{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:6UM2HCBMGYSL6E2LMWTBNQIOQ6","short_pith_number":"pith:6UM2HCBM","schema_version":"1.0","canonical_sha256":"f519a3882c3624bf134b65a616c10e87b05d66991cd0dc545271a9a6d384f2d0","source":{"kind":"arxiv","id":"1404.1402","version":1},"attestation_state":"computed","paper":{"title":"ALMA Observations of Warm Molecular Gas and Cold Dust in NGC 34","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. S. Evans, B. Schulz, C. Cao, C. K. Xu (IPAC), D. B. Sanders, E. J. Murphy, J. Chu, J. M. Mazzarella, L. Armus, N. Lu, P. Appleton, P. van der Werf, R. Meijerink, S. Haan, S. Lord, S. Stierwalt, T. Diaz-Santos, V. Charmandaris, Y. Gao, Y.-H. Zhao","submitted_at":"2014-04-04T22:05:19Z","abstract_excerpt":"We present ALMA Cycle-0 observations of the CO (6-5) line emission (rest-frame frequency = 691.473 GHz) and of the 435$\\mu m$ dust continuum emission in the nuclear region of NGC 34, a local luminous infrared galaxy (LIRG) at a distance of 84 Mpc (1\" = 407 pc) which contains a Seyfert 2 active galactic nucleus (AGN) and a nuclear starburst. The CO emission is well resolved by the ALMA beam ($\\rm 0.\"26\\times 0.\"23$), with an integrated flux of $\\rm f_{CO~(6-5)} = 1004\\; (\\pm 151) \\; Jy\\; km\\; s^{-1}$. Both the morphology and kinematics of the CO (6-5) emission are rather regular, consistent wit"},"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":"1404.1402","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-04-04T22:05:19Z","cross_cats_sorted":[],"title_canon_sha256":"fc38f37ee91f204083a066c635c7428c31fed20a366f939f3d06c86921da0893","abstract_canon_sha256":"b2d0265d37d2856d72316eb2467edb63b5018d477b2b8088f686111dbbd49025"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:37.388236Z","signature_b64":"SmJc4AZGszHDQ6XuCTaNAHJH1n/7gv3h/seo2qb9xeBWxZwpRPTSdqzFNzj22Zx+4Yum5k0VeSCwL4O4VjTDBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f519a3882c3624bf134b65a616c10e87b05d66991cd0dc545271a9a6d384f2d0","last_reissued_at":"2026-05-18T01:43:37.387612Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:37.387612Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"ALMA Observations of Warm Molecular Gas and Cold Dust in NGC 34","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. S. Evans, B. Schulz, C. Cao, C. K. Xu (IPAC), D. B. Sanders, E. J. Murphy, J. Chu, J. M. Mazzarella, L. Armus, N. Lu, P. Appleton, P. van der Werf, R. Meijerink, S. Haan, S. Lord, S. Stierwalt, T. Diaz-Santos, V. Charmandaris, Y. Gao, Y.-H. Zhao","submitted_at":"2014-04-04T22:05:19Z","abstract_excerpt":"We present ALMA Cycle-0 observations of the CO (6-5) line emission (rest-frame frequency = 691.473 GHz) and of the 435$\\mu m$ dust continuum emission in the nuclear region of NGC 34, a local luminous infrared galaxy (LIRG) at a distance of 84 Mpc (1\" = 407 pc) which contains a Seyfert 2 active galactic nucleus (AGN) and a nuclear starburst. The CO emission is well resolved by the ALMA beam ($\\rm 0.\"26\\times 0.\"23$), with an integrated flux of $\\rm f_{CO~(6-5)} = 1004\\; (\\pm 151) \\; Jy\\; km\\; s^{-1}$. Both the morphology and kinematics of the CO (6-5) emission are rather regular, consistent wit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.1402","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":"1404.1402","created_at":"2026-05-18T01:43:37.387701+00:00"},{"alias_kind":"arxiv_version","alias_value":"1404.1402v1","created_at":"2026-05-18T01:43:37.387701+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.1402","created_at":"2026-05-18T01:43:37.387701+00:00"},{"alias_kind":"pith_short_12","alias_value":"6UM2HCBMGYSL","created_at":"2026-05-18T12:28:16.859392+00:00"},{"alias_kind":"pith_short_16","alias_value":"6UM2HCBMGYSL6E2L","created_at":"2026-05-18T12:28:16.859392+00:00"},{"alias_kind":"pith_short_8","alias_value":"6UM2HCBM","created_at":"2026-05-18T12:28:16.859392+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/6UM2HCBMGYSL6E2LMWTBNQIOQ6","json":"https://pith.science/pith/6UM2HCBMGYSL6E2LMWTBNQIOQ6.json","graph_json":"https://pith.science/api/pith-number/6UM2HCBMGYSL6E2LMWTBNQIOQ6/graph.json","events_json":"https://pith.science/api/pith-number/6UM2HCBMGYSL6E2LMWTBNQIOQ6/events.json","paper":"https://pith.science/paper/6UM2HCBM"},"agent_actions":{"view_html":"https://pith.science/pith/6UM2HCBMGYSL6E2LMWTBNQIOQ6","download_json":"https://pith.science/pith/6UM2HCBMGYSL6E2LMWTBNQIOQ6.json","view_paper":"https://pith.science/paper/6UM2HCBM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1404.1402&json=true","fetch_graph":"https://pith.science/api/pith-number/6UM2HCBMGYSL6E2LMWTBNQIOQ6/graph.json","fetch_events":"https://pith.science/api/pith-number/6UM2HCBMGYSL6E2LMWTBNQIOQ6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6UM2HCBMGYSL6E2LMWTBNQIOQ6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6UM2HCBMGYSL6E2LMWTBNQIOQ6/action/storage_attestation","attest_author":"https://pith.science/pith/6UM2HCBMGYSL6E2LMWTBNQIOQ6/action/author_attestation","sign_citation":"https://pith.science/pith/6UM2HCBMGYSL6E2LMWTBNQIOQ6/action/citation_signature","submit_replication":"https://pith.science/pith/6UM2HCBMGYSL6E2LMWTBNQIOQ6/action/replication_record"}},"created_at":"2026-05-18T01:43:37.387701+00:00","updated_at":"2026-05-18T01:43:37.387701+00:00"}