{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:3ATAGBM6SLZ62O2KEXTSEOTT5Z","short_pith_number":"pith:3ATAGBM6","schema_version":"1.0","canonical_sha256":"d82603059e92f3ed3b4a25e7223a73ee5b7e6c778e2c18c87c12a704a9cab658","source":{"kind":"arxiv","id":"2404.01271","version":1},"attestation_state":"computed","paper":{"title":"Energy, strength, and alpha width measurements of $E_{\\rm{c.m.}} = 1323$ and $1487$ keV resonances in $^{15}$N($\\alpha,\\gamma$)$^{19}$F","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"nucl-ex","authors_text":"A. Sanchez, D. Robertson, E. Stech, J. G\\\"orres, J. Koros, J. P. McDonaugh, J. Rufino, K. Lee, K. Manukyan, M. Couder, M. Matney, R. Fang, R. J. deBoer, S. Carmichael, S. Moylan, T. L. Bailey","submitted_at":"2024-04-01T17:47:08Z","abstract_excerpt":"The $^{15}$N($\\alpha,\\gamma$)$^{19}$F reaction produces $^{19}$F in asymptotic giant branch (AGB) stars, where the low energy tails of two resonances at $E_{\\rm{c.m.}} = 1323 \\pm 2$ and $1487 \\pm 1.7$ keV are estimated to contribute about $30\\%$ of the total reaction rate in these environments. However, recent measurements have shown discrepancies in the energies, the strengths, and the corresponding alpha widths of these two resonances, resulting in an increase in the systematic uncertainty of the extrapolated cross section to helium burning energies. With this motivation, we have undertaken "},"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":"2404.01271","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"nucl-ex","submitted_at":"2024-04-01T17:47:08Z","cross_cats_sorted":[],"title_canon_sha256":"e3a7a77ad7d2c0d36f8bf9f62ac7a74ed7791cf5b50c04e78ad8174b606282e8","abstract_canon_sha256":"3b2bec2c3e5f02bfeabd75314591a03c390c2b87d750fc78b9171de38766b2f1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:03:03.821407Z","signature_b64":"tXewOKY2l9jFhw7OjOo53gwh+6h1U3TSsMPcM37MgYwEtV4CQLgt/Ph5vkdVP/9wj/Bu38nfLM9S6mjhP/K5Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d82603059e92f3ed3b4a25e7223a73ee5b7e6c778e2c18c87c12a704a9cab658","last_reissued_at":"2026-07-05T08:03:03.820945Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:03:03.820945Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Energy, strength, and alpha width measurements of $E_{\\rm{c.m.}} = 1323$ and $1487$ keV resonances in $^{15}$N($\\alpha,\\gamma$)$^{19}$F","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"nucl-ex","authors_text":"A. Sanchez, D. Robertson, E. Stech, J. G\\\"orres, J. Koros, J. P. McDonaugh, J. Rufino, K. Lee, K. Manukyan, M. Couder, M. Matney, R. Fang, R. J. deBoer, S. Carmichael, S. Moylan, T. L. Bailey","submitted_at":"2024-04-01T17:47:08Z","abstract_excerpt":"The $^{15}$N($\\alpha,\\gamma$)$^{19}$F reaction produces $^{19}$F in asymptotic giant branch (AGB) stars, where the low energy tails of two resonances at $E_{\\rm{c.m.}} = 1323 \\pm 2$ and $1487 \\pm 1.7$ keV are estimated to contribute about $30\\%$ of the total reaction rate in these environments. However, recent measurements have shown discrepancies in the energies, the strengths, and the corresponding alpha widths of these two resonances, resulting in an increase in the systematic uncertainty of the extrapolated cross section to helium burning energies. With this motivation, we have undertaken "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2404.01271","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/2404.01271/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":"2404.01271","created_at":"2026-07-05T08:03:03.821006+00:00"},{"alias_kind":"arxiv_version","alias_value":"2404.01271v1","created_at":"2026-07-05T08:03:03.821006+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2404.01271","created_at":"2026-07-05T08:03:03.821006+00:00"},{"alias_kind":"pith_short_12","alias_value":"3ATAGBM6SLZ6","created_at":"2026-07-05T08:03:03.821006+00:00"},{"alias_kind":"pith_short_16","alias_value":"3ATAGBM6SLZ62O2K","created_at":"2026-07-05T08:03:03.821006+00:00"},{"alias_kind":"pith_short_8","alias_value":"3ATAGBM6","created_at":"2026-07-05T08:03:03.821006+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/3ATAGBM6SLZ62O2KEXTSEOTT5Z","json":"https://pith.science/pith/3ATAGBM6SLZ62O2KEXTSEOTT5Z.json","graph_json":"https://pith.science/api/pith-number/3ATAGBM6SLZ62O2KEXTSEOTT5Z/graph.json","events_json":"https://pith.science/api/pith-number/3ATAGBM6SLZ62O2KEXTSEOTT5Z/events.json","paper":"https://pith.science/paper/3ATAGBM6"},"agent_actions":{"view_html":"https://pith.science/pith/3ATAGBM6SLZ62O2KEXTSEOTT5Z","download_json":"https://pith.science/pith/3ATAGBM6SLZ62O2KEXTSEOTT5Z.json","view_paper":"https://pith.science/paper/3ATAGBM6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2404.01271&json=true","fetch_graph":"https://pith.science/api/pith-number/3ATAGBM6SLZ62O2KEXTSEOTT5Z/graph.json","fetch_events":"https://pith.science/api/pith-number/3ATAGBM6SLZ62O2KEXTSEOTT5Z/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3ATAGBM6SLZ62O2KEXTSEOTT5Z/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3ATAGBM6SLZ62O2KEXTSEOTT5Z/action/storage_attestation","attest_author":"https://pith.science/pith/3ATAGBM6SLZ62O2KEXTSEOTT5Z/action/author_attestation","sign_citation":"https://pith.science/pith/3ATAGBM6SLZ62O2KEXTSEOTT5Z/action/citation_signature","submit_replication":"https://pith.science/pith/3ATAGBM6SLZ62O2KEXTSEOTT5Z/action/replication_record"}},"created_at":"2026-07-05T08:03:03.821006+00:00","updated_at":"2026-07-05T08:03:03.821006+00:00"}