{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:GBDA25KB436PFIK4T7OYEYFDKM","short_pith_number":"pith:GBDA25KB","schema_version":"1.0","canonical_sha256":"30460d7541e6fcf2a15c9fdd8260a353058f9a36b0b4aea73b7c4b60605314a9","source":{"kind":"arxiv","id":"1205.5794","version":2},"attestation_state":"computed","paper":{"title":"Cosmological Constraints from Moments of the Thermal Sunyaev-Zel'dovich Effect","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Blake D. Sherwin, J. Colin Hill","submitted_at":"2012-05-25T19:57:28Z","abstract_excerpt":"In this paper, we explain how moments of the thermal Sunyaev-Zel'dovich (tSZ) effect can constrain both cosmological parameters and the astrophysics of the intracluster medium (ICM). As the tSZ signal is strongly non-Gaussian, higher moments of tSZ maps contain useful information. We first calculate the dependence of the tSZ moments on cosmological parameters, finding that higher moments scale more steeply with sigma_8 and are sourced by more massive galaxy clusters. Taking advantage of the different dependence of the variance and skewness on cosmological and astrophysical parameters, we const"},"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":"1205.5794","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-05-25T19:57:28Z","cross_cats_sorted":[],"title_canon_sha256":"543316159a4998b9dc774b56f5043dedcd1c67245ee599b1a6f57ad81122abaf","abstract_canon_sha256":"798c75ddc4ab407e9c7cc043c547e1781b2ffb909b3db38d18566f7767ee2a1f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:22:28.232956Z","signature_b64":"9ZYE7RcrjnsGer6JTwxnVrsbOlxF3Q0sLCCFwwh/NK0sGEFVwHgIWdft1eusgjCe1OhnYveB0/IOh6Mvg6uiCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"30460d7541e6fcf2a15c9fdd8260a353058f9a36b0b4aea73b7c4b60605314a9","last_reissued_at":"2026-05-18T03:22:28.232511Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:22:28.232511Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmological Constraints from Moments of the Thermal Sunyaev-Zel'dovich Effect","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Blake D. Sherwin, J. Colin Hill","submitted_at":"2012-05-25T19:57:28Z","abstract_excerpt":"In this paper, we explain how moments of the thermal Sunyaev-Zel'dovich (tSZ) effect can constrain both cosmological parameters and the astrophysics of the intracluster medium (ICM). As the tSZ signal is strongly non-Gaussian, higher moments of tSZ maps contain useful information. We first calculate the dependence of the tSZ moments on cosmological parameters, finding that higher moments scale more steeply with sigma_8 and are sourced by more massive galaxy clusters. Taking advantage of the different dependence of the variance and skewness on cosmological and astrophysical parameters, we const"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1205.5794","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":"1205.5794","created_at":"2026-05-18T03:22:28.232571+00:00"},{"alias_kind":"arxiv_version","alias_value":"1205.5794v2","created_at":"2026-05-18T03:22:28.232571+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1205.5794","created_at":"2026-05-18T03:22:28.232571+00:00"},{"alias_kind":"pith_short_12","alias_value":"GBDA25KB436P","created_at":"2026-05-18T12:27:06.952714+00:00"},{"alias_kind":"pith_short_16","alias_value":"GBDA25KB436PFIK4","created_at":"2026-05-18T12:27:06.952714+00:00"},{"alias_kind":"pith_short_8","alias_value":"GBDA25KB","created_at":"2026-05-18T12:27:06.952714+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/GBDA25KB436PFIK4T7OYEYFDKM","json":"https://pith.science/pith/GBDA25KB436PFIK4T7OYEYFDKM.json","graph_json":"https://pith.science/api/pith-number/GBDA25KB436PFIK4T7OYEYFDKM/graph.json","events_json":"https://pith.science/api/pith-number/GBDA25KB436PFIK4T7OYEYFDKM/events.json","paper":"https://pith.science/paper/GBDA25KB"},"agent_actions":{"view_html":"https://pith.science/pith/GBDA25KB436PFIK4T7OYEYFDKM","download_json":"https://pith.science/pith/GBDA25KB436PFIK4T7OYEYFDKM.json","view_paper":"https://pith.science/paper/GBDA25KB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1205.5794&json=true","fetch_graph":"https://pith.science/api/pith-number/GBDA25KB436PFIK4T7OYEYFDKM/graph.json","fetch_events":"https://pith.science/api/pith-number/GBDA25KB436PFIK4T7OYEYFDKM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GBDA25KB436PFIK4T7OYEYFDKM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GBDA25KB436PFIK4T7OYEYFDKM/action/storage_attestation","attest_author":"https://pith.science/pith/GBDA25KB436PFIK4T7OYEYFDKM/action/author_attestation","sign_citation":"https://pith.science/pith/GBDA25KB436PFIK4T7OYEYFDKM/action/citation_signature","submit_replication":"https://pith.science/pith/GBDA25KB436PFIK4T7OYEYFDKM/action/replication_record"}},"created_at":"2026-05-18T03:22:28.232571+00:00","updated_at":"2026-05-18T03:22:28.232571+00:00"}