{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:NJX6HUPS6SBN476AMYGLGGJB3T","short_pith_number":"pith:NJX6HUPS","schema_version":"1.0","canonical_sha256":"6a6fe3d1f2f482de7fc0660cb31921dcc96d7803c0844a92ca7e9dee78d45bbb","source":{"kind":"arxiv","id":"1911.11841","version":2},"attestation_state":"computed","paper":{"title":"Cross Correlation of the Extragalactic Gamma-ray Background with Thermal Sunyaev-Zel'dovich Effect in the Cosmic Microwave Background","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"Masato Shirasaki, Naoki Yoshida, Oscar Macias, Shin'ichiro Ando, Shunsaku Horiuchi","submitted_at":"2019-11-26T21:33:56Z","abstract_excerpt":"Cosmic rays in galaxy clusters are unique probes of energetic processes operating with large-scale structures in the Universe. Precise measurements of cosmic rays in galaxy clusters are essential for improving our understanding of non-thermal components in the intracluster-medium (ICM) as well as the accuracy of cluster mass estimates in cosmological analyses. In this paper, we perform a cross-correlation analysis with the extragalactic gamma-ray background and the thermal Sunyaev-Zel'dovich (tSZ) effect in the cosmic microwave background. The expected cross-correlation signal would contain ri"},"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":"1911.11841","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2019-11-26T21:33:56Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"62bc3cf5898dde74a02db6daed2f10581f33fda1607a7df7b2326dcbfbb70b0f","abstract_canon_sha256":"53e3b56c8465bc0bcb71f004344cea3d6330b91938305138073989daaf060696"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:05:39.246088Z","signature_b64":"2OZJmJJsMiV+pTYE5rAzLgOQcqX1z02/Aer9fA676RJOaKUig8PlQQpfp7/us0DDCuiHhVjYDQujmQLvm+fcCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6a6fe3d1f2f482de7fc0660cb31921dcc96d7803c0844a92ca7e9dee78d45bbb","last_reissued_at":"2026-07-05T01:05:39.245595Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:05:39.245595Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cross Correlation of the Extragalactic Gamma-ray Background with Thermal Sunyaev-Zel'dovich Effect in the Cosmic Microwave Background","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"Masato Shirasaki, Naoki Yoshida, Oscar Macias, Shin'ichiro Ando, Shunsaku Horiuchi","submitted_at":"2019-11-26T21:33:56Z","abstract_excerpt":"Cosmic rays in galaxy clusters are unique probes of energetic processes operating with large-scale structures in the Universe. Precise measurements of cosmic rays in galaxy clusters are essential for improving our understanding of non-thermal components in the intracluster-medium (ICM) as well as the accuracy of cluster mass estimates in cosmological analyses. In this paper, we perform a cross-correlation analysis with the extragalactic gamma-ray background and the thermal Sunyaev-Zel'dovich (tSZ) effect in the cosmic microwave background. The expected cross-correlation signal would contain ri"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1911.11841","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/1911.11841/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":"1911.11841","created_at":"2026-07-05T01:05:39.245663+00:00"},{"alias_kind":"arxiv_version","alias_value":"1911.11841v2","created_at":"2026-07-05T01:05:39.245663+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1911.11841","created_at":"2026-07-05T01:05:39.245663+00:00"},{"alias_kind":"pith_short_12","alias_value":"NJX6HUPS6SBN","created_at":"2026-07-05T01:05:39.245663+00:00"},{"alias_kind":"pith_short_16","alias_value":"NJX6HUPS6SBN476A","created_at":"2026-07-05T01:05:39.245663+00:00"},{"alias_kind":"pith_short_8","alias_value":"NJX6HUPS","created_at":"2026-07-05T01:05:39.245663+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/NJX6HUPS6SBN476AMYGLGGJB3T","json":"https://pith.science/pith/NJX6HUPS6SBN476AMYGLGGJB3T.json","graph_json":"https://pith.science/api/pith-number/NJX6HUPS6SBN476AMYGLGGJB3T/graph.json","events_json":"https://pith.science/api/pith-number/NJX6HUPS6SBN476AMYGLGGJB3T/events.json","paper":"https://pith.science/paper/NJX6HUPS"},"agent_actions":{"view_html":"https://pith.science/pith/NJX6HUPS6SBN476AMYGLGGJB3T","download_json":"https://pith.science/pith/NJX6HUPS6SBN476AMYGLGGJB3T.json","view_paper":"https://pith.science/paper/NJX6HUPS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1911.11841&json=true","fetch_graph":"https://pith.science/api/pith-number/NJX6HUPS6SBN476AMYGLGGJB3T/graph.json","fetch_events":"https://pith.science/api/pith-number/NJX6HUPS6SBN476AMYGLGGJB3T/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NJX6HUPS6SBN476AMYGLGGJB3T/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NJX6HUPS6SBN476AMYGLGGJB3T/action/storage_attestation","attest_author":"https://pith.science/pith/NJX6HUPS6SBN476AMYGLGGJB3T/action/author_attestation","sign_citation":"https://pith.science/pith/NJX6HUPS6SBN476AMYGLGGJB3T/action/citation_signature","submit_replication":"https://pith.science/pith/NJX6HUPS6SBN476AMYGLGGJB3T/action/replication_record"}},"created_at":"2026-07-05T01:05:39.245663+00:00","updated_at":"2026-07-05T01:05:39.245663+00:00"}