{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:DREZCWCLLA572CV2JPQNY4MCAH","short_pith_number":"pith:DREZCWCL","schema_version":"1.0","canonical_sha256":"1c4991584b583bfd0aba4be0dc718201ce4c2c8f0c1100a7614fc4779d44adda","source":{"kind":"arxiv","id":"2305.09861","version":1},"attestation_state":"computed","paper":{"title":"An optimized search for dark matter in the galactic halo with HAWC","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.IM","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"A. Albert, A. Carraminana, A. Iriarte, A.L. Longinotti, A. Nayerhoda, A. Peisker, A. Sandoval, B.L. Dingus, C. Alvarez, C. De Leon, C.D. Rho, C. Espinoza, D. Avila Rojas, D. Huang, D. Rosa-Gonzalez, D. Salazar-Gallegos, E. Belmont-Moreno, E. De la Fuente, E.G. Perez-Perez, E. Moreno, F. Garfias, F. Hueyotl-Zahuantitla, F. Urena-Mena, G.J. Kunde, G. Luis-Raya, H.A. Ayala Solares, H. Leon Vargas, H. Salazar, H. Zhou, I. Torres, J.A. Garc{\\i}a-Gonzalez, J.A. Goodman, J.A. Matthews, J.C. Arteaga-Velazquez, J.C. D{\\i}az-Velez, J. Cotzomi, J. Lee, J. Lundeen, J. Mart{\\i}nez-Castro, J.P. Harding, J. Serna-Franco, J.T. Linnemann, K.L. Fan, K. Malone, K.S. Caballero-Mora, K. Tollefson, L. Nellen, L. Villasenor, M.A. DuVernois, M. Durocher, M.M. Gonzalez, M. Mostafa, N. Fraija, O. Chaparro-Amaro, O. Martinez, O. Tibolla, R. Alfaro, R. Diaz Hernandez, R. Torres-Escobedo, R. Turner, R.W. Springer, S. Casanova, T. Capistran, U. Cotti, V. Joshi, X. Wang","submitted_at":"2023-05-17T00:14:29Z","abstract_excerpt":"The Galactic Halo is a key target for indirect dark matter detection. The High Altitude Water Cherenkov (HAWC) observatory is a high-energy (~300 GeV to >100 TeV) gamma-ray detector located in central Mexico. HAWC operates via the water Cherenkov technique and has both a wide field of view of 2 sr and a >95% duty cycle, making it ideal for analyses of highly extended sources. We made use of these properties of HAWC and a new background-estimation technique optimized for extended sources to probe a large region of the Galactic Halo for dark matter signals. With this approach, we set improved co"},"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":"2305.09861","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-05-17T00:14:29Z","cross_cats_sorted":["astro-ph.CO","astro-ph.IM","hep-ph"],"title_canon_sha256":"7eead7083f59b5f3eaaefd75f37d7bc09bac50bae5c45a7597ba2e6e7e470691","abstract_canon_sha256":"34bdf44a00ac03edb241bd75e34ccf4ac7811a6f4f1b21b374b881481f872631"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:11:21.957833Z","signature_b64":"k8oShT1nZkBaSbBiQtlAj1okKXlk+7wM9eodYdylPSYQhmUzaJIp/SFFDVrmKh+dP6PBO34DGYu9tViwdlVDCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1c4991584b583bfd0aba4be0dc718201ce4c2c8f0c1100a7614fc4779d44adda","last_reissued_at":"2026-07-05T06:11:21.957370Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:11:21.957370Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"An optimized search for dark matter in the galactic halo with HAWC","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.IM","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"A. Albert, A. Carraminana, A. Iriarte, A.L. Longinotti, A. Nayerhoda, A. Peisker, A. Sandoval, B.L. Dingus, C. Alvarez, C. De Leon, C.D. Rho, C. Espinoza, D. Avila Rojas, D. Huang, D. Rosa-Gonzalez, D. Salazar-Gallegos, E. Belmont-Moreno, E. De la Fuente, E.G. Perez-Perez, E. Moreno, F. Garfias, F. Hueyotl-Zahuantitla, F. Urena-Mena, G.J. Kunde, G. Luis-Raya, H.A. Ayala