{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:FNMFN4NSLZXDKERHQMVQE7FXQB","short_pith_number":"pith:FNMFN4NS","schema_version":"1.0","canonical_sha256":"2b5856f1b25e6e351227832b027cb780504d49b893bac64f96075bf506b602f2","source":{"kind":"arxiv","id":"1103.4829","version":2},"attestation_state":"computed","paper":{"title":"Cosmological Parameters from Observations of Galaxy Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adam B. Mantz, August E. Evrard, Steven W. Allen","submitted_at":"2011-03-24T18:20:05Z","abstract_excerpt":"Studies of galaxy clusters have proved crucial in helping to establish the standard model of cosmology, with a universe dominated by dark matter and dark energy. A theoretical basis that describes clusters as massive, multi-component, quasi-equilibrium systems is growing in its capability to interpret multi-wavelength observations of expanding scope and sensitivity. We review current cosmological results, including contributions to fundamental physics, obtained from observations of galaxy clusters. These results are consistent with and complementary to those from other methods. We highlight se"},"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":"1103.4829","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-03-24T18:20:05Z","cross_cats_sorted":[],"title_canon_sha256":"a958ed7efc7f72efb3fb0e927d9dda79016cfe520e9dab1f7c22d4d53b59f0c2","abstract_canon_sha256":"5b48b5b04bc9ddc13de5afee1842ea8294b937d0cd0cf57f92442c543b424b77"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:12:32.268906Z","signature_b64":"y6j8Kca36cMWMQvT4nkzz/4xcXvF9QHpymrnAo9gJVRY2++CFLqqwjWA1XWou8UvUrSlsyZOQuegqtFzFATXCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2b5856f1b25e6e351227832b027cb780504d49b893bac64f96075bf506b602f2","last_reissued_at":"2026-05-18T04:12:32.268169Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:12:32.268169Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmological Parameters from Observations of Galaxy Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adam B. Mantz, August E. Evrard, Steven W. Allen","submitted_at":"2011-03-24T18:20:05Z","abstract_excerpt":"Studies of galaxy clusters have proved crucial in helping to establish the standard model of cosmology, with a universe dominated by dark matter and dark energy. A theoretical basis that describes clusters as massive, multi-component, quasi-equilibrium systems is growing in its capability to interpret multi-wavelength observations of expanding scope and sensitivity. We review current cosmological results, including contributions to fundamental physics, obtained from observations of galaxy clusters. These results are consistent with and complementary to those from other methods. We highlight se"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1103.4829","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":"1103.4829","created_at":"2026-05-18T04:12:32.268270+00:00"},{"alias_kind":"arxiv_version","alias_value":"1103.4829v2","created_at":"2026-05-18T04:12:32.268270+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1103.4829","created_at":"2026-05-18T04:12:32.268270+00:00"},{"alias_kind":"pith_short_12","alias_value":"FNMFN4NSLZXD","created_at":"2026-05-18T12:26:28.662955+00:00"},{"alias_kind":"pith_short_16","alias_value":"FNMFN4NSLZXDKERH","created_at":"2026-05-18T12:26:28.662955+00:00"},{"alias_kind":"pith_short_8","alias_value":"FNMFN4NS","created_at":"2026-05-18T12:26:28.662955+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.20779","citing_title":"A MINOT-based Study of Gamma-ray emission from SPT-CL J2012-5649/Abell 3667","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2510.00753","citing_title":"Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters","ref_index":6,"is_internal_anchor":true},{"citing_arxiv_id":"1106.2476","citing_title":"Modified Gravity and Cosmology","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2605.06267","citing_title":"Revisiting the Constancy of the Speed of Light: Galaxy Cluster Mass Bias Implications","ref_index":27,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FNMFN4NSLZXDKERHQMVQE7FXQB","json":"https://pith.science/pith/FNMFN4NSLZXDKERHQMVQE7FXQB.json","graph_json":"https://pith.science/api/pith-number/FNMFN4NSLZXDKERHQMVQE7FXQB/graph.json","events_json":"https://pith.science/api/pith-number/FNMFN4NSLZXDKERHQMVQE7FXQB/events.json","paper":"https://pith.science/paper/FNMFN4NS"},"agent_actions":{"view_html":"https://pith.science/pith/FNMFN4NSLZXDKERHQMVQE7FXQB","download_json":"https://pith.science/pith/FNMFN4NSLZXDKERHQMVQE7FXQB.json","view_paper":"https://pith.science/paper/FNMFN4NS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1103.4829&json=true","fetch_graph":"https://pith.science/api/pith-number/FNMFN4NSLZXDKERHQMVQE7FXQB/graph.json","fetch_events":"https://pith.science/api/pith-number/FNMFN4NSLZXDKERHQMVQE7FXQB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FNMFN4NSLZXDKERHQMVQE7FXQB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FNMFN4NSLZXDKERHQMVQE7FXQB/action/storage_attestation","attest_author":"https://pith.science/pith/FNMFN4NSLZXDKERHQMVQE7FXQB/action/author_attestation","sign_citation":"https://pith.science/pith/FNMFN4NSLZXDKERHQMVQE7FXQB/action/citation_signature","submit_replication":"https://pith.science/pith/FNMFN4NSLZXDKERHQMVQE7FXQB/action/replication_record"}},"created_at":"2026-05-18T04:12:32.268270+00:00","updated_at":"2026-05-18T04:12:32.268270+00:00"}