{"as_of":"2026-08-10T14:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bf742033885b1b3f54f6a02a8b72cc224159e00f6893188f72de124a74747096","coverage":[{"denominator":115,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T14:45:20.337478Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2507.18128/citation-record","integrity":"/paper/2507.18128/integrity","json":"/paper/2507.18128/citation-record.json","paper":"/paper/2507.18128"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.056474Z","title":"Asteroseismology; 2010","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.056474Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:4218440703e1b35a8d79c4aeffd41fb612db950882f14a90dbff6cde02d7d26f","observation_id":"ab79478b-4443-41c7-bf33-ca42068ed7d8","resolution":{"observed_at":"2026-08-06T14:45:20.056474Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.059809Z","title":"Asteroseismology Across the Hertzsprung-Russell Diagram","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.059809Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:e961a724a21c84e99a1ff203d07906a51bfa9d846b3ac8df4e2371e46f47b9c5","observation_id":"dd39a893-5be8-40a5-b047-92b00f1844e4","resolution":{"observed_at":"2026-08-06T14:45:20.059809Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.0335","last_updated":"2011-08-31T17:10:41Z","snapshot_observed_at":"2026-08-07T13:59:36.658844Z","submitted_at":"2011-07-01T20:54:15Z","title":"The Kepler characterization of the variability among A- and F-type stars. I. General overview","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1107.0335","snapshot_observed_at":"2026-08-06T14:45:20.064272Z","title":"The Kepler characterization of the variability among A- and F-type stars","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.064272Z"},"links":{"cited_paper":"/paper/1107.0335","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:0dadf10e55f89729268bc1c4675198ff072e3ca0993615d2ef30fad87b4e0b6d","observation_id":"3789b493-f3e2-4a77-87af-5641902cd6b6","resolution":{"observed_at":"2026-08-06T14:45:20.064272Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stt1981","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Low frequencies in Kepler δ Scuti stars","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"fe324da3-cc05-405b-a49d-6fb9420b45a3","year":2014},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.070170Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:3215fa3387dd4d904a6fcea0f3b5325d84f2cde2651d0d57a3c9ca5e4451a287","observation_id":"864d7e6a-8b76-4a09-a604-8320031728e6","resolution":{"observed_at":"2026-08-06T14:45:20.580466Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1505.07216","last_updated":"2015-05-27T08:17:32Z","snapshot_observed_at":"2026-07-06T04:19:02.060352Z","submitted_at":"2015-05-27T08:17:32Z","title":"Pulsation frequency distribution in Delta Scuti stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.07216","snapshot_observed_at":"2026-08-06T14:45:20.073132Z","title":"Pulsation frequency distribution inδ Scuti stars","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.073132Z"},"links":{"cited_paper":"/paper/1505.07216","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:5fb00611dde4278d89e67aa689bfa999c785d9cdce0c028469f5d476df022e10","observation_id":"f5c7090f-8d45-4589-bd6c-92599d92b0fe","resolution":{"observed_at":"2026-08-06T14:45:20.073132Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.076602Z","title":"Convection-pulsation coupling","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.076602Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:a0e08100e7752fe795b171be2a854892405ee062b1abc214fd1b7e69700455e3","observation_id":"1bc1c779-3101-4615-a9dc-ae50256cc24d","resolution":{"observed_at":"2026-08-06T14:45:20.076602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.079408Z","title":"The MOST Asteroseismology Mission: Ultraprecise Photometry from Space","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.079408Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:ee08da7eee5be0362dbcd5a53148201fa7b89a0fe2e1dbef3555b98181d24b14","observation_id":"6a041643-3445-4b25-9686-6f2c118ec922","resolution":{"observed_at":"2026-08-06T14:45:20.079408Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.2206","last_updated":"2009-01-15T14:08:26Z","snapshot_observed_at":"2026-07-06T01:50:46.078469Z","submitted_at":"2009-01-15T14:08:26Z","title":"The CoRoT satellite in flight : description and performance","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.2206","snapshot_observed_at":"2026-08-06T14:45:20.081974Z","title":"The CoRoT satellite in flight: description and performance","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.081974Z"},"links":{"cited_paper":"/paper/0901.2206","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:aa98cdc197cd8c622558d44ebb53e94a96ef4ba25f95b116307ba6f5af3a43b9","observation_id":"ee3678f4-665a-41d5-8a97-3a2e151378a9","resolution":{"observed_at":"2026-08-06T14:45:20.081974Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.085200Z","title":"Kepler Planet-Detection Mission: Introduction and First Results","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.085200Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:2ea0ed2ff9fb98794d25a0ee9198e59678f2c2119864e3930788a0de7ed34314","observation_id":"82193842-4019-478f-a6f6-be1b06e5b5f9","resolution":{"observed_at":"2026-08-06T14:45:20.085200Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.087947Z","title":"Transiting Exoplanet Survey Satellite (TESS)","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.087947Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:3fc15f60cb5081ef134511b1a60f57760acfaa9df6d53eca5e64c69cee8242f5","observation_id":"76356097-cc38-4ed5-ab83-a50dec2d4c7b","resolution":{"observed_at":"2026-08-06T14:45:20.087947Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.090482Z","title":"Asteroseismic inferences from the study of non-linearities in Delta Sct stars","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.090482Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:9b2ecabf4a6ee527cf15742e8d01cc13a50f62dfe2a1be81c9083b04e8d701d6","observation_id":"d3298a4f-782d-4582-85a6-33edf0d9c14a","resolution":{"observed_at":"2026-08-06T14:45:20.090482Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac86c9","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"KIC 2857323: A Double-mode High-amplitudeδ Scuti Star with Amplitude Decline of the First Overtone Mode","venue":"The Astrophysical Journal","work_id":"c1030491-cda0-4575-9b83-1e8d7af1b91d","year":2022},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.093272Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:bebd7c4de19a07b306a4b74080f7a9eba5bf3883050a90e302caf205d12d20b0","observation_id":"3486878e-47e2-411b-b24f-d54387031421","resolution":{"observed_at":"2026-08-06T14:45:20.545715Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.05831","last_updated":"2023-10-09T16:19:29Z","snapshot_observed_at":"2026-07-06T16:29:55.892584Z","submitted_at":"2023-10-09T16:19:29Z","title":"Unveiling the Intricate Symphony of Nonlinear Pulsation Mode Interactions in High-Amplitude $\\delta$ Scuti Stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.05831","snapshot_observed_at":"2026-08-06T14:45:20.095838Z","title":"Unveiling the intricate symphony of nonlinear pulsation mode interactions in high-amplitude δ Scuti stars","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.095838Z"},"links":{"cited_paper":"/paper/2310.05831","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:3ac0e27d2144ad3d58018cd6599e2c35801aec8108891c8e63666690c82d2f2d","observation_id":"97b8dff4-d676-4c27-b0b3-6b7510cdfb0f","resolution":{"observed_at":"2026-08-06T14:45:20.095838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.5603","last_updated":"2012-12-21T21:00:01Z","snapshot_observed_at":"2026-07-06T03:02:40.338020Z","submitted_at":"2012-12-21T21:00:01Z","title":"Super-Nyquist asteroseismology with the Kepler Space Telescope","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.5603","snapshot_observed_at":"2026-08-06T14:45:20.098953Z","title":"Super-Nyquist asteroseismology with the Kepler Space Telescope","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.098953Z"},"links":{"cited_paper":"/paper/1212.5603","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:37d2c20d7264bf826d0182d3ba21f2769f993f29ba19d2d4e64f56f041b4c3a8","observation_id":"3b820c99-a09c-4e4f-b11a-b4861d27650d","resolution":{"observed_at":"2026-08-06T14:45:20.098953Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.02717","last_updated":"2015-08-11T20:06:46Z","snapshot_observed_at":"2026-07-06T04:26:27.164004Z","submitted_at":"2015-08-11T20:06:46Z","title":"The