{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:6GDKGCIJXPHCJ7H6UQYTXZ23VX","short_pith_number":"pith:6GDKGCIJ","schema_version":"1.0","canonical_sha256":"f186a30909bbce24fcfea4313be75baddea9fd077e495fb09cd965f92629004f","source":{"kind":"arxiv","id":"1105.3543","version":1},"attestation_state":"computed","paper":{"title":"Physical properties of the circumnuclear starburst ring in the barred Galaxy NGC 1097","license":"http://creativecommons.org/licenses/by/3.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Guilin Liu, Nagisa Oi, Paul T. P. Ho, Pei-Ying Hsieh, Satoki Matsushita, Ya-Lin Wu","submitted_at":"2011-05-18T06:23:43Z","abstract_excerpt":"We report high resolution 12CO(J = 2-1), 13CO(J = 2-1), and 12CO(J = 3-2) imaging of the Seyfert 1/starburst ring galaxy NGC 1097 with the Submillimeter Array to study the physical and kinematic properties of the 1-kpc circumnuclear starburst ring. Individual star clusters as detected in the HST map of Pa_alpha line emission have been used to determine the star formation rate, and are compared with the properties of the molecular gas. The molecular ring has been resolved into individual clumps at GMA-scale of 200--300 pc in all three CO lines. The intersection between the dust lanes and the st"},"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":"1105.3543","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/3.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-05-18T06:23:43Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"840f1884b6536a372cdaacc76f6ee329b12c348d9625bdf1a0bf74405413a336","abstract_canon_sha256":"5053bbe6edb76f3997dbc88f0ee8fd98c867f06c22ddee36b35e1fa480f2c0cc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:56.695278Z","signature_b64":"EmBvY37msKu02EhjOjMTxCj04g1kzaVeycra2mOM5dec5+sJiRP3SJ/Fmsfm9aZ5NA+OPt6VTM6mJVXsB0C6Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f186a30909bbce24fcfea4313be75baddea9fd077e495fb09cd965f92629004f","last_reissued_at":"2026-05-18T02:01:56.694713Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:56.694713Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Physical properties of the circumnuclear starburst ring in the barred Galaxy NGC 1097","license":"http://creativecommons.org/licenses/by/3.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Guilin Liu, Nagisa Oi, Paul T. P. Ho, Pei-Ying Hsieh, Satoki Matsushita, Ya-Lin Wu","submitted_at":"2011-05-18T06:23:43Z","abstract_excerpt":"We report high resolution 12CO(J = 2-1), 13CO(J = 2-1), and 12CO(J = 3-2) imaging of the Seyfert 1/starburst ring galaxy NGC 1097 with the Submillimeter Array to study the physical and kinematic properties of the 1-kpc circumnuclear starburst ring. Individual star clusters as detected in the HST map of Pa_alpha line emission have been used to determine the star formation rate, and are compared with the properties of the molecular gas. The molecular ring has been resolved into individual clumps at GMA-scale of 200--300 pc in all three CO lines. The intersection between the dust lanes and the st"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1105.3543","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":"1105.3543","created_at":"2026-05-18T02:01:56.694797+00:00"},{"alias_kind":"arxiv_version","alias_value":"1105.3543v1","created_at":"2026-05-18T02:01:56.694797+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1105.3543","created_at":"2026-05-18T02:01:56.694797+00:00"},{"alias_kind":"pith_short_12","alias_value":"6GDKGCIJXPHC","created_at":"2026-05-18T12:26:22.705136+00:00"},{"alias_kind":"pith_short_16","alias_value":"6GDKGCIJXPHCJ7H6","created_at":"2026-05-18T12:26:22.705136+00:00"},{"alias_kind":"pith_short_8","alias_value":"6GDKGCIJ","created_at":"2026-05-18T12:26:22.705136+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/6GDKGCIJXPHCJ7H6UQYTXZ23VX","json":"https://pith.science/pith/6GDKGCIJXPHCJ7H6UQYTXZ23VX.json","graph_json":"https://pith.science/api/pith-number/6GDKGCIJXPHCJ7H6UQYTXZ23VX/graph.json","events_json":"https://pith.science/api/pith-number/6GDKGCIJXPHCJ7H6UQYTXZ23VX/events.json","paper":"https://pith.science/paper/6GDKGCIJ"},"agent_actions":{"view_html":"https://pith.science/pith/6GDKGCIJXPHCJ7H6UQYTXZ23VX","download_json":"https://pith.science/pith/6GDKGCIJXPHCJ7H6UQYTXZ23VX.json","view_paper":"https://pith.science/paper/6GDKGCIJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1105.3543&json=true","fetch_graph":"https://pith.science/api/pith-number/6GDKGCIJXPHCJ7H6UQYTXZ23VX/graph.json","fetch_events":"https://pith.science/api/pith-number/6GDKGCIJXPHCJ7H6UQYTXZ23VX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6GDKGCIJXPHCJ7H6UQYTXZ23VX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6GDKGCIJXPHCJ7H6UQYTXZ23VX/action/storage_attestation","attest_author":"https://pith.science/pith/6GDKGCIJXPHCJ7H6UQYTXZ23VX/action/author_attestation","sign_citation":"https://pith.science/pith/6GDKGCIJXPHCJ7H6UQYTXZ23VX/action/citation_signature","submit_replication":"https://pith.science/pith/6GDKGCIJXPHCJ7H6UQYTXZ23VX/action/replication_record"}},"created_at":"2026-05-18T02:01:56.694797+00:00","updated_at":"2026-05-18T02:01:56.694797+00:00"}