{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:EOWSQXZGT26TQAAFXEYFG6NK25","short_pith_number":"pith:EOWSQXZG","schema_version":"1.0","canonical_sha256":"23ad285f269ebd380005b9305379aad7721cf9f3b5ef0008f03fdb947b6030da","source":{"kind":"arxiv","id":"1101.5590","version":1},"attestation_state":"computed","paper":{"title":"Sunyaev-Zel'dovich observations of LoCuSS clusters with the Arcminute Microkelvin Imager: high X-ray luminosity sample","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Anna M. M. Scaife, Anthony N. Lasenby, Carmen Rodriguez-Gonzalvez, David J. Titterington, Elizabeth M. Waldram, Farhan Feroz, Guy Pooley, Keith J. B. Grainge, Malak Olamaie, Matthew L. Davies, Michael P. Hobson, Michel P. Schammel, Natasha Hurley-Walker, Paul F. Scott, Richard D. E. Saunders, The AMI Consortium: Timothy W. Shimwell, Thomas M. O. Franzen","submitted_at":"2011-01-28T17:52:47Z","abstract_excerpt":"We present observations from the Small Array of the Arcminute Microkelvin Imager (AMI) of eight high X-ray luminosity galaxy cluster systems selected from the Local Cluster Substructure Survey (LoCuSS) sample.We detect the Sunyaev-Zel'dovich (SZ) effect in seven of these clusters. With the assumptions that galaxy clusters are isothermal, have a density profile described by a spherical b -model and obey the theoretical M-T relation, we are able to derive cluster parameters at r200 from our SZ data. With the additional assumption of hydrostatic equilibrium we are able to derive parameters at r50"},"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":"1101.5590","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-01-28T17:52:47Z","cross_cats_sorted":[],"title_canon_sha256":"e32e817852a5faccdc4b1b72cc95006f6403bb3fb306287c5c2d25110e9a5557","abstract_canon_sha256":"0b40c1bbeb7cebb33b7c66aa077caa50a05a90530a68ad3da8adf16975781412"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:22:42.200627Z","signature_b64":"7nkmjwV2pmJOsrSQg36gLxpL0CZACEHlQgQbC7qtzcBRzvVnHgwPffnpjiTY5f5DJhESKJlXSkHpn9s6FAHCBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"23ad285f269ebd380005b9305379aad7721cf9f3b5ef0008f03fdb947b6030da","last_reissued_at":"2026-05-18T02:22:42.199938Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:22:42.199938Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Sunyaev-Zel'dovich observations of LoCuSS clusters with the Arcminute Microkelvin Imager: high X-ray luminosity sample","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Anna M. M. Scaife, Anthony N. Lasenby, Carmen Rodriguez-Gonzalvez, David J. Titterington, Elizabeth M. Waldram, Farhan Feroz, Guy Pooley, Keith J. B. Grainge, Malak Olamaie, Matthew L. Davies, Michael P. Hobson, Michel P. Schammel, Natasha Hurley-Walker, Paul F. Scott, Richard D. E. Saunders, The AMI Consortium: Timothy W. Shimwell, Thomas M. O. Franzen","submitted_at":"2011-01-28T17:52:47Z","abstract_excerpt":"We present observations from the Small Array of the Arcminute Microkelvin Imager (AMI) of eight high X-ray luminosity galaxy cluster systems selected from the Local Cluster Substructure Survey (LoCuSS) sample.We detect the Sunyaev-Zel'dovich (SZ) effect in seven of these clusters. With the assumptions that galaxy clusters are isothermal, have a density profile described by a spherical b -model and obey the theoretical M-T relation, we are able to derive cluster parameters at r200 from our SZ data. With the additional assumption of hydrostatic equilibrium we are able to derive parameters at r50"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.5590","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":"1101.5590","created_at":"2026-05-18T02:22:42.200041+00:00"},{"alias_kind":"arxiv_version","alias_value":"1101.5590v1","created_at":"2026-05-18T02:22:42.200041+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.5590","created_at":"2026-05-18T02:22:42.200041+00:00"},{"alias_kind":"pith_short_12","alias_value":"EOWSQXZGT26T","created_at":"2026-05-18T12:26:28.662955+00:00"},{"alias_kind":"pith_short_16","alias_value":"EOWSQXZGT26TQAAF","created_at":"2026-05-18T12:26:28.662955+00:00"},{"alias_kind":"pith_short_8","alias_value":"EOWSQXZG","created_at":"2026-05-18T12:26:28.662955+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/EOWSQXZGT26TQAAFXEYFG6NK25","json":"https://pith.science/pith/EOWSQXZGT26TQAAFXEYFG6NK25.json","graph_json":"https://pith.science/api/pith-number/EOWSQXZGT26TQAAFXEYFG6NK25/graph.json","events_json":"https://pith.science/api/pith-number/EOWSQXZGT26TQAAFXEYFG6NK25/events.json","paper":"https://pith.science/paper/EOWSQXZG"},"agent_actions":{"view_html":"https://pith.science/pith/EOWSQXZGT26TQAAFXEYFG6NK25","download_json":"https://pith.science/pith/EOWSQXZGT26TQAAFXEYFG6NK25.json","view_paper":"https://pith.science/paper/EOWSQXZG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1101.5590&json=true","fetch_graph":"https://pith.science/api/pith-number/EOWSQXZGT26TQAAFXEYFG6NK25/graph.json","fetch_events":"https://pith.science/api/pith-number/EOWSQXZGT26TQAAFXEYFG6NK25/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EOWSQXZGT26TQAAFXEYFG6NK25/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EOWSQXZGT26TQAAFXEYFG6NK25/action/storage_attestation","attest_author":"https://pith.science/pith/EOWSQXZGT26TQAAFXEYFG6NK25/action/author_attestation","sign_citation":"https://pith.science/pith/EOWSQXZGT26TQAAFXEYFG6NK25/action/citation_signature","submit_replication":"https://pith.science/pith/EOWSQXZGT26TQAAFXEYFG6NK25/action/replication_record"}},"created_at":"2026-05-18T02:22:42.200041+00:00","updated_at":"2026-05-18T02:22:42.200041+00:00"}