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We determine Li and Be abundances for this star and evaluate its radial velocity time series, activity cycle, and spectral energy distribution in search of clues regarding the origin of this enigmatic star. Methods. Li and Be abundances were determined via spectral synthesis of their resonance lines using HARPS and UVES spectra"},"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":"2411.15650","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2024-11-23T21:04:33Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"7d95e7a3b4b9e82409afc83c82229cab964f98140deab983146d72aedd5dcf8d","abstract_canon_sha256":"6eee3d522d5dcdbd57bb3d22cc73bb72ea17b55a3c8fda80e76a0f8a3d9a8e80"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:39:38.511741Z","signature_b64":"9WlQekDQPL+fmjS8Txa+uy9qCNK18oMsnIrh/R/UMTL7by29KmAK9BWfZ4Zh6qApfVN0vUKcW3n1U3PW9MU/AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"459cd2e19d5461658f0ffa2903013b1d1eff7ec1a20e81a645c964004bfed934","last_reissued_at":"2026-07-05T09:39:38.511266Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:39:38.511266Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Beryllium: The smoking gun of a rejuvenated star","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Amanda I. 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