, Pierre Guillard, Raffaella Morganti, Tom Oosterloo","submitted_at":"2012-01-06T21:00:23Z","abstract_excerpt":"Observations of ionized and neutral gas outflows in radio-galaxies (RGs) suggest that AGN radio jet feedback has a galaxy-scale impact on the host ISM, but it is still unclear how the molecular gas is affected. We present deep Spitzer IRS spectroscopy of 8 RGs that show fast HI outflows. All of these HI-outflow RGs have bright H2 mid-IR lines that cannot be accounted for by UV or X-ray heating. This suggests that the radio jet, which drives the HI outflow, is also responsible for the shock-excitation of the warm H2 gas. In addition, the warm H2 gas does not share the kinematics of the ionized/"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.1503","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":"1201.1503","created_at":"2026-05-18T01:58:54.702626+00:00"},{"alias_kind":"arxiv_version","alias_value":"1201.1503v1","created_at":"2026-05-18T01:58:54.702626+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.1503","created_at":"2026-05-18T01:58:54.702626+00:00"},{"alias_kind":"pith_short_12","alias_value":"IEMXHHYIPP6W","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_16","alias_value":"IEMXHHYIPP6WGBIU","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_8","alias_value":"IEMXHHYI","created_at":"2026-05-18T12:27:09.501522+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/IEMXHHYIPP6WGBIUPD2BIYEWN6","json":"https://pith.science/pith/IEMXHHYIPP6WGBIUPD2BIYEWN6.json","graph_json":"https://pith.science/api/pith-number/IEMXHHYIPP6WGBIUPD2BIYEWN6/graph.json","events_json":"https://pith.science/api/pith-number/IEMXHHYIPP6WGBIUPD2BIYEWN6/events.json","paper":"https://pith.science/paper/IEMXHHYI"},"agent_actions":{"view_html":"https://pith.science/pith/IEMXHHYIPP6WGBIUPD2BIYEWN6","download_json":"https://pith.science/pith/IEMXHHYIPP6WGBIUPD2BIYEWN6.json","view_paper":"https://pith.science/paper/IEMXHHYI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1201.1503&json=true","fetch_graph":"https://pith.science/api/pith-number/IEMXHHYIPP6WGBIUPD2BIYEWN6/graph.json","fetch_events":"https://pith.science/api/pith-number/IEMXHHYIPP6WGBIUPD2BIYEWN6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IEMXHHYIPP6WGBIUPD2BIYEWN6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IEMXHHYIPP6WGBIUPD2BIYEWN6/action/storage_attestation","attest_author":"https://pith.science/pith/IEMXHHYIPP6WGBIUPD2BIYEWN6/action/author_attestation","sign_citation":"https://pith.science/pith/IEMXHHYIPP6WGBIUPD2BIYEWN6/action/citation_signature","submit_replication":"https://pith.science/pith/IEMXHHYIPP6WGBIUPD2BIYEWN6/action/replication_record"}},"created_at":"2026-05-18T01:58:54.702626+00:00","updated_at":"2026-05-18T01:58:54.702626+00:00"}