{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:PMA4YEJFQ2S736L3VZ5UYPZGL3","short_pith_number":"pith:PMA4YEJF","schema_version":"1.0","canonical_sha256":"7b01cc112586a5fdf97bae7b4c3f265edd3c8afe4a793436f58bced5fce29c3d","source":{"kind":"arxiv","id":"1505.05843","version":1},"attestation_state":"computed","paper":{"title":"Abundances in the atmosphere of the metal-rich planet-host star HD 77338","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"H.R.A. Jones, I.O. Kushniruk, J.S. Jenkins, Ya.V. Pavlenko","submitted_at":"2015-05-21T19:00:40Z","abstract_excerpt":"Abundances of Fe, Si, Ni, Ti, Na, Mg, Cu, Zn, Mn, Cr and Ca in the atmosphere of the K-dwarf HD 77338 are determined and discussed. HD 77338 hosts a hot Uranus-like planet and is currently the most metal-rich single star to host any planet. Determination of abundances was carried out in the framework of a self-consistent approach developed by Pavlenko et al. (2012). Abundances were computed iteratively by the program ABEL8, and the process converged after 4 iterations. We find that most elements follow the iron abundance, however some of the iron peak elements are found to be over-abundant in "},"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":"1505.05843","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-05-21T19:00:40Z","cross_cats_sorted":[],"title_canon_sha256":"a53ffe7724c2d2da1f16c204b775cf5f91410b776dacedab9952d59d42034656","abstract_canon_sha256":"031585bb64f800f7666b9a9b8c00e0e25baabf5f72bca47e1e43c717e6ca7702"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:36:49.613988Z","signature_b64":"0g3SegA0USc/BdJ9CLl8RWwo4/4RH5AUIQ2/gj7bt6IuWtf3KBTWaCE5dVEdt81/JntyQqarn3sDO1BmVs77Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7b01cc112586a5fdf97bae7b4c3f265edd3c8afe4a793436f58bced5fce29c3d","last_reissued_at":"2026-05-18T01:36:49.613584Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:36:49.613584Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Abundances in the atmosphere of the metal-rich planet-host star HD 77338","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"H.R.A. Jones, I.O. Kushniruk, J.S. Jenkins, Ya.V. Pavlenko","submitted_at":"2015-05-21T19:00:40Z","abstract_excerpt":"Abundances of Fe, Si, Ni, Ti, Na, Mg, Cu, Zn, Mn, Cr and Ca in the atmosphere of the K-dwarf HD 77338 are determined and discussed. HD 77338 hosts a hot Uranus-like planet and is currently the most metal-rich single star to host any planet. Determination of abundances was carried out in the framework of a self-consistent approach developed by Pavlenko et al. (2012). Abundances were computed iteratively by the program ABEL8, and the process converged after 4 iterations. We find that most elements follow the iron abundance, however some of the iron peak elements are found to be over-abundant in "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1505.05843","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":"1505.05843","created_at":"2026-05-18T01:36:49.613655+00:00"},{"alias_kind":"arxiv_version","alias_value":"1505.05843v1","created_at":"2026-05-18T01:36:49.613655+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1505.05843","created_at":"2026-05-18T01:36:49.613655+00:00"},{"alias_kind":"pith_short_12","alias_value":"PMA4YEJFQ2S7","created_at":"2026-05-18T12:29:37.295048+00:00"},{"alias_kind":"pith_short_16","alias_value":"PMA4YEJFQ2S736L3","created_at":"2026-05-18T12:29:37.295048+00:00"},{"alias_kind":"pith_short_8","alias_value":"PMA4YEJF","created_at":"2026-05-18T12:29:37.295048+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/PMA4YEJFQ2S736L3VZ5UYPZGL3","json":"https://pith.science/pith/PMA4YEJFQ2S736L3VZ5UYPZGL3.json","graph_json":"https://pith.science/api/pith-number/PMA4YEJFQ2S736L3VZ5UYPZGL3/graph.json","events_json":"https://pith.science/api/pith-number/PMA4YEJFQ2S736L3VZ5UYPZGL3/events.json","paper":"https://pith.science/paper/PMA4YEJF"},"agent_actions":{"view_html":"https://pith.science/pith/PMA4YEJFQ2S736L3VZ5UYPZGL3","download_json":"https://pith.science/pith/PMA4YEJFQ2S736L3VZ5UYPZGL3.json","view_paper":"https://pith.science/paper/PMA4YEJF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1505.05843&json=true","fetch_graph":"https://pith.science/api/pith-number/PMA4YEJFQ2S736L3VZ5UYPZGL3/graph.json","fetch_events":"https://pith.science/api/pith-number/PMA4YEJFQ2S736L3VZ5UYPZGL3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PMA4YEJFQ2S736L3VZ5UYPZGL3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PMA4YEJFQ2S736L3VZ5UYPZGL3/action/storage_attestation","attest_author":"https://pith.science/pith/PMA4YEJFQ2S736L3VZ5UYPZGL3/action/author_attestation","sign_citation":"https://pith.science/pith/PMA4YEJFQ2S736L3VZ5UYPZGL3/action/citation_signature","submit_replication":"https://pith.science/pith/PMA4YEJFQ2S736L3VZ5UYPZGL3/action/replication_record"}},"created_at":"2026-05-18T01:36:49.613655+00:00","updated_at":"2026-05-18T01:36:49.613655+00:00"}