{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:X2D7XUUGN462VLKDJMUCOL6M2H","short_pith_number":"pith:X2D7XUUG","schema_version":"1.0","canonical_sha256":"be87fbd2866f3daaad434b28272fccd1cd7d66a8b8131c667cd630927bcb9e0e","source":{"kind":"arxiv","id":"1403.0724","version":1},"attestation_state":"computed","paper":{"title":"The molecular gas content of ULIRG type 2 quasars at z < 1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Humphrey, B. Emonts, G. Drouart, M. I. Rodr\\'iguez, M. P\\'erez Torres, M. Villar-Mart\\'in, S. Garc\\'ia Burillo","submitted_at":"2014-03-04T09:15:23Z","abstract_excerpt":"We present new results of CO(1-0) spectroscopic observations of 4 SDSS type 2 quasars (QSO2) at z$\\sim$0.3, observed with the 30m IRAM telescope. The QSO2 have infrared luminosities in the ULIRG (UltraLuminous Infrared Galaxies) regime. We confirm the CO(1-0) detection in one of our 4 QSO2, SDSS J1543-00, with $L'_{CO}$ and $M_{H_2}$ (1.2$\\pm$0.2) $\\times$10$^{10}$ K km s$^{-1}$ pc$^2$ and (9.4$\\pm$1.4)$\\times$10$^9$ M$_{\\odot}$, respectively. The CO(1-0) line has $FWHM=$575$\\pm$102 km s$^{-1}$. No CO(1-0) emission is detected in SDSS J0903+02, SDSS J1337-01, SDSS J1520-01 above 3 sigma, yield"},"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":"1403.0724","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-03-04T09:15:23Z","cross_cats_sorted":[],"title_canon_sha256":"ee35250f6cae3d6ee21760a85ac91c5d2902fa9333cebe9faf86d469ea822ad0","abstract_canon_sha256":"e5659b56687f1b1b7c33a312ca8709dd73d8c9c41f19d7fafe4751b73546618f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:44:20.400454Z","signature_b64":"KUSorNcoUYtMyPqaSVFsTWgXWz7+x1CpaCszt+osqPp5iJEI5ZwhBApGOG1fMmESPEqt3ZKFeGsfYcrD5AKnCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"be87fbd2866f3daaad434b28272fccd1cd7d66a8b8131c667cd630927bcb9e0e","last_reissued_at":"2026-05-18T01:44:20.399763Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:44:20.399763Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The molecular gas content of ULIRG type 2 quasars at z < 1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Humphrey, B. Emonts, G. Drouart, M. I. Rodr\\'iguez, M. P\\'erez Torres, M. Villar-Mart\\'in, S. Garc\\'ia Burillo","submitted_at":"2014-03-04T09:15:23Z","abstract_excerpt":"We present new results of CO(1-0) spectroscopic observations of 4 SDSS type 2 quasars (QSO2) at z$\\sim$0.3, observed with the 30m IRAM telescope. The QSO2 have infrared luminosities in the ULIRG (UltraLuminous Infrared Galaxies) regime. We confirm the CO(1-0) detection in one of our 4 QSO2, SDSS J1543-00, with $L'_{CO}$ and $M_{H_2}$ (1.2$\\pm$0.2) $\\times$10$^{10}$ K km s$^{-1}$ pc$^2$ and (9.4$\\pm$1.4)$\\times$10$^9$ M$_{\\odot}$, respectively. The CO(1-0) line has $FWHM=$575$\\pm$102 km s$^{-1}$. No CO(1-0) emission is detected in SDSS J0903+02, SDSS J1337-01, SDSS J1520-01 above 3 sigma, yield"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.0724","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":"1403.0724","created_at":"2026-05-18T01:44:20.399874+00:00"},{"alias_kind":"arxiv_version","alias_value":"1403.0724v1","created_at":"2026-05-18T01:44:20.399874+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1403.0724","created_at":"2026-05-18T01:44:20.399874+00:00"},{"alias_kind":"pith_short_12","alias_value":"X2D7XUUGN462","created_at":"2026-05-18T12:28:54.890064+00:00"},{"alias_kind":"pith_short_16","alias_value":"X2D7XUUGN462VLKD","created_at":"2026-05-18T12:28:54.890064+00:00"},{"alias_kind":"pith_short_8","alias_value":"X2D7XUUG","created_at":"2026-05-18T12:28:54.890064+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/X2D7XUUGN462VLKDJMUCOL6M2H","json":"https://pith.science/pith/X2D7XUUGN462VLKDJMUCOL6M2H.json","graph_json":"https://pith.science/api/pith-number/X2D7XUUGN462VLKDJMUCOL6M2H/graph.json","events_json":"https://pith.science/api/pith-number/X2D7XUUGN462VLKDJMUCOL6M2H/events.json","paper":"https://pith.science/paper/X2D7XUUG"},"agent_actions":{"view_html":"https://pith.science/pith/X2D7XUUGN462VLKDJMUCOL6M2H","download_json":"https://pith.science/pith/X2D7XUUGN462VLKDJMUCOL6M2H.json","view_paper":"https://pith.science/paper/X2D7XUUG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1403.0724&json=true","fetch_graph":"https://pith.science/api/pith-number/X2D7XUUGN462VLKDJMUCOL6M2H/graph.json","fetch_events":"https://pith.science/api/pith-number/X2D7XUUGN462VLKDJMUCOL6M2H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/X2D7XUUGN462VLKDJMUCOL6M2H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/X2D7XUUGN462VLKDJMUCOL6M2H/action/storage_attestation","attest_author":"https://pith.science/pith/X2D7XUUGN462VLKDJMUCOL6M2H/action/author_attestation","sign_citation":"https://pith.science/pith/X2D7XUUGN462VLKDJMUCOL6M2H/action/citation_signature","submit_replication":"https://pith.science/pith/X2D7XUUGN462VLKDJMUCOL6M2H/action/replication_record"}},"created_at":"2026-05-18T01:44:20.399874+00:00","updated_at":"2026-05-18T01:44:20.399874+00:00"}