{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:QGLOSNET225ON2GUGBSWH5O3JH","short_pith_number":"pith:QGLOSNET","schema_version":"1.0","canonical_sha256":"8196e93493d6bae6e8d4306563f5db49e0b20a0d0281109a0d2d5f4c79aeb940","source":{"kind":"arxiv","id":"2102.12510","version":1},"attestation_state":"computed","paper":{"title":"An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Amvrosiadis, A. M. Swinbank, Chian-Chou Chen, C. J. Conselice, D. Farrah, Durham), E. A. Cooke, I. Smail, J. E. Birkin, J. E. Geach, J. L. Wardlow, J. S. Dunlop, K. E. K. Coppin, O. Almaini, R. J. Ivison, S. Ikarashi, S. M. Stach (CEA, U. Dudzevi\\v{c}i\\=ut\\.e","submitted_at":"2021-02-24T19:02:00Z","abstract_excerpt":"We present an analysis of the spatial clustering of a large sample of high-resolution, interferometically identified, submillimetre galaxies (SMGs). We measure the projected cross-correlation function of ~350 SMGs in the UKIDSS Ultra Deep-Survey Field across a redshift range of $z=1.5-3$ utilising a method that incorporates the uncertainties in the redshift measurements for both the SMGs and cross-correlated galaxies through sampling their full probability distribution functions. By measuring the absolute linear bias of the SMGs we derive halo masses of $\\log_{10}(M_{\\rm halo}[{h^{-1}\\,\\rm M_{"},"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":"2102.12510","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2021-02-24T19:02:00Z","cross_cats_sorted":[],"title_canon_sha256":"d39194bff8fa0fe5b60413f081677715116b494851e3c5c3262ce5589a0df18c","abstract_canon_sha256":"2313eb45af48f92cbcafe3585c379456d56d69c6e665cd7648e5903b3202380d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:23:27.729959Z","signature_b64":"2b1DDzMC8oUWrloamtfIoubcIC+bEM9YOWSJNnB3dw2u6W0C0L76yAOzXMOW8XU2ycvM0QNR4mIyoUnKCTX9AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8196e93493d6bae6e8d4306563f5db49e0b20a0d0281109a0d2d5f4c79aeb940","last_reissued_at":"2026-07-05T02:23:27.729515Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:23:27.729515Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Amvrosiadis, A. M. Swinbank, Chian-Chou Chen, C. J. Conselice, D. Farrah, Durham), E. A. Cooke, I. Smail, J. E. Birkin, J. E. Geach, J. L. Wardlow, J. S. Dunlop, K. E. K. Coppin, O. Almaini, R. J. Ivison, S. Ikarashi, S. M. Stach (CEA, U. Dudzevi\\v{c}i\\=ut\\.e","submitted_at":"2021-02-24T19:02:00Z","abstract_excerpt":"We present an analysis of the spatial clustering of a large sample of high-resolution, interferometically identified, submillimetre galaxies (SMGs). We measure the projected cross-correlation function of ~350 SMGs in the UKIDSS Ultra Deep-Survey Field across a redshift range of $z=1.5-3$ utilising a method that incorporates the uncertainties in the redshift measurements for both the SMGs and cross-correlated galaxies through sampling their full probability distribution functions. By measuring the absolute linear bias of the SMGs we derive halo masses of $\\log_{10}(M_{\\rm halo}[{h^{-1}\\,\\rm M_{"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2102.12510","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2102.12510/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2102.12510","created_at":"2026-07-05T02:23:27.729582+00:00"},{"alias_kind":"arxiv_version","alias_value":"2102.12510v1","created_at":"2026-07-05T02:23:27.729582+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2102.12510","created_at":"2026-07-05T02:23:27.729582+00:00"},{"alias_kind":"pith_short_12","alias_value":"QGLOSNET225O","created_at":"2026-07-05T02:23:27.729582+00:00"},{"alias_kind":"pith_short_16","alias_value":"QGLOSNET225ON2GU","created_at":"2026-07-05T02:23:27.729582+00:00"},{"alias_kind":"pith_short_8","alias_value":"QGLOSNET","created_at":"2026-07-05T02:23:27.729582+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/QGLOSNET225ON2GUGBSWH5O3JH","json":"https://pith.science/pith/QGLOSNET225ON2GUGBSWH5O3JH.json","graph_json":"https://pith.science/api/pith-number/QGLOSNET225ON2GUGBSWH5O3JH/graph.json","events_json":"https://pith.science/api/pith-number/QGLOSNET225ON2GUGBSWH5O3JH/events.json","paper":"https://pith.science/paper/QGLOSNET"},"agent_actions":{"view_html":"https://pith.science/pith/QGLOSNET225ON2GUGBSWH5O3JH","download_json":"https://pith.science/pith/QGLOSNET225ON2GUGBSWH5O3JH.json","view_paper":"https://pith.science/paper/QGLOSNET","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2102.12510&json=true","fetch_graph":"https://pith.science/api/pith-number/QGLOSNET225ON2GUGBSWH5O3JH/graph.json","fetch_events":"https://pith.science/api/pith-number/QGLOSNET225ON2GUGBSWH5O3JH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QGLOSNET225ON2GUGBSWH5O3JH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QGLOSNET225ON2GUGBSWH5O3JH/action/storage_attestation","attest_author":"https://pith.science/pith/QGLOSNET225ON2GUGBSWH5O3JH/action/author_attestation","sign_citation":"https://pith.science/pith/QGLOSNET225ON2GUGBSWH5O3JH/action/citation_signature","submit_replication":"https://pith.science/pith/QGLOSNET225ON2GUGBSWH5O3JH/action/replication_record"}},"created_at":"2026-07-05T02:23:27.729582+00:00","updated_at":"2026-07-05T02:23:27.729582+00:00"}