{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:QSCMWIDRCALS5AZK4NTH3AQTUG","short_pith_number":"pith:QSCMWIDR","schema_version":"1.0","canonical_sha256":"8484cb207110172e832ae3667d8213a18fb3027b8191efa638569fa393f374bf","source":{"kind":"arxiv","id":"1407.4516","version":3},"attestation_state":"computed","paper":{"title":"Weighing the Giants IV: Cosmology and Neutrino Mass","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) KIPAC Stanford/SLAC, 3), (3) DARK Cosmology Centre, (4) Bonn, (5) UC Berkeley, (6) Heidelberg, (7) IGC Penn. State, (8) IfA Hawaii), Adam B. Mantz (1), Adam Wright (2) ((1) KICP Chicago, Anja von der Linden (2, David A. Rapetti (3), David Donovon (8), David L. Burke (2), Douglas E. Applegate (4), Harald Ebeling (8), Mark T. Allen (2), Matteo Cataneo (3), Patricia R. Burchat (2), Patrick L. Kelly (5), R. Glenn Morris (2), Robert W. Schmidt (6), Sarah Shandera (7), Saroj Adhikari (7), Steven W. Allen (2)","submitted_at":"2014-07-16T22:26:18Z","abstract_excerpt":"We employ robust weak gravitational lensing measurements to improve cosmological constraints from measurements of the galaxy cluster mass function and its evolution, using X-ray selected clusters detected in the ROSAT All-Sky Survey. Our lensing analysis constrains the absolute mass scale of such clusters at the 8 per cent level, including both statistical and systematic uncertainties. Combining it with the survey data and X-ray follow-up observations, we find a tight constraint on a combination of the mean matter density and late-time normalization of the matter power spectrum, $\\sigma_8(\\Ome"},"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":"1407.4516","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-07-16T22:26:18Z","cross_cats_sorted":[],"title_canon_sha256":"c222c647c51288f2bd6d8ca466a8f97422479a1ceb2a207ec5b49f1748506168","abstract_canon_sha256":"4007f7f7971805407ba059076b3cbfb0ca76ecf2380828849b3d5e4df586609e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:35.935841Z","signature_b64":"o/baIk/Q3v/4kKILJHuVZ3EDSeC1Br9wlIZ+mCP/4LqV7Y46dGtXqsODP00xOPvl6G94YmovL09vs401R5VNDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8484cb207110172e832ae3667d8213a18fb3027b8191efa638569fa393f374bf","last_reissued_at":"2026-05-18T01:42:35.935355Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:35.935355Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Weighing the Giants IV: Cosmology and Neutrino Mass","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) KIPAC Stanford/SLAC, 3), (3) DARK Cosmology Centre, (4) Bonn, (5) UC Berkeley, (6) Heidelberg, (7) IGC Penn. State, (8) IfA Hawaii), Adam B. Mantz (1), Adam Wright (2) ((1) KICP Chicago, Anja von der Linden (2, David A. Rapetti (3), David Donovon (8), David L. Burke (2), Douglas E. Applegate (4), Harald Ebeling (8), Mark T. Allen (2), Matteo Cataneo (3), Patricia R. Burchat (2), Patrick L. Kelly (5), R. Glenn Morris (2), Robert W. Schmidt (6), Sarah Shandera (7), Saroj Adhikari (7), Steven W. Allen (2)","submitted_at":"2014-07-16T22:26:18Z","abstract_excerpt":"We employ robust weak gravitational lensing measurements to improve cosmological constraints from measurements of the galaxy cluster mass function and its evolution, using X-ray selected clusters detected in the ROSAT All-Sky Survey. Our lensing analysis constrains the absolute mass scale of such clusters at the 8 per cent level, including both statistical and systematic uncertainties. Combining it with the survey data and X-ray follow-up observations, we find a tight constraint on a combination of the mean matter density and late-time normalization of the matter power spectrum, $\\sigma_8(\\Ome"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.4516","kind":"arxiv","version":3},"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":"1407.4516","created_at":"2026-05-18T01:42:35.935437+00:00"},{"alias_kind":"arxiv_version","alias_value":"1407.4516v3","created_at":"2026-05-18T01:42:35.935437+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.4516","created_at":"2026-05-18T01:42:35.935437+00:00"},{"alias_kind":"pith_short_12","alias_value":"QSCMWIDRCALS","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"QSCMWIDRCALS5AZK","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"QSCMWIDR","created_at":"2026-05-18T12:28:46.137349+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2105.13549","citing_title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","ref_index":105,"is_internal_anchor":true},{"citing_arxiv_id":"1807.06209","citing_title":"Planck 2018 results. VI. Cosmological parameters","ref_index":231,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QSCMWIDRCALS5AZK4NTH3AQTUG","json":"https://pith.science/pith/QSCMWIDRCALS5AZK4NTH3AQTUG.json","graph_json":"https://pith.science/api/pith-number/QSCMWIDRCALS5AZK4NTH3AQTUG/graph.json","events_json":"https://pith.science/api/pith-number/QSCMWIDRCALS5AZK4NTH3AQTUG/events.json","paper":"https://pith.science/paper/QSCMWIDR"},"agent_actions":{"view_html":"https://pith.science/pith/QSCMWIDRCALS5AZK4NTH3AQTUG","download_json":"https://pith.science/pith/QSCMWIDRCALS5AZK4NTH3AQTUG.json","view_paper":"https://pith.science/paper/QSCMWIDR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1407.4516&json=true","fetch_graph":"https://pith.science/api/pith-number/QSCMWIDRCALS5AZK4NTH3AQTUG/graph.json","fetch_events":"https://pith.science/api/pith-number/QSCMWIDRCALS5AZK4NTH3AQTUG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QSCMWIDRCALS5AZK4NTH3AQTUG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QSCMWIDRCALS5AZK4NTH3AQTUG/action/storage_attestation","attest_author":"https://pith.science/pith/QSCMWIDRCALS5AZK4NTH3AQTUG/action/author_attestation","sign_citation":"https://pith.science/pith/QSCMWIDRCALS5AZK4NTH3AQTUG/action/citation_signature","submit_replication":"https://pith.science/pith/QSCMWIDRCALS5AZK4NTH3AQTUG/action/replication_record"}},"created_at":"2026-05-18T01:42:35.935437+00:00","updated_at":"2026-05-18T01:42:35.935437+00:00"}