potential for super-Nyquist asteroseismology with TESS","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.02717","snapshot_observed_at":"2026-08-06T14:45:20.102437Z","title":"The potential for super-Nyquist asteroseismology with TESS","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.102437Z"},"links":{"cited_paper":"/paper/1508.02717","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:8bd7894122cbe1b4e5b3c255e9e0cc5febda41df182052b84f503f920f0fcb1f","observation_id":"cbb22989-899f-45b0-9e5a-0a36c627c102","resolution":{"observed_at":"2026-08-06T14:45:20.102437Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.03955","last_updated":"2016-05-12T19:56:24Z","snapshot_observed_at":"2026-08-10T09:46:22.818791Z","submitted_at":"2016-05-12T19:56:24Z","title":"Amplitude modulation in $\\delta$ Sct stars: statistics from an ensemble study of Kepler targets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.03955","snapshot_observed_at":"2026-08-06T14:45:20.105233Z","title":"Amplitude modulation in δ Sct stars: statistics from an ensemble study of Kepler targets","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.105233Z"},"links":{"cited_paper":"/paper/1605.03955","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:bb3681c0c5d795fa1bc521a1a3aa7a3ba8f00434768cde2a7de14e8ef93a1c11","observation_id":"65508713-8d4f-4c27-babb-768633051125","resolution":{"observed_at":"2026-08-06T14:45:20.105233Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.04713","last_updated":"2021-03-08T12:41:51Z","snapshot_observed_at":"2026-08-07T17:17:02.405572Z","submitted_at":"2021-03-08T12:41:51Z","title":"Amplitude and frequency modulation of super-Nyquist frequency from Kepler photometric sampling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.04713","snapshot_observed_at":"2026-08-06T14:45:20.107845Z","title":"Amplitude and Frequency Modulation of Super-Nyquist Frequency from Kepler Photometric Sampling","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.107845Z"},"links":{"cited_paper":"/paper/2103.04713","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:b1d621d3856fc2d86864287076dd2a359df9144bef770ab9663c584e2cc4f86e","observation_id":"8ba7dd85-2bdb-4a3f-9a45-f534ae67783a","resolution":{"observed_at":"2026-08-06T14:45:20.107845Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.12481","last_updated":"2024-11-19T13:03:16Z","snapshot_observed_at":"2026-07-06T19:52:33.374340Z","submitted_at":"2024-11-19T13:03:16Z","title":"Distinguishing super-Nyquist frequencies via their temporal variation in $\\gamma$ Doradus stars from continuous photometry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.12481","snapshot_observed_at":"2026-08-06T14:45:20.110562Z","title":"Distinguishing super-Nyquist frequencies via their temporal varia- tion in γ Doradus stars from continuous photometry","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.110562Z"},"links":{"cited_paper":"/paper/2411.12481","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:4e4a1e5159eeef85292f397d4ce42b00419abffb97316f1e29c2cee0caa4bdf4","observation_id":"b4a309f8-c0a2-4c48-9e99-b0f35100703d","resolution":{"observed_at":"2026-08-06T14:45:20.110562Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.113524Z","title":"Kepler Instrument Handbook","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.113524Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:4a3ec83cc613d38990ad835dc1e0b4aba1b5a7a9bd9787a38b689d6929633c90","observation_id":"d0f7fadc-b5fa-4fe9-9476-d509bf2924f2","resolution":{"observed_at":"2026-08-06T14:45:20.113524Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.0142","last_updated":"2009-12-31T14:37:23Z","snapshot_observed_at":"2026-07-31T17:01:33.330335Z","submitted_at":"2009-12-31T14:37:23Z","title":"Initial Characteristics of Kepler Short Cadence Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.0142","snapshot_observed_at":"2026-08-06T14:45:20.115974Z","title":"Initial Characteristics of Kepler Short Cadence Data","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.115974Z"},"links":{"cited_paper":"/paper/1001.0142","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:762a77cb79e755bf06ccc2378c6d92917a12392febc2cfb372bb1f0fe6161ab5","observation_id":"f9384f84-38ee-43cb-bdc0-402a2d672e12","resolution":{"observed_at":"2026-08-06T14:45:20.115974Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.118498Z","title":"KIC 10975348: A Double-mode or Triple-mode High-amplitude δ Scuti Star? The Astronomical Journal 2021, 161, 27, [arXiv:astro-ph.SR/2011.09091]","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.118498Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:00e9e084fd4dc78aa708e346a6f4ba38757e8818975fed67f519940290a8c8b6","observation_id":"4ceb1e94-c0c0-46d7-b851-74a98faab3b5","resolution":{"observed_at":"2026-08-06T14:45:20.118498Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.05283","last_updated":"2022-08-10T11:32:18Z","snapshot_observed_at":"2026-08-04T10:01:05.366786Z","submitted_at":"2022-08-10T11:32:18Z","title":"KIC 10417986: Spectroscopic confirmation of the nature of the binary system with a {\\delta} Scuti component","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.05283","snapshot_observed_at":"2026-08-06T14:45:20.121321Z","title":"KIC 10417986: Spectroscopic Confirmation of the Nature of the Binary System with a δ Scuti Component","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.121321Z"},"links":{"cited_paper":"/paper/2208.05283","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:4758369d4bf9ed16062b65fe4513013a1521b500fddf622adcdc39bd9dd3642b","observation_id":"435f639b-bd3f-4814-bb94-90297268a1f9","resolution":{"observed_at":"2026-08-06T14:45:20.121321Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.11060","last_updated":"2024-06-16T20:24:36Z","snapshot_observed_at":"2026-07-06T18:31:49.437336Z","submitted_at":"2024-06-16T20:24:36Z","title":"Asteroseismology of the fast-rotating high-amplitude $\\delta$ Scuti star V2367 Cygni","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.11060","snapshot_observed_at":"2026-08-06T14:45:20.125025Z","title":"Asteroseismology of the fast-rotating high-amplitude δ Scuti star V2367 Cygni","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.125025Z"},"links":{"cited_paper":"/paper/2406.11060","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:2981d378921670cd89c72bb286a8457badac6840450c8b2aca5652c6bcaab1be","observation_id":"6ffe18c8-59eb-4a2d-990f-d967a054ffda","resolution":{"observed_at":"2026-08-06T14:45:20.125025Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/staa2207","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Linear and non-linear tidal oscillations and mode identification in the eccentric binary system KIC 3858884","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"79c73a32-d39b-4694-8add-a9dbcb9ba4d8","year":2020},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.127624Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:436ec035c44e30b02089e18fe1b53728b801577912fe1e314bf6bd2ba964827f","observation_id":"555b71db-669b-45b4-b0d2-71a01505f9d3","resolution":{"observed_at":"2026-08-06T14:45:20.537025Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.00126","last_updated":"2024-08-06T15:42:44Z","snapshot_observed_at":"2026-08-10T13:01:05.162484Z","submitted_at":"2024-07-31T19:29:16Z","title":"Characterization of the $\\delta$ Scuti eclipsing binary KIC 4851217 and its tertiary companion as well as detection of tidally tilted pulsations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.00126","snapshot_observed_at":"2026-08-06T14:45:20.130370Z","title":"Characterization of the δ Scuti eclipsing binary KIC 4851217 and its tertiary companion as well as detection of tidally tilted pulsations","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.130370Z"},"links":{"cited_paper":"/paper/2408.00126","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:f322e2925e4c6d81bc5def7b79a6e79f015a211f91b816b3adb1b04d767eb2b9","observation_id":"55cebfb4-12e7-4ec8-b0ae-3c0c2214e766","resolution":{"observed_at":"2026-08-06T14:45:20.130370Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.06118","last_updated":"2024-08-12T12:59:54Z","snapshot_observed_at":"2026-08-10T08:42:20.867253Z","submitted_at":"2024-08-12T12:59:54Z","title":"Analysis of KIC 7023917 -- spotted low-mass ratio eclipsing binary with $\\delta$ Scuti pulsations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.06118","snapshot_observed_at":"2026-08-06T14:45:20.133168Z","title":"Analysis of KIC 7023917: