{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:RJGGOZCJ4QN5BX7WDQPH366LSP","short_pith_number":"pith:RJGGOZCJ","schema_version":"1.0","canonical_sha256":"8a4c676449e41bd0dff61c1e7dfbcb93c031f07dcb9f0f8a905b42a568667a59","source":{"kind":"arxiv","id":"1303.4727","version":5},"attestation_state":"computed","paper":{"title":"Removal of two large scale Cosmic Microwave Background anomalies after subtraction of the Integrated Sachs Wolfe effect","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Rassat, F.-X. Dupe, J.-L. Starck","submitted_at":"2013-03-19T19:59:08Z","abstract_excerpt":"Though debated, the existence of claimed large-scale anomalies in the CMB is not totally dismissed. In parallel to the debate over their statistical significance, recent work focussed on masks and secondary anisotropies as potential sources of these anomalies. In this work we investigate simultaneously the impact of the method used to account for masked regions and the impact of the ISW effect, which is the large-scale secondary anisotropy most likely to affect the CMB anomalies. In this sense, our work is an update of both Francis & Peacock 2010 and Kim et al. 2012. Our aim is to identify tre"},"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":"1303.4727","kind":"arxiv","version":5},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-03-19T19:59:08Z","cross_cats_sorted":[],"title_canon_sha256":"e53f1415570e66be914699cac20612c365ea5007b7af8d0baa3c5c44458054b6","abstract_canon_sha256":"e31e4ee91c584d19e7e6412ddc45428e413fd849c475411cf2eb512d28bff54c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:00.624235Z","signature_b64":"j5Zeje5wdCGpeqaHen/DeNwNiPsse2nNcybZm3r5azBbtYPztac8Umdt929Myisxhgn/tVkE9Xzc6NGMOPfnBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8a4c676449e41bd0dff61c1e7dfbcb93c031f07dcb9f0f8a905b42a568667a59","last_reissued_at":"2026-05-18T01:51:00.623832Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:00.623832Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Removal of two large scale Cosmic Microwave Background anomalies after subtraction of the Integrated Sachs Wolfe effect","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Rassat, F.-X. Dupe, J.-L. Starck","submitted_at":"2013-03-19T19:59:08Z","abstract_excerpt":"Though debated, the existence of claimed large-scale anomalies in the CMB is not totally dismissed. In parallel to the debate over their statistical significance, recent work focussed on masks and secondary anisotropies as potential sources of these anomalies. In this work we investigate simultaneously the impact of the method used to account for masked regions and the impact of the ISW effect, which is the large-scale secondary anisotropy most likely to affect the CMB anomalies. In this sense, our work is an update of both Francis & Peacock 2010 and Kim et al. 2012. Our aim is to identify tre"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.4727","kind":"arxiv","version":5},"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":"1303.4727","created_at":"2026-05-18T01:51:00.623898+00:00"},{"alias_kind":"arxiv_version","alias_value":"1303.4727v5","created_at":"2026-05-18T01:51:00.623898+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.4727","created_at":"2026-05-18T01:51:00.623898+00:00"},{"alias_kind":"pith_short_12","alias_value":"RJGGOZCJ4QN5","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_16","alias_value":"RJGGOZCJ4QN5BX7W","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_8","alias_value":"RJGGOZCJ","created_at":"2026-05-18T12:27:57.521954+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.20699","citing_title":"Forecasts of CMB $E$-mode anomalies for AliCPT-1","ref_index":27,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RJGGOZCJ4QN5BX7WDQPH366LSP","json":"https://pith.science/pith/RJGGOZCJ4QN5BX7WDQPH366LSP.json","graph_json":"https://pith.science/api/pith-number/RJGGOZCJ4QN5BX7WDQPH366LSP/graph.json","events_json":"https://pith.science/api/pith-number/RJGGOZCJ4QN5BX7WDQPH366LSP/events.json","paper":"https://pith.science/paper/RJGGOZCJ"},"agent_actions":{"view_html":"https://pith.science/pith/RJGGOZCJ4QN5BX7WDQPH366LSP","download_json":"https://pith.science/pith/RJGGOZCJ4QN5BX7WDQPH366LSP.json","view_paper":"https://pith.science/paper/RJGGOZCJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1303.4727&json=true","fetch_graph":"https://pith.science/api/pith-number/RJGGOZCJ4QN5BX7WDQPH366LSP/graph.json","fetch_events":"https://pith.science/api/pith-number/RJGGOZCJ4QN5BX7WDQPH366LSP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RJGGOZCJ4QN5BX7WDQPH366LSP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RJGGOZCJ4QN5BX7WDQPH366LSP/action/storage_attestation","attest_author":"https://pith.science/pith/RJGGOZCJ4QN5BX7WDQPH366LSP/action/author_attestation","sign_citation":"https://pith.science/pith/RJGGOZCJ4QN5BX7WDQPH366LSP/action/citation_signature","submit_replication":"https://pith.science/pith/RJGGOZCJ4QN5BX7WDQPH366LSP/action/replication_record"}},"created_at":"2026-05-18T01:51:00.623898+00:00","updated_at":"2026-05-18T01:51:00.623898+00:00"}