{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:J5FXVKGGVOWLPCOD427UK2ZZUI","short_pith_number":"pith:J5FXVKGG","schema_version":"1.0","canonical_sha256":"4f4b7aa8c6abacb789c3e6bf456b39a214864ddfb9240a26d675ddb04f713352","source":{"kind":"arxiv","id":"1707.08967","version":1},"attestation_state":"computed","paper":{"title":"The most distant, luminous, dusty star-forming galaxies: redshifts from NOEMA and ALMA spectral scans","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Omont, A. Weiss, B. Stalder, D. L. Clements, D. Riechers, E. Valiante, F. Bertoldi, H. Dannerbauer, I. Oteo, I. P\\'erez-Fournon, J. Greenslade, J. M. Simpson, L. Christensen, L. Dunne, M. Bremer, M. Krips, M. Michalowski, P. Martinez-Navajas, P. van der Werf, R. J. Ivison, S. A. Eales, S. C. Chapman, S. Maddox, V. Arumugam, Y. Fudamoto, Z. Y. Zhang","submitted_at":"2017-07-27T18:00:06Z","abstract_excerpt":"We present 1.3- and/or 3-mm continuum images and 3-mm spectral scans, obtained using NOEMA and ALMA, of 21 distant, dusty, star-forming galaxies (DSFGs). Our sample is a subset of the galaxies selected by Ivison et al. (2016) on the basis of their extremely red far-infrared (far-IR) colours and low {\\it Herschel} flux densities; most are thus expected to be unlensed, extraordinarily luminous starbursts at $z \\gtrsim 4$, modulo the considerable cross-section to gravitational lensing implied by their redshift. We observed 17 of these galaxies with NOEMA and four with ALMA, scanning through the 3"},"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":"1707.08967","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-07-27T18:00:06Z","cross_cats_sorted":[],"title_canon_sha256":"034b4623f9a66b80c3025aefdd1a3b2620289cb0a8b30251da05c6e74d716842","abstract_canon_sha256":"a41b4ab150c2a39a01fd67b638343bc3f1cd14d38dcd9a985ae498daa6d3b05c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:35:30.764093Z","signature_b64":"5AvfGAOilWxms5wCOX2Ly36h5fGVP2QGLdZaRKH4TEP1m6Oxp7W5REQtxRRJ4O90oEqHrHdCd5+jge7pQrGjAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4f4b7aa8c6abacb789c3e6bf456b39a214864ddfb9240a26d675ddb04f713352","last_reissued_at":"2026-05-18T00:35:30.763702Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:35:30.763702Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The most distant, luminous, dusty star-forming galaxies: redshifts from NOEMA and ALMA spectral scans","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Omont, A. Weiss, B. Stalder, D. L. Clements, D. Riechers, E. Valiante, F. Bertoldi, H. Dannerbauer, I. Oteo, I. P\\'erez-Fournon, J. Greenslade, J. M. Simpson, L. Christensen, L. Dunne, M. Bremer, M. Krips, M. Michalowski, P. Martinez-Navajas, P. van der Werf, R. J. Ivison, S. A. Eales, S. C. Chapman, S. Maddox, V. Arumugam, Y. Fudamoto, Z. Y. Zhang","submitted_at":"2017-07-27T18:00:06Z","abstract_excerpt":"We present 1.3- and/or 3-mm continuum images and 3-mm spectral scans, obtained using NOEMA and ALMA, of 21 distant, dusty, star-forming galaxies (DSFGs). Our sample is a subset of the galaxies selected by Ivison et al. (2016) on the basis of their extremely red far-infrared (far-IR) colours and low {\\it Herschel} flux densities; most are thus expected to be unlensed, extraordinarily luminous starbursts at $z \\gtrsim 4$, modulo the considerable cross-section to gravitational lensing implied by their redshift. We observed 17 of these galaxies with NOEMA and four with ALMA, scanning through the 3"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.08967","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":"1707.08967","created_at":"2026-05-18T00:35:30.763761+00:00"},{"alias_kind":"arxiv_version","alias_value":"1707.08967v1","created_at":"2026-05-18T00:35:30.763761+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1707.08967","created_at":"2026-05-18T00:35:30.763761+00:00"},{"alias_kind":"pith_short_12","alias_value":"J5FXVKGGVOWL","created_at":"2026-05-18T12:31:21.493067+00:00"},{"alias_kind":"pith_short_16","alias_value":"J5FXVKGGVOWLPCOD","created_at":"2026-05-18T12:31:21.493067+00:00"},{"alias_kind":"pith_short_8","alias_value":"J5FXVKGG","created_at":"2026-05-18T12:31:21.493067+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/J5FXVKGGVOWLPCOD427UK2ZZUI","json":"https://pith.science/pith/J5FXVKGGVOWLPCOD427UK2ZZUI.json","graph_json":"https://pith.science/api/pith-number/J5FXVKGGVOWLPCOD427UK2ZZUI/graph.json","events_json":"https://pith.science/api/pith-number/J5FXVKGGVOWLPCOD427UK2ZZUI/events.json","paper":"https://pith.science/paper/J5FXVKGG"},"agent_actions":{"view_html":"https://pith.science/pith/J5FXVKGGVOWLPCOD427UK2ZZUI","download_json":"https://pith.science/pith/J5FXVKGGVOWLPCOD427UK2ZZUI.json","view_paper":"https://pith.science/paper/J5FXVKGG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1707.08967&json=true","fetch_graph":"https://pith.science/api/pith-number/J5FXVKGGVOWLPCOD427UK2ZZUI/graph.json","fetch_events":"https://pith.science/api/pith-number/J5FXVKGGVOWLPCOD427UK2ZZUI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/J5FXVKGGVOWLPCOD427UK2ZZUI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/J5FXVKGGVOWLPCOD427UK2ZZUI/action/storage_attestation","attest_author":"https://pith.science/pith/J5FXVKGGVOWLPCOD427UK2ZZUI/action/author_attestation","sign_citation":"https://pith.science/pith/J5FXVKGGVOWLPCOD427UK2ZZUI/action/citation_signature","submit_replication":"https://pith.science/pith/J5FXVKGGVOWLPCOD427UK2ZZUI/action/replication_record"}},"created_at":"2026-05-18T00:35:30.763761+00:00","updated_at":"2026-05-18T00:35:30.763761+00:00"}