{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:PVV2Q6RQYWPPAYXEU3EAINYLW7","short_pith_number":"pith:PVV2Q6RQ","schema_version":"1.0","canonical_sha256":"7d6ba87a30c59ef062e4a6c804370bb7d2bf75c4e7f4d7c838728c48f4fcfe36","source":{"kind":"arxiv","id":"1003.2369","version":1},"attestation_state":"computed","paper":{"title":"Detections of CO Molecular Gas in 24um-Bright ULIRGs at z~2 in the Spitzer First Look Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Omont (Univ. Paris), A. Sajina (Haverford College), D. Lutz (MPE), K.~M. Dasyra (CEA), Lin Yan (Caltech) L.~J. Tacconi (MPE), M. Zamojski (Caltech), N. Fiolet (Univ. Paris), P. Cox (IRAM), R. Neri (IRAM)","submitted_at":"2010-03-11T17:41:10Z","abstract_excerpt":"We present CO observations of 9 ULIRGs at z~2 with S(24\\mu m)>1mJy, previously confirmed with the mid-IR spectra in the Spitzer First Look Survey.  All targets are required to have accurate redshifts from Keck/GEMINI near-IR spectra. Using the Plateau de Bure millimeter-wave Interferometer (PdBI) at IRAM,  we detect CO J(3-2) [7 objects] or J(2-1) [1 object] line emission from 8 sources with integrated intensities Ic ~(5-9)sigma. The CO detected sources have a variety of mid-IR spectra, including strong PAH, deep silicate absorption and power-law continuum, implying that these molecular gas ri"},"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":"1003.2369","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-03-11T17:41:10Z","cross_cats_sorted":[],"title_canon_sha256":"48170e1eef797c26e9c8fbb3f763369a4ee416b8a1f74db6e4d8db1920ff2829","abstract_canon_sha256":"04565ca91ac9c254dfe92ffa96afa26a21aeffe27836ce1429279a4d35ae4446"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:08:34.929584Z","signature_b64":"KNDwlYDEVeKYp4Ozx+GIFuAXpZsDtxJSuSDxf9kVn7HSwLbTaz/4IiORUFn2JnodFfA7M7ZeCQx5/G55kCUVAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7d6ba87a30c59ef062e4a6c804370bb7d2bf75c4e7f4d7c838728c48f4fcfe36","last_reissued_at":"2026-05-18T02:08:34.928964Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:08:34.928964Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detections of CO Molecular Gas in 24um-Bright ULIRGs at z~2 in the Spitzer First Look Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Omont (Univ. Paris), A. Sajina (Haverford College), D. Lutz (MPE), K.~M. Dasyra (CEA), Lin Yan (Caltech) L.~J. Tacconi (MPE), M. Zamojski (Caltech), N. Fiolet (Univ. Paris), P. Cox (IRAM), R. Neri (IRAM)","submitted_at":"2010-03-11T17:41:10Z","abstract_excerpt":"We present CO observations of 9 ULIRGs at z~2 with S(24\\mu m)>1mJy, previously confirmed with the mid-IR spectra in the Spitzer First Look Survey.  All targets are required to have accurate redshifts from Keck/GEMINI near-IR spectra. Using the Plateau de Bure millimeter-wave Interferometer (PdBI) at IRAM,  we detect CO J(3-2) [7 objects] or J(2-1) [1 object] line emission from 8 sources with integrated intensities Ic ~(5-9)sigma. The CO detected sources have a variety of mid-IR spectra, including strong PAH, deep silicate absorption and power-law continuum, implying that these molecular gas ri"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1003.2369","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":"1003.2369","created_at":"2026-05-18T02:08:34.929071+00:00"},{"alias_kind":"arxiv_version","alias_value":"1003.2369v1","created_at":"2026-05-18T02:08:34.929071+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1003.2369","created_at":"2026-05-18T02:08:34.929071+00:00"},{"alias_kind":"pith_short_12","alias_value":"PVV2Q6RQYWPP","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_16","alias_value":"PVV2Q6RQYWPPAYXE","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_8","alias_value":"PVV2Q6RQ","created_at":"2026-05-18T12:26:12.377268+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/PVV2Q6RQYWPPAYXEU3EAINYLW7","json":"https://pith.science/pith/PVV2Q6RQYWPPAYXEU3EAINYLW7.json","graph_json":"https://pith.science/api/pith-number/PVV2Q6RQYWPPAYXEU3EAINYLW7/graph.json","events_json":"https://pith.science/api/pith-number/PVV2Q6RQYWPPAYXEU3EAINYLW7/events.json","paper":"https://pith.science/paper/PVV2Q6RQ"},"agent_actions":{"view_html":"https://pith.science/pith/PVV2Q6RQYWPPAYXEU3EAINYLW7","download_json":"https://pith.science/pith/PVV2Q6RQYWPPAYXEU3EAINYLW7.json","view_paper":"https://pith.science/paper/PVV2Q6RQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1003.2369&json=true","fetch_graph":"https://pith.science/api/pith-number/PVV2Q6RQYWPPAYXEU3EAINYLW7/graph.json","fetch_events":"https://pith.science/api/pith-number/PVV2Q6RQYWPPAYXEU3EAINYLW7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PVV2Q6RQYWPPAYXEU3EAINYLW7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PVV2Q6RQYWPPAYXEU3EAINYLW7/action/storage_attestation","attest_author":"https://pith.science/pith/PVV2Q6RQYWPPAYXEU3EAINYLW7/action/author_attestation","sign_citation":"https://pith.science/pith/PVV2Q6RQYWPPAYXEU3EAINYLW7/action/citation_signature","submit_replication":"https://pith.science/pith/PVV2Q6RQYWPPAYXEU3EAINYLW7/action/replication_record"}},"created_at":"2026-05-18T02:08:34.929071+00:00","updated_at":"2026-05-18T02:08:34.929071+00:00"}