{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:7F4EDRYWQ7MXEDRBKVIADEQLK6","short_pith_number":"pith:7F4EDRYW","schema_version":"1.0","canonical_sha256":"f97841c71687d9720e21555001920b57b584b61acb3003a45130359e5d7ee297","source":{"kind":"arxiv","id":"astro-ph/0501412","version":1},"attestation_state":"computed","paper":{"title":"Dark Matter particles in the galactic halo: results and implications from DAMA/NaI","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) Univ., (3) IHEP Beijing), A. Incicchitti (2), C.J. Dai (3), D. Prosperi (2), F. Cappella (1), F. Montecchia (1), F. Nozzoli (1), H.H. Kuang (3), INFN Roma, INFN Roma2, J.M. Ma (3), P. Belli (1), R. Bernabei (1), R. Cerulli (1), Z.P. Ye (3) ((1) Univ.","submitted_at":"2005-01-19T13:59:10Z","abstract_excerpt":"The DAMA/NaI experiment (about 100 kg highly radiopure NaI(Tl)) was proposed, designed and realised to effectively investigate in a model independent way the presence of a Dark Matter particle component in the galactic halo by exploiting the annual modulation signature. With a total exposure of 107731 kg day, collected over seven annual cycles deep underground at the Gran Sasso National Laboratory of the I.N.F.N., it has pointed out -- at 6.3 sigma C.L. -- an effect which satisfies all the peculiarities of the signature and neither systematic effects nor side reactions able to mimic the signat"},"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":"astro-ph/0501412","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-01-19T13:59:10Z","cross_cats_sorted":[],"title_canon_sha256":"f9cae58eb377d5167177b45b0e81d87d9359af4c11fa7fad3104902f8be11342","abstract_canon_sha256":"5e95b184cbec492c41b10ab4182f0191f64cb27691e6cbe40241052e9ef6d36e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:40:25.882335Z","signature_b64":"rVednfCNFg+OZA/vIJNBxOG+mebLb55G9WCV0E7xtbX2iqYiBShEQByjOvhDdP8E1Vq7bRRwkmYtJtTiOkZKBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f97841c71687d9720e21555001920b57b584b61acb3003a45130359e5d7ee297","last_reissued_at":"2026-05-18T02:40:25.881929Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:40:25.881929Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark Matter particles in the galactic halo: results and implications from DAMA/NaI","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) Univ., (3) IHEP Beijing), A. Incicchitti (2), C.J. Dai (3), D. Prosperi (2), F. Cappella (1), F. Montecchia (1), F. Nozzoli (1), H.H. Kuang (3), INFN Roma, INFN Roma2, J.M. Ma (3), P. Belli (1), R. Bernabei (1), R. Cerulli (1), Z.P. Ye (3) ((1) Univ.","submitted_at":"2005-01-19T13:59:10Z","abstract_excerpt":"The DAMA/NaI experiment (about 100 kg highly radiopure NaI(Tl)) was proposed, designed and realised to effectively investigate in a model independent way the presence of a Dark Matter particle component in the galactic halo by exploiting the annual modulation signature. With a total exposure of 107731 kg day, collected over seven annual cycles deep underground at the Gran Sasso National Laboratory of the I.N.F.N., it has pointed out -- at 6.3 sigma C.L. -- an effect which satisfies all the peculiarities of the signature and neither systematic effects nor side reactions able to mimic the signat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0501412","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":""},"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":"astro-ph/0501412","created_at":"2026-05-18T02:40:25.881990+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0501412v1","created_at":"2026-05-18T02:40:25.881990+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0501412","created_at":"2026-05-18T02:40:25.881990+00:00"},{"alias_kind":"pith_short_12","alias_value":"7F4EDRYWQ7MX","created_at":"2026-05-18T12:25:53.335082+00:00"},{"alias_kind":"pith_short_16","alias_value":"7F4EDRYWQ7MXEDRB","created_at":"2026-05-18T12:25:53.335082+00:00"},{"alias_kind":"pith_short_8","alias_value":"7F4EDRYW","created_at":"2026-05-18T12:25:53.335082+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2406.01705","citing_title":"Dark Matter","ref_index":97,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7F4EDRYWQ7MXEDRBKVIADEQLK6","json":"https://pith.science/pith/7F4EDRYWQ7MXEDRBKVIADEQLK6.json","graph_json":"https://pith.science/api/pith-number/7F4EDRYWQ7MXEDRBKVIADEQLK6/graph.json","events_json":"https://pith.science/api/pith-number/7F4EDRYWQ7MXEDRBKVIADEQLK6/events.json","paper":"https://pith.science/paper/7F4EDRYW"},"agent_actions":{"view_html":"https://pith.science/pith/7F4EDRYWQ7MXEDRBKVIADEQLK6","download_json":"https://pith.science/pith/7F4EDRYWQ7MXEDRBKVIADEQLK6.json","view_paper":"https://pith.science/paper/7F4EDRYW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0501412&json=true","fetch_graph":"https://pith.science/api/pith-number/7F4EDRYWQ7MXEDRBKVIADEQLK6/graph.json","fetch_events":"https://pith.science/api/pith-number/7F4EDRYWQ7MXEDRBKVIADEQLK6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7F4EDRYWQ7MXEDRBKVIADEQLK6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7F4EDRYWQ7MXEDRBKVIADEQLK6/action/storage_attestation","attest_author":"https://pith.science/pith/7F4EDRYWQ7MXEDRBKVIADEQLK6/action/author_attestation","sign_citation":"https://pith.science/pith/7F4EDRYWQ7MXEDRBKVIADEQLK6/action/citation_signature","submit_replication":"https://pith.science/pith/7F4EDRYWQ7MXEDRBKVIADEQLK6/action/replication_record"}},"created_at":"2026-05-18T02:40:25.881990+00:00","updated_at":"2026-05-18T02:40:25.881990+00:00"}