Spotted Low-mass Ratio Eclipsing Binary with δ Scuti Pulsations","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.133168Z"},"links":{"cited_paper":"/paper/2408.06118","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:37a56c7bacd5346a4e454fa1c6bda23c262fe84b8e045d610f588c2847416079","observation_id":"3f780554-c09c-42eb-ab1c-566b46890c6d","resolution":{"observed_at":"2026-08-06T14:45:20.133168Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.06773","last_updated":"2019-08-19T12:57:08Z","snapshot_observed_at":"2026-08-07T16:00:00.504355Z","submitted_at":"2019-08-19T12:57:08Z","title":"Systematic search for stellar pulsators in the eclipsing binaries observed by Kepler","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.06773","snapshot_observed_at":"2026-08-06T14:45:20.138625Z","title":"Systematic search for stellar pulsators in the eclipsing binaries observed by Kepler","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.138625Z"},"links":{"cited_paper":"/paper/1908.06773","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:a1b696832c28ccf6dcc2ef46f59241339ecf15bf6bceef99efe92a36e0796292","observation_id":"9296deee-3574-4738-973d-203b0c7d580f","resolution":{"observed_at":"2026-08-06T14:45:20.138625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.00763","last_updated":"2024-10-01T15:00:29Z","snapshot_observed_at":"2026-07-06T19:25:19.661028Z","submitted_at":"2024-10-01T15:00:29Z","title":"The catalogue of $\\delta$ Sct pulsators in binary systems in 2024","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.00763","snapshot_observed_at":"2026-08-06T14:45:20.141427Z","title":"A catalogue of δ Sct pulsators in binary systems in 2024","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.141427Z"},"links":{"cited_paper":"/paper/2410.00763","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:01b88e5794dc92f8e9ffa54f882e4defb1576ff655e49117fc747ac2766c2830","observation_id":"59002d01-41e6-465e-8def-9c512cd6d7a8","resolution":{"observed_at":"2026-08-06T14:45:20.141427Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.144473Z","title":"Nonradial pulsation of the unevolved hot δ Scuti star CD-24 7599 discovered with the Whole Earth Telescope","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.144473Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:f4f8074c285756df7b0d658dac736ef026dd48636b47fb33bdfa12c91d3bc3b3","observation_id":"a7fd0045-9450-4845-a9af-3bfdf993383c","resolution":{"observed_at":"2026-08-06T14:45:20.144473Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.146936Z","title":"δ Scuti pulsations in β Pictoris","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.146936Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:21ad70201b8eca2a18f647a06e076059d558a9397550b4ca0231eba20c31b137","observation_id":"b3ac2baa-73b7-479d-b716-a8285a518245","resolution":{"observed_at":"2026-08-06T14:45:20.146936Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.1383","last_updated":"2012-03-07T05:35:37Z","snapshot_observed_at":"2026-08-02T10:31:52.545012Z","submitted_at":"2012-03-07T05:35:37Z","title":"Kepler Presearch Data Conditioning II - A Bayesian Approach to Systematic Error Correction","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.1383","snapshot_observed_at":"2026-08-06T14:45:20.149548Z","title":"Kepler Presearch Data Conditioning II - A Bayesian Approach to Systematic Error Correction","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.149548Z"},"links":{"cited_paper":"/paper/1203.1383","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:ba352bc67feb6a216926dd70b26b19310ed707f605a63122135c2e5f02979673","observation_id":"8f7db658-fbc1-4067-8fde-227e73bacc10","resolution":{"observed_at":"2026-08-06T14:45:20.149548Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.152531Z","title":"Lightkurve: Kepler and TESS time series analysis in Python","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.152531Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:06692f53b2e1653d3266a3565b9ae659da9e15c38db9ad3ed60ccea53829165e","observation_id":"2aab845b-c4af-499c-8a4a-42dbc90d3dc0","resolution":{"observed_at":"2026-08-06T14:45:20.152531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.16018","last_updated":"2024-02-25T07:35:02Z","snapshot_observed_at":"2026-07-06T17:35:06.195492Z","submitted_at":"2024-02-25T07:35:02Z","title":"Flares hunting in hot subdwarf and white dwarf stars from Cycles 1-5 of TESS photometry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.16018","snapshot_observed_at":"2026-08-06T14:45:20.154882Z","title":"Flare Hunting in Hot Subdwarf and White Dwarf Stars from Cycles 1–5 of TESS Photometry","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.154882Z"},"links":{"cited_paper":"/paper/2402.16018","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:a0d9f3866666155762e17adddca8dc05e1596e47307f15addf4656382e518f52","observation_id":"ed253e2a-f133-4334-a783-5e640f830739","resolution":{"observed_at":"2026-08-06T14:45:20.154882Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.00966","last_updated":"2019-08-07T17:50:27Z","snapshot_observed_at":"2026-07-06T07:57:34.683633Z","submitted_at":"2019-06-03T18:00:00Z","title":"Wotan: Comprehensive time-series de-trending in Python","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.00966","snapshot_observed_at":"2026-08-06T14:45:20.157810Z","title":"W¯otan: Comprehensive Time-series Detrending in Python","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.157810Z"},"links":{"cited_paper":"/paper/1906.00966","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:0522296f6575e0491e090cb02c5336eb80767d662ff60fcb21420c5f59eff895","observation_id":"ea2bdbc6-1d8b-4824-910d-932bfaedfde6","resolution":{"observed_at":"2026-08-06T14:45:20.157810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac8c30","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"KIC 3440495: A Rapidly Rotating δ Scuti-γ Doradus Hybrid Pulsator in a Binary System","venue":"The Astrophysical Journal","work_id":"5e6e9a58-4fd3-4ea4-9f18-48a9add43466","year":2022},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.160453Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:055e8bdcd5e22dcfc5ce001133a52096633ce9e90078bd81901a68f455bac831","observation_id":"1395e15c-9736-4ea6-8014-f00af34909a4","resolution":{"observed_at":"2026-08-06T14:45:20.527491Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.03490","last_updated":"2019-04-06T16:43:45Z","snapshot_observed_at":"2026-07-30T20:37:16.012955Z","submitted_at":"2019-04-06T16:43:45Z","title":"Spectroscopic confirmation of the binary nature of the hybrid pulsator KIC 5709664 found with the frequency modulation method","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.03490","snapshot_observed_at":"2026-08-06T14:45:20.163100Z","title":"Spectroscopic confirmation of the binary nature of the hybrid pulsator KIC 5709664 found with the frequency modulation method","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.163100Z"},"links":{"cited_paper":"/paper/1904.03490","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:52885616cfac15fbb76f1f83300d63446d3fd8fd27699fe6da73e365023f4f09","observation_id":"977fb6af-a865-42e0-b449-64e0eda0babd","resolution":{"observed_at":"2026-08-06T14:45:20.163100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stz1033","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Two new R CMa-type eclipsing binaries containing a possible low-mass Helium white dwarf precursor: KIC 7368103 and KIC 8823397","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"4ecefd8e-e9de-4547-a49d-e1ef1c79a5d4","year":2019},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.166058Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:a3c2bc4b30e23ebe49d3148439af769ae665764034a165ba62c9d7e467f80466","observation_id":"9fb76a24-384d-423f-8a9d-ef2fbf3b340b","resolution":{"observed_at":"2026-08-06T14:45:20.519258Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.00367","last_updated":"2019-03-31T09:39:30Z","snapshot_observed_at":"2026-07-06T07:42:49.750708Z","submitted_at":"2019-03-31T09:39:30Z","title":"A study of Variability of the Marginal Am star HD 176843 observed in the Kepler field","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.00367","snapshot_observed_at":"2026-08-06T14:45:20.168634Z","title":"A study of variability of the marginal Am star HD 176843 observed in the Kepler