{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:NXC5WPT3VLA55EXOLWPC65O56D","short_pith_number":"pith:NXC5WPT3","schema_version":"1.0","canonical_sha256":"6dc5db3e7baac1de92ee5d9e2f75ddf0d669cfe12b584462d5b49f76cdd6ede0","source":{"kind":"arxiv","id":"1404.5469","version":1},"attestation_state":"computed","paper":{"title":"CFHTLenS: Cosmological constraints from a combination of cosmic shear two-point and three-point correlations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Barnaby Rowe, Catherine Heymans, Elisabetta Semboloni, Hendrik Hildebrandt, Henk Hoekstra, Jean Coupon, Joachim Harnois-D\\'eraps, Konrad Kuijken, Lance Miller, Liping Fu, Ludovic Van Waerbeke, Malin Velander, Martin Kilbinger, Michael J. Hudson, Patrick Simon, Sanaz Vafaei, Thomas D. Kitching, Thomas Erben, Tim Schrabback, Yannick Mellier","submitted_at":"2014-04-22T12:30:09Z","abstract_excerpt":"Higher-order, non-Gaussian aspects of the large-scale structure carry valuable information on structure formation and cosmology, which is complementary to second-order statistics. In this work we measure second- and third-order weak-lensing aperture-mass moments from CFHTLenS and combine those with CMB anisotropy probes. The third moment is measured with a significance of $2\\sigma$. The combined constraint on $\\Sigma_8 = \\sigma_8 (\\Omega_{\\rm m}/0.27)^\\alpha$ is improved by 10%, in comparison to the second-order only, and the allowed ranges for $\\Omega_{\\rm m}$ and $\\sigma_8$ are substantially"},"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":"1404.5469","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-04-22T12:30:09Z","cross_cats_sorted":[],"title_canon_sha256":"62b7b5a9aac9c9c8de1866b63bf09da6892e9ce3f0ecff3a503d7842eead42f0","abstract_canon_sha256":"956194b7e48082b32712d8f01292a326a431245bedef574a7c7c5822712fd4bb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:26.459520Z","signature_b64":"CeZxu3j5D0xhXQLIUWx3Tp93w/ofllTZIVDLTbj2MG+J/yvBA2AhOF7CwtZcVk/3Rs9TZ4UGU3VK4jxzGKz7BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6dc5db3e7baac1de92ee5d9e2f75ddf0d669cfe12b584462d5b49f76cdd6ede0","last_reissued_at":"2026-05-18T01:43:26.458968Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:26.458968Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CFHTLenS: Cosmological constraints from a combination of cosmic shear two-point and three-point correlations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Barnaby Rowe, Catherine Heymans, Elisabetta Semboloni, Hendrik Hildebrandt, Henk Hoekstra, Jean Coupon, Joachim Harnois-D\\'eraps, Konrad Kuijken, Lance Miller, Liping Fu, Ludovic Van Waerbeke, Malin Velander, Martin Kilbinger, Michael J. Hudson, Patrick Simon, Sanaz Vafaei, Thomas D. Kitching, Thomas Erben, Tim Schrabback, Yannick Mellier","submitted_at":"2014-04-22T12:30:09Z","abstract_excerpt":"Higher-order, non-Gaussian aspects of the large-scale structure carry valuable information on structure formation and cosmology, which is complementary to second-order statistics. In this work we measure second- and third-order weak-lensing aperture-mass moments from CFHTLenS and combine those with CMB anisotropy probes. The third moment is measured with a significance of $2\\sigma$. The combined constraint on $\\Sigma_8 = \\sigma_8 (\\Omega_{\\rm m}/0.27)^\\alpha$ is improved by 10%, in comparison to the second-order only, and the allowed ranges for $\\Omega_{\\rm m}$ and $\\sigma_8$ are substantially"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.5469","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":"1404.5469","created_at":"2026-05-18T01:43:26.459052+00:00"},{"alias_kind":"arxiv_version","alias_value":"1404.5469v1","created_at":"2026-05-18T01:43:26.459052+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.5469","created_at":"2026-05-18T01:43:26.459052+00:00"},{"alias_kind":"pith_short_12","alias_value":"NXC5WPT3VLA5","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_16","alias_value":"NXC5WPT3VLA55EXO","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_8","alias_value":"NXC5WPT3","created_at":"2026-05-18T12:28:41.024544+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/NXC5WPT3VLA55EXOLWPC65O56D","json":"https://pith.science/pith/NXC5WPT3VLA55EXOLWPC65O56D.json","graph_json":"https://pith.science/api/pith-number/NXC5WPT3VLA55EXOLWPC65O56D/graph.json","events_json":"https://pith.science/api/pith-number/NXC5WPT3VLA55EXOLWPC65O56D/events.json","paper":"https://pith.science/paper/NXC5WPT3"},"agent_actions":{"view_html":"https://pith.science/pith/NXC5WPT3VLA55EXOLWPC65O56D","download_json":"https://pith.science/pith/NXC5WPT3VLA55EXOLWPC65O56D.json","view_paper":"https://pith.science/paper/NXC5WPT3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1404.5469&json=true","fetch_graph":"https://pith.science/api/pith-number/NXC5WPT3VLA55EXOLWPC65O56D/graph.json","fetch_events":"https://pith.science/api/pith-number/NXC5WPT3VLA55EXOLWPC65O56D/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NXC5WPT3VLA55EXOLWPC65O56D/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NXC5WPT3VLA55EXOLWPC65O56D/action/storage_attestation","attest_author":"https://pith.science/pith/NXC5WPT3VLA55EXOLWPC65O56D/action/author_attestation","sign_citation":"https://pith.science/pith/NXC5WPT3VLA55EXOLWPC65O56D/action/citation_signature","submit_replication":"https://pith.science/pith/NXC5WPT3VLA55EXOLWPC65O56D/action/replication_record"}},"created_at":"2026-05-18T01:43:26.459052+00:00","updated_at":"2026-05-18T01:43:26.459052+00:00"}