{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:KPCDQPM3RXTGV235W3MUDCXHTP","short_pith_number":"pith:KPCDQPM3","schema_version":"1.0","canonical_sha256":"53c4383d9b8de66aeb7db6d9418ae79be9c58a28ed12965a69eeeaa837a253bd","source":{"kind":"arxiv","id":"1702.05158","version":1},"attestation_state":"computed","paper":{"title":"Search for exoplanets around pulsating stars of A--F type in Kepler Short Cadence data and the case of KIC 8197761","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"Bart{\\l}omiej D\\k{e}bski, David Jones, Gerald Handler, Marie Van de Sande, Paulina Sowicka, P\\'eter I. P\\'apics","submitted_at":"2017-02-16T21:15:31Z","abstract_excerpt":"We searched for extrasolar planets around pulsating stars by examining $\\textit{Kepler}$ data for transit-like events hidden in the intrinsic variability. All Short Cadence observations for targets with 6000 K $< T_{\\rm eff} <$ 8500 K were visually inspected for transit-like events following the removal of pulsational signals by sinusoidal fits. Clear transit-like events were detected in KIC 5613330 and KIC 8197761. KIC 5613330 is a confirmed exoplanet host (Kepler-635b), where the transit period determined here is consistent with the literature value. KIC 8197761 is a $\\gamma$ Doradus - $\\del"},"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":"1702.05158","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-02-16T21:15:31Z","cross_cats_sorted":["astro-ph.EP"],"title_canon_sha256":"9e8997582afbd501ef496fca452da792eb7b930bd7558a85f1cd29d7e580183c","abstract_canon_sha256":"751b8f2c20c5435d92c324d312f926d0ea5c8dc8d1d886a5e460422afc0f4416"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:47:45.807543Z","signature_b64":"s8Q09ZUpL4RQj7CS2V9CvnaxJkfQhcEGZRGaikx1r3Br3VGWMGsqOsE6vDOeFl4dfv3MoIbTB4NZxxCnE3LwAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"53c4383d9b8de66aeb7db6d9418ae79be9c58a28ed12965a69eeeaa837a253bd","last_reissued_at":"2026-05-18T00:47:45.806881Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:47:45.806881Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Search for exoplanets around pulsating stars of A--F type in Kepler Short Cadence data and the case of KIC 8197761","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"Bart{\\l}omiej D\\k{e}bski, David Jones, Gerald Handler, Marie Van de Sande, Paulina Sowicka, P\\'eter I. P\\'apics","submitted_at":"2017-02-16T21:15:31Z","abstract_excerpt":"We searched for extrasolar planets around pulsating stars by examining $\\textit{Kepler}$ data for transit-like events hidden in the intrinsic variability. All Short Cadence observations for targets with 6000 K $< T_{\\rm eff} <$ 8500 K were visually inspected for transit-like events following the removal of pulsational signals by sinusoidal fits. Clear transit-like events were detected in KIC 5613330 and KIC 8197761. KIC 5613330 is a confirmed exoplanet host (Kepler-635b), where the transit period determined here is consistent with the literature value. KIC 8197761 is a $\\gamma$ Doradus - $\\del"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1702.05158","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":"1702.05158","created_at":"2026-05-18T00:47:45.806977+00:00"},{"alias_kind":"arxiv_version","alias_value":"1702.05158v1","created_at":"2026-05-18T00:47:45.806977+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1702.05158","created_at":"2026-05-18T00:47:45.806977+00:00"},{"alias_kind":"pith_short_12","alias_value":"KPCDQPM3RXTG","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_16","alias_value":"KPCDQPM3RXTGV235","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_8","alias_value":"KPCDQPM3","created_at":"2026-05-18T12:31:24.725408+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.18128","citing_title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","ref_index":56,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KPCDQPM3RXTGV235W3MUDCXHTP","json":"https://pith.science/pith/KPCDQPM3RXTGV235W3MUDCXHTP.json","graph_json":"https://pith.science/api/pith-number/KPCDQPM3RXTGV235W3MUDCXHTP/graph.json","events_json":"https://pith.science/api/pith-number/KPCDQPM3RXTGV235W3MUDCXHTP/events.json","paper":"https://pith.science/paper/KPCDQPM3"},"agent_actions":{"view_html":"https://pith.science/pith/KPCDQPM3RXTGV235W3MUDCXHTP","download_json":"https://pith.science/pith/KPCDQPM3RXTGV235W3MUDCXHTP.json","view_paper":"https://pith.science/paper/KPCDQPM3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1702.05158&json=true","fetch_graph":"https://pith.science/api/pith-number/KPCDQPM3RXTGV235W3MUDCXHTP/graph.json","fetch_events":"https://pith.science/api/pith-number/KPCDQPM3RXTGV235W3MUDCXHTP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KPCDQPM3RXTGV235W3MUDCXHTP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KPCDQPM3RXTGV235W3MUDCXHTP/action/storage_attestation","attest_author":"https://pith.science/pith/KPCDQPM3RXTGV235W3MUDCXHTP/action/author_attestation","sign_citation":"https://pith.science/pith/KPCDQPM3RXTGV235W3MUDCXHTP/action/citation_signature","submit_replication":"https://pith.science/pith/KPCDQPM3RXTGV235W3MUDCXHTP/action/replication_record"}},"created_at":"2026-05-18T00:47:45.806977+00:00","updated_at":"2026-05-18T00:47:45.806977+00:00"}