{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:W6MBNE7WREILUJPP765D3I4AAQ","short_pith_number":"pith:W6MBNE7W","schema_version":"1.0","canonical_sha256":"b7981693f68910ba25efffba3da380042a780afbe63c172c67cd460d62f9ea76","source":{"kind":"arxiv","id":"1707.05329","version":1},"attestation_state":"computed","paper":{"title":"Low-redshift analogs of submm galaxies: a diverse population","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Cooray, D. L. Clements, D. Riechers, H. Dannerbauer, I. Oteo, I. Smail, L. Dunne, L. Wang, M. J. Micha{\\l}owski, N. Bourne, P. van der Werf, R. J. Ivison, T. Hughes, Z-Y. Zhang","submitted_at":"2017-07-17T18:00:04Z","abstract_excerpt":"We have combined the wide-area Herschel-ATLAS far-IR survey with spectroscopic redshifts from GAMA and SDSS to define a sample of 21 low--redshift ($z_{\\rm spec} < 0.5$) analogs of submm galaxies (SMGs). These have been selected because their dust temperatures and total IR luminosities are similar to those for the classical high-redshift SMG population. As well as presenting the sample, in this paper we report $^{12}$CO(2-1) and $^{12}$CO(1-0) observations of 16 low-redshift analogs of SMGs taken with the IRAM-30m telescope. We have obtained that low-redshift analogs of SMGs represent a very d"},"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":"1707.05329","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-07-17T18:00:04Z","cross_cats_sorted":[],"title_canon_sha256":"3b70dc70acd2bae2a7a8c07697be1355fd7935649b64afed2e8773e9cb226b9b","abstract_canon_sha256":"d04300d4736318b73b927f672994425b01ce75ca722eaaa6101722c6f35d8b4e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:40:02.600765Z","signature_b64":"CzrTSefl02THuvfDizmpQi/cVHiYzG8eaCWG1I5H3WA9SY191mfyh925obAGlOLemVoN++3uJPWA7QO+BiQ8CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b7981693f68910ba25efffba3da380042a780afbe63c172c67cd460d62f9ea76","last_reissued_at":"2026-05-18T00:40:02.600232Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:40:02.600232Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Low-redshift analogs of submm galaxies: a diverse population","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Cooray, D. L. Clements, D. Riechers, H. Dannerbauer, I. Oteo, I. Smail, L. Dunne, L. Wang, M. J. Micha{\\l}owski, N. Bourne, P. van der Werf, R. J. Ivison, T. Hughes, Z-Y. Zhang","submitted_at":"2017-07-17T18:00:04Z","abstract_excerpt":"We have combined the wide-area Herschel-ATLAS far-IR survey with spectroscopic redshifts from GAMA and SDSS to define a sample of 21 low--redshift ($z_{\\rm spec} < 0.5$) analogs of submm galaxies (SMGs). These have been selected because their dust temperatures and total IR luminosities are similar to those for the classical high-redshift SMG population. As well as presenting the sample, in this paper we report $^{12}$CO(2-1) and $^{12}$CO(1-0) observations of 16 low-redshift analogs of SMGs taken with the IRAM-30m telescope. We have obtained that low-redshift analogs of SMGs represent a very d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.05329","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":"1707.05329","created_at":"2026-05-18T00:40:02.600297+00:00"},{"alias_kind":"arxiv_version","alias_value":"1707.05329v1","created_at":"2026-05-18T00:40:02.600297+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1707.05329","created_at":"2026-05-18T00:40:02.600297+00:00"},{"alias_kind":"pith_short_12","alias_value":"W6MBNE7WREIL","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_16","alias_value":"W6MBNE7WREILUJPP","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_8","alias_value":"W6MBNE7W","created_at":"2026-05-18T12:31:53.515858+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/W6MBNE7WREILUJPP765D3I4AAQ","json":"https://pith.science/pith/W6MBNE7WREILUJPP765D3I4AAQ.json","graph_json":"https://pith.science/api/pith-number/W6MBNE7WREILUJPP765D3I4AAQ/graph.json","events_json":"https://pith.science/api/pith-number/W6MBNE7WREILUJPP765D3I4AAQ/events.json","paper":"https://pith.science/paper/W6MBNE7W"},"agent_actions":{"view_html":"https://pith.science/pith/W6MBNE7WREILUJPP765D3I4AAQ","download_json":"https://pith.science/pith/W6MBNE7WREILUJPP765D3I4AAQ.json","view_paper":"https://pith.science/paper/W6MBNE7W","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1707.05329&json=true","fetch_graph":"https://pith.science/api/pith-number/W6MBNE7WREILUJPP765D3I4AAQ/graph.json","fetch_events":"https://pith.science/api/pith-number/W6MBNE7WREILUJPP765D3I4AAQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/W6MBNE7WREILUJPP765D3I4AAQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/W6MBNE7WREILUJPP765D3I4AAQ/action/storage_attestation","attest_author":"https://pith.science/pith/W6MBNE7WREILUJPP765D3I4AAQ/action/author_attestation","sign_citation":"https://pith.science/pith/W6MBNE7WREILUJPP765D3I4AAQ/action/citation_signature","submit_replication":"https://pith.science/pith/W6MBNE7WREILUJPP765D3I4AAQ/action/replication_record"}},"created_at":"2026-05-18T00:40:02.600297+00:00","updated_at":"2026-05-18T00:40:02.600297+00:00"}