{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:W2EOR6X7AYRBCKLX7TRQEE2VH6","short_pith_number":"pith:W2EOR6X7","schema_version":"1.0","canonical_sha256":"b688e8faff0622112977fce30213553fb196c899d761c2b683f39eaa7696c6d2","source":{"kind":"arxiv","id":"astro-ph/0611388","version":3},"attestation_state":"computed","paper":{"title":"Measurements of 0.2 to 20 GeV/n cosmic-ray proton and helium spectra from 1997 through 2002 with the BESS spectrometer","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. A. Moiseev, A. Yamamoto, E. S. Seo, H. Fuke, J. F. Ormes, J. Nishimura, J. Suzuki, J. W. Mitchell, K. Abe, K. C. Kim, K. Tanaka, K. Yoshimura, M. Nozaki, M. Sasaki, R. E. Streitmatter, S. Haino, S. Matsuda, S. Orito, T. Hams, T. Sanuki, T. Yamagami, T. Yoshida, Y. Makida, Y. Shikaze","submitted_at":"2006-11-13T14:49:18Z","abstract_excerpt":"We measured low energy cosmic-ray proton and helium spectra in the kinetic energy range 0.215 - 21.5 GeV/n at different solar activities during a period from 1997 to 2002. The observations were carried out with the BESS spectrometer launched on a balloon at Lynn Lake, Canada. A calculation for the correction of secondary particle backgrounds from the overlying atmosphere was improved by using the measured spectra at small atmospheric depths ranging from 5 through 37 g/cm^2. The uncertainties including statistical and systematic errors of the obtained spectra at the top of atmosphere are 5-7 % "},"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/0611388","kind":"arxiv","version":3},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-11-13T14:49:18Z","cross_cats_sorted":[],"title_canon_sha256":"ad2aaf13e67c6130ffa0c174b00dd4a55d08b49abd0704534da9bf496ff4bf73","abstract_canon_sha256":"f8b6e1139356b4cd84e0a1a03752cb592fe902a2028fc3596a737583e9ffeb62"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:21:49.087977Z","signature_b64":"UIknDF/tiLNJPsksbfPOOKrFyloHgChD0/5RR1VFZC8ZnRTn+5r3tshdxdfSye+WZQwrTgCulnJColoP85BvDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b688e8faff0622112977fce30213553fb196c899d761c2b683f39eaa7696c6d2","last_reissued_at":"2026-07-04T15:21:49.087552Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:21:49.087552Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Measurements of 0.2 to 20 GeV/n cosmic-ray proton and helium spectra from 1997 through 2002 with the BESS spectrometer","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. A. Moiseev, A. Yamamoto, E. S. Seo, H. Fuke, J. F. Ormes, J. Nishimura, J. Suzuki, J. W. Mitchell, K. Abe, K. C. Kim, K. Tanaka, K. Yoshimura, M. Nozaki, M. Sasaki, R. E. Streitmatter, S. Haino, S. Matsuda, S. Orito, T. Hams, T. Sanuki, T. Yamagami, T. Yoshida, Y. Makida, Y. Shikaze","submitted_at":"2006-11-13T14:49:18Z","abstract_excerpt":"We measured low energy cosmic-ray proton and helium spectra in the kinetic energy range 0.215 - 21.5 GeV/n at different solar activities during a period from 1997 to 2002. The observations were carried out with the BESS spectrometer launched on a balloon at Lynn Lake, Canada. A calculation for the correction of secondary particle backgrounds from the overlying atmosphere was improved by using the measured spectra at small atmospheric depths ranging from 5 through 37 g/cm^2. The uncertainties including statistical and systematic errors of the obtained spectra at the top of atmosphere are 5-7 % "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0611388","kind":"arxiv","version":3},"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/astro-ph/0611388/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":"astro-ph/0611388","created_at":"2026-07-04T15:21:49.087609+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0611388v3","created_at":"2026-07-04T15:21:49.087609+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0611388","created_at":"2026-07-04T15:21:49.087609+00:00"},{"alias_kind":"pith_short_12","alias_value":"W2EOR6X7AYRB","created_at":"2026-07-04T15:21:49.087609+00:00"},{"alias_kind":"pith_short_16","alias_value":"W2EOR6X7AYRBCKLX","created_at":"2026-07-04T15:21:49.087609+00:00"},{"alias_kind":"pith_short_8","alias_value":"W2EOR6X7","created_at":"2026-07-04T15:21:49.087609+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/W2EOR6X7AYRBCKLX7TRQEE2VH6","json":"https://pith.science/pith/W2EOR6X7AYRBCKLX7TRQEE2VH6.json","graph_json":"https://pith.science/api/pith-number/W2EOR6X7AYRBCKLX7TRQEE2VH6/graph.json","events_json":"https://pith.science/api/pith-number/W2EOR6X7AYRBCKLX7TRQEE2VH6/events.json","paper":"https://pith.science/paper/W2EOR6X7"},"agent_actions":{"view_html":"https://pith.science/pith/W2EOR6X7AYRBCKLX7TRQEE2VH6","download_json":"https://pith.science/pith/W2EOR6X7AYRBCKLX7TRQEE2VH6.json","view_paper":"https://pith.science/paper/W2EOR6X7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0611388&json=true","fetch_graph":"https://pith.science/api/pith-number/W2EOR6X7AYRBCKLX7TRQEE2VH6/graph.json","fetch_events":"https://pith.science/api/pith-number/W2EOR6X7AYRBCKLX7TRQEE2VH6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/W2EOR6X7AYRBCKLX7TRQEE2VH6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/W2EOR6X7AYRBCKLX7TRQEE2VH6/action/storage_attestation","attest_author":"https://pith.science/pith/W2EOR6X7AYRBCKLX7TRQEE2VH6/action/author_attestation","sign_citation":"https://pith.science/pith/W2EOR6X7AYRBCKLX7TRQEE2VH6/action/citation_signature","submit_replication":"https://pith.science/pith/W2EOR6X7AYRBCKLX7TRQEE2VH6/action/replication_record"}},"created_at":"2026-07-04T15:21:49.087609+00:00","updated_at":"2026-07-04T15:21:49.087609+00:00"}