{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:BBQRPRTLWEND7GGS4VZID53RJU","short_pith_number":"pith:BBQRPRTL","schema_version":"1.0","canonical_sha256":"086117c66bb11a3f98d2e57281f7714d382cd0a86c34d094e36fda5d32d9da7d","source":{"kind":"arxiv","id":"1604.08537","version":1},"attestation_state":"computed","paper":{"title":"Stark broadening of B IV spectral lines","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Andjelka Kovacevic, Magdalena Christova, Milan S. Dimitrijevic, Sylvie Sahal-Brechot, Zoran Simic","submitted_at":"2016-04-28T18:00:21Z","abstract_excerpt":"Stark broadening parameters for 157 multiplets of helium like boron (B IV) have been calculated using the impact semiclassical perturbation formalism. Obtained results have been used to investigate the regularities within spectral series. An example of the influence of Stark broadening on B IV lines in DO white dwarfs is given."},"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":"1604.08537","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-04-28T18:00:21Z","cross_cats_sorted":[],"title_canon_sha256":"fac343e7d39a15b4aa18cda204709a0b4d49327d7b25c08ce0e6f6ff5a34ba17","abstract_canon_sha256":"82d14469565512347c30850ecf649fe6c3f47d0501c69779361714a4515fff86"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:13:47.365924Z","signature_b64":"vFOCB/WxBEorORk6zu8rbVPrKR2d/fH8YNOTsa32g+lPqwOVwwagH9MLo9SFYpCq71jUrTM39aNsls1EZXRfAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"086117c66bb11a3f98d2e57281f7714d382cd0a86c34d094e36fda5d32d9da7d","last_reissued_at":"2026-05-18T01:13:47.365218Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:13:47.365218Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stark broadening of B IV spectral lines","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Andjelka Kovacevic, Magdalena Christova, Milan S. Dimitrijevic, Sylvie Sahal-Brechot, Zoran Simic","submitted_at":"2016-04-28T18:00:21Z","abstract_excerpt":"Stark broadening parameters for 157 multiplets of helium like boron (B IV) have been calculated using the impact semiclassical perturbation formalism. Obtained results have been used to investigate the regularities within spectral series. An example of the influence of Stark broadening on B IV lines in DO white dwarfs is given."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.08537","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":"1604.08537","created_at":"2026-05-18T01:13:47.365325+00:00"},{"alias_kind":"arxiv_version","alias_value":"1604.08537v1","created_at":"2026-05-18T01:13:47.365325+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1604.08537","created_at":"2026-05-18T01:13:47.365325+00:00"},{"alias_kind":"pith_short_12","alias_value":"BBQRPRTLWEND","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_16","alias_value":"BBQRPRTLWEND7GGS","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_8","alias_value":"BBQRPRTL","created_at":"2026-05-18T12:30:07.202191+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/BBQRPRTLWEND7GGS4VZID53RJU","json":"https://pith.science/pith/BBQRPRTLWEND7GGS4VZID53RJU.json","graph_json":"https://pith.science/api/pith-number/BBQRPRTLWEND7GGS4VZID53RJU/graph.json","events_json":"https://pith.science/api/pith-number/BBQRPRTLWEND7GGS4VZID53RJU/events.json","paper":"https://pith.science/paper/BBQRPRTL"},"agent_actions":{"view_html":"https://pith.science/pith/BBQRPRTLWEND7GGS4VZID53RJU","download_json":"https://pith.science/pith/BBQRPRTLWEND7GGS4VZID53RJU.json","view_paper":"https://pith.science/paper/BBQRPRTL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1604.08537&json=true","fetch_graph":"https://pith.science/api/pith-number/BBQRPRTLWEND7GGS4VZID53RJU/graph.json","fetch_events":"https://pith.science/api/pith-number/BBQRPRTLWEND7GGS4VZID53RJU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BBQRPRTLWEND7GGS4VZID53RJU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BBQRPRTLWEND7GGS4VZID53RJU/action/storage_attestation","attest_author":"https://pith.science/pith/BBQRPRTLWEND7GGS4VZID53RJU/action/author_attestation","sign_citation":"https://pith.science/pith/BBQRPRTLWEND7GGS4VZID53RJU/action/citation_signature","submit_replication":"https://pith.science/pith/BBQRPRTLWEND7GGS4VZID53RJU/action/replication_record"}},"created_at":"2026-05-18T01:13:47.365325+00:00","updated_at":"2026-05-18T01:13:47.365325+00:00"}