{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:UBTBSUV5BE2RARJEHCTM6FJIRR","short_pith_number":"pith:UBTBSUV5","schema_version":"1.0","canonical_sha256":"a0661952bd093510452438a6cf15288c6bb091fc5681c25104b74e4ed0f7ef93","source":{"kind":"arxiv","id":"1605.06433","version":1},"attestation_state":"computed","paper":{"title":"H-ATLAS: A Candidate High Redshift Cluster/Protocluster of Star-Forming Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Cooray, A. Dariush, A. Omont, B. Morris, B. O'Halloran, D.L. Clements, D. Riechers, E. Ibar, E. Valiante, F. Braglia, G. de Zotti, G. Petitpas, H. Dannerbauer, I.Oteo, I. Perez-Fournon D. Herranz, I. Valtchanov, J.D. Vieira, J. Fritz, J. Gonzalez-Nuevo, J. Greenslade, J. Holdship, J. Wardlow, L. Dunne, L.L. Leeuw, M. Baes, M. Bremer, M.J. Michaowski M. Negrello, N. Bourne, P. van der Werf, R. Hopwood, R.J. Ivison, S. Eales, S. Maddox, S. Serjeant","submitted_at":"2016-05-20T16:54:21Z","abstract_excerpt":"We investigate the region around the Planck-detected z=3.26 gravitationally lensed galaxy HATLAS J114637.9-001132 (hereinafter HATLAS12-00) using both archival Herschel data from the H-ATLAS survey and using submm data obtained with both LABOCA and SCUBA2. The lensed source is found to be surrounded by a strong overdensity of both Herschel-SPIRE sources and submm sources. We detect 17 bright (S_870 >~7 mJy) sources at >4sigma closer than 5 arcmin to the lensed object at 850/870 microns. Ten of these sources have good cross-identifications with objects detected by Herschel-SPIRE which have redd"},"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":"1605.06433","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-05-20T16:54:21Z","cross_cats_sorted":[],"title_canon_sha256":"2c9b2921b96a71ff3d58671bf80c517d208f5d0a920b5d36eac1926271c5cf03","abstract_canon_sha256":"d5b7381e8ccb9fd69bc964823722414ae60aa73112deb10f1ce451b751287b87"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:14:18.915764Z","signature_b64":"zYy0ZSNRJiYIPN2NPO8EWNPeCkwJ44OGRpRRiH+xHIfcNSNevVOGyszNONvNwAtY4c7uAUSucMWiaO/hj/TxAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a0661952bd093510452438a6cf15288c6bb091fc5681c25104b74e4ed0f7ef93","last_reissued_at":"2026-05-18T01:14:18.914850Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:14:18.914850Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"H-ATLAS: A Candidate High Redshift Cluster/Protocluster of Star-Forming Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Cooray, A. Dariush, A. Omont, B. Morris, B. O'Halloran, D.L. Clements, D. Riechers, E. Ibar, E. Valiante, F. Braglia, G. de Zotti, G. Petitpas, H. Dannerbauer, I.Oteo, I. Perez-Fournon D. Herranz, I. Valtchanov, J.D. Vieira, J. Fritz, J. Gonzalez-Nuevo, J. Greenslade, J. Holdship, J. Wardlow, L. Dunne, L.L. Leeuw, M. Baes, M. Bremer, M.J. Michaowski M. Negrello, N. Bourne, P. van der Werf, R. Hopwood, R.J. Ivison, S. Eales, S. Maddox, S. Serjeant","submitted_at":"2016-05-20T16:54:21Z","abstract_excerpt":"We investigate the region around the Planck-detected z=3.26 gravitationally lensed galaxy HATLAS J114637.9-001132 (hereinafter HATLAS12-00) using both archival Herschel data from the H-ATLAS survey and using submm data obtained with both LABOCA and SCUBA2. The lensed source is found to be surrounded by a strong overdensity of both Herschel-SPIRE sources and submm sources. We detect 17 bright (S_870 >~7 mJy) sources at >4sigma closer than 5 arcmin to the lensed object at 850/870 microns. Ten of these sources have good cross-identifications with objects detected by Herschel-SPIRE which have redd"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.06433","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":"1605.06433","created_at":"2026-05-18T01:14:18.914988+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.06433v1","created_at":"2026-05-18T01:14:18.914988+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.06433","created_at":"2026-05-18T01:14:18.914988+00:00"},{"alias_kind":"pith_short_12","alias_value":"UBTBSUV5BE2R","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_16","alias_value":"UBTBSUV5BE2RARJE","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_8","alias_value":"UBTBSUV5","created_at":"2026-05-18T12:30:46.583412+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/UBTBSUV5BE2RARJEHCTM6FJIRR","json":"https://pith.science/pith/UBTBSUV5BE2RARJEHCTM6FJIRR.json","graph_json":"https://pith.science/api/pith-number/UBTBSUV5BE2RARJEHCTM6FJIRR/graph.json","events_json":"https://pith.science/api/pith-number/UBTBSUV5BE2RARJEHCTM6FJIRR/events.json","paper":"https://pith.science/paper/UBTBSUV5"},"agent_actions":{"view_html":"https://pith.science/pith/UBTBSUV5BE2RARJEHCTM6FJIRR","download_json":"https://pith.science/pith/UBTBSUV5BE2RARJEHCTM6FJIRR.json","view_paper":"https://pith.science/paper/UBTBSUV5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.06433&json=true","fetch_graph":"https://pith.science/api/pith-number/UBTBSUV5BE2RARJEHCTM6FJIRR/graph.json","fetch_events":"https://pith.science/api/pith-number/UBTBSUV5BE2RARJEHCTM6FJIRR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UBTBSUV5BE2RARJEHCTM6FJIRR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UBTBSUV5BE2RARJEHCTM6FJIRR/action/storage_attestation","attest_author":"https://pith.science/pith/UBTBSUV5BE2RARJEHCTM6FJIRR/action/author_attestation","sign_citation":"https://pith.science/pith/UBTBSUV5BE2RARJEHCTM6FJIRR/action/citation_signature","submit_replication":"https://pith.science/pith/UBTBSUV5BE2RARJEHCTM6FJIRR/action/replication_record"}},"created_at":"2026-05-18T01:14:18.914988+00:00","updated_at":"2026-05-18T01:14:18.914988+00:00"}