Solares, H. Leon Vargas, H. Salazar, H. Zhou, I. Torres, J.A. Garc{\\i}a-Gonzalez, J.A. Goodman, J.A. Matthews, J.C. Arteaga-Velazquez, J.C. D{\\i}az-Velez, J. Cotzomi, J. Lee, J. Lundeen, J. Mart{\\i}nez-Castro, J.P. Harding, J. Serna-Franco, J.T. Linnemann, K.L. Fan, K. Malone, K.S. Caballero-Mora, K. Tollefson, L. Nellen, L. Villasenor, M.A. DuVernois, M. Durocher, M.M. Gonzalez, M. Mostafa, N. Fraija, O. Chaparro-Amaro, O. Martinez, O. Tibolla, R. Alfaro, R. Diaz Hernandez, R. Torres-Escobedo, R. Turner, R.W. Springer, S. Casanova, T. Capistran, U. Cotti, V. Joshi, X. Wang","submitted_at":"2023-05-17T00:14:29Z","abstract_excerpt":"The Galactic Halo is a key target for indirect dark matter detection. The High Altitude Water Cherenkov (HAWC) observatory is a high-energy (~300 GeV to >100 TeV) gamma-ray detector located in central Mexico. HAWC operates via the water Cherenkov technique and has both a wide field of view of 2 sr and a >95% duty cycle, making it ideal for analyses of highly extended sources. We made use of these properties of HAWC and a new background-estimation technique optimized for extended sources to probe a large region of the Galactic Halo for dark matter signals. With this approach, we set improved co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2305.09861","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/2305.09861/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":"2305.09861","created_at":"2026-07-05T06:11:21.957436+00:00"},{"alias_kind":"arxiv_version","alias_value":"2305.09861v1","created_at":"2026-07-05T06:11:21.957436+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2305.09861","created_at":"2026-07-05T06:11:21.957436+00:00"},{"alias_kind":"pith_short_12","alias_value":"DREZCWCLLA57","created_at":"2026-07-05T06:11:21.957436+00:00"},{"alias_kind":"pith_short_16","alias_value":"DREZCWCLLA572CV2","created_at":"2026-07-05T06:11:21.957436+00:00"},{"alias_kind":"pith_short_8","alias_value":"DREZCWCL","created_at":"2026-07-05T06:11:21.957436+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/DREZCWCLLA572CV2JPQNY4MCAH","json":"https://pith.science/pith/DREZCWCLLA572CV2JPQNY4MCAH.json","graph_json":"https://pith.science/api/pith-number/DREZCWCLLA572CV2JPQNY4MCAH/graph.json","events_json":"https://pith.science/api/pith-number/DREZCWCLLA572CV2JPQNY4MCAH/events.json","paper":"https://pith.science/paper/DREZCWCL"},"agent_actions":{"view_html":"https://pith.science/pith/DREZCWCLLA572CV2JPQNY4MCAH","download_json":"https://pith.science/pith/DREZCWCLLA572CV2JPQNY4MCAH.json","view_paper":"https://pith.science/paper/DREZCWCL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2305.09861&json=true","fetch_graph":"https://pith.science/api/pith-number/DREZCWCLLA572CV2JPQNY4MCAH/graph.json","fetch_events":"https://pith.science/api/pith-number/DREZCWCLLA572CV2JPQNY4MCAH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DREZCWCLLA572CV2JPQNY4MCAH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DREZCWCLLA572CV2JPQNY4MCAH/action/storage_attestation","attest_author":"https://pith.science/pith/DREZCWCLLA572CV2JPQNY4MCAH/action/author_attestation","sign_citation":"https://pith.science/pith/DREZCWCLLA572CV2JPQNY4MCAH/action/citation_signature","submit_replication":"https://pith.science/pith/DREZCWCLLA572CV2JPQNY4MCAH/action/replication_record"}},"created_at":"2026-07-05T06:11:21.957436+00:00","updated_at":"2026-07-05T06:11:21.957436+00:00"}