{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:M7QASGQRUAJTM2H27FE3K5YMEC","short_pith_number":"pith:M7QASGQR","schema_version":"1.0","canonical_sha256":"67e0091a11a0133668faf949b5770c20baca1a14bf72814d86ab418a52d035e3","source":{"kind":"arxiv","id":"1506.06208","version":1},"attestation_state":"computed","paper":{"title":"Correlation Analysis between Tibet AS-$\\gamma$ TeV Cosmic Ray and WMAP Nine-year Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Qian-Qing Yin, Shuang-Nan Zhang","submitted_at":"2015-06-20T07:18:57Z","abstract_excerpt":"The Wilkinson Microwave Anisotropy Probe (WMAP) team subtracted template-based foreground models to produce foreground-reduced maps, and masked point sources and uncertain sky regions directly; however, whether foreground residuals exist in the WMAP foreground-reduced maps is still an open question. Here, we use Pearson correlation coefficient (PCC) analysis with AS-$\\gamma$ TeV cosmic ray (CR) data to probe possible foreground residuals in the WMAP nine-year data. The correlation results between the CR and foreground-contained maps (WMAP foreground-unreduced maps, WMAP template-based and MEM "},"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":"1506.06208","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-06-20T07:18:57Z","cross_cats_sorted":["astro-ph.GA","astro-ph.IM"],"title_canon_sha256":"bda8a969a244c24a8c0acf188b36983c888df52ddd57d539a2ad985ed293b98b","abstract_canon_sha256":"f34b7b22856549e2aa6031b6b0bd0fc9c7b9e4b24639bf6e8b7a00c3fdfdcd76"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:29:31.512885Z","signature_b64":"62bWNZWZlxB1r7XFk8LUr4UzROuMHjJgTDUldzwldLdx0PaCY2pThKkAYGOZG/ZQI8mXbDdMK8XBE85Cufl6Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"67e0091a11a0133668faf949b5770c20baca1a14bf72814d86ab418a52d035e3","last_reissued_at":"2026-05-18T01:29:31.512156Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:29:31.512156Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Correlation Analysis between Tibet AS-$\\gamma$ TeV Cosmic Ray and WMAP Nine-year Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Qian-Qing Yin, Shuang-Nan Zhang","submitted_at":"2015-06-20T07:18:57Z","abstract_excerpt":"The Wilkinson Microwave Anisotropy Probe (WMAP) team subtracted template-based foreground models to produce foreground-reduced maps, and masked point sources and uncertain sky regions directly; however, whether foreground residuals exist in the WMAP foreground-reduced maps is still an open question. Here, we use Pearson correlation coefficient (PCC) analysis with AS-$\\gamma$ TeV cosmic ray (CR) data to probe possible foreground residuals in the WMAP nine-year data. The correlation results between the CR and foreground-contained maps (WMAP foreground-unreduced maps, WMAP template-based and MEM "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1506.06208","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":"1506.06208","created_at":"2026-05-18T01:29:31.512303+00:00"},{"alias_kind":"arxiv_version","alias_value":"1506.06208v1","created_at":"2026-05-18T01:29:31.512303+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.06208","created_at":"2026-05-18T01:29:31.512303+00:00"},{"alias_kind":"pith_short_12","alias_value":"M7QASGQRUAJT","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_16","alias_value":"M7QASGQRUAJTM2H2","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_8","alias_value":"M7QASGQR","created_at":"2026-05-18T12:29:32.376354+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/M7QASGQRUAJTM2H27FE3K5YMEC","json":"https://pith.science/pith/M7QASGQRUAJTM2H27FE3K5YMEC.json","graph_json":"https://pith.science/api/pith-number/M7QASGQRUAJTM2H27FE3K5YMEC/graph.json","events_json":"https://pith.science/api/pith-number/M7QASGQRUAJTM2H27FE3K5YMEC/events.json","paper":"https://pith.science/paper/M7QASGQR"},"agent_actions":{"view_html":"https://pith.science/pith/M7QASGQRUAJTM2H27FE3K5YMEC","download_json":"https://pith.science/pith/M7QASGQRUAJTM2H27FE3K5YMEC.json","view_paper":"https://pith.science/paper/M7QASGQR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1506.06208&json=true","fetch_graph":"https://pith.science/api/pith-number/M7QASGQRUAJTM2H27FE3K5YMEC/graph.json","fetch_events":"https://pith.science/api/pith-number/M7QASGQRUAJTM2H27FE3K5YMEC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/M7QASGQRUAJTM2H27FE3K5YMEC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/M7QASGQRUAJTM2H27FE3K5YMEC/action/storage_attestation","attest_author":"https://pith.science/pith/M7QASGQRUAJTM2H27FE3K5YMEC/action/author_attestation","sign_citation":"https://pith.science/pith/M7QASGQRUAJTM2H27FE3K5YMEC/action/citation_signature","submit_replication":"https://pith.science/pith/M7QASGQRUAJTM2H27FE3K5YMEC/action/replication_record"}},"created_at":"2026-05-18T01:29:31.512303+00:00","updated_at":"2026-05-18T01:29:31.512303+00:00"}