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Combined with a stellar rotation period of $23.47\\pm0.29$ days measured with photometry from the Tierras Observatory, this yields a stellar inclination of $90^{\\circ} \\pm 13^{\\circ}$ and a true obliquity $\\psi = 15.6$$^\\circ$$^{+7.7^\\circ}_{-7.3^\\circ}$, indicating that "},"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":"2505.03628","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2025-05-06T15:28:08Z","cross_cats_sorted":[],"title_canon_sha256":"ec746cb31faf4941c95923cf51215d053341311ec1e4e7a9fa4af090a0cf7e5a","abstract_canon_sha256":"fb83865b8445d24bf2204f9a8401689d517dae5dafb10cea3645b6ecb497012d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:59:19.584085Z","signature_b64":"SVM4Dqnm6mHx7Nfaw5z2r93zX3ILJDDyOz939RWsXqgqGtR4qkVtuNfVEOEuxUnj74AWTmsKSwTkGGFlL/LaDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0724c995c5088b3f8e7ad29fe27678d8ef9073b629284dc3b8b4b91fc4923cc5","last_reissued_at":"2026-07-05T10:59:19.583528Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:59:19.583528Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The True Stellar Obliquity of a Sub-Saturn Planet from the Tierras Observatory and KPF","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Aaron Householder, Allyson Bieryla, Andrew W. 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