{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:HMPMSUBON5JWNIGXWVV54CVUYH","short_pith_number":"pith:HMPMSUBO","schema_version":"1.0","canonical_sha256":"3b1ec9502e6f5366a0d7b56bde0ab4c1c69c3a5d5baa1aa040b142f5e0629e72","source":{"kind":"arxiv","id":"1608.04351","version":2},"attestation_state":"computed","paper":{"title":"Planck Lensing and Cosmic Infrared Background Cross-Correlation with Fermi-LAT: Tracing Dark Matter Signals in the Gamma-Ray Background","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Asantha Cooray, Brian Keating, Chang Feng","submitted_at":"2016-08-15T18:16:18Z","abstract_excerpt":"The extragalactic $\\gamma$-ray background and its spatial anisotropy could potentially contain a signature of dark matter (DM) annihilation or particle decay. Astrophysical foregrounds, such as blazars and star-forming galaxies (SFGs), however, dominate the $\\gamma$-ray background, precluding an easy detection of the signal associated with the DM annihilation or decay in the background intensity spectrum. The DM imprint on the $\\gamma$-ray background is expected to be correlated with large-scale structure tracers. In some cases, such a cross-correlation is even expected to have a higher signal"},"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":"1608.04351","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-08-15T18:16:18Z","cross_cats_sorted":[],"title_canon_sha256":"8f2023d2f1e4dd1705a72b98de7a529f9f2747f54bb858fe90cf88b62e633df7","abstract_canon_sha256":"6d5420554061f6d515463bcd7507f1dcd4254aff1089a77c8cf9b6b467dc665a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:50:19.453429Z","signature_b64":"QqDCH3gg21PD8wyshTwtTJsyK/kBU1cZbFCbU3uyfmTYdvqVrGtQZp0p3GvryshzjhhWgPyXvV0gTGv12ZrVDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3b1ec9502e6f5366a0d7b56bde0ab4c1c69c3a5d5baa1aa040b142f5e0629e72","last_reissued_at":"2026-05-18T00:50:19.452903Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:50:19.452903Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Planck Lensing and Cosmic Infrared Background Cross-Correlation with Fermi-LAT: Tracing Dark Matter Signals in the Gamma-Ray Background","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Asantha Cooray, Brian Keating, Chang Feng","submitted_at":"2016-08-15T18:16:18Z","abstract_excerpt":"The extragalactic $\\gamma$-ray background and its spatial anisotropy could potentially contain a signature of dark matter (DM) annihilation or particle decay. Astrophysical foregrounds, such as blazars and star-forming galaxies (SFGs), however, dominate the $\\gamma$-ray background, precluding an easy detection of the signal associated with the DM annihilation or decay in the background intensity spectrum. The DM imprint on the $\\gamma$-ray background is expected to be correlated with large-scale structure tracers. In some cases, such a cross-correlation is even expected to have a higher signal"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.04351","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":"1608.04351","created_at":"2026-05-18T00:50:19.452991+00:00"},{"alias_kind":"arxiv_version","alias_value":"1608.04351v2","created_at":"2026-05-18T00:50:19.452991+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1608.04351","created_at":"2026-05-18T00:50:19.452991+00:00"},{"alias_kind":"pith_short_12","alias_value":"HMPMSUBON5JW","created_at":"2026-05-18T12:30:19.053100+00:00"},{"alias_kind":"pith_short_16","alias_value":"HMPMSUBON5JWNIGX","created_at":"2026-05-18T12:30:19.053100+00:00"},{"alias_kind":"pith_short_8","alias_value":"HMPMSUBO","created_at":"2026-05-18T12:30:19.053100+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/HMPMSUBON5JWNIGXWVV54CVUYH","json":"https://pith.science/pith/HMPMSUBON5JWNIGXWVV54CVUYH.json","graph_json":"https://pith.science/api/pith-number/HMPMSUBON5JWNIGXWVV54CVUYH/graph.json","events_json":"https://pith.science/api/pith-number/HMPMSUBON5JWNIGXWVV54CVUYH/events.json","paper":"https://pith.science/paper/HMPMSUBO"},"agent_actions":{"view_html":"https://pith.science/pith/HMPMSUBON5JWNIGXWVV54CVUYH","download_json":"https://pith.science/pith/HMPMSUBON5JWNIGXWVV54CVUYH.json","view_paper":"https://pith.science/paper/HMPMSUBO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1608.04351&json=true","fetch_graph":"https://pith.science/api/pith-number/HMPMSUBON5JWNIGXWVV54CVUYH/graph.json","fetch_events":"https://pith.science/api/pith-number/HMPMSUBON5JWNIGXWVV54CVUYH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HMPMSUBON5JWNIGXWVV54CVUYH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HMPMSUBON5JWNIGXWVV54CVUYH/action/storage_attestation","attest_author":"https://pith.science/pith/HMPMSUBON5JWNIGXWVV54CVUYH/action/author_attestation","sign_citation":"https://pith.science/pith/HMPMSUBON5JWNIGXWVV54CVUYH/action/citation_signature","submit_replication":"https://pith.science/pith/HMPMSUBON5JWNIGXWVV54CVUYH/action/replication_record"}},"created_at":"2026-05-18T00:50:19.452991+00:00","updated_at":"2026-05-18T00:50:19.452991+00:00"}