{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:UZOJTBAVKQXXJDFNFOASDQ62PK","short_pith_number":"pith:UZOJTBAV","schema_version":"1.0","canonical_sha256":"a65c998415542f748cad2b8121c3da7aa28179c58db5218a15a9824c7c60dced","source":{"kind":"arxiv","id":"1310.3815","version":2},"attestation_state":"computed","paper":{"title":"Current Dark Matter Annihilation Constraints from CMB and Low-Redshift Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"(2) MIT), Mathew S. Madhavacheril (1), Neelima Sehgal (1), Tracy R. Slatyer (2) ((1) Stony Brook","submitted_at":"2013-10-14T20:00:00Z","abstract_excerpt":"Updated constraints on dark matter cross section and mass are presented combining CMB power spectrum measurements from Planck, WMAP9, ACT, and SPT as well as several low-redshift datasets (BAO, HST, supernovae). For the CMB datasets, we combine WMAP9 temperature and polarization data for l <= 431 with Planck temperature data for 432 < l < 2500, ACT and SPT data for l > 2500, and Planck CMB four-point lensing measurements. We allow for redshift-dependent energy deposition from dark matter annihilation by using a `universal' energy absorption curve. We also include an updated treatment of the ex"},"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":"1310.3815","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-10-14T20:00:00Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"f1b7fc1afdd30520d3a1aa0a4a981b7e9e8a6a6fd495febd5ec60933a0a564c6","abstract_canon_sha256":"dc47e1c01b777cb3efd74e3f7478ae4f7174f1792a3af5b39463f0d598a08e35"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:32:38.998788Z","signature_b64":"Tfk2KZE1QYWPHdjUZf6eNkJ3j4dKBHrnrmD+RGdKsNOcO+u+45G4Eu/MnS/wv2QRI+HxLObNP4/vd8HKamrEAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a65c998415542f748cad2b8121c3da7aa28179c58db5218a15a9824c7c60dced","last_reissued_at":"2026-05-18T02:32:38.998309Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:32:38.998309Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Current Dark Matter Annihilation Constraints from CMB and Low-Redshift Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"(2) MIT), Mathew S. Madhavacheril (1), Neelima Sehgal (1), Tracy R. Slatyer (2) ((1) Stony Brook","submitted_at":"2013-10-14T20:00:00Z","abstract_excerpt":"Updated constraints on dark matter cross section and mass are presented combining CMB power spectrum measurements from Planck, WMAP9, ACT, and SPT as well as several low-redshift datasets (BAO, HST, supernovae). For the CMB datasets, we combine WMAP9 temperature and polarization data for l <= 431 with Planck temperature data for 432 < l < 2500, ACT and SPT data for l > 2500, and Planck CMB four-point lensing measurements. We allow for redshift-dependent energy deposition from dark matter annihilation by using a `universal' energy absorption curve. We also include an updated treatment of the ex"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.3815","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":"1310.3815","created_at":"2026-05-18T02:32:38.998416+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.3815v2","created_at":"2026-05-18T02:32:38.998416+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.3815","created_at":"2026-05-18T02:32:38.998416+00:00"},{"alias_kind":"pith_short_12","alias_value":"UZOJTBAVKQXX","created_at":"2026-05-18T12:28:02.375192+00:00"},{"alias_kind":"pith_short_16","alias_value":"UZOJTBAVKQXXJDFN","created_at":"2026-05-18T12:28:02.375192+00:00"},{"alias_kind":"pith_short_8","alias_value":"UZOJTBAV","created_at":"2026-05-18T12:28:02.375192+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2508.02642","citing_title":"Lepton parity dark matter and naturally unstable domain walls","ref_index":29,"is_internal_anchor":true},{"citing_arxiv_id":"2605.08080","citing_title":"CMB Limits on the Absorption of Light Vector and Axial-Vector Dark Matter","ref_index":30,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UZOJTBAVKQXXJDFNFOASDQ62PK","json":"https://pith.science/pith/UZOJTBAVKQXXJDFNFOASDQ62PK.json","graph_json":"https://pith.science/api/pith-number/UZOJTBAVKQXXJDFNFOASDQ62PK/graph.json","events_json":"https://pith.science/api/pith-number/UZOJTBAVKQXXJDFNFOASDQ62PK/events.json","paper":"https://pith.science/paper/UZOJTBAV"},"agent_actions":{"view_html":"https://pith.science/pith/UZOJTBAVKQXXJDFNFOASDQ62PK","download_json":"https://pith.science/pith/UZOJTBAVKQXXJDFNFOASDQ62PK.json","view_paper":"https://pith.science/paper/UZOJTBAV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.3815&json=true","fetch_graph":"https://pith.science/api/pith-number/UZOJTBAVKQXXJDFNFOASDQ62PK/graph.json","fetch_events":"https://pith.science/api/pith-number/UZOJTBAVKQXXJDFNFOASDQ62PK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UZOJTBAVKQXXJDFNFOASDQ62PK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UZOJTBAVKQXXJDFNFOASDQ62PK/action/storage_attestation","attest_author":"https://pith.science/pith/UZOJTBAVKQXXJDFNFOASDQ62PK/action/author_attestation","sign_citation":"https://pith.science/pith/UZOJTBAVKQXXJDFNFOASDQ62PK/action/citation_signature","submit_replication":"https://pith.science/pith/UZOJTBAVKQXXJDFNFOASDQ62PK/action/replication_record"}},"created_at":"2026-05-18T02:32:38.998416+00:00","updated_at":"2026-05-18T02:32:38.998416+00:00"}