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We analyzed the TESS light curves, finding that the previously determined frequency is a Nyquist alias. The revised pulsation frequency is $191.5151 \\pm 0.0005$d$^{-1}$ ($P = 7.52$min) and the rotation frequency is $0.32229 \\pm 0.00005$d$^{-1}$ ($P_{\\rm rot} = 3.1028$d). The star is an oblique pulsator with pulsation amplitude modulated by the rotation, reaching pulsat"},"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":"2008.05619","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2020-08-13T00:21:13Z","cross_cats_sorted":[],"title_canon_sha256":"73fcae8c0536efd6e25e188e68be51a2de5c82e0924a04f181e07166791d2460","abstract_canon_sha256":"124d6062cb496179785599ffb815d206d2460320677e93a4334546c0d281a72e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:26:55.259434Z","signature_b64":"6gLTMYMCmIEJDFjMm0ZKMqtJMlF6U8BwA4VSlNnyC8flLp6Hry2g4ZwXB9FiO44S5M3rQhoxMIeqlayr7iVEBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"34d11fffc7be99c179957c5be3a5e7b8c79b57d1a3ff64d228f0aef0fa7bd57f","last_reissued_at":"2026-07-05T01:26:55.259018Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:26:55.259018Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Pulsations of the roAp star KIC 10685175 revisited by TESS","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Donald Kurtz, Fangfei Shi, Hideyuki Saio, Huawei Zhang, Jianning Fu","submitted_at":"2020-08-13T00:21:13Z","abstract_excerpt":"KIC 10685175 (TIC 264509538) was discovered to be a rapidly oscillating Ap star from {\\it Kepler} long cadence data using super-Nyquist frequency analysis. 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