{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:IDVMOG567TYWAEKP3NBFAXBKYV","short_pith_number":"pith:IDVMOG56","schema_version":"1.0","canonical_sha256":"40eac71bbefcf160114fdb42505c2ac54d0f33722bc886a093edf2dd03ca3ea6","source":{"kind":"arxiv","id":"1601.00115","version":2},"attestation_state":"computed","paper":{"title":"Revisiting CFHTLenS cosmic shear: Optimal E/B mode decomposition using COSEBIs and compressed COSEBIs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Catherine Heymans, Chris Blake, Joachim Harnois-Deraps, Ludovic Van Waerbeke, Marika Asgari, Peter Schneider","submitted_at":"2016-01-01T20:59:47Z","abstract_excerpt":"We present a re-analysis of the CFHTLenS weak gravitational lensing survey using Complete Orthogonal Sets of E/B-mode Integrals, known as COSEBIs. COSEBIs provide a complete set of functions to efficiently separate E-modes from B-modes and hence allow for robust and stringent tests for systematic errors in the data. This analysis reveals significant B-modes on large angular scales that were not previously seen using the standard E/B decomposition analyses. We find that the significance of the B-modes is enhanced when the data is split by galaxy type and analysed in tomographic redshift bins. A"},"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":"1601.00115","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-01-01T20:59:47Z","cross_cats_sorted":[],"title_canon_sha256":"670e3950950a19479f1726ee2dac6bcfdcb5423228b1a5858803e3aa0140b1f1","abstract_canon_sha256":"29f87e6c6159f070e24fd11dcf5ebb139f30279e4a6867c3a36be37ea8b41554"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:54:15.813211Z","signature_b64":"JrWgUsA/IuM3atING8OjrvhQYKVh430h0VPe9wMRpDfRf7COnRwPxBh3hqaWvJb2wAWgmOrlpL162pDfccz8Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"40eac71bbefcf160114fdb42505c2ac54d0f33722bc886a093edf2dd03ca3ea6","last_reissued_at":"2026-05-18T00:54:15.812786Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:54:15.812786Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Revisiting CFHTLenS cosmic shear: Optimal E/B mode decomposition using COSEBIs and compressed COSEBIs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Catherine Heymans, Chris Blake, Joachim Harnois-Deraps, Ludovic Van Waerbeke, Marika Asgari, Peter Schneider","submitted_at":"2016-01-01T20:59:47Z","abstract_excerpt":"We present a re-analysis of the CFHTLenS weak gravitational lensing survey using Complete Orthogonal Sets of E/B-mode Integrals, known as COSEBIs. COSEBIs provide a complete set of functions to efficiently separate E-modes from B-modes and hence allow for robust and stringent tests for systematic errors in the data. This analysis reveals significant B-modes on large angular scales that were not previously seen using the standard E/B decomposition analyses. We find that the significance of the B-modes is enhanced when the data is split by galaxy type and analysed in tomographic redshift bins. A"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1601.00115","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":"1601.00115","created_at":"2026-05-18T00:54:15.812859+00:00"},{"alias_kind":"arxiv_version","alias_value":"1601.00115v2","created_at":"2026-05-18T00:54:15.812859+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1601.00115","created_at":"2026-05-18T00:54:15.812859+00:00"},{"alias_kind":"pith_short_12","alias_value":"IDVMOG567TYW","created_at":"2026-05-18T12:30:22.444734+00:00"},{"alias_kind":"pith_short_16","alias_value":"IDVMOG567TYWAEKP","created_at":"2026-05-18T12:30:22.444734+00:00"},{"alias_kind":"pith_short_8","alias_value":"IDVMOG56","created_at":"2026-05-18T12:30:22.444734+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/IDVMOG567TYWAEKP3NBFAXBKYV","json":"https://pith.science/pith/IDVMOG567TYWAEKP3NBFAXBKYV.json","graph_json":"https://pith.science/api/pith-number/IDVMOG567TYWAEKP3NBFAXBKYV/graph.json","events_json":"https://pith.science/api/pith-number/IDVMOG567TYWAEKP3NBFAXBKYV/events.json","paper":"https://pith.science/paper/IDVMOG56"},"agent_actions":{"view_html":"https://pith.science/pith/IDVMOG567TYWAEKP3NBFAXBKYV","download_json":"https://pith.science/pith/IDVMOG567TYWAEKP3NBFAXBKYV.json","view_paper":"https://pith.science/paper/IDVMOG56","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1601.00115&json=true","fetch_graph":"https://pith.science/api/pith-number/IDVMOG567TYWAEKP3NBFAXBKYV/graph.json","fetch_events":"https://pith.science/api/pith-number/IDVMOG567TYWAEKP3NBFAXBKYV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IDVMOG567TYWAEKP3NBFAXBKYV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IDVMOG567TYWAEKP3NBFAXBKYV/action/storage_attestation","attest_author":"https://pith.science/pith/IDVMOG567TYWAEKP3NBFAXBKYV/action/author_attestation","sign_citation":"https://pith.science/pith/IDVMOG567TYWAEKP3NBFAXBKYV/action/citation_signature","submit_replication":"https://pith.science/pith/IDVMOG567TYWAEKP3NBFAXBKYV/action/replication_record"}},"created_at":"2026-05-18T00:54:15.812859+00:00","updated_at":"2026-05-18T00:54:15.812859+00:00"}