{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:TPJOCKBY5BLISLTQYE3FGTM5QW","short_pith_number":"pith:TPJOCKBY","schema_version":"1.0","canonical_sha256":"9bd2e12838e856892e70c136534d9d85932ef31c366432307b865fe7e52d2117","source":{"kind":"arxiv","id":"2312.01936","version":1},"attestation_state":"computed","paper":{"title":"Radio Jet Feedback on the Inner Disk of Virgo Spiral Galaxy Messier 58","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aditya Togi, Grant Donnelly, Ivan E. Lopez, Javier Roman, J. D. T. Smith, Lauranne Lanz, Osmin Caceres, Patrick M. Ogle, Philip N. Appleton, R. Michael Rich, Victoria Reynaldi, Zhuofu (Chester) Li","submitted_at":"2023-12-04T14:50:55Z","abstract_excerpt":"Spitzer spectral maps reveal a disk of highly luminous, warm (>150 K) H2 in the center of the massive spiral galaxy Messier 58, which hosts a radio-loud AGN. The inner 2.6 kpc of the galaxy appears to be overrun by shocks from the radio jet cocoon. Gemini NIRI imaging of the H2 1-0 S(1) emission line, ALMA CO 2-1, and HST multiband imagery indicate that much of the molecular gas is shocked in-situ, corresponding to lanes of dusty molecular gas that spiral towards the galaxy nucleus. The CO 2-1 and ionized gas kinematics are highly disturbed, with velocity dispersion up to 300 km/s. Dissipation"},"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":"2312.01936","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-12-04T14:50:55Z","cross_cats_sorted":[],"title_canon_sha256":"8be672ba455fdab35d6c8b8744ff4bff8b0a2377a6213acd4c56cf0df68f399f","abstract_canon_sha256":"922382a20f6cf54190766bccd74059c7deea112ff64bd70bcc59324f5d672cb7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:20:01.992734Z","signature_b64":"iZXC3TUGF/SxTohjfU2qoPYB6Hx0/JqpvSXcCrRzDNCfU8sJgf1wsiB0JGXoL1o3e/Ns/kH3NXKjWYI1h1GQDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9bd2e12838e856892e70c136534d9d85932ef31c366432307b865fe7e52d2117","last_reissued_at":"2026-07-05T07:20:01.992268Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:20:01.992268Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Radio Jet Feedback on the Inner Disk of Virgo Spiral Galaxy Messier 58","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aditya Togi, Grant Donnelly, Ivan E. Lopez, Javier Roman, J. D. T. Smith, Lauranne Lanz, Osmin Caceres, Patrick M. Ogle, Philip N. Appleton, R. Michael Rich, Victoria Reynaldi, Zhuofu (Chester) Li","submitted_at":"2023-12-04T14:50:55Z","abstract_excerpt":"Spitzer spectral maps reveal a disk of highly luminous, warm (>150 K) H2 in the center of the massive spiral galaxy Messier 58, which hosts a radio-loud AGN. The inner 2.6 kpc of the galaxy appears to be overrun by shocks from the radio jet cocoon. Gemini NIRI imaging of the H2 1-0 S(1) emission line, ALMA CO 2-1, and HST multiband imagery indicate that much of the molecular gas is shocked in-situ, corresponding to lanes of dusty molecular gas that spiral towards the galaxy nucleus. The CO 2-1 and ionized gas kinematics are highly disturbed, with velocity dispersion up to 300 km/s. Dissipation"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2312.01936","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2312.01936/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":"2312.01936","created_at":"2026-07-05T07:20:01.992326+00:00"},{"alias_kind":"arxiv_version","alias_value":"2312.01936v1","created_at":"2026-07-05T07:20:01.992326+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2312.01936","created_at":"2026-07-05T07:20:01.992326+00:00"},{"alias_kind":"pith_short_12","alias_value":"TPJOCKBY5BLI","created_at":"2026-07-05T07:20:01.992326+00:00"},{"alias_kind":"pith_short_16","alias_value":"TPJOCKBY5BLISLTQ","created_at":"2026-07-05T07:20:01.992326+00:00"},{"alias_kind":"pith_short_8","alias_value":"TPJOCKBY","created_at":"2026-07-05T07:20:01.992326+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/TPJOCKBY5BLISLTQYE3FGTM5QW","json":"https://pith.science/pith/TPJOCKBY5BLISLTQYE3FGTM5QW.json","graph_json":"https://pith.science/api/pith-number/TPJOCKBY5BLISLTQYE3FGTM5QW/graph.json","events_json":"https://pith.science/api/pith-number/TPJOCKBY5BLISLTQYE3FGTM5QW/events.json","paper":"https://pith.science/paper/TPJOCKBY"},"agent_actions":{"view_html":"https://pith.science/pith/TPJOCKBY5BLISLTQYE3FGTM5QW","download_json":"https://pith.science/pith/TPJOCKBY5BLISLTQYE3FGTM5QW.json","view_paper":"https://pith.science/paper/TPJOCKBY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2312.01936&json=true","fetch_graph":"https://pith.science/api/pith-number/TPJOCKBY5BLISLTQYE3FGTM5QW/graph.json","fetch_events":"https://pith.science/api/pith-number/TPJOCKBY5BLISLTQYE3FGTM5QW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TPJOCKBY5BLISLTQYE3FGTM5QW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TPJOCKBY5BLISLTQYE3FGTM5QW/action/storage_attestation","attest_author":"https://pith.science/pith/TPJOCKBY5BLISLTQYE3FGTM5QW/action/author_attestation","sign_citation":"https://pith.science/pith/TPJOCKBY5BLISLTQYE3FGTM5QW/action/citation_signature","submit_replication":"https://pith.science/pith/TPJOCKBY5BLISLTQYE3FGTM5QW/action/replication_record"}},"created_at":"2026-07-05T07:20:01.992326+00:00","updated_at":"2026-07-05T07:20:01.992326+00:00"}