{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:VRY5FL5CO2L66XUPNOQFSQUQC7","short_pith_number":"pith:VRY5FL5C","schema_version":"1.0","canonical_sha256":"ac71d2afa27697ef5e8f6ba059429017e99dea6be109d830a926e110611ffa14","source":{"kind":"arxiv","id":"1405.5013","version":2},"attestation_state":"computed","paper":{"title":"Comparison of Sunyaev-Zel'dovich measurements from Planck and from the Arcminute Microkelvin Imager for 99 galaxy clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Hempel, A. N. Lasenby, B. Comis, C. J. MacTavish, C. Rumsey, D. Harrison, D. J. Titterington, D. Sutton, E. M. Waldram, E. Pointecouteau, F. Feroz, G. Chon, G. G. Pooley, G. Hurier, G. W. Pratt, H. Aussel, H. B\\\"ohringer, H. Dahle, I. Bikmaev, I. Khamitov, J. A. Rubi\\~no-Mart\\'in, J.-B. Melin, J. Democles, J. F. Mac\\'ias-P\\'erez, K. J. B. Grainge, M. Arnaud, M. Ashdown, M. Douspis, M. L. Brown, M. Olamaie, M. P. Hobson, M. P. Schammel, N. Aghanim, P. Carvalho, P. F. Scott, R. Barrena, R. Burenin, R. D. E. Saunders, R. Kneissl, T. W. Shimwell, V. Stolyarov, Y. C. Perrott","submitted_at":"2014-05-20T09:42:00Z","abstract_excerpt":"We present observations and analysis of a sample of 123 galaxy clusters from the 2013 Planck catalogue of Sunyaev-Zel'dovich sources with the Arcminute Microkelvin Imager (AMI), a ground-based radio interferometer. AMI provides an independent measurement with higher angular resolution, 3 arcmin compared to the Planck beams of 5-10 arcmin. The AMI observations thus provide validation of the cluster detections, improved positional estimates, and a consistency check on the fitted 'size' ($\\theta_{s}$) and 'flux' ($Y_{\\rm tot}$) parameters in the Generalised Navarro, Frenk and White (GNFW) model. "},"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":"1405.5013","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-05-20T09:42:00Z","cross_cats_sorted":[],"title_canon_sha256":"1e740a1e70add03a5a6e64d85485806183018df2a4409e5e80d651fd4b5c058f","abstract_canon_sha256":"3ab65a64914d2f660bf95cc3589b56f3972d782020ea4d7c10ec89557a5dc654"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:35:32.972945Z","signature_b64":"uvLpLsfV8Hx/Mblpfc07GYcn+hZ36cMvbz8JhBmFHXTd3TVzinOCoPON9l/6JjNyvZtS2212RnPWqb7P9eNgAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ac71d2afa27697ef5e8f6ba059429017e99dea6be109d830a926e110611ffa14","last_reissued_at":"2026-05-18T01:35:32.972300Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:35:32.972300Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Comparison of Sunyaev-Zel'dovich measurements from Planck and from the Arcminute Microkelvin Imager for 99 galaxy clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Hempel, A. N. Lasenby, B. Comis, C. J. MacTavish, C. Rumsey, D. Harrison, D. J. Titterington, D. Sutton, E. M. Waldram, E. Pointecouteau, F. Feroz, G. Chon, G. G. Pooley, G. Hurier, G. W. Pratt, H. Aussel, H. B\\\"ohringer, H. Dahle, I. Bikmaev, I. Khamitov, J. A. Rubi\\~no-Mart\\'in, J.-B. Melin, J. Democles, J. F. Mac\\'ias-P\\'erez, K. J. B. Grainge, M. Arnaud, M. Ashdown, M. Douspis, M. L. Brown, M. Olamaie, M. P. Hobson, M. P. Schammel, N. Aghanim, P. Carvalho, P. F. Scott, R. Barrena, R. Burenin, R. D. E. Saunders, R. Kneissl, T. W. Shimwell, V. Stolyarov, Y. C. Perrott","submitted_at":"2014-05-20T09:42:00Z","abstract_excerpt":"We present observations and analysis of a sample of 123 galaxy clusters from the 2013 Planck catalogue of Sunyaev-Zel'dovich sources with the Arcminute Microkelvin Imager (AMI), a ground-based radio interferometer. AMI provides an independent measurement with higher angular resolution, 3 arcmin compared to the Planck beams of 5-10 arcmin. The AMI observations thus provide validation of the cluster detections, improved positional estimates, and a consistency check on the fitted 'size' ($\\theta_{s}$) and 'flux' ($Y_{\\rm tot}$) parameters in the Generalised Navarro, Frenk and White (GNFW) model. "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.5013","kind":"arxiv","version":2},"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":"1405.5013","created_at":"2026-05-18T01:35:32.972418+00:00"},{"alias_kind":"arxiv_version","alias_value":"1405.5013v2","created_at":"2026-05-18T01:35:32.972418+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.5013","created_at":"2026-05-18T01:35:32.972418+00:00"},{"alias_kind":"pith_short_12","alias_value":"VRY5FL5CO2L6","created_at":"2026-05-18T12:28:54.890064+00:00"},{"alias_kind":"pith_short_16","alias_value":"VRY5FL5CO2L66XUP","created_at":"2026-05-18T12:28:54.890064+00:00"},{"alias_kind":"pith_short_8","alias_value":"VRY5FL5C","created_at":"2026-05-18T12:28:54.890064+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/VRY5FL5CO2L66XUPNOQFSQUQC7","json":"https://pith.science/pith/VRY5FL5CO2L66XUPNOQFSQUQC7.json","graph_json":"https://pith.science/api/pith-number/VRY5FL5CO2L66XUPNOQFSQUQC7/graph.json","events_json":"https://pith.science/api/pith-number/VRY5FL5CO2L66XUPNOQFSQUQC7/events.json","paper":"https://pith.science/paper/VRY5FL5C"},"agent_actions":{"view_html":"https://pith.science/pith/VRY5FL5CO2L66XUPNOQFSQUQC7","download_json":"https://pith.science/pith/VRY5FL5CO2L66XUPNOQFSQUQC7.json","view_paper":"https://pith.science/paper/VRY5FL5C","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1405.5013&json=true","fetch_graph":"https://pith.science/api/pith-number/VRY5FL5CO2L66XUPNOQFSQUQC7/graph.json","fetch_events":"https://pith.science/api/pith-number/VRY5FL5CO2L66XUPNOQFSQUQC7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VRY5FL5CO2L66XUPNOQFSQUQC7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VRY5FL5CO2L66XUPNOQFSQUQC7/action/storage_attestation","attest_author":"https://pith.science/pith/VRY5FL5CO2L66XUPNOQFSQUQC7/action/author_attestation","sign_citation":"https://pith.science/pith/VRY5FL5CO2L66XUPNOQFSQUQC7/action/citation_signature","submit_replication":"https://pith.science/pith/VRY5FL5CO2L66XUPNOQFSQUQC7/action/replication_record"}},"created_at":"2026-05-18T01:35:32.972418+00:00","updated_at":"2026-05-18T01:35:32.972418+00:00"}