{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:XEEUNBN77XS5J2Q3BFJGJ2V52Z","short_pith_number":"pith:XEEUNBN7","schema_version":"1.0","canonical_sha256":"b9094685bffde5d4ea1b095264eabdd658500e9936eb557bea69a0e796f16783","source":{"kind":"arxiv","id":"2207.09182","version":1},"attestation_state":"computed","paper":{"title":"Iterative-Bayesian unfolding of isotopic cosmic-ray fluxes measured by AMS-02","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"astro-ph.IM","authors_text":"E. F. Bueno, F. Bar\\~ao, M. Vecchi","submitted_at":"2022-07-19T10:42:05Z","abstract_excerpt":"The measurement of the isotopic composition of cosmic rays (CRs) provides essential insights the understanding of the origin and propagation of these particles, namely the CR source spectra, the propagation processes and the galactic halo size. The Alpha Magnetic Spectrometer (AMS-02), a CR detector operating aboard the International Space Station since May 2011, has the capability of performing these measurements due to its precise determination of the velocity provided by its Time of Flight (TOF) and Ring Imaging Cherenkov (RICH) detector. The correct interpretation of the data requires the "},"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":"2207.09182","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.IM","submitted_at":"2022-07-19T10:42:05Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"74455c4fa697013c22b5e70629c7bb3ea577f98c22ccee769ce63f73e22118a2","abstract_canon_sha256":"321b849529bf347ea225df03ee826dae2bff07fe60124b9e1573db116309086b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:20:43.199687Z","signature_b64":"cEbJmtIHkp5QH7esf4jZWZHRcsDYZ+TuUXbrb1mtj6kQWw60bkihyj79gZCIp1pQeNayg+4ZBVUpPhpJkeNHCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b9094685bffde5d4ea1b095264eabdd658500e9936eb557bea69a0e796f16783","last_reissued_at":"2026-07-05T05:20:43.198993Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:20:43.198993Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Iterative-Bayesian unfolding of isotopic cosmic-ray fluxes measured by AMS-02","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"astro-ph.IM","authors_text":"E. F. Bueno, F. Bar\\~ao, M. Vecchi","submitted_at":"2022-07-19T10:42:05Z","abstract_excerpt":"The measurement of the isotopic composition of cosmic rays (CRs) provides essential insights the understanding of the origin and propagation of these particles, namely the CR source spectra, the propagation processes and the galactic halo size. The Alpha Magnetic Spectrometer (AMS-02), a CR detector operating aboard the International Space Station since May 2011, has the capability of performing these measurements due to its precise determination of the velocity provided by its Time of Flight (TOF) and Ring Imaging Cherenkov (RICH) detector. The correct interpretation of the data requires the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2207.09182","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/2207.09182/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":"2207.09182","created_at":"2026-07-05T05:20:43.199110+00:00"},{"alias_kind":"arxiv_version","alias_value":"2207.09182v1","created_at":"2026-07-05T05:20:43.199110+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2207.09182","created_at":"2026-07-05T05:20:43.199110+00:00"},{"alias_kind":"pith_short_12","alias_value":"XEEUNBN77XS5","created_at":"2026-07-05T05:20:43.199110+00:00"},{"alias_kind":"pith_short_16","alias_value":"XEEUNBN77XS5J2Q3","created_at":"2026-07-05T05:20:43.199110+00:00"},{"alias_kind":"pith_short_8","alias_value":"XEEUNBN7","created_at":"2026-07-05T05:20:43.199110+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/XEEUNBN77XS5J2Q3BFJGJ2V52Z","json":"https://pith.science/pith/XEEUNBN77XS5J2Q3BFJGJ2V52Z.json","graph_json":"https://pith.science/api/pith-number/XEEUNBN77XS5J2Q3BFJGJ2V52Z/graph.json","events_json":"https://pith.science/api/pith-number/XEEUNBN77XS5J2Q3BFJGJ2V52Z/events.json","paper":"https://pith.science/paper/XEEUNBN7"},"agent_actions":{"view_html":"https://pith.science/pith/XEEUNBN77XS5J2Q3BFJGJ2V52Z","download_json":"https://pith.science/pith/XEEUNBN77XS5J2Q3BFJGJ2V52Z.json","view_paper":"https://pith.science/paper/XEEUNBN7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2207.09182&json=true","fetch_graph":"https://pith.science/api/pith-number/XEEUNBN77XS5J2Q3BFJGJ2V52Z/graph.json","fetch_events":"https://pith.science/api/pith-number/XEEUNBN77XS5J2Q3BFJGJ2V52Z/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XEEUNBN77XS5J2Q3BFJGJ2V52Z/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XEEUNBN77XS5J2Q3BFJGJ2V52Z/action/storage_attestation","attest_author":"https://pith.science/pith/XEEUNBN77XS5J2Q3BFJGJ2V52Z/action/author_attestation","sign_citation":"https://pith.science/pith/XEEUNBN77XS5J2Q3BFJGJ2V52Z/action/citation_signature","submit_replication":"https://pith.science/pith/XEEUNBN77XS5J2Q3BFJGJ2V52Z/action/replication_record"}},"created_at":"2026-07-05T05:20:43.199110+00:00","updated_at":"2026-07-05T05:20:43.199110+00:00"}