field","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.168634Z"},"links":{"cited_paper":"/paper/1904.00367","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:4d78642876a6b245d6d20d9a0886b416fd67efd43bf2bb78262a0b6a8f4bab60","observation_id":"92012200-9fae-4786-bb63-68db56b90364","resolution":{"observed_at":"2026-08-06T14:45:20.168634Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.01801","last_updated":"2024-12-09T03:08:50Z","snapshot_observed_at":"2026-07-06T18:09:08.963593Z","submitted_at":"2024-05-03T01:16:29Z","title":"KIC 7914906: An Eclipsing Heartbeat Star with Tidally Excited Oscillations and Gamma Doradus/Delta Scuti Hybrid Pulsations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.01801","snapshot_observed_at":"2026-08-06T14:45:20.171423Z","title":"KIC 7914906: An eclipsing heartbeat star with tidally excited oscillations and gamma Doradus/delta Scuti hybrid pulsations","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.171423Z"},"links":{"cited_paper":"/paper/2405.01801","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:ac9cd4d4dfd21ae534a8efe8dffa81ad5b894e872cdeb3ca992a478cb0c9caa3","observation_id":"9729e76a-28df-4251-bfd4-3c61c7901b51","resolution":{"observed_at":"2026-08-06T14:45:20.171423Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.174041Z","title":"Pulsation modes of three Delta Scuti stars using Kepler project data: KIC3429637, KIC10451090, KIC2987660","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.174041Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:39a66d95ab8b4af17fb50380461df53b841e45f3b68f0f32a9df070ea6122ffa","observation_id":"039afe43-4982-4210-bbd9-f6f89cae3965","resolution":{"observed_at":"2026-08-06T14:45:20.174041Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.03908","last_updated":"2019-09-09T15:01:33Z","snapshot_observed_at":"2026-07-06T08:20:16.101101Z","submitted_at":"2019-09-09T15:01:33Z","title":"KIC 4142768: An Evolved Gamma Doradus/Delta Scuti Hybrid Pulsating Eclipsing Binary with Tidally Excited Oscillations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.03908","snapshot_observed_at":"2026-08-06T14:45:20.176665Z","title":"KIC 4142768: An Evolved Gamma Doradus/Delta Scuti Hybrid Pulsating Eclipsing Binary with Tidally Excited Oscillations","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.176665Z"},"links":{"cited_paper":"/paper/1909.03908","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:e3d3eb4cd0facf8cf2032cb06294ba1a034d957c1eb64fad23cd1bc34f52a560","observation_id":"3bfdebfd-94d5-46d4-bd08-9eef2f344ccb","resolution":{"observed_at":"2026-08-06T14:45:20.176665Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.179466Z","title":"The effect of tides on self-driven stellar pulsations","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.179466Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:7a8641278e3a3e81019c5480d6fc1b9dcc9370bfa08d2134832a8aeef0945d48","observation_id":"d500cda5-43c4-49e6-a7b3-aa3fc8f88b30","resolution":{"observed_at":"2026-08-06T14:45:20.179466Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.1493","last_updated":"2012-09-07T11:01:47Z","snapshot_observed_at":"2026-07-06T02:55:10.476799Z","submitted_at":"2012-09-07T11:01:47Z","title":"Pulsational amplitude growth of the star KIC 3429637 (HD 178875) in the context of Am and rho Puppis stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.1493","snapshot_observed_at":"2026-08-06T14:45:20.184932Z","title":"Pulsational amplitude growth of the star KIC 3429637 (HD 178875) in the context of Am and ρ Pup stars","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.184932Z"},"links":{"cited_paper":"/paper/1209.1493","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:94822f32e1fa211ccecc42984772458c950b6871c97606d3d0d248c70af0bd26","observation_id":"35d75f89-8674-474f-9156-999a1fe9fd97","resolution":{"observed_at":"2026-08-06T14:45:20.184932Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.188015Z","title":"Discovery and Seismic Analysis of an EL CVn-type Binary with Hybrid δ Sct-γ Dor Pulsations","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.188015Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:491ca20535dcc3c351882e790000e14b20fd143de71e6fd5e421f9bfb2e0b49b","observation_id":"d5d9f9fb-bfe1-4d84-88a0-7424fe5f9b1b","resolution":{"observed_at":"2026-08-06T14:45:20.188015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.08931","last_updated":"2019-07-05T09:54:45Z","snapshot_observed_at":"2026-07-06T07:54:35.511356Z","submitted_at":"2019-05-22T02:53:34Z","title":"A double-modulation effect detected in a double-mode high-amplitude $\\delta$ Scuti star: KIC 10284901","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.08931","snapshot_observed_at":"2026-08-06T14:45:20.190632Z","title":"A Double-modulation Effect Detected in a Double-mode High-amplitude δ Scuti Star: KIC 10284901","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.190632Z"},"links":{"cited_paper":"/paper/1905.08931","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:c385f31471136686b710a28cf5683ad27cea0b0964d0f43c85c2e1c1d35ec06b","observation_id":"119a637c-df30-4d6c-bb41-ed03c3312621","resolution":{"observed_at":"2026-08-06T14:45:20.190632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.00740","last_updated":"2020-08-03T09:42:35Z","snapshot_observed_at":"2026-08-07T17:18:24.922149Z","submitted_at":"2020-08-03T09:42:35Z","title":"Asteroseismology of two Kepler detached eclipsing binaries","version":1},"cited_work":{"arxiv_id":"2008.00740","doi":null,"metadata_source":"pith","pith_arxiv_id":"2008.00740","snapshot_observed_at":"2026-08-06T14:45:23.373135Z","title":"Asteroseismology of two Kepler detached eclipsing binaries","venue":"astro-ph.SR","work_id":"16620411-41c0-49df-852e-4f769a8cb0d1","year":2020},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.193348Z"},"links":{"cited_paper":"/paper/2008.00740","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:d0b53b5ea7273fba73724a399e37ef006455303dbdfc08a4bf191e4ddc53a262","observation_id":"8a3cb009-14d2-4b90-9d0a-63c607f7b9e7","resolution":{"observed_at":"2026-08-06T14:45:23.471945Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.01029","last_updated":"2019-07-29T22:28:09Z","snapshot_observed_at":"2026-08-09T16:33:04.673025Z","submitted_at":"2019-06-03T19:12:46Z","title":"Dealing With $\\delta$-Scuti Variables: Transit Light Curve Analysis of Planets Orbiting Rapidly-Rotating, Seismically Active A/F Stars","version":2},"cited_work":{"arxiv_id":"1906.01029","doi":null,"metadata_source":"pith","pith_arxiv_id":"1906.01029","snapshot_observed_at":"2026-08-06T14:45:23.198227Z","title":"Dealing With $\\delta$-Scuti Variables: Transit Light Curve Analysis of Planets Orbiting Rapidly-Rotating, Seismically Active A/F Stars","venue":"astro-ph.SR","work_id":"2a17b009-5636-446c-93a7-0721a3de35ac","year":2019},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.195892Z"},"links":{"cited_paper":"/paper/1906.01029","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:b41cf4be155c8d07d870ba302a10f635a9b74a0de65d4f2e5cb08cb8d36dbba0","observation_id":"4c94c388-15a7-4e74-b3a3-f09b51b4f1a1","resolution":{"observed_at":"2026-08-06T14:45:23.265490Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stx3206","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Equally spaced periods in the δ Scuti star KIC 5123889","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"dec9946b-86b5-45b3-a63c-e2b725e5b983","year":2018},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.198522Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:6b0fd4c5fb300dfbfbffc7e8a899734f306b3f1e9267124f9d87b62885e8ca78","observation_id":"7c2cd9a4-7933-401a-aa4c-91909cd936bc","resolution":{"observed_at":"2026-08-06T14:45:20.498499Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.201166Z","title":"Kepler observations of the high-amplitude δ Scuti star V2367 Cyg","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.201166Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:1d68398f54bf91205ebff94c44e1acfb16c71cc4aed47d1199315eb43c99065d","observation_id":"c5d7334d-91bf-45e8-a33d-385ed238a7a2","resolution":{"observed_at":"2026-08-06T14:45:20.201166Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.32023/0001-5237/68.4.6","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Hybrid Pulsations and Tidal Splitting detected in the Kepler Eclipsing and Spotted Binary System KIC 6048106","venue":"Acta Astronomica","work_id":"4f660a11-952f-49d0-941b-485d9de04726","year":2018},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.204118Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:171ab90b381f4c233d0316d6a67382b0cc636abb6e420aea26902efc6a5f2661","observation_id":"cef7f4ac-618f-44f5-98b1-865fdf068f09","resolution":{"observed_at":"2026-08-06T14:45:20.490996Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.02064","last_updated":"2023-11-07T18:49:38Z","snapshot_observed_at":"2026-07-31T03:17:55.891893Z","submitted_at":"2023-11-03T17:47:38Z","title":"Physical