{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:Z3SGXWGD6ASUBO3RXHMUKFKO5W","short_pith_number":"pith:Z3SGXWGD","schema_version":"1.0","canonical_sha256":"cee46bd8c3f02540bb71b9d945154eed82af996471bc10d1b91c689dbd2aa6f4","source":{"kind":"arxiv","id":"1402.0999","version":1},"attestation_state":"computed","paper":{"title":"The molecular circumnuclear disk (CND) in Centaurus A: A multi-transition CO and [CI] survey with Herschel, APEX, JCMT, and SEST","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A.F. Loenen, A. Harris, A. Weiss, C. Kramer, F.P. Israel, J. Martin-Pintado, J. Stutzki, M.A. Requena-Torres, P. van der Werf, R. Guesten, R. Meijerink","submitted_at":"2014-02-05T10:24:02Z","abstract_excerpt":"We present new CO and C^o line measurements of the compact circumnuclear disk in the center of NGC 128 (Centaurus~A) obtained with the Herschel Space Observatory, as well as SEST, JCMT, and APEX. The Cen A center CO ladder is quite different from those of either star-burst galaxies or AGNs. In addition, the relative intensity of the central Cen A [CI] emission lines is much greate than that in any other galaxy. The CO surface brightness of the compact circumnuclear disk (CND) is significantly higher than that of the much more extended thin disk (ETD) in the same line of sight. Our LVG and PDR/"},"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":"1402.0999","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-02-05T10:24:02Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"028043a4111d10f886bf940faf0c040cb02d3cc7e3cd2792d59f5df16d921aea","abstract_canon_sha256":"3ef376dc370f4112407416e7cc8f92a3ee90462600085cf9c48059f3c0e42d97"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:44:47.573435Z","signature_b64":"xjQuC1L3kKshOrLKoA3mfnMJx8hIvk+oEjn87kxAhCn0YXkgAf7rvIfQldcjyHOeyx3FK+QqE01W8PGYneyvBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cee46bd8c3f02540bb71b9d945154eed82af996471bc10d1b91c689dbd2aa6f4","last_reissued_at":"2026-05-18T01:44:47.572791Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:44:47.572791Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The molecular circumnuclear disk (CND) in Centaurus A: A multi-transition CO and [CI] survey with Herschel, APEX, JCMT, and SEST","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A.F. Loenen, A. Harris, A. Weiss, C. Kramer, F.P. Israel, J. Martin-Pintado, J. Stutzki, M.A. Requena-Torres, P. van der Werf, R. Guesten, R. Meijerink","submitted_at":"2014-02-05T10:24:02Z","abstract_excerpt":"We present new CO and C^o line measurements of the compact circumnuclear disk in the center of NGC 128 (Centaurus~A) obtained with the Herschel Space Observatory, as well as SEST, JCMT, and APEX. The Cen A center CO ladder is quite different from those of either star-burst galaxies or AGNs. In addition, the relative intensity of the central Cen A [CI] emission lines is much greate than that in any other galaxy. The CO surface brightness of the compact circumnuclear disk (CND) is significantly higher than that of the much more extended thin disk (ETD) in the same line of sight. Our LVG and PDR/"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1402.0999","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":"1402.0999","created_at":"2026-05-18T01:44:47.572895+00:00"},{"alias_kind":"arxiv_version","alias_value":"1402.0999v1","created_at":"2026-05-18T01:44:47.572895+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1402.0999","created_at":"2026-05-18T01:44:47.572895+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z3SGXWGD6ASU","created_at":"2026-05-18T12:28:59.999130+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z3SGXWGD6ASUBO3R","created_at":"2026-05-18T12:28:59.999130+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z3SGXWGD","created_at":"2026-05-18T12:28:59.999130+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/Z3SGXWGD6ASUBO3RXHMUKFKO5W","json":"https://pith.science/pith/Z3SGXWGD6ASUBO3RXHMUKFKO5W.json","graph_json":"https://pith.science/api/pith-number/Z3SGXWGD6ASUBO3RXHMUKFKO5W/graph.json","events_json":"https://pith.science/api/pith-number/Z3SGXWGD6ASUBO3RXHMUKFKO5W/events.json","paper":"https://pith.science/paper/Z3SGXWGD"},"agent_actions":{"view_html":"https://pith.science/pith/Z3SGXWGD6ASUBO3RXHMUKFKO5W","download_json":"https://pith.science/pith/Z3SGXWGD6ASUBO3RXHMUKFKO5W.json","view_paper":"https://pith.science/paper/Z3SGXWGD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1402.0999&json=true","fetch_graph":"https://pith.science/api/pith-number/Z3SGXWGD6ASUBO3RXHMUKFKO5W/graph.json","fetch_events":"https://pith.science/api/pith-number/Z3SGXWGD6ASUBO3RXHMUKFKO5W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z3SGXWGD6ASUBO3RXHMUKFKO5W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z3SGXWGD6ASUBO3RXHMUKFKO5W/action/storage_attestation","attest_author":"https://pith.science/pith/Z3SGXWGD6ASUBO3RXHMUKFKO5W/action/author_attestation","sign_citation":"https://pith.science/pith/Z3SGXWGD6ASUBO3RXHMUKFKO5W/action/citation_signature","submit_replication":"https://pith.science/pith/Z3SGXWGD6ASUBO3RXHMUKFKO5W/action/replication_record"}},"created_at":"2026-05-18T01:44:47.572895+00:00","updated_at":"2026-05-18T01:44:47.572895+00:00"}