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HD 86950b has a period of 1270$\\pm$57 days at $a=2.72\\pm$0.08 AU, and m sin $i=3.6\\pm$0.7 Mjup. HD 222076b has $P=871\\pm$19 days at $a=1.83\\pm$0.03 AU, and m sin $i=1.56\\pm$0.11 Mjup. These two giant planets are typical of the population of planets known to orbit evolved stars. In addition, we find a high-amplitude periodic velocity signal ($K\\sim$50 m/s) in HD 29399, and show that it is due to stellar variabi"},"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":"1611.07648","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2016-11-23T05:21:18Z","cross_cats_sorted":[],"title_canon_sha256":"eb47d4a7bc004078bf597145f753f13c776927bea367741e4875bc6c8497301f","abstract_canon_sha256":"6a5521320269578037307580030aed997c894fb9126e5bd02fcc9fb7428ecc86"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:52:37.701336Z","signature_b64":"UniQl5sjOTDljjR2PKoSsSB9aX16a/THn3Zsy7D3eRbhvwghiwQzuedKzuenmOgUysmzQtargTkTPzWrTDYnCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ecd15edcc69b0b8afa2972eff6df199e2d2b4f9aa29234205c4928e1693bbc4a","last_reissued_at":"2026-05-18T00:52:37.700733Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:52:37.700733Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Pan-Pacific Planet Search VI: Giant planets orbiting HD 86950 and HD 222076","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"C.G. 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