{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:S2IORVU5KC6W735T5WIEOGDFWA","short_pith_number":"pith:S2IORVU5","schema_version":"1.0","canonical_sha256":"9690e8d69d50bd6fefb3ed90471865b029d3d3c611c8ef8bd1ddd438d73caa31","source":{"kind":"arxiv","id":"astro-ph/0504361","version":2},"attestation_state":"computed","paper":{"title":"Search for Cosmic-Ray Antideuterons","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. A. Moiseev, A. Yamamoto, E. S. Seo, H. Fuke, H. Matsumoto, J. F. Ormes, J. Nishimura, J. Suzuki, J. W. Mitchell, K. Abe, K. Tanaka, K. Tanizaki, K. Yamato, K. Yoshimura, M. Nozaki, M. Sasaki, R. E. Streitmatter, S. Haino, S. Matsuda, S. Orito, T. Maeno, T. Yamagami, T. Yoshida, Y. Makida, Y. Shikaze, Y. Yamamoto","submitted_at":"2005-04-16T03:58:52Z","abstract_excerpt":"We performed a search for cosmic-ray antideuterons using data collected during four BESS balloon flights from 1997 to 2000. No candidate was found. We derived, for the first time, an upper limit of 1.9E-4 (m^2 s sr GeV/nucleon)^(-1) for the differential flux of cosmic-ray antideuterons, at the 95% confidence level, between 0.17 and 1.15 GeV/nucleon at the top of the atmosphere."},"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/0504361","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-04-16T03:58:52Z","cross_cats_sorted":[],"title_canon_sha256":"bed7003129fb7a2c7faac67395daa06b578a87e7b367199e655277086007e521","abstract_canon_sha256":"06153e2bf11f21ea6fe2aa31877b7df5257ff54cf080ebb5982a86c0a2958460"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:18:02.764405Z","signature_b64":"ckX1y8mOBNcjc9r16za74EpFbQqSjweVfwDyQZPEWupwMVkokZPlLlpD9hqX5uZTMHsIJ97f9IjMBulp+MhACg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9690e8d69d50bd6fefb3ed90471865b029d3d3c611c8ef8bd1ddd438d73caa31","last_reissued_at":"2026-05-18T04:18:02.763652Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:18:02.763652Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Search for Cosmic-Ray Antideuterons","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. A. Moiseev, A. Yamamoto, E. S. Seo, H. Fuke, H. Matsumoto, J. F. Ormes, J. Nishimura, J. Suzuki, J. W. Mitchell, K. Abe, K. Tanaka, K. Tanizaki, K. Yamato, K. Yoshimura, M. Nozaki, M. Sasaki, R. E. Streitmatter, S. Haino, S. Matsuda, S. Orito, T. Maeno, T. Yamagami, T. Yoshida, Y. Makida, Y. Shikaze, Y. Yamamoto","submitted_at":"2005-04-16T03:58:52Z","abstract_excerpt":"We performed a search for cosmic-ray antideuterons using data collected during four BESS balloon flights from 1997 to 2000. No candidate was found. We derived, for the first time, an upper limit of 1.9E-4 (m^2 s sr GeV/nucleon)^(-1) for the differential flux of cosmic-ray antideuterons, at the 95% confidence level, between 0.17 and 1.15 GeV/nucleon at the top of the atmosphere."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0504361","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":"astro-ph/0504361","created_at":"2026-05-18T04:18:02.763781+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0504361v2","created_at":"2026-05-18T04:18:02.763781+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0504361","created_at":"2026-05-18T04:18:02.763781+00:00"},{"alias_kind":"pith_short_12","alias_value":"S2IORVU5KC6W","created_at":"2026-05-18T12:25:53.335082+00:00"},{"alias_kind":"pith_short_16","alias_value":"S2IORVU5KC6W735T","created_at":"2026-05-18T12:25:53.335082+00:00"},{"alias_kind":"pith_short_8","alias_value":"S2IORVU5","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":"2509.06892","citing_title":"Asymmetric Cannibal Dark Matter: Constraints from Neutron Star","ref_index":23,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/S2IORVU5KC6W735T5WIEOGDFWA","json":"https://pith.science/pith/S2IORVU5KC6W735T5WIEOGDFWA.json","graph_json":"https://pith.science/api/pith-number/S2IORVU5KC6W735T5WIEOGDFWA/graph.json","events_json":"https://pith.science/api/pith-number/S2IORVU5KC6W735T5WIEOGDFWA/events.json","paper":"https://pith.science/paper/S2IORVU5"},"agent_actions":{"view_html":"https://pith.science/pith/S2IORVU5KC6W735T5WIEOGDFWA","download_json":"https://pith.science/pith/S2IORVU5KC6W735T5WIEOGDFWA.json","view_paper":"https://pith.science/paper/S2IORVU5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0504361&json=true","fetch_graph":"https://pith.science/api/pith-number/S2IORVU5KC6W735T5WIEOGDFWA/graph.json","fetch_events":"https://pith.science/api/pith-number/S2IORVU5KC6W735T5WIEOGDFWA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/S2IORVU5KC6W735T5WIEOGDFWA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/S2IORVU5KC6W735T5WIEOGDFWA/action/storage_attestation","attest_author":"https://pith.science/pith/S2IORVU5KC6W735T5WIEOGDFWA/action/author_attestation","sign_citation":"https://pith.science/pith/S2IORVU5KC6W735T5WIEOGDFWA/action/citation_signature","submit_replication":"https://pith.science/pith/S2IORVU5KC6W735T5WIEOGDFWA/action/replication_record"}},"created_at":"2026-05-18T04:18:02.763781+00:00","updated_at":"2026-05-18T04:18:02.763781+00:00"}