{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:VCQM6V25NFBDYB23UBKQWBLX74","short_pith_number":"pith:VCQM6V25","schema_version":"1.0","canonical_sha256":"a8a0cf575d69423c075ba0550b0577ff29e2f243f31fbea2d53100409d3cd859","source":{"kind":"arxiv","id":"2410.05958","version":1},"attestation_state":"computed","paper":{"title":"Collisional and Radiative Data for Tellurium ions in Kilonovae modelling and Laboratory Benchmarks","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","physics.atom-ph"],"primary_cat":"astro-ph.SR","authors_text":"Catherine A. Ramsbottom, Connor P. Ballance, Fiona McNeill, Leo Patrick Mulholland, Stuart A. Sim","submitted_at":"2024-10-08T12:12:20Z","abstract_excerpt":"Tellurium is a primary candidate for the identification of the 2.1 $\\mu$m emission line in kilonovae (KNe) spectra AT2017gfo and GRB230307A. Despite this, there is currently an insufficient amount of atomic data available for this species. We calculate the required atomic structure and collisional data, particularly the data required for accurate Non-Local-Thermodynamic-Equilibrium (NLTE) modelling of the low temperatures and densities in KNe. We use a Multi-Configurational-Dirac-Hartree-Fock method to produce optimised one-electron orbitals for Te {\\sc i}-{\\sc iii}.\n  As a result energy level"},"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":"2410.05958","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2024-10-08T12:12:20Z","cross_cats_sorted":["astro-ph.HE","physics.atom-ph"],"title_canon_sha256":"7a32deb3f8d836f9ce3b17526d5cf9dd70b9fe1c28abd62a71e671e6f28067ff","abstract_canon_sha256":"394d0831a51cf48c53b30cfa53d1ce5583c341c700d517c75b38f46a85d39bfb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:17:53.707723Z","signature_b64":"MIg1C5kF6cqaq+6nAL/BSyWfPaCGpdLjyW0iPHp+XEaEaZBvBiNdnBh8i2db0YMk5aEFqbd/p88hBueSVMpvDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a8a0cf575d69423c075ba0550b0577ff29e2f243f31fbea2d53100409d3cd859","last_reissued_at":"2026-07-05T09:17:53.707222Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:17:53.707222Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Collisional and Radiative Data for Tellurium ions in Kilonovae modelling and Laboratory Benchmarks","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","physics.atom-ph"],"primary_cat":"astro-ph.SR","authors_text":"Catherine A. Ramsbottom, Connor P. Ballance, Fiona McNeill, Leo Patrick Mulholland, Stuart A. Sim","submitted_at":"2024-10-08T12:12:20Z","abstract_excerpt":"Tellurium is a primary candidate for the identification of the 2.1 $\\mu$m emission line in kilonovae (KNe) spectra AT2017gfo and GRB230307A. Despite this, there is currently an insufficient amount of atomic data available for this species. We calculate the required atomic structure and collisional data, particularly the data required for accurate Non-Local-Thermodynamic-Equilibrium (NLTE) modelling of the low temperatures and densities in KNe. We use a Multi-Configurational-Dirac-Hartree-Fock method to produce optimised one-electron orbitals for Te {\\sc i}-{\\sc iii}.\n  As a result energy level"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2410.05958","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/2410.05958/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":"2410.05958","created_at":"2026-07-05T09:17:53.707271+00:00"},{"alias_kind":"arxiv_version","alias_value":"2410.05958v1","created_at":"2026-07-05T09:17:53.707271+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2410.05958","created_at":"2026-07-05T09:17:53.707271+00:00"},{"alias_kind":"pith_short_12","alias_value":"VCQM6V25NFBD","created_at":"2026-07-05T09:17:53.707271+00:00"},{"alias_kind":"pith_short_16","alias_value":"VCQM6V25NFBDYB23","created_at":"2026-07-05T09:17:53.707271+00:00"},{"alias_kind":"pith_short_8","alias_value":"VCQM6V25","created_at":"2026-07-05T09:17:53.707271+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.10818","citing_title":"Late-time emission-line profiles from kilonova models","ref_index":35,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VCQM6V25NFBDYB23UBKQWBLX74","json":"https://pith.science/pith/VCQM6V25NFBDYB23UBKQWBLX74.json","graph_json":"https://pith.science/api/pith-number/VCQM6V25NFBDYB23UBKQWBLX74/graph.json","events_json":"https://pith.science/api/pith-number/VCQM6V25NFBDYB23UBKQWBLX74/events.json","paper":"https://pith.science/paper/VCQM6V25"},"agent_actions":{"view_html":"https://pith.science/pith/VCQM6V25NFBDYB23UBKQWBLX74","download_json":"https://pith.science/pith/VCQM6V25NFBDYB23UBKQWBLX74.json","view_paper":"https://pith.science/paper/VCQM6V25","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2410.05958&json=true","fetch_graph":"https://pith.science/api/pith-number/VCQM6V25NFBDYB23UBKQWBLX74/graph.json","fetch_events":"https://pith.science/api/pith-number/VCQM6V25NFBDYB23UBKQWBLX74/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VCQM6V25NFBDYB23UBKQWBLX74/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VCQM6V25NFBDYB23UBKQWBLX74/action/storage_attestation","attest_author":"https://pith.science/pith/VCQM6V25NFBDYB23UBKQWBLX74/action/author_attestation","sign_citation":"https://pith.science/pith/VCQM6V25NFBDYB23UBKQWBLX74/action/citation_signature","submit_replication":"https://pith.science/pith/VCQM6V25NFBDYB23UBKQWBLX74/action/replication_record"}},"created_at":"2026-07-05T09:17:53.707271+00:00","updated_at":"2026-07-05T09:17:53.707271+00:00"}