properties of the eclipsing binary KIC 9851944 and analysis of its tidally-perturbed p- and g-mode pulsations","version":2},"cited_work":{"arxiv_id":"2311.02064","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.02064","snapshot_observed_at":"2026-08-06T14:45:22.994256Z","title":"Physical properties of the eclipsing binary KIC 9851944 and analysis of its tidally-perturbed p- and g-mode pulsations","venue":"astro-ph.SR","work_id":"123af181-9585-4b03-8957-9bcf8f049384","year":2023},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.207033Z"},"links":{"cited_paper":"/paper/2311.02064","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:9694116a14d5c8acc060133f97a7713f95d1c41887275162f22379d64add879f","observation_id":"2ac7a221-ae5f-48c5-96be-d6e36b27263d","resolution":{"observed_at":"2026-08-06T14:45:23.049290Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1805.00798","last_updated":"2018-05-02T13:35:19Z","snapshot_observed_at":"2026-07-06T06:36:54.436252Z","submitted_at":"2018-05-02T13:35:19Z","title":"KIC 8553788: A pulsating Algol with an extreme mass ratio","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.00798","snapshot_observed_at":"2026-08-06T14:45:20.210256Z","title":"KIC 8553788: A pulsating Algol with an extreme mass ratio","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.210256Z"},"links":{"cited_paper":"/paper/1805.00798","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:ce403d04fa558165d0ecdd8dc15c58b6cf76d27b5a247f7835011f261130440f","observation_id":"43b98c6c-bc78-4951-907f-e9b6155112fe","resolution":{"observed_at":"2026-08-06T14:45:20.210256Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.00831","last_updated":"2016-06-02T19:58:32Z","snapshot_observed_at":"2026-07-06T04:58:34.126702Z","submitted_at":"2016-06-02T19:58:32Z","title":"Kepler Eclipsing Binaries with $\\delta$ Scuti/$\\gamma$ Doradus Pulsating Components 1: KIC 9851944","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.00831","snapshot_observed_at":"2026-08-06T14:45:20.213039Z","title":"Kepler Eclipsing Binaries with Delta Scuti/Gamma Doradus Pulsating Components I: KIC 9851944","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.213039Z"},"links":{"cited_paper":"/paper/1606.00831","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:8614ff3b58f1fb5ad881940a944ca0c03867545e09219fbb9df091a181ba7468","observation_id":"23951bc9-c730-4100-b52f-7b331c22ae19","resolution":{"observed_at":"2026-08-06T14:45:20.213039Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.05158","last_updated":"2017-02-16T21:15:31Z","snapshot_observed_at":"2026-08-02T16:05:11.155894Z","submitted_at":"2017-02-16T21:15:31Z","title":"Search for exoplanets around pulsating stars of A--F type in Kepler Short Cadence data and the case of KIC 8197761","version":1},"cited_work":{"arxiv_id":"1702.05158","doi":null,"metadata_source":"pith","pith_arxiv_id":"1702.05158","snapshot_observed_at":"2026-08-06T14:45:22.748065Z","title":"Search for exoplanets around pulsating stars of A--F type in Kepler Short Cadence data and the case of KIC 8197761","venue":"astro-ph.SR","work_id":"4ec224b3-d48c-4b2f-a697-f49d53fea39c","year":2017},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.215834Z"},"links":{"cited_paper":"/paper/1702.05158","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:0a10cfa134be89ccbad1b6eaeb51d23d63852a0561e65773d892659b2d0c0114","observation_id":"e756e1e6-6b86-48d0-9baf-dae453c3d1a4","resolution":{"observed_at":"2026-08-06T14:45:22.838320Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ad93bc","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Hilbert Transform Reveals Unusual Modulation in Delta Scuti Star KIC 10407873","venue":"The Astrophysical Journal","work_id":"829be95d-52d4-4e5e-bb5b-980d0f6724b3","year":2024},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.218589Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:d7344aa1c3f842b3bc2502551c486153d57ee9040a0a78a0cb068bd6eeb1977e","observation_id":"bc6302b3-11bc-4292-b02e-d6aa728f6321","resolution":{"observed_at":"2026-08-06T14:45:20.483490Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1704.03789","last_updated":"2017-10-31T10:39:46Z","snapshot_observed_at":"2026-07-06T05:37:35.795581Z","submitted_at":"2017-04-12T15:01:59Z","title":"Gravity Modes Reveal the Internal Rotation of a Post-mass Transfer Gamma Doradus/Delta Scuti Hybrid Pulsator in Kepler Eclipsing Binary KIC 9592855","version":2},"cited_work":{"arxiv_id":"1704.03789","doi":null,"metadata_source":"pith","pith_arxiv_id":"1704.03789","snapshot_observed_at":"2026-08-06T14:45:22.537438Z","title":"Gravity Modes Reveal the Internal Rotation of a Post-mass Transfer Gamma Doradus/Delta Scuti Hybrid Pulsator in Kepler Eclipsing Binary KIC 9592855","venue":"astro-ph.SR","work_id":"1c780d1b-823c-41e1-9637-7d59aab77255","year":2017},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.221085Z"},"links":{"cited_paper":"/paper/1704.03789","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:7cf9d1c847167b539be1449bc02ef6a5cdda915b48e43ab1b82e73ceafa033b9","observation_id":"f7a35fa9-b833-48db-8ac9-e67a16f87bbd","resolution":{"observed_at":"2026-08-06T14:45:22.635166Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.20834","last_updated":"2024-11-04T08:00:00Z","snapshot_observed_at":"2026-07-06T19:40:39.348570Z","submitted_at":"2024-10-28T08:33:19Z","title":"KIC 10855535: An elegant Delta Scuti pulsator with Amplitude and Phase Modulation","version":2},"cited_work":{"arxiv_id":"2410.20834","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.20834","snapshot_observed_at":"2026-08-06T14:45:22.355881Z","title":"KIC 10855535: An elegant Delta Scuti pulsator with Amplitude and Phase Modulation","venue":"astro-ph.SR","work_id":"c264f6b2-1dcd-4ebc-a0c1-c537628a065c","year":2024},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.223917Z"},"links":{"cited_paper":"/paper/2410.20834","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:1685977a6f8ef49b1346ab6530145d606eaa7188bf47e70560ed4c553f343016","observation_id":"0ebdca9d-0a0c-4f48-8974-d1ecfab99d22","resolution":{"observed_at":"2026-08-06T14:45:22.429084Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/aa9577","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Low-mass Pre-He White Dwarf Stars in Kepler Eclipsing Binaries with Multi-periodic Pulsations","venue":"The Astrophysical Journal","work_id":"cf7b5b65-709b-4866-b07c-e8ed177c2368","year":2017},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.226428Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:7ed5c8ee54d2e6ba1ffdb929e851311819270ed22e54e41e7bbe6978e0cec371","observation_id":"b8b538fc-5634-4635-9beb-1b5a5531f52d","resolution":{"observed_at":"2026-08-06T14:45:20.476076Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ad7","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.464689Z","title":"KIC 8840638: A Newly Discovered Eclipsing Binary with δ Scuti–Type Oscillations","venue":null,"work_id":"cf6b26e6-8271-4e60-94df-632d2a60881e","year":2024},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.228849Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:0bdd8508e4fc1f86c3016479c45e63420e1645eddd2e43a3a503b7e852b44418","observation_id":"f8421d31-76a2-4f20-b73a-0fa9520e5146","resolution":{"observed_at":"2026-08-06T14:45:20.467668Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.08102","last_updated":"2023-09-15T01:44:24Z","snapshot_observed_at":"2026-07-06T16:18:45.451203Z","submitted_at":"2023-09-15T01:44:24Z","title":"KIC 9845907: A $\\delta$ Scuti star with the first overtone as the dominant frequency and with many equidistant structures in its spectrum","version":1},"cited_work":{"arxiv_id":"2309.08102","doi":null,"metadata_source":"pith","pith_arxiv_id":"2309.08102","snapshot_observed_at":"2026-08-06T14:45:22.171280Z","title":"KIC 9845907: A $\\delta$ Scuti star with the first overtone as the dominant frequency and with many equidistant structures in its spectrum","venue":"astro-ph.SR","work_id":"04471509-d7da-4293-8149-7914c74d4bd2","year":2023},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.231915Z"},"links":{"cited_paper":"/paper/2309.08102","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:538093535fdebbd63ebc50311566c943b9e98d7bc1af450230073add720998b7","observation_id":"e27631bf-5700-4f93-bc34-bfccc65c3efa","resolution":{"observed_at":"2026-08-06T14:45:22.272179Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.00350","last_updated":"2017-02-18T08:45:36Z","snapshot_observed_at":"2026-08-10T10:20:59.993498Z","submitted_at":"2016-10-02T21:04:34Z","title":"KIC 