{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:AUXPNWDZHD43WJRQBQAQGT3X7C","short_pith_number":"pith:AUXPNWDZ","schema_version":"1.0","canonical_sha256":"052ef6d87938f9bb26300c01034f77f8a1a730e5e282277fb06e5562807c32ab","source":{"kind":"arxiv","id":"2311.04982","version":1},"attestation_state":"computed","paper":{"title":"Legacy Analysis of Dark Matter Annihilation from the Milky Way Dwarf Spheroidal Galaxies with 14 Years of Fermi-LAT Data","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Alex Drlica-Wagner, Alex McDaniel, Christopher M. Karwin, Marco Ajello, Mattia Di Mauro, Miguel A. Sanchez-Conde","submitted_at":"2023-11-08T19:03:43Z","abstract_excerpt":"The Milky Way (MW) dwarf spheroidal satellite galaxies (dSphs) are particularly intriguing targets to search for gamma rays from Weakly Interacting Massive Particle (WIMP) dark matter (DM) annihilation or decay. They are nearby, DM-dominated, and lack significant emission from standard astrophysical processes. Previous studies using the Fermi-Large Area Telescope (LAT) of DM emission from dSphs have provided the most robust and stringent constraints on the DM annihilation cross section and mass. We report an analysis of the MW dSphs using over 14 years of LAT data and an updated census of dSph"},"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":"2311.04982","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-11-08T19:03:43Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"00d76e2b990a09053beff606c8eabc15f5d1d0ce6587c58c93f7de24e776d65c","abstract_canon_sha256":"08e472671af6d5d6a540ac6272551787b99c87d401e3592ba0053e3fc16acde3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:10:52.969872Z","signature_b64":"1HPI+8Pvp798tCbpNt5jAGt6IibQAab0y5GiAvtr2hDnqS8iNONnO/uNg1dpLEBkIQXGSCvAvEDXBEjlhGGZCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"052ef6d87938f9bb26300c01034f77f8a1a730e5e282277fb06e5562807c32ab","last_reissued_at":"2026-07-05T07:10:52.969408Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:10:52.969408Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Legacy Analysis of Dark Matter Annihilation from the Milky Way Dwarf Spheroidal Galaxies with 14 Years of Fermi-LAT Data","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Alex Drlica-Wagner, Alex McDaniel, Christopher M. Karwin, Marco Ajello, Mattia Di Mauro, Miguel A. Sanchez-Conde","submitted_at":"2023-11-08T19:03:43Z","abstract_excerpt":"The Milky Way (MW) dwarf spheroidal satellite galaxies (dSphs) are particularly intriguing targets to search for gamma rays from Weakly Interacting Massive Particle (WIMP) dark matter (DM) annihilation or decay. They are nearby, DM-dominated, and lack significant emission from standard astrophysical processes. Previous studies using the Fermi-Large Area Telescope (LAT) of DM emission from dSphs have provided the most robust and stringent constraints on the DM annihilation cross section and mass. We report an analysis of the MW dSphs using over 14 years of LAT data and an updated census of dSph"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.04982","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2311.04982/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":"2311.04982","created_at":"2026-07-05T07:10:52.969460+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.04982v1","created_at":"2026-07-05T07:10:52.969460+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.04982","created_at":"2026-07-05T07:10:52.969460+00:00"},{"alias_kind":"pith_short_12","alias_value":"AUXPNWDZHD43","created_at":"2026-07-05T07:10:52.969460+00:00"},{"alias_kind":"pith_short_16","alias_value":"AUXPNWDZHD43WJRQ","created_at":"2026-07-05T07:10:52.969460+00:00"},{"alias_kind":"pith_short_8","alias_value":"AUXPNWDZ","created_at":"2026-07-05T07:10:52.969460+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":14,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.08552","citing_title":"The 