{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:3DIVYHBP7FK3UC7WUJY4P63WKJ","short_pith_number":"pith:3DIVYHBP","schema_version":"1.0","canonical_sha256":"d8d15c1c2ff955ba0bf6a271c7fb76527272bd7115dd4de3c2ccd25c44c1bddf","source":{"kind":"arxiv","id":"astro-ph/0208192","version":1},"attestation_state":"computed","paper":{"title":"Cosmology with the Sunyaev-Zel'dovich Effect","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Erik D. Reese (UC Berkeley), Gilbert P. Holder (IAS), John E. Carlstrom (Chicago)","submitted_at":"2002-08-08T20:23:16Z","abstract_excerpt":"The Sunyaev-Zel'dovich effect (SZE) provides a unique way to map the large-scale structure of the universe as traced by massive clusters of galaxies. As a spectral distortion of the cosmic microwave background, the SZE is insensitive to the redshift of the galaxy cluster, making it well-suited for studies of clusters at all redshifts, and especially at reasonably high redshifts (z > 1) where the abundance of clusters is critically dependent on the underlying cosmology. Recent high signal-to-noise detections of the SZE have enabled interesting constraints on the Hubble constant and the matter d"},"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":"astro-ph/0208192","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2002-08-08T20:23:16Z","cross_cats_sorted":[],"title_canon_sha256":"c821de8a11ce042c223531b06f91da90b45d7eeb3ae69136150acd3f505aa677","abstract_canon_sha256":"26a781f22e7f9611455363b5c95b5d7cae641608bbd07399e78698300d08de2b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:23:01.136589Z","signature_b64":"o4QTTQwN+7dYYuxtf154xnAA7aHfDPcssGXHjEC3323yUl3uylv8XJMC4TDHKXUQ5e51Vy6xJ10KtRaJyZ6IDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d8d15c1c2ff955ba0bf6a271c7fb76527272bd7115dd4de3c2ccd25c44c1bddf","last_reissued_at":"2026-05-18T04:23:01.135907Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:23:01.135907Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmology with the Sunyaev-Zel'dovich Effect","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Erik D. Reese (UC Berkeley), Gilbert P. Holder (IAS), John E. Carlstrom (Chicago)","submitted_at":"2002-08-08T20:23:16Z","abstract_excerpt":"The Sunyaev-Zel'dovich effect (SZE) provides a unique way to map the large-scale structure of the universe as traced by massive clusters of galaxies. As a spectral distortion of the cosmic microwave background, the SZE is insensitive to the redshift of the galaxy cluster, making it well-suited for studies of clusters at all redshifts, and especially at reasonably high redshifts (z > 1) where the abundance of clusters is critically dependent on the underlying cosmology. Recent high signal-to-noise detections of the SZE have enabled interesting constraints on the Hubble constant and the matter d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0208192","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":"astro-ph/0208192","created_at":"2026-05-18T04:23:01.136035+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0208192v1","created_at":"2026-05-18T04:23:01.136035+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0208192","created_at":"2026-05-18T04:23:01.136035+00:00"},{"alias_kind":"pith_short_12","alias_value":"3DIVYHBP7FK3","created_at":"2026-05-18T12:25:50.845339+00:00"},{"alias_kind":"pith_short_16","alias_value":"3DIVYHBP7FK3UC7W","created_at":"2026-05-18T12:25:50.845339+00:00"},{"alias_kind":"pith_short_8","alias_value":"3DIVYHBP","created_at":"2026-05-18T12:25:50.845339+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.09967","citing_title":"Reconstructing the Thermal Sunyaev Zeldovich Power Spectrum from Planck using the ABS Method","ref_index":6,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3DIVYHBP7FK3UC7WUJY4P63WKJ","json":"https://pith.science/pith/3DIVYHBP7FK3UC7WUJY4P63WKJ.json","graph_json":"https://pith.science/api/pith-number/3DIVYHBP7FK3UC7WUJY4P63WKJ/graph.json","events_json":"https://pith.science/api/pith-number/3DIVYHBP7FK3UC7WUJY4P63WKJ/events.json","paper":"https://pith.science/paper/3DIVYHBP"},"agent_actions":{"view_html":"https://pith.science/pith/3DIVYHBP7FK3UC7WUJY4P63WKJ","download_json":"https://pith.science/pith/3DIVYHBP7FK3UC7WUJY4P63WKJ.json","view_paper":"https://pith.science/paper/3DIVYHBP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0208192&json=true","fetch_graph":"https://pith.science/api/pith-number/3DIVYHBP7FK3UC7WUJY4P63WKJ/graph.json","fetch_events":"https://pith.science/api/pith-number/3DIVYHBP7FK3UC7WUJY4P63WKJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3DIVYHBP7FK3UC7WUJY4P63WKJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3DIVYHBP7FK3UC7WUJY4P63WKJ/action/storage_attestation","attest_author":"https://pith.science/pith/3DIVYHBP7FK3UC7WUJY4P63WKJ/action/author_attestation","sign_citation":"https://pith.science/pith/3DIVYHBP7FK3UC7WUJY4P63WKJ/action/citation_signature","submit_replication":"https://pith.science/pith/3DIVYHBP7FK3UC7WUJY4P63WKJ/action/replication_record"}},"created_at":"2026-05-18T04:23:01.136035+00:00","updated_at":"2026-05-18T04:23:01.136035+00:00"}