{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:FX4OXI7HPESEUUPZBLAAOGETZC","short_pith_number":"pith:FX4OXI7H","schema_version":"1.0","canonical_sha256":"2df8eba3e779244a51f90ac0071893c895d203e99fcc1a551db88f5e684f76e3","source":{"kind":"arxiv","id":"1403.5860","version":1},"attestation_state":"computed","paper":{"title":"Why is there a Dearth of Close-In Planets around Fast-Rotating stars?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Arieh K\\\"onigl, Seth Teitler","submitted_at":"2014-03-24T05:51:38Z","abstract_excerpt":"We propose that the reported dearth of $Kepler$ Objects of Interest (KOIs) with orbital periods $P_{\\rm orb} \\lesssim 2-3\\;$days around stars with rotation periods $P_{\\rm rot} \\lesssim 5-10\\;$days can be attributed to tidal ingestion of close-in planets by their host stars. We show that the planet distribution in this region of the $\\log{P_{\\rm orb}}-\\log{P_{\\rm rot}}$ plane is qualitatively reproduced with a model that incorporates tidal interaction and magnetic braking as well as the dependence on the stellar core--envelope coupling timescale. We demonstrate the consistency of this scenario"},"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":"1403.5860","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2014-03-24T05:51:38Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"2d2e782830772d773ccd99a4598023ce5a712bfe4de2585fbd6f0228ccad2014","abstract_canon_sha256":"1042f8e77014da7b68338175e1704df68ff687145577196646a3630200c4b395"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:52.024589Z","signature_b64":"R3BRFhBeDqq56w5tp/0CIuZpoVBNUvnuD68LraCN0Vf6lnv0aNIaQvGNIyRsaBwMQkcEbRbG4HFkPr42NJ5QAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2df8eba3e779244a51f90ac0071893c895d203e99fcc1a551db88f5e684f76e3","last_reissued_at":"2026-05-18T01:43:52.023812Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:52.023812Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Why is there a Dearth of Close-In Planets around Fast-Rotating stars?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Arieh K\\\"onigl, Seth Teitler","submitted_at":"2014-03-24T05:51:38Z","abstract_excerpt":"We propose that the reported dearth of $Kepler$ Objects of Interest (KOIs) with orbital periods $P_{\\rm orb} \\lesssim 2-3\\;$days around stars with rotation periods $P_{\\rm rot} \\lesssim 5-10\\;$days can be attributed to tidal ingestion of close-in planets by their host stars. We show that the planet distribution in this region of the $\\log{P_{\\rm orb}}-\\log{P_{\\rm rot}}$ plane is qualitatively reproduced with a model that incorporates tidal interaction and magnetic braking as well as the dependence on the stellar core--envelope coupling timescale. We demonstrate the consistency of this scenario"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.5860","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":"1403.5860","created_at":"2026-05-18T01:43:52.023932+00:00"},{"alias_kind":"arxiv_version","alias_value":"1403.5860v1","created_at":"2026-05-18T01:43:52.023932+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1403.5860","created_at":"2026-05-18T01:43:52.023932+00:00"},{"alias_kind":"pith_short_12","alias_value":"FX4OXI7HPESE","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_16","alias_value":"FX4OXI7HPESEUUPZ","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_8","alias_value":"FX4OXI7H","created_at":"2026-05-18T12:28:28.263976+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FX4OXI7HPESEUUPZBLAAOGETZC","json":"https://pith.science/pith/FX4OXI7HPESEUUPZBLAAOGETZC.json","graph_json":"https://pith.science/api/pith-number/FX4OXI7HPESEUUPZBLAAOGETZC/graph.json","events_json":"https://pith.science/api/pith-number/FX4OXI7HPESEUUPZBLAAOGETZC/events.json","paper":"https://pith.science/paper/FX4OXI7H"},"agent_actions":{"view_html":"https://pith.science/pith/FX4OXI7HPESEUUPZBLAAOGETZC","download_json":"https://pith.science/pith/FX4OXI7HPESEUUPZBLAAOGETZC.json","view_paper":"https://pith.science/paper/FX4OXI7H","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1403.5860&json=true","fetch_graph":"https://pith.science/api/pith-number/FX4OXI7HPESEUUPZBLAAOGETZC/graph.json","fetch_events":"https://pith.science/api/pith-number/FX4OXI7HPESEUUPZBLAAOGETZC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FX4OXI7HPESEUUPZBLAAOGETZC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FX4OXI7HPESEUUPZBLAAOGETZC/action/storage_attestation","attest_author":"https://pith.science/pith/FX4OXI7HPESEUUPZBLAAOGETZC/action/author_attestation","sign_citation":"https://pith.science/pith/FX4OXI7HPESEUUPZBLAAOGETZC/action/citation_signature","submit_replication":"https://pith.science/pith/FX4OXI7HPESEUUPZBLAAOGETZC/action/replication_record"}},"created_at":"2026-05-18T01:43:52.023932+00:00","updated_at":"2026-05-18T01:43:52.023932+00:00"}