8262223: A Post-Mass Transfer Eclipsing Binary Consisting of a Delta Scuti Pulsator and a Helium White Dwarf Precursor","version":2},"cited_work":{"arxiv_id":"1610.00350","doi":null,"metadata_source":"pith","pith_arxiv_id":"1610.00350","snapshot_observed_at":"2026-08-06T14:45:21.975428Z","title":"KIC 8262223: A Post-Mass Transfer Eclipsing Binary Consisting of a Delta Scuti Pulsator and a Helium White Dwarf Precursor","venue":"astro-ph.SR","work_id":"a43527eb-2c70-4e3f-ad5c-30197622bf6a","year":2016},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.234690Z"},"links":{"cited_paper":"/paper/1610.00350","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:bf7fdaab90434f4cdad8669a93dca95a995c03c6929de65d97a7f35f87e807cd","observation_id":"faa47961-c144-4cd4-84e0-e1da25cb5301","resolution":{"observed_at":"2026-08-06T14:45:22.062831Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/acb056","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Hidden Companions Detected by Asteroseismology","venue":"The Astrophysical Journal Letters","work_id":"ed895afc-6b28-4f4c-aa0a-23909b123b85","year":2023},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.237280Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:3fb913b8447f07b97c399acf7bbfcedccc0e610b54bb5a06e1ca40eb3a99d09b","observation_id":"d47c7d79-8e83-4903-99c0-7c00012271c1","resolution":{"observed_at":"2026-08-06T14:45:20.459074Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1612.09408","last_updated":"2016-12-30T07:13:49Z","snapshot_observed_at":"2026-07-06T05:24:32.693553Z","submitted_at":"2016-12-30T07:13:49Z","title":"KIC 11401845: An Eclipsing Binary with Multiperiodic Pulsations and Light Travel Time","version":1},"cited_work":{"arxiv_id":"1612.09408","doi":null,"metadata_source":"pith","pith_arxiv_id":"1612.09408","snapshot_observed_at":"2026-08-06T14:45:21.794237Z","title":"KIC 11401845: An Eclipsing Binary with Multiperiodic Pulsations and Light Travel Time","venue":"astro-ph.SR","work_id":"b9ae10ff-a5ac-4f78-83b2-373a63e57294","year":2016},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.239721Z"},"links":{"cited_paper":"/paper/1612.09408","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:667616131695751a40c4a340d6c00da1b4c176d17145953016622cdd7cc74023","observation_id":"db35bd46-37ce-40d8-aeb1-7d4a579f739c","resolution":{"observed_at":"2026-08-06T14:45:21.887385Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1605.09076","last_updated":"2016-05-29T23:41:55Z","snapshot_observed_at":"2026-07-06T04:57:59.683530Z","submitted_at":"2016-05-29T23:41:55Z","title":"KIC 6220497: A New Algol-type Eclipsing Binary with Multiperiodic Pulsations","version":1},"cited_work":{"arxiv_id":"1605.09076","doi":null,"metadata_source":"pith","pith_arxiv_id":"1605.09076","snapshot_observed_at":"2026-08-06T14:45:21.575004Z","title":"KIC 6220497: A New Algol-type Eclipsing Binary with Multiperiodic Pulsations","venue":"astro-ph.SR","work_id":"3ebf8fb3-ea93-42f6-9350-f8fb916dd548","year":2016},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.242287Z"},"links":{"cited_paper":"/paper/1605.09076","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:5c2e0641673b7ce1d3d2017110b1330e760188549ff6f9ea0c7da5b2e41a47c1","observation_id":"638217f0-61e7-49e6-a5c7-5ac1f579854d","resolution":{"observed_at":"2026-08-06T14:45:21.674310Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1511.03764","last_updated":"2015-11-12T02:48:47Z","snapshot_observed_at":"2026-07-06T04:36:12.154027Z","submitted_at":"2015-11-12T02:48:47Z","title":"KIC 4739791: A New R CMa-type Eclipsing Binary with a Pulsating Component","version":1},"cited_work":{"arxiv_id":"1511.03764","doi":null,"metadata_source":"pith","pith_arxiv_id":"1511.03764","snapshot_observed_at":"2026-08-06T14:45:21.378397Z","title":"KIC 4739791: A New R CMa-type Eclipsing Binary with a Pulsating Component","venue":"astro-ph.SR","work_id":"a2edbae0-d27d-426a-96cd-289ed7334616","year":2015},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.244845Z"},"links":{"cited_paper":"/paper/1511.03764","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:dec6df051e182d280d46a43da80baacb960fbf4e4e9685a9a15c96bcb5600590","observation_id":"fe304760-946d-4502-91ba-1c5dec5846ca","resolution":{"observed_at":"2026-08-06T14:45:21.456834Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2102.10259","last_updated":"2022-10-26T15:13:03Z","snapshot_observed_at":"2026-07-06T10:43:05.412194Z","submitted_at":"2021-02-20T05:15:06Z","title":"A rapidly evolving high-amplitude $\\delta$ Scuti star crossing the Hertzsprung Gap","version":2},"cited_work":{"arxiv_id":"2102.10259","doi":null,"metadata_source":"pith","pith_arxiv_id":"2102.10259","snapshot_observed_at":"2026-08-06T14:45:21.308948Z","title":"A rapidly evolving high-amplitude $\\delta$ Scuti star crossing the Hertzsprung Gap","venue":"astro-ph.SR","work_id":"6c2d1526-9f36-4033-8ffe-9df0ccf48c02","year":2021},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.247236Z"},"links":{"cited_paper":"/paper/2102.10259","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:165ebf1ce3f48c13d89b88ac85bfeda2ba26909523e67119b48631bb1b5c6675","observation_id":"459214b2-9d62-4dd9-8a1a-ff77f786a8c6","resolution":{"observed_at":"2026-08-06T14:45:21.318274Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1412.5362","last_updated":"2014-12-17T12:36:43Z","snapshot_observed_at":"2026-08-10T06:38:46.469720Z","submitted_at":"2014-12-17T12:36:43Z","title":"Asteroseismic measurement of slow, nearly-uniform surface-to-core rotation in the main sequence F star KIC 9244992","version":1},"cited_work":{"arxiv_id":"1412.5362","doi":null,"metadata_source":"pith","pith_arxiv_id":"1412.5362","snapshot_observed_at":"2026-08-06T14:45:21.279356Z","title":"Asteroseismic measurement of slow, nearly-uniform surface-to-core rotation in the main sequence F star KIC 9244992","venue":"astro-ph.SR","work_id":"44ea3af4-ddcb-4734-8557-20772a1cf467","year":2014},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.249832Z"},"links":{"cited_paper":"/paper/1412.5362","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:e9eed7479a4880a0c02de052b9f48905cf25e60aa22d01e330c776448ded7251","observation_id":"bc83494a-b2d2-4fa8-97d2-da823a470163","resolution":{"observed_at":"2026-08-06T14:45:21.289603Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1304.6993","last_updated":"2013-04-25T19:51:37Z","snapshot_observed_at":"2026-07-06T03:12:02.850583Z","submitted_at":"2013-04-25T19:51:37Z","title":"Multi-site photometric campaign on the high amplitude {\\delta} Scuti star KIC 6382916","version":1},"cited_work":{"arxiv_id":"1304.6993","doi":null,"metadata_source":"pith","pith_arxiv_id":"1304.6993","snapshot_observed_at":"2026-08-06T14:45:21.242971Z","title":"Multi-site photometric campaign on the high amplitude {\\delta} Scuti star KIC 6382916","venue":"astro-ph.SR","work_id":"a0e51ed0-c2b0-4195-992a-78fab737f350","year":2013},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.252895Z"},"links":{"cited_paper":"/paper/1304.6993","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:64e636257e416153dc3c71ddeca8c1960abe4c718af3890906f03d4d9436275a","observation_id":"d5a42b9c-42a4-483f-856b-a7851351765e","resolution":{"observed_at":"2026-08-06T14:45:21.256878Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1410.8699","last_updated":"2014-10-31T10:46:37Z","snapshot_observed_at":"2026-08-10T09:46:27.799864Z","submitted_at":"2014-10-31T10:46:37Z","title":"Validation of the Frequency Modulation technique applied to the pulsating delta Sct - gamma Dor eclipsing binary star KIC 8569819","version":1},"cited_work":{"arxiv_id":"1410.8699","doi":null,"metadata_source":"pith","pith_arxiv_id":"1410.8699","snapshot_observed_at":"2026-08-06T14:45:21.195122Z","title":"Validation of the Frequency Modulation technique applied to the pulsating delta Sct - gamma Dor eclipsing binary star KIC 8569819","venue":"astro-ph.SR","work_id":"cb249f97-bb78-4342-be0b-3ecc5e555756","year":2014},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.255650Z"},"links":{"cited_paper":"/paper/1410.8699","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:7e5cef7bc23807fe02b77cad146dbdad4cdcadfc14c092521b5160e20bcc46ff","observation_id":"52b006c8-bae2-4b23-9649-fe2cfb78a284","resolution":{"observed_at":"2026-08-06T14:45:21.214958Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.258334Z","title":"Amplitude Modulation in the δ Sct star KIC 