{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:AABVSEEXEWJA4NBVNGWCMMFIBJ","short_pith_number":"pith:AABVSEEX","schema_version":"1.0","canonical_sha256":"000359109725920e343569ac2630a80a52f9d1df102c0616481306f8633f711a","source":{"kind":"arxiv","id":"1706.06099","version":1},"attestation_state":"computed","paper":{"title":"Multiwavelength characterisation of an ACT-selected, lensed dusty star-forming galaxy at z=2.64","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. J. Baker, A. Sievers, A. Wei{\\ss}, C. Jim\\'enez, E. J. Wollack, F. Nati, G. W. Roberts-Borsani, G. W. Wilson, I. Aretxaga, J. \\'Alvarez-M\\'arquez, J. P. Hughes, J. Rivera, K. Alatalo, M. Dapr\\`a, M. Gralla, M. Hilton, M. J. Jim\\'enez-Donaire, M. S. Yun, N. Laporte, P. A. Gallardo, S. Fujimoto, T. A. Marriage","submitted_at":"2017-06-19T18:00:00Z","abstract_excerpt":"We present \\ci\\,(2--1) and multi-transition $^{12}$CO observations of a dusty star-forming galaxy, ACT\\,J2029+0120, which we spectroscopically confirm to lie at $z$\\,=\\,2.64. We detect CO(3--2), CO(5--4), CO(7--6), CO(8--7), and \\ci\\,(2--1) at high significance, tentatively detect HCO$^{+}$(4--3), and place strong upper limits on the integrated strength of dense gas tracers (HCN(4--3) and CS(7--6)). Multi-transition CO observations and dense gas tracers can provide valuable constraints on the molecular gas content and excitation conditions in high-redshift galaxies. We therefore use this uniqu"},"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":"1706.06099","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-19T18:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"61e8da4b6f81ed964cf0a935a611d935bfa2ca422c72861cabbc2e14b35cef99","abstract_canon_sha256":"d9f05bce339961052e0dab02233701b26c990e122b7275f3747bd1c5ba28a977"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:38:02.126106Z","signature_b64":"imQlxLci4DSRO5M/G/+u7l4ODAsvRz69MbyQAW1DfHql8FqYmyhvn6C3uAz39+TjtrplOog3xk6z1ZY6bab8DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"000359109725920e343569ac2630a80a52f9d1df102c0616481306f8633f711a","last_reissued_at":"2026-05-18T00:38:02.125202Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:38:02.125202Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multiwavelength characterisation of an ACT-selected, lensed dusty star-forming galaxy at z=2.64","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. J. Baker, A. Sievers, A. Wei{\\ss}, C. Jim\\'enez, E. J. Wollack, F. Nati, G. W. Roberts-Borsani, G. W. Wilson, I. Aretxaga, J. \\'Alvarez-M\\'arquez, J. P. Hughes, J. Rivera, K. Alatalo, M. Dapr\\`a, M. Gralla, M. Hilton, M. J. Jim\\'enez-Donaire, M. S. Yun, N. Laporte, P. A. Gallardo, S. Fujimoto, T. A. Marriage","submitted_at":"2017-06-19T18:00:00Z","abstract_excerpt":"We present \\ci\\,(2--1) and multi-transition $^{12}$CO observations of a dusty star-forming galaxy, ACT\\,J2029+0120, which we spectroscopically confirm to lie at $z$\\,=\\,2.64. We detect CO(3--2), CO(5--4), CO(7--6), CO(8--7), and \\ci\\,(2--1) at high significance, tentatively detect HCO$^{+}$(4--3), and place strong upper limits on the integrated strength of dense gas tracers (HCN(4--3) and CS(7--6)). Multi-transition CO observations and dense gas tracers can provide valuable constraints on the molecular gas content and excitation conditions in high-redshift galaxies. We therefore use this uniqu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.06099","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":"1706.06099","created_at":"2026-05-18T00:38:02.125354+00:00"},{"alias_kind":"arxiv_version","alias_value":"1706.06099v1","created_at":"2026-05-18T00:38:02.125354+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.06099","created_at":"2026-05-18T00:38:02.125354+00:00"},{"alias_kind":"pith_short_12","alias_value":"AABVSEEXEWJA","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_16","alias_value":"AABVSEEXEWJA4NBV","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_8","alias_value":"AABVSEEX","created_at":"2026-05-18T12:31:05.417338+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/AABVSEEXEWJA4NBVNGWCMMFIBJ","json":"https://pith.science/pith/AABVSEEXEWJA4NBVNGWCMMFIBJ.json","graph_json":"https://pith.science/api/pith-number/AABVSEEXEWJA4NBVNGWCMMFIBJ/graph.json","events_json":"https://pith.science/api/pith-number/AABVSEEXEWJA4NBVNGWCMMFIBJ/events.json","paper":"https://pith.science/paper/AABVSEEX"},"agent_actions":{"view_html":"https://pith.science/pith/AABVSEEXEWJA4NBVNGWCMMFIBJ","download_json":"https://pith.science/pith/AABVSEEXEWJA4NBVNGWCMMFIBJ.json","view_paper":"https://pith.science/paper/AABVSEEX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1706.06099&json=true","fetch_graph":"https://pith.science/api/pith-number/AABVSEEXEWJA4NBVNGWCMMFIBJ/graph.json","fetch_events":"https://pith.science/api/pith-number/AABVSEEXEWJA4NBVNGWCMMFIBJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AABVSEEXEWJA4NBVNGWCMMFIBJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AABVSEEXEWJA4NBVNGWCMMFIBJ/action/storage_attestation","attest_author":"https://pith.science/pith/AABVSEEXEWJA4NBVNGWCMMFIBJ/action/author_attestation","sign_citation":"https://pith.science/pith/AABVSEEXEWJA4NBVNGWCMMFIBJ/action/citation_signature","submit_replication":"https://pith.science/pith/AABVSEEXEWJA4NBVNGWCMMFIBJ/action/replication_record"}},"created_at":"2026-05-18T00:38:02.125354+00:00","updated_at":"2026-05-18T00:38:02.125354+00:00"}