{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:3BXH337LBXUNCKEEMIOHOGRC6L","short_pith_number":"pith:3BXH337L","schema_version":"1.0","canonical_sha256":"d86e7defeb0de8d12884621c771a22f2c4ba7b5407a0cb518465ced7300bfb5f","source":{"kind":"arxiv","id":"astro-ph/0309337","version":2},"attestation_state":"computed","paper":{"title":"Beyond the Damping Tail: Cross-Correlating the Kinetic Sunyaev-Zel'dovich Effect with Cosmic Shear","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"David N. Spergel (Princeton), Joseph F. Hennawi, Olivier Dor\\'e","submitted_at":"2003-09-11T22:03:29Z","abstract_excerpt":"Secondary anisotropies of the CMB have the potential to reveal intricate details about the history of our universe between the present and recombination epochs. However, because the CMB we observe is the projected sum of a multitude of effects, the interpretation of small scale anisotropies by future high resolution experiments will be marred by uncertainty and speculation without the handles provided by other observations. In this paper we show that cross correlating the CMB with an overlapping weak lensing survey will isolate the elusive kinetic Sunyaev-Zel'dovich Effect from secondary aniso"},"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/0309337","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2003-09-11T22:03:29Z","cross_cats_sorted":[],"title_canon_sha256":"2951e5e792ae5f80f8ac734f58c54c90120a2d0fbf81e49706ba9ad82cbe6411","abstract_canon_sha256":"1b6099ce97f10b648acae17cd038f1a045a594e941aaf056b8a8cd7671a3f40a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:51:38.537841Z","signature_b64":"pqHwjJNfa8yUTXLBZivIc1wDF+yg3PKWyeVAMlgWjl7ISAvOzlTwj4Q7Cdj7TcyqVcCn9jqK4IGOl1DO1jVSAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d86e7defeb0de8d12884621c771a22f2c4ba7b5407a0cb518465ced7300bfb5f","last_reissued_at":"2026-07-04T16:51:38.537467Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:51:38.537467Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Beyond the Damping Tail: Cross-Correlating the Kinetic Sunyaev-Zel'dovich Effect with Cosmic Shear","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"David N. Spergel (Princeton), Joseph F. Hennawi, Olivier Dor\\'e","submitted_at":"2003-09-11T22:03:29Z","abstract_excerpt":"Secondary anisotropies of the CMB have the potential to reveal intricate details about the history of our universe between the present and recombination epochs. However, because the CMB we observe is the projected sum of a multitude of effects, the interpretation of small scale anisotropies by future high resolution experiments will be marred by uncertainty and speculation without the handles provided by other observations. In this paper we show that cross correlating the CMB with an overlapping weak lensing survey will isolate the elusive kinetic Sunyaev-Zel'dovich Effect from secondary aniso"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0309337","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0309337/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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/0309337","created_at":"2026-07-04T16:51:38.537531+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0309337v2","created_at":"2026-07-04T16:51:38.537531+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0309337","created_at":"2026-07-04T16:51:38.537531+00:00"},{"alias_kind":"pith_short_12","alias_value":"3BXH337LBXUN","created_at":"2026-07-04T16:51:38.537531+00:00"},{"alias_kind":"pith_short_16","alias_value":"3BXH337LBXUNCKEE","created_at":"2026-07-04T16:51:38.537531+00:00"},{"alias_kind":"pith_short_8","alias_value":"3BXH337L","created_at":"2026-07-04T16:51:38.537531+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2509.03458","citing_title":"Comparison of Halo Model and Simulation Predictions for Projected-Field Kinematic Sunyaev-Zel'dovich Cross-Correlations","ref_index":10,"is_internal_anchor":true},{"citing_arxiv_id":"2510.13752","citing_title":"Effects of primordial magnetic fields on 21 cm multifrequency angular power spectra","ref_index":50,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3BXH337LBXUNCKEEMIOHOGRC6L","json":"https://pith.science/pith/3BXH337LBXUNCKEEMIOHOGRC6L.json","graph_json":"https://pith.science/api/pith-number/3BXH337LBXUNCKEEMIOHOGRC6L/graph.json","events_json":"https://pith.science/api/pith-number/3BXH337LBXUNCKEEMIOHOGRC6L/events.json","paper":"https://pith.science/paper/3BXH337L"},"agent_actions":{"view_html":"https://pith.science/pith/3BXH337LBXUNCKEEMIOHOGRC6L","download_json":"https://pith.science/pith/3BXH337LBXUNCKEEMIOHOGRC6L.json","view_paper":"https://pith.science/paper/3BXH337L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0309337&json=true","fetch_graph":"https://pith.science/api/pith-number/3BXH337LBXUNCKEEMIOHOGRC6L/graph.json","fetch_events":"https://pith.science/api/pith-number/3BXH337LBXUNCKEEMIOHOGRC6L/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3BXH337LBXUNCKEEMIOHOGRC6L/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3BXH337LBXUNCKEEMIOHOGRC6L/action/storage_attestation","attest_author":"https://pith.science/pith/3BXH337LBXUNCKEEMIOHOGRC6L/action/author_attestation","sign_citation":"https://pith.science/pith/3BXH337LBXUNCKEEMIOHOGRC6L/action/citation_signature","submit_replication":"https://pith.science/pith/3BXH337LBXUNCKEEMIOHOGRC6L/action/replication_record"}},"created_at":"2026-07-04T16:51:38.537531+00:00","updated_at":"2026-07-04T16:51:38.537531+00:00"}