{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:2HLBVIOPG775SRZHFNCVGJE4OW","short_pith_number":"pith:2HLBVIOP","schema_version":"1.0","canonical_sha256":"d1d61aa1cf37ffd947272b4553249c75a4d61b56a27ea6e2eefad17cdf5e4908","source":{"kind":"arxiv","id":"1306.1819","version":1},"attestation_state":"computed","paper":{"title":"KIC 4544587: an Eccentric, Short Period Binary System with delta Sct Pulsations and Tidally Excited Modes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Prsa, D. W. Kurtz, J. A. Guzik, J. Fuller, J. Southworth, K. Conroy, K. M. Hambleton, K. Pavlovski, S. Bloemen, S. P. Littlefair","submitted_at":"2013-06-07T19:50:44Z","abstract_excerpt":"We present Kepler photometry and ground based spectroscopy of KIC 4544587, a short-period eccentric eclipsing binary system with self-excited pressure and gravity modes, tidally excited modes, tidally influenced p modes, and rapid apsidal motion of 182 y per cycle. The primary and secondary components of KIC 4544587 reside within the delta Scuti and gamma Dor instability region of the Hurtzsprung-Russell diagram, respectively. By applying the binary modelling software PHOEBE to prewhitened Kepler photometric data and radial velocity data obtained using the William Herschel Telescope and 4-m Ma"},"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":"1306.1819","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-06-07T19:50:44Z","cross_cats_sorted":[],"title_canon_sha256":"270b300c60e57446ea7f77a8858fee7b34efed0a7dce0f1c93fce26a89a3ab9c","abstract_canon_sha256":"5356bf9e27841522a0445e2d1116527d9e80c7b52ad73866fb4cbde45f4362a7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:49:24.824007Z","signature_b64":"Yx/mu51qFGSVWcJl1CZ/+krD/PYTRf8CYIdexXgesLbtSEwcYddq9TE7d2wavl7sYasJ1OZF5misLl0Ah4FMBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d1d61aa1cf37ffd947272b4553249c75a4d61b56a27ea6e2eefad17cdf5e4908","last_reissued_at":"2026-05-18T01:49:24.823376Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:49:24.823376Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"KIC 4544587: an Eccentric, Short Period Binary System with delta Sct Pulsations and Tidally Excited Modes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Prsa, D. W. Kurtz, J. A. Guzik, J. Fuller, J. Southworth, K. Conroy, K. M. Hambleton, K. Pavlovski, S. Bloemen, S. P. Littlefair","submitted_at":"2013-06-07T19:50:44Z","abstract_excerpt":"We present Kepler photometry and ground based spectroscopy of KIC 4544587, a short-period eccentric eclipsing binary system with self-excited pressure and gravity modes, tidally excited modes, tidally influenced p modes, and rapid apsidal motion of 182 y per cycle. The primary and secondary components of KIC 4544587 reside within the delta Scuti and gamma Dor instability region of the Hurtzsprung-Russell diagram, respectively. By applying the binary modelling software PHOEBE to prewhitened Kepler photometric data and radial velocity data obtained using the William Herschel Telescope and 4-m Ma"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1306.1819","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":"1306.1819","created_at":"2026-05-18T01:49:24.823485+00:00"},{"alias_kind":"arxiv_version","alias_value":"1306.1819v1","created_at":"2026-05-18T01:49:24.823485+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1306.1819","created_at":"2026-05-18T01:49:24.823485+00:00"},{"alias_kind":"pith_short_12","alias_value":"2HLBVIOPG775","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_16","alias_value":"2HLBVIOPG775SRZH","created_at":"2026-05-18T12:27:30.460161+00:00"},{"alias_kind":"pith_short_8","alias_value":"2HLBVIOP","created_at":"2026-05-18T12:27:30.460161+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":93,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2HLBVIOPG775SRZHFNCVGJE4OW","json":"https://pith.science/pith/2HLBVIOPG775SRZHFNCVGJE4OW.json","graph_json":"https://pith.science/api/pith-number/2HLBVIOPG775SRZHFNCVGJE4OW/graph.json","events_json":"https://pith.science/api/pith-number/2HLBVIOPG775SRZHFNCVGJE4OW/events.json","paper":"https://pith.science/paper/2HLBVIOP"},"agent_actions":{"view_html":"https://pith.science/pith/2HLBVIOPG775SRZHFNCVGJE4OW","download_json":"https://pith.science/pith/2HLBVIOPG775SRZHFNCVGJE4OW.json","view_paper":"https://pith.science/paper/2HLBVIOP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1306.1819&json=true","fetch_graph":"https://pith.science/api/pith-number/2HLBVIOPG775SRZHFNCVGJE4OW/graph.json","fetch_events":"https://pith.science/api/pith-number/2HLBVIOPG775SRZHFNCVGJE4OW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2HLBVIOPG775SRZHFNCVGJE4OW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2HLBVIOPG775SRZHFNCVGJE4OW/action/storage_attestation","attest_author":"https://pith.science/pith/2HLBVIOPG775SRZHFNCVGJE4OW/action/author_attestation","sign_citation":"https://pith.science/pith/2HLBVIOPG775SRZHFNCVGJE4OW/action/citation_signature","submit_replication":"https://pith.science/pith/2HLBVIOPG775SRZHFNCVGJE4OW/action/replication_record"}},"created_at":"2026-05-18T01:49:24.823485+00:00","updated_at":"2026-05-18T01:49:24.823485+00:00"}