7106205","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.258334Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:b1dcce5f7463a8d49a283150deb93f14f48ae84c91bd31cf718ebf4c65974f2b","observation_id":"4461e595-f520-4572-b776-618dc0aecec1","resolution":{"observed_at":"2026-08-06T14:45:20.258334Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.00571","last_updated":"2022-05-01T22:08:01Z","snapshot_observed_at":"2026-08-09T13:41:55.073184Z","submitted_at":"2022-05-01T22:08:01Z","title":"Frequency analysis of KIC 1573174 : shedding light on the nature of HADS stars","version":1},"cited_work":{"arxiv_id":"2205.00571","doi":null,"metadata_source":"pith","pith_arxiv_id":"2205.00571","snapshot_observed_at":"2026-08-06T14:45:21.089478Z","title":"Frequency analysis of KIC 1573174 : shedding light on the nature of HADS stars","venue":"astro-ph.SR","work_id":"a6aaf374-fdf2-473e-8687-913b9cce242b","year":2022},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.260789Z"},"links":{"cited_paper":"/paper/2205.00571","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:8c3504c15b48dbbc54db7e3cd3d7c4b72717410d5bd7a0c7c4477d8296e480d3","observation_id":"fd9831d1-0a4c-4262-9d1d-fc288fc3a756","resolution":{"observed_at":"2026-08-06T14:45:21.097018Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1408.0715","last_updated":"2014-08-04T15:46:07Z","snapshot_observed_at":"2026-08-10T06:22:03.205693Z","submitted_at":"2014-08-04T15:46:07Z","title":"Pulsational Frequency and Amplitude Modulation in the $\\delta$\\,Sct star KIC\\,7106205","version":1},"cited_work":{"arxiv_id":"1408.0715","doi":null,"metadata_source":"pith","pith_arxiv_id":"1408.0715","snapshot_observed_at":"2026-08-06T14:45:21.065150Z","title":"Pulsational Frequency and Amplitude Modulation in the $\\delta$\\,Sct star KIC\\,7106205","venue":"astro-ph.SR","work_id":"004a06f6-5c09-45d3-b13f-e5475459d62b","year":2014},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.263818Z"},"links":{"cited_paper":"/paper/1408.0715","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:6636ee7d95568b497ac99685febd95bb65c90595c832f3f3f4586228d9cff379","observation_id":"05e54552-3e51-4f8f-8355-65a8957dba62","resolution":{"observed_at":"2026-08-06T14:45:21.073245Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-3881/ac6fde","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"KIC 5768203: Aδ Sct Pulsator Modulated by Rotation and Spots","venue":"The Astronomical Journal","work_id":"885aaa43-dfda-46e8-bdb9-1bdd6e43c07d","year":2022},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.266274Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:5b91d3995fab9f76616a0593b1d264b4bffdfdd6bdad2af5b2097955002953db","observation_id":"47ee02fe-042a-41cd-9b58-b9911602b3de","resolution":{"observed_at":"2026-08-06T14:45:20.450711Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00781","last_updated":"2015-09-24T13:01:37Z","snapshot_observed_at":"2026-07-06T04:28:35.430029Z","submitted_at":"2015-09-02T16:53:34Z","title":"KIC 10080943: An eccentric binary system containing two pressure- and gravity-mode hybrid pulsators","version":2},"cited_work":{"arxiv_id":"1509.00781","doi":null,"metadata_source":"pith","pith_arxiv_id":"1509.00781","snapshot_observed_at":"2026-08-06T14:45:21.053960Z","title":"KIC 10080943: An eccentric binary system containing two pressure- and gravity-mode hybrid pulsators","venue":"astro-ph.SR","work_id":"bb4c8896-1b49-408e-b84b-550514b3cef0","year":2015},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.268759Z"},"links":{"cited_paper":"/paper/1509.00781","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:2e212e4678f0ec6a8534f3450476d5e208ae6042effd321213e0a2db786b0054","observation_id":"47b8b43b-86b2-4715-9b1b-63df09fea0f6","resolution":{"observed_at":"2026-08-06T14:45:21.056978Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.04651","last_updated":"2022-09-10T12:40:43Z","snapshot_observed_at":"2026-08-08T23:13:20.954531Z","submitted_at":"2022-09-10T12:40:43Z","title":"KIC 6951642: confirmed Kepler $\\gamma$ Doradus-$\\delta$ Scuti star with intermediate to fast rotation in a possible single-lined binary system","version":1},"cited_work":{"arxiv_id":"2209.04651","doi":null,"metadata_source":"pith","pith_arxiv_id":"2209.04651","snapshot_observed_at":"2026-08-06T14:45:21.041693Z","title":"KIC 6951642: confirmed Kepler $\\gamma$ Doradus-$\\delta$ Scuti star with intermediate to fast rotation in a possible single-lined binary system","venue":"astro-ph.SR","work_id":"8c023d58-f2d8-4165-87b5-2e76b51958a4","year":2022},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.271500Z"},"links":{"cited_paper":"/paper/2209.04651","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:fbb1d544499ffc80a09cc154de4ad5f24a6e2f573ec21def188ef1c96c029b76","observation_id":"a30cabda-b963-44a1-a97c-3321f6115a3e","resolution":{"observed_at":"2026-08-06T14:45:21.045185Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1506.01668","last_updated":"2015-06-04T17:48:54Z","snapshot_observed_at":"2026-07-06T04:19:55.079206Z","submitted_at":"2015-06-04T17:48:54Z","title":"KIC 9533489: a genuine gamma Doradus-delta Scuti Kepler hybrid pulsator with transit events","version":1},"cited_work":{"arxiv_id":"1506.01668","doi":null,"metadata_source":"pith","pith_arxiv_id":"1506.01668","snapshot_observed_at":"2026-08-06T14:45:21.030309Z","title":"KIC 9533489: a genuine gamma Doradus-delta Scuti Kepler hybrid pulsator with transit events","venue":"astro-ph.SR","work_id":"97926b21-eeca-4ba4-8a98-7823df80e057","year":2015},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.274304Z"},"links":{"cited_paper":"/paper/1506.01668","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:b1d467d8f0729fd9537bd3d73104eafc26c412dc8163d61520418d5f38c8b206","observation_id":"cb171519-224c-47c6-98d3-aa53de8841a1","resolution":{"observed_at":"2026-08-06T14:45:21.033560Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1674-4527/21/9/224","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"KIC 5197256: an eclipsing binary containing aδ Scuti variable star","venue":"Research in Astronomy and Astrophysics","work_id":"86c69c2c-316a-4163-8839-58e6a8a19e22","year":2021},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.277159Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:5eb3ba1d0bba2af66d2942f9fd15dfcf37f7a2e5fec88cb00f5cdb312bd3bd3a","observation_id":"45caf346-1515-455c-8d64-68a597efb328","resolution":{"observed_at":"2026-08-06T14:45:20.442761Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1506.00543","last_updated":"2015-06-15T10:48:28Z","snapshot_observed_at":"2026-07-06T04:19:32.838540Z","submitted_at":"2015-06-01T15:42:56Z","title":"Evidence of amplitude modulation due to Resonant Mode Coupling in the delta Scuti star KIC5892969","version":2},"cited_work":{"arxiv_id":"1506.00543","doi":null,"metadata_source":"pith","pith_arxiv_id":"1506.00543","snapshot_observed_at":"2026-08-06T14:45:21.018028Z","title":"Evidence of amplitude modulation due to Resonant Mode Coupling in the delta Scuti star KIC5892969","venue":"astro-ph.SR","work_id":"084e480b-5a5e-4a71-a342-abe896db4db0","year":2015},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.279649Z"},"links":{"cited_paper":"/paper/1506.00543","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:be0838cf32322095a9674f29148c004e54a93428b7f1488421ffa1999b019375","observation_id":"7696f198-467d-4e62-ac9d-dac0f33438ba","resolution":{"observed_at":"2026-08-06T14:45:21.021178Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.282247Z","title":"The δ Scuti Pulsation Periods in KIC 5197256","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.282247Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:ca8aef8fe879ac5d078553e884c979a088d1877f0c55607ea8329ca74258a4a9","observation_id":"25eade5c-0a3c-44f7-808f-d275a2bb7b28","resolution":{"observed_at":"2026-08-06T14:45:20.282247Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.0155","last_updated":"2014-07-14T12:27:17Z","snapshot_observed_at":"2026-07-06T03:42:35.765182Z","submitted_at":"2014-05-01T13:12:27Z","title":"Asteroseismic measurement of surface-to-core rotation in a main sequence A star, KIC 11145123","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.0155","snapshot_observed_at":"2026-08-06T14:45:20.284832Z","title":"Asteroseismic measurement of surface-to-core rotation in a main-sequence A star, KIC 11145123","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.284832Z"},"links":{"cited_paper":"/paper/1405.0155","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:ebc3841f141c200bbcf9eb425eff422de9999c42ab0ce65f694db20811877752","observation_id":"c6b07f30-f660-43f9-84c9-60ebbabdf154","resolution":{"observed_at":"2026-08-06T14:45:20.284832Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.13577","last_updated":"2021-05-28T04:04:06Z","snapshot_observed_at":"2026-08-03T04:35:12.908780Z","submitted_at":"2021-05-28T04:04:06Z","title":"A