{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:NFXNSPCCNCXROIIUVAOATQ6A5O","short_pith_number":"pith:NFXNSPCC","schema_version":"1.0","canonical_sha256":"696ed93c4268af172114a81c09c3c0eb9d863b14801fe8e9de311565fc4cfa1b","source":{"kind":"arxiv","id":"1408.3688","version":1},"attestation_state":"computed","paper":{"title":"The Karlsruhe Astrophysical Database of Nucleosynthesis in Stars Project - Status and Prospects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex"],"primary_cat":"astro-ph.SR","authors_text":"Franz K\\\"appeler, Iris Dillmann, Ralf Plag, Tamas Sz\\\"ucs, Thomas Rauscher, Zsolt F\\\"ul\\\"op","submitted_at":"2014-08-16T00:35:43Z","abstract_excerpt":"The KADoNiS (Karlsruhe Astrophysical Database of Nucleosynthesis in Stars) project is an astrophysical online database for cross sections relevant for nucleosynthesis in the $s$ process and the $\\gamma$ process. The $s$-process database (www.kadonis.org) was started in 2005 and is presently facing its 4th update (KADoNiS v1.0). The $\\gamma$-process database (KADoNiS-p, www.kadonis.org/pprocess) was recently revised and re-launched in March 2013.\n  Both databases are compilations for experimental cross sections with relevance to heavy ion nucleosynthesis. For the $s$ process recommended Maxwell"},"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":"1408.3688","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-08-16T00:35:43Z","cross_cats_sorted":["nucl-ex"],"title_canon_sha256":"8942f1ab8368ba54f13f2dd5d10facd232d16366237a67559123edbda47e736d","abstract_canon_sha256":"d4e3d669fa64ac96e53790835852f57c2f08b4c426563fbcd915f52ceb6a1633"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:45:03.575815Z","signature_b64":"NrlGujm30yUfiff2XKyaW8uhFC9eo060xIZX/jaZpc+l8YO8ycceSMfKTXpA4UHlkyZebNtJDCflV2DUTNAmDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"696ed93c4268af172114a81c09c3c0eb9d863b14801fe8e9de311565fc4cfa1b","last_reissued_at":"2026-05-18T02:45:03.575277Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:45:03.575277Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Karlsruhe Astrophysical Database of Nucleosynthesis in Stars Project - Status and Prospects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex"],"primary_cat":"astro-ph.SR","authors_text":"Franz K\\\"appeler, Iris Dillmann, Ralf Plag, Tamas Sz\\\"ucs, Thomas Rauscher, Zsolt F\\\"ul\\\"op","submitted_at":"2014-08-16T00:35:43Z","abstract_excerpt":"The KADoNiS (Karlsruhe Astrophysical Database of Nucleosynthesis in Stars) project is an astrophysical online database for cross sections relevant for nucleosynthesis in the $s$ process and the $\\gamma$ process. The $s$-process database (www.kadonis.org) was started in 2005 and is presently facing its 4th update (KADoNiS v1.0). The $\\gamma$-process database (KADoNiS-p, www.kadonis.org/pprocess) was recently revised and re-launched in March 2013.\n  Both databases are compilations for experimental cross sections with relevance to heavy ion nucleosynthesis. For the $s$ process recommended Maxwell"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1408.3688","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":""},"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":"1408.3688","created_at":"2026-05-18T02:45:03.575370+00:00"},{"alias_kind":"arxiv_version","alias_value":"1408.3688v1","created_at":"2026-05-18T02:45:03.575370+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1408.3688","created_at":"2026-05-18T02:45:03.575370+00:00"},{"alias_kind":"pith_short_12","alias_value":"NFXNSPCCNCXR","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_16","alias_value":"NFXNSPCCNCXROIIU","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_8","alias_value":"NFXNSPCC","created_at":"2026-05-18T12:28:41.024544+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/NFXNSPCCNCXROIIUVAOATQ6A5O","json":"https://pith.science/pith/NFXNSPCCNCXROIIUVAOATQ6A5O.json","graph_json":"https://pith.science/api/pith-number/NFXNSPCCNCXROIIUVAOATQ6A5O/graph.json","events_json":"https://pith.science/api/pith-number/NFXNSPCCNCXROIIUVAOATQ6A5O/events.json","paper":"https://pith.science/paper/NFXNSPCC"},"agent_actions":{"view_html":"https://pith.science/pith/NFXNSPCCNCXROIIUVAOATQ6A5O","download_json":"https://pith.science/pith/NFXNSPCCNCXROIIUVAOATQ6A5O.json","view_paper":"https://pith.science/paper/NFXNSPCC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1408.3688&json=true","fetch_graph":"https://pith.science/api/pith-number/NFXNSPCCNCXROIIUVAOATQ6A5O/graph.json","fetch_events":"https://pith.science/api/pith-number/NFXNSPCCNCXROIIUVAOATQ6A5O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NFXNSPCCNCXROIIUVAOATQ6A5O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NFXNSPCCNCXROIIUVAOATQ6A5O/action/storage_attestation","attest_author":"https://pith.science/pith/NFXNSPCCNCXROIIUVAOATQ6A5O/action/author_attestation","sign_citation":"https://pith.science/pith/NFXNSPCCNCXROIIUVAOATQ6A5O/action/citation_signature","submit_replication":"https://pith.science/pith/NFXNSPCCNCXROIIUVAOATQ6A5O/action/replication_record"}},"created_at":"2026-05-18T02:45:03.575370+00:00","updated_at":"2026-05-18T02:45:03.575370+00:00"}