{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:FQEHBA2GSZBG7ZQQUKIB2INRGW","short_pith_number":"pith:FQEHBA2G","schema_version":"1.0","canonical_sha256":"2c0870834696426fe610a2901d21b1359d4f8e27eff562802b323ab01969f78e","source":{"kind":"arxiv","id":"2009.00877","version":1},"attestation_state":"computed","paper":{"title":"SCUBA2 High Redshift Bright Quasar Survey: Far-infrared Properties and Weak-line Features","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alain Omont, Bram Venemans, Chengpeng Zhang, Chiara Mazzucchelli, Eduardo Banados, Frank Bertoldi, Jeff Wagg, Jianan Li, Linhua Jiang, Qiong Li, Ran Wang, Roberto Decarli, Xiaohui Fan, Xue-Bing Wu, Yali Shao, Yunhao Zhang","submitted_at":"2020-09-02T08:01:48Z","abstract_excerpt":"We present a submillimetre continuum survey ('SCUBA2 High rEdshift bRight quasaR surveY', hereafter SHERRY) of 54 high redshift quasars at $5.6<z<6.9$ with quasar bolometric luminosities in a range of (0.2$-$$ 5)\\times10^{14}\\,L_{\\odot}$, using the Submillimetre Common-User Bolometer Array-2 (SCUBA2) on the James Clerk Maxwell Telescope. About 30% (16/54) of the sources are detected with a typical 850$\\mu$m rms sensitivity of 1.2 $\\rm mJy\\,beam^{-1}$ ($S\\rm _{\\nu,850\\,\\mu m} = 4$-5 mJy, at $>3.5\\sigma$). The new SHERRY detections indicate far-infrared (FIR) luminosities of $\\rm 3.5\\times10^{12"},"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":"2009.00877","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2020-09-02T08:01:48Z","cross_cats_sorted":[],"title_canon_sha256":"ff269be3248356295b5c46b68af63cc4cae9f2d34d8a131e43bad2e9504e360e","abstract_canon_sha256":"e168e21c95e73eb36a7354d28fcf7d5c6665472474c53b39c08ae2f7bd7330de"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:32:29.739378Z","signature_b64":"Xc4ZOPQwn2Tksf6sK+9s+J4MXiROsskKVEOFSS/x+FnmUUpDswrS876sVNS2tTctBcAHJTEByd6VhLemNcgXDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2c0870834696426fe610a2901d21b1359d4f8e27eff562802b323ab01969f78e","last_reissued_at":"2026-07-05T01:32:29.738954Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:32:29.738954Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"SCUBA2 High Redshift Bright Quasar Survey: Far-infrared Properties and Weak-line Features","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alain Omont, Bram Venemans, Chengpeng Zhang, Chiara Mazzucchelli, Eduardo Banados, Frank Bertoldi, Jeff Wagg, Jianan Li, Linhua Jiang, Qiong Li, Ran Wang, Roberto Decarli, Xiaohui Fan, Xue-Bing Wu, Yali Shao, Yunhao Zhang","submitted_at":"2020-09-02T08:01:48Z","abstract_excerpt":"We present a submillimetre continuum survey ('SCUBA2 High rEdshift bRight quasaR surveY', hereafter SHERRY) of 54 high redshift quasars at $5.6<z<6.9$ with quasar bolometric luminosities in a range of (0.2$-$$ 5)\\times10^{14}\\,L_{\\odot}$, using the Submillimetre Common-User Bolometer Array-2 (SCUBA2) on the James Clerk Maxwell Telescope. About 30% (16/54) of the sources are detected with a typical 850$\\mu$m rms sensitivity of 1.2 $\\rm mJy\\,beam^{-1}$ ($S\\rm _{\\nu,850\\,\\mu m} = 4$-5 mJy, at $>3.5\\sigma$). The new SHERRY detections indicate far-infrared (FIR) luminosities of $\\rm 3.5\\times10^{12"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2009.00877","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/2009.00877/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":"2009.00877","created_at":"2026-07-05T01:32:29.739001+00:00"},{"alias_kind":"arxiv_version","alias_value":"2009.00877v1","created_at":"2026-07-05T01:32:29.739001+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2009.00877","created_at":"2026-07-05T01:32:29.739001+00:00"},{"alias_kind":"pith_short_12","alias_value":"FQEHBA2GSZBG","created_at":"2026-07-05T01:32:29.739001+00:00"},{"alias_kind":"pith_short_16","alias_value":"FQEHBA2GSZBG7ZQQ","created_at":"2026-07-05T01:32:29.739001+00:00"},{"alias_kind":"pith_short_8","alias_value":"FQEHBA2G","created_at":"2026-07-05T01:32:29.739001+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/FQEHBA2GSZBG7ZQQUKIB2INRGW","json":"https://pith.science/pith/FQEHBA2GSZBG7ZQQUKIB2INRGW.json","graph_json":"https://pith.science/api/pith-number/FQEHBA2GSZBG7ZQQUKIB2INRGW/graph.json","events_json":"https://pith.science/api/pith-number/FQEHBA2GSZBG7ZQQUKIB2INRGW/events.json","paper":"https://pith.science/paper/FQEHBA2G"},"agent_actions":{"view_html":"https://pith.science/pith/FQEHBA2GSZBG7ZQQUKIB2INRGW","download_json":"https://pith.science/pith/FQEHBA2GSZBG7ZQQUKIB2INRGW.json","view_paper":"https://pith.science/paper/FQEHBA2G","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2009.00877&json=true","fetch_graph":"https://pith.science/api/pith-number/FQEHBA2GSZBG7ZQQUKIB2INRGW/graph.json","fetch_events":"https://pith.science/api/pith-number/FQEHBA2GSZBG7ZQQUKIB2INRGW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FQEHBA2GSZBG7ZQQUKIB2INRGW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FQEHBA2GSZBG7ZQQUKIB2INRGW/action/storage_attestation","attest_author":"https://pith.science/pith/FQEHBA2GSZBG7ZQQUKIB2INRGW/action/author_attestation","sign_citation":"https://pith.science/pith/FQEHBA2GSZBG7ZQQUKIB2INRGW/action/citation_signature","submit_replication":"https://pith.science/pith/FQEHBA2GSZBG7ZQQUKIB2INRGW/action/replication_record"}},"created_at":"2026-07-05T01:32:29.739001+00:00","updated_at":"2026-07-05T01:32:29.739001+00:00"}