{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:DZOYSVZLRITQRKUJXVKKNIVX6N","short_pith_number":"pith:DZOYSVZL","schema_version":"1.0","canonical_sha256":"1e5d89572b8a2708aa89bd54a6a2b7f347ce7cb38a90cb6b0e78a742da3369f6","source":{"kind":"arxiv","id":"2203.06894","version":2},"attestation_state":"computed","paper":{"title":"Snowmass2021 Cosmic Frontier: The landscape of cosmic-ray and high-energy photon probes of particle dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ex","authors_text":"Andrew W. Strong, Atsushi Takada, Brandon Roach, Chris Karwin, Daniel Salazar-Gallegos, David A. Williams, Esra Bulbul, Fiorenza Donato, James Buckley, Jason Kumar, John Tomsick, J. Patrick Harding, Julie McEnry, Kerstin Perez, Miguel A. Sanchez-Conde, Mirko Boezio, Philip von Doetinchem, Rebecca K. Leane, Shigeki Matsumoto, Stefano Profumo, Tom Melia, Tom Shutt, Toru Tanimori, Tsuguo Aramaki, Yu Watanabe","submitted_at":"2022-03-14T07:31:38Z","abstract_excerpt":"This white paper discusses the current landscape and prospects for experiments sensitive to particle dark matter processes producing photons and cosmic rays. Much of the gamma-ray sky remains unexplored on a level of sensitivity that would enable the discovery of a dark matter signal. Currently operating GeV-TeV observatories, such as Fermi-LAT, atmospheric Cherenkov telescopes, and water Cherenkov detector arrays continue to target several promising dark matter-rich environments within and beyond the Galaxy. Soon, several new experiments will continue to explore, with increased sensitivity, e"},"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":"2203.06894","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ex","submitted_at":"2022-03-14T07:31:38Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"04da6086f3e7b779b17883299829edf4e15dbaa770ce5bf037112d2555f21be1","abstract_canon_sha256":"1985786ce1d91e06188ab786671f1fb5f517c8dcfca21af4c9016b301bb2a6b1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:34:36.728901Z","signature_b64":"D1C5EwuXZj4o20Zx7Z2Bnm38oIrpQqJ0CCU+JxAp+ZIKkeWvMvXc+qKbuYHpNNM3BXHcA/xf70fAGkbGZYcJCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1e5d89572b8a2708aa89bd54a6a2b7f347ce7cb38a90cb6b0e78a742da3369f6","last_reissued_at":"2026-07-05T04:34:36.728396Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:34:36.728396Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Snowmass2021 Cosmic Frontier: The landscape of cosmic-ray and high-energy photon probes of particle dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ex","authors_text":"Andrew W. Strong, Atsushi Takada, Brandon Roach, Chris Karwin, Daniel Salazar-Gallegos, David A. Williams, Esra Bulbul, Fiorenza Donato, James Buckley, Jason Kumar, John Tomsick, J. Patrick Harding, Julie McEnry, Kerstin Perez, Miguel A. Sanchez-Conde, Mirko Boezio, Philip von Doetinchem, Rebecca K. Leane, Shigeki Matsumoto, Stefano Profumo, Tom Melia, Tom Shutt, Toru Tanimori, Tsuguo Aramaki, Yu Watanabe","submitted_at":"2022-03-14T07:31:38Z","abstract_excerpt":"This white paper discusses the current landscape and prospects for experiments sensitive to particle dark matter processes producing photons and cosmic rays. Much of the gamma-ray sky remains unexplored on a level of sensitivity that would enable the discovery of a dark matter signal. Currently operating GeV-TeV observatories, such as Fermi-LAT, atmospheric Cherenkov telescopes, and water Cherenkov detector arrays continue to target several promising dark matter-rich environments within and beyond the Galaxy. Soon, several new experiments will continue to explore, with increased sensitivity, e"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2203.06894","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/2203.06894/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":"2203.06894","created_at":"2026-07-05T04:34:36.728462+00:00"},{"alias_kind":"arxiv_version","alias_value":"2203.06894v2","created_at":"2026-07-05T04:34:36.728462+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2203.06894","created_at":"2026-07-05T04:34:36.728462+00:00"},{"alias_kind":"pith_short_12","alias_value":"DZOYSVZLRITQ","created_at":"2026-07-05T04:34:36.728462+00:00"},{"alias_kind":"pith_short_16","alias_value":"DZOYSVZLRITQRKUJ","created_at":"2026-07-05T04:34:36.728462+00:00"},{"alias_kind":"pith_short_8","alias_value":"DZOYSVZL","created_at":"2026-07-05T04:34:36.728462+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.09976","citing_title":"Too Heavy to Hide: Gamma-Ray Constraints on Annihilating Dark Matter beyond Unitarity","ref_index":52,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DZOYSVZLRITQRKUJXVKKNIVX6N","json":"https://pith.science/pith/DZOYSVZLRITQRKUJXVKKNIVX6N.json","graph_json":"https://pith.science/api/pith-number/DZOYSVZLRITQRKUJXVKKNIVX6N/graph.json","events_json":"https://pith.science/api/pith-number/DZOYSVZLRITQRKUJXVKKNIVX6N/events.json","paper":"https://pith.science/paper/DZOYSVZL"},"agent_actions":{"view_html":"https://pith.science/pith/DZOYSVZLRITQRKUJXVKKNIVX6N","download_json":"https://pith.science/pith/DZOYSVZLRITQRKUJXVKKNIVX6N.json","view_paper":"https://pith.science/paper/DZOYSVZL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2203.06894&json=true","fetch_graph":"https://pith.science/api/pith-number/DZOYSVZLRITQRKUJXVKKNIVX6N/graph.json","fetch_events":"https://pith.science/api/pith-number/DZOYSVZLRITQRKUJXVKKNIVX6N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DZOYSVZLRITQRKUJXVKKNIVX6N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DZOYSVZLRITQRKUJXVKKNIVX6N/action/storage_attestation","attest_author":"https://pith.science/pith/DZOYSVZLRITQRKUJXVKKNIVX6N/action/author_attestation","sign_citation":"https://pith.science/pith/DZOYSVZLRITQRKUJXVKKNIVX6N/action/citation_signature","submit_replication":"https://pith.science/pith/DZOYSVZLRITQRKUJXVKKNIVX6N/action/replication_record"}},"created_at":"2026-07-05T04:34:36.728462+00:00","updated_at":"2026-07-05T04:34:36.728462+00:00"}