20 GeV Galactic Halo Excess: Pixel-Level Confirmation and Consistency with Sub-TeV WIMP Annihilation","ref_index":17,"is_internal_anchor":true},{"citing_arxiv_id":"2606.25033","citing_title":"Gravitational ultra-relativistic freeze-out during general reheating","ref_index":12,"is_internal_anchor":false},{"citing_arxiv_id":"2606.23457","citing_title":"Charting Dark Matter down to the neutrino floor/fog in the 2HD+a scenario","ref_index":28,"is_internal_anchor":false},{"citing_arxiv_id":"2606.01853","citing_title":"Possible High-Energy Neutrino Emission from Dark Matter Annihilation in the Disrupting Dwarf Galaxy Bo\\\"{o}tes~III","ref_index":46,"is_internal_anchor":false},{"citing_arxiv_id":"2507.11376","citing_title":"GeV-scale thermal dark matter from dark photons: tightly constrained, yet allowed","ref_index":106,"is_internal_anchor":false},{"citing_arxiv_id":"2509.08043","citing_title":"Testing Viability of Benchmark Dark Matter Models for the Galactic Center Excess","ref_index":29,"is_internal_anchor":false},{"citing_arxiv_id":"2511.21808","citing_title":"A Comprehensive Study of WIMP Models Explaining the Fermi-LAT Galactic Center Excess","ref_index":48,"is_internal_anchor":false},{"citing_arxiv_id":"2406.01705","citing_title":"Dark Matter","ref_index":136,"is_internal_anchor":false},{"citing_arxiv_id":"2605.04890","citing_title":"Sensitivity of the Cherenkov Telescope Array Observatory to Gamma-Ray Signals in Dwarf Irregular Galaxies","ref_index":6,"is_internal_anchor":false},{"citing_arxiv_id":"2604.21976","citing_title":"Cosmic-Ray Signatures of Annihilating and Semi-Annihilating Dark Matter via One-Step Cascades","ref_index":44,"is_internal_anchor":false},{"citing_arxiv_id":"2604.05016","citing_title":"Electroweak Doublet Dark Matter for a Galactic Halo Gamma-Ray Excess","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14794","citing_title":"Deeper analysis of Fermi-LAT unassociated 4FGL J2112.5-3043 for possible identification","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2604.16595","citing_title":"On the Gamma-ray Efficiency of Superluminous Supernovae: Potential Detections and Population-Level Constraints","ref_index":37,"is_internal_anchor":false},{"citing_arxiv_id":"2604.20086","citing_title":"Photon and neutrino fluxes from spheroidal dwarf galaxies in a decaying DM model","ref_index":24,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AUXPNWDZHD43WJRQBQAQGT3X7C","json":"https://pith.science/pith/AUXPNWDZHD43WJRQBQAQGT3X7C.json","graph_json":"https://pith.science/api/pith-number/AUXPNWDZHD43WJRQBQAQGT3X7C/graph.json","events_json":"https://pith.science/api/pith-number/AUXPNWDZHD43WJRQBQAQGT3X7C/events.json","paper":"https://pith.science/paper/AUXPNWDZ"},"agent_actions":{"view_html":"https://pith.science/pith/AUXPNWDZHD43WJRQBQAQGT3X7C","download_json":"https://pith.science/pith/AUXPNWDZHD43WJRQBQAQGT3X7C.json","view_paper":"https://pith.science/paper/AUXPNWDZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.04982&json=true","fetch_graph":"https://pith.science/api/pith-number/AUXPNWDZHD43WJRQBQAQGT3X7C/graph.json","fetch_events":"https://pith.science/api/pith-number/AUXPNWDZHD43WJRQBQAQGT3X7C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AUXPNWDZHD43WJRQBQAQGT3X7C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AUXPNWDZHD43WJRQBQAQGT3X7C/action/storage_attestation","attest_author":"https://pith.science/pith/AUXPNWDZHD43WJRQBQAQGT3X7C/action/author_attestation","sign_citation":"https://pith.science/pith/AUXPNWDZHD43WJRQBQAQGT3X7C/action/citation_signature","submit_replication":"https://pith.science/pith/AUXPNWDZHD43WJRQBQAQGT3X7C/action/replication_record"}},"created_at":"2026-07-05T07:10:52.969460+00:00","updated_at":"2026-07-05T07:10:52.969460+00:00"}