{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:BOE3QDTH4KASP4QXIFRKQ7YVB5","short_pith_number":"pith:BOE3QDTH","schema_version":"1.0","canonical_sha256":"0b89b80e67e28127f2174162a87f150f4a07c5cafdcad73b178d026a495c1343","source":{"kind":"arxiv","id":"1311.1330","version":1},"attestation_state":"computed","paper":{"title":"Stark broadening of B IV lines for astrophysical and laboratory plasma research","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.atom-ph"],"primary_cat":"astro-ph.SR","authors_text":"Andjelka Kova\\v{c}evi\\'c, Magdalena Christova, Milan S. Dimitrijevi\\'c, Sylvie Sahal-Br\\'echot, Zoran Simi\\'c","submitted_at":"2013-11-06T09:58:13Z","abstract_excerpt":"Stark broadening parameters for 36 multiplets of B IV have been calculated using the semi-classical perturbation formalism. Obtained results have been used to investigate the regularities within spectral series and temperature dependence."},"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":"1311.1330","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-11-06T09:58:13Z","cross_cats_sorted":["physics.atom-ph"],"title_canon_sha256":"f79323f6ec39fc3b2110c02719a9f37ffc1584470d69954e84ec3e5798b8502d","abstract_canon_sha256":"380fecb335977d078eadfc75070541db6d65a0ad27da86d1473d9779f3a9c66a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:46:38.387903Z","signature_b64":"DuR5xamJJpko1n1Ad1rrIRsyWPyWQa+3svz85z4sNGNgkHTLv08dxm69uMjh/CRloZS5zA7o4w9G8nksUGQ+AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0b89b80e67e28127f2174162a87f150f4a07c5cafdcad73b178d026a495c1343","last_reissued_at":"2026-05-18T01:46:38.387473Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:46:38.387473Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stark broadening of B IV lines for astrophysical and laboratory plasma research","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.atom-ph"],"primary_cat":"astro-ph.SR","authors_text":"Andjelka Kova\\v{c}evi\\'c, Magdalena Christova, Milan S. Dimitrijevi\\'c, Sylvie Sahal-Br\\'echot, Zoran Simi\\'c","submitted_at":"2013-11-06T09:58:13Z","abstract_excerpt":"Stark broadening parameters for 36 multiplets of B IV have been calculated using the semi-classical perturbation formalism. Obtained results have been used to investigate the regularities within spectral series and temperature dependence."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1311.1330","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":"1311.1330","created_at":"2026-05-18T01:46:38.387536+00:00"},{"alias_kind":"arxiv_version","alias_value":"1311.1330v1","created_at":"2026-05-18T01:46:38.387536+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1311.1330","created_at":"2026-05-18T01:46:38.387536+00:00"},{"alias_kind":"pith_short_12","alias_value":"BOE3QDTH4KAS","created_at":"2026-05-18T12:27:40.988391+00:00"},{"alias_kind":"pith_short_16","alias_value":"BOE3QDTH4KASP4QX","created_at":"2026-05-18T12:27:40.988391+00:00"},{"alias_kind":"pith_short_8","alias_value":"BOE3QDTH","created_at":"2026-05-18T12:27:40.988391+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/BOE3QDTH4KASP4QXIFRKQ7YVB5","json":"https://pith.science/pith/BOE3QDTH4KASP4QXIFRKQ7YVB5.json","graph_json":"https://pith.science/api/pith-number/BOE3QDTH4KASP4QXIFRKQ7YVB5/graph.json","events_json":"https://pith.science/api/pith-number/BOE3QDTH4KASP4QXIFRKQ7YVB5/events.json","paper":"https://pith.science/paper/BOE3QDTH"},"agent_actions":{"view_html":"https://pith.science/pith/BOE3QDTH4KASP4QXIFRKQ7YVB5","download_json":"https://pith.science/pith/BOE3QDTH4KASP4QXIFRKQ7YVB5.json","view_paper":"https://pith.science/paper/BOE3QDTH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1311.1330&json=true","fetch_graph":"https://pith.science/api/pith-number/BOE3QDTH4KASP4QXIFRKQ7YVB5/graph.json","fetch_events":"https://pith.science/api/pith-number/BOE3QDTH4KASP4QXIFRKQ7YVB5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BOE3QDTH4KASP4QXIFRKQ7YVB5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BOE3QDTH4KASP4QXIFRKQ7YVB5/action/storage_attestation","attest_author":"https://pith.science/pith/BOE3QDTH4KASP4QXIFRKQ7YVB5/action/author_attestation","sign_citation":"https://pith.science/pith/BOE3QDTH4KASP4QXIFRKQ7YVB5/action/citation_signature","submit_replication":"https://pith.science/pith/BOE3QDTH4KASP4QXIFRKQ7YVB5/action/replication_record"}},"created_at":"2026-05-18T01:46:38.387536+00:00","updated_at":"2026-05-18T01:46:38.387536+00:00"}