{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:5Y6L3OW7JDE4HGI44V4YJNHHTT","short_pith_number":"pith:5Y6L3OW7","schema_version":"1.0","canonical_sha256":"ee3cbdbadf48c9c3991ce57984b4e79ccf12954d06049d1956f2b1881e261e71","source":{"kind":"arxiv","id":"nucl-th/0406011","version":2},"attestation_state":"computed","paper":{"title":"Determination of S17(0) from published data","license":"","headline":"","cross_cats":["astro-ph","nucl-ex"],"primary_cat":"nucl-th","authors_text":"B. Davids, B. K. Jennings, R. H. Cyburt","submitted_at":"2004-06-03T20:00:50Z","abstract_excerpt":"The experimental landscape for the 7Be+p radiative capture reaction is rapidly changing as new high precision data become available. We present an evaluation of existing data, detailing the treatment of systematic errors and discrepancies, and show how they constrain the astrophysical S factor (S17), independent of any nuclear structure model. With theoretical models robustly determining the behavior of the sub-threshold pole, the extrapolation error can be reduced and a constraint placed on the slope of S17. Using only radiative capture data, we find S17(0) = 20.7 +/- 0.6 (stat) +/- 1.0 (syst"},"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":"nucl-th/0406011","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"nucl-th","submitted_at":"2004-06-03T20:00:50Z","cross_cats_sorted":["astro-ph","nucl-ex"],"title_canon_sha256":"2cf029dae16e6bc7c3ded24132c8fee12c14251a937c9594ff8f6194284fee11","abstract_canon_sha256":"3e0f4e5d7b8cac13a60ecc26bab5693c6f6b9c14133ed9aa45448dd689d12f80"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:49:39.743055Z","signature_b64":"TpUwW9ilJNqnmAE/r/vqGR0cWV2WecJPRLNRQwhhXBTlvoE3tHBFuTbgZuOWyv2q19pAUsaLKa+Tyi9rDeMuCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ee3cbdbadf48c9c3991ce57984b4e79ccf12954d06049d1956f2b1881e261e71","last_reissued_at":"2026-07-04T16:49:39.742709Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:49:39.742709Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Determination of S17(0) from published data","license":"","headline":"","cross_cats":["astro-ph","nucl-ex"],"primary_cat":"nucl-th","authors_text":"B. Davids, B. K. Jennings, R. H. Cyburt","submitted_at":"2004-06-03T20:00:50Z","abstract_excerpt":"The experimental landscape for the 7Be+p radiative capture reaction is rapidly changing as new high precision data become available. We present an evaluation of existing data, detailing the treatment of systematic errors and discrepancies, and show how they constrain the astrophysical S factor (S17), independent of any nuclear structure model. With theoretical models robustly determining the behavior of the sub-threshold pole, the extrapolation error can be reduced and a constraint placed on the slope of S17. Using only radiative capture data, we find S17(0) = 20.7 +/- 0.6 (stat) +/- 1.0 (syst"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"nucl-th/0406011","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/nucl-th/0406011/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":"nucl-th/0406011","created_at":"2026-07-04T16:49:39.742772+00:00"},{"alias_kind":"arxiv_version","alias_value":"nucl-th/0406011v2","created_at":"2026-07-04T16:49:39.742772+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.nucl-th/0406011","created_at":"2026-07-04T16:49:39.742772+00:00"},{"alias_kind":"pith_short_12","alias_value":"5Y6L3OW7JDE4","created_at":"2026-07-04T16:49:39.742772+00:00"},{"alias_kind":"pith_short_16","alias_value":"5Y6L3OW7JDE4HGI4","created_at":"2026-07-04T16:49:39.742772+00:00"},{"alias_kind":"pith_short_8","alias_value":"5Y6L3OW7","created_at":"2026-07-04T16:49:39.742772+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/5Y6L3OW7JDE4HGI44V4YJNHHTT","json":"https://pith.science/pith/5Y6L3OW7JDE4HGI44V4YJNHHTT.json","graph_json":"https://pith.science/api/pith-number/5Y6L3OW7JDE4HGI44V4YJNHHTT/graph.json","events_json":"https://pith.science/api/pith-number/5Y6L3OW7JDE4HGI44V4YJNHHTT/events.json","paper":"https://pith.science/paper/5Y6L3OW7"},"agent_actions":{"view_html":"https://pith.science/pith/5Y6L3OW7JDE4HGI44V4YJNHHTT","download_json":"https://pith.science/pith/5Y6L3OW7JDE4HGI44V4YJNHHTT.json","view_paper":"https://pith.science/paper/5Y6L3OW7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=nucl-th/0406011&json=true","fetch_graph":"https://pith.science/api/pith-number/5Y6L3OW7JDE4HGI44V4YJNHHTT/graph.json","fetch_events":"https://pith.science/api/pith-number/5Y6L3OW7JDE4HGI44V4YJNHHTT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5Y6L3OW7JDE4HGI44V4YJNHHTT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5Y6L3OW7JDE4HGI44V4YJNHHTT/action/storage_attestation","attest_author":"https://pith.science/pith/5Y6L3OW7JDE4HGI44V4YJNHHTT/action/author_attestation","sign_citation":"https://pith.science/pith/5Y6L3OW7JDE4HGI44V4YJNHHTT/action/citation_signature","submit_replication":"https://pith.science/pith/5Y6L3OW7JDE4HGI44V4YJNHHTT/action/replication_record"}},"created_at":"2026-07-04T16:49:39.742772+00:00","updated_at":"2026-07-04T16:49:39.742772+00:00"}