binary with a $\\delta$~Scuti star and an oscillating red giant: orbit and asteroseismology of KIC9773821","version":1},"cited_work":{"arxiv_id":"2105.13577","doi":null,"metadata_source":"pith","pith_arxiv_id":"2105.13577","snapshot_observed_at":"2026-08-06T14:45:21.000051Z","title":"A binary with a $\\delta$~Scuti star and an oscillating red giant: orbit and asteroseismology of KIC9773821","venue":"astro-ph.SR","work_id":"e0203c81-d8ee-4817-ab4a-90d648a0ef52","year":2021},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.287299Z"},"links":{"cited_paper":"/paper/2105.13577","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:4039f4d410925eed730df08b54004bde7956c0533e06d64515ae5b72fe6ace21","observation_id":"f38e8930-2394-4ecf-b367-99b16fd3fde4","resolution":{"observed_at":"2026-08-06T14:45:21.003008Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1402.0833","last_updated":"2014-02-04T19:01:50Z","snapshot_observed_at":"2026-07-06T03:35:08.378080Z","submitted_at":"2014-02-04T19:01:50Z","title":"Evidence of resonant mode coupling and the relationship between low and high frequencies in a rapidly rotating A star","version":1},"cited_work":{"arxiv_id":"1402.0833","doi":null,"metadata_source":"pith","pith_arxiv_id":"1402.0833","snapshot_observed_at":"2026-08-06T14:45:20.989689Z","title":"Evidence of resonant mode coupling and the relationship between low and high frequencies in a rapidly rotating A star","venue":"astro-ph.SR","work_id":"85cc69a3-960e-4ff6-8e93-d4ed6df80bba","year":2014},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.290179Z"},"links":{"cited_paper":"/paper/1402.0833","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:1e1dcf71bd820416fb58ab7f94ebfa0c3b7182147916f8d9b7916a32e48e56e9","observation_id":"4889284d-da59-4bba-8099-0057c2c7b463","resolution":{"observed_at":"2026-08-06T14:45:20.992778Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.09279","last_updated":"2021-04-19T13:20:05Z","snapshot_observed_at":"2026-07-06T11:01:38.535657Z","submitted_at":"2021-04-19T13:20:05Z","title":"KIC5950759: a high-amplitude $\\delta$ Sct star with amplitude and frequency modulation near the terminal age main sequence","version":1},"cited_work":{"arxiv_id":"2104.09279","doi":null,"metadata_source":"pith","pith_arxiv_id":"2104.09279","snapshot_observed_at":"2026-08-06T14:45:20.978840Z","title":"KIC5950759: a high-amplitude $\\delta$ Sct star with amplitude and frequency modulation near the terminal age main sequence","venue":"astro-ph.SR","work_id":"49eff275-5c1c-4320-89a6-e9322844bbbc","year":2021},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.293029Z"},"links":{"cited_paper":"/paper/2104.09279","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:2117568465d54d2edf3a7a97477f020f0299a40cbb56ec5dded343d69e7e62d8","observation_id":"ab81cbb1-e3c4-4a41-a1cc-0ebcc1409289","resolution":{"observed_at":"2026-08-06T14:45:20.982175Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1209.4836","last_updated":"2012-09-21T14:54:06Z","snapshot_observed_at":"2026-07-06T02:56:05.416759Z","submitted_at":"2012-09-21T14:54:06Z","title":"Relationship between low and high frequencies in Delta Scuti stars: Photometric Kepler and spectroscopic analyses of the rapid rotator KIC 8054146","version":1},"cited_work":{"arxiv_id":"1209.4836","doi":null,"metadata_source":"pith","pith_arxiv_id":"1209.4836","snapshot_observed_at":"2026-08-06T14:45:20.967731Z","title":"Relationship between low and high frequencies in Delta Scuti stars: Photometric Kepler and spectroscopic analyses of the rapid rotator KIC 8054146","venue":"astro-ph.SR","work_id":"91c750c0-e5a0-4867-a59d-db1e1c2cdccf","year":2012},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.295818Z"},"links":{"cited_paper":"/paper/1209.4836","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:0a4d3a68f751486dfed681c927cd3299efc73bb38d72cbdeb765012e55e2f603","observation_id":"8ec58a8c-3aa6-4396-9aed-0c6e80f140f5","resolution":{"observed_at":"2026-08-06T14:45:20.971203Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1807.03946","last_updated":"2018-08-25T03:00:58Z","snapshot_observed_at":"2026-08-01T14:48:26.558072Z","submitted_at":"2018-07-11T04:20:43Z","title":"A Weak Modulation Effect Detected in the Light Curves of KIC 5950759: Intrinsic or Instrumental Effect?","version":4},"cited_work":{"arxiv_id":"1807.03946","doi":null,"metadata_source":"pith","pith_arxiv_id":"1807.03946","snapshot_observed_at":"2026-08-06T14:45:20.956408Z","title":"A Weak Modulation Effect Detected in the Light Curves of KIC 5950759: Intrinsic or Instrumental Effect?","venue":"astro-ph.SR","work_id":"5e7b9a66-4c43-462b-a96e-5f9b4a8b30cb","year":2018},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.298311Z"},"links":{"cited_paper":"/paper/1807.03946","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:eb9f44aac3e2c11080213b9ea29bdcd10d336a12510b40aa6c325084edd33429","observation_id":"c694e69c-fbee-40b2-9b13-6343d2f78ad9","resolution":{"observed_at":"2026-08-06T14:45:20.959494Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1002/asna.201412122","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Relationship between low and high frequencies in the δ Scuti star KIC 9764965","venue":"Astronomische Nachrichten","work_id":"b4a2b7a1-8e64-45be-88c0-c12be7b1114e","year":2014},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.300904Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:021d0aaa83491207568d140b0429ee8450303f3f700499129d8a4e7f4fb7e5d8","observation_id":"3b8cd316-f186-4745-9f65-90d13bb14ebc","resolution":{"observed_at":"2026-08-06T14:45:20.434097Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.11389","last_updated":"2021-10-21T18:15:23Z","snapshot_observed_at":"2026-08-09T13:26:49.298035Z","submitted_at":"2021-10-21T18:15:23Z","title":"KIC 12602250: A low-amplitude Double-mode $\\delta$ Scuti star with Amplitude Modulation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.11389","snapshot_observed_at":"2026-08-06T14:45:20.303376Z","title":"KIC 12602250: A Low-amplitude Double-mode Delta Scuti Star with Amplitude Modulation","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.303376Z"},"links":{"cited_paper":"/paper/2110.11389","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:3b5d14320f83f6a0e79b9fe2198696daffcfc6ea984dbc7c5ad13385bfe7dada","observation_id":"c48ebe82-fb33-47e8-b9f6-c73c9c3d7015","resolution":{"observed_at":"2026-08-06T14:45:20.303376Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.0246","last_updated":"2011-07-01T14:55:47Z","snapshot_observed_at":"2026-07-06T02:30:15.224615Z","submitted_at":"2011-07-01T14:55:47Z","title":"SuperWASP observations of pulsating Am stars","version":1},"cited_work":{"arxiv_id":"1107.0246","doi":null,"metadata_source":"pith","pith_arxiv_id":"1107.0246","snapshot_observed_at":"2026-08-06T14:45:20.938464Z","title":"SuperWASP observations of pulsating Am stars","venue":"astro-ph.SR","work_id":"a910f560-7fb6-489c-9dc1-4b5d57e8de65","year":2011},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.305867Z"},"links":{"cited_paper":"/paper/1107.0246","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:356c2a660423ad4230e285d301de5a93d5218f017768291f8da2714207e5937c","observation_id":"d075df3f-fa04-424a-b480-5e544f2b473b","resolution":{"observed_at":"2026-08-06T14:45:20.941280Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1401.3130","last_updated":"2014-01-14T10:45:01Z","snapshot_observed_at":"2026-07-06T03:33:13.469117Z","submitted_at":"2014-01-14T10:45:01Z","title":"KIC 3858884: a hybrid {\\delta} Sct pulsator in a highly eccentric eclipsing binary","version":1},"cited_work":{"arxiv_id":"1401.3130","doi":null,"metadata_source":"pith","pith_arxiv_id":"1401.3130","snapshot_observed_at":"2026-08-06T14:45:20.927927Z","title":"KIC 3858884: a hybrid {\\delta} Sct pulsator in a highly eccentric eclipsing binary","venue":"astro-ph.SR","work_id":"a7d4dc9e-f795-4514-9656-528d59418a60","year":2014},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.308355Z"},"links":{"cited_paper":"/paper/1401.3130","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:57c19b5a9e2d3cc8b91f564a058c788618f6fd5432e053784665711c4d12315c","observation_id":"d156fe2c-4e15-4810-ba8e-878ff93ffaa6","resolution":{"observed_at":"2026-08-06T14:45:20.930886Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.10187","last_updated":"2020-10-20T10:51:58Z","snapshot_observed_at":"2026-07-06T10:06:09.269237Z","submitted_at":"2020-10-20T10:51:58Z","title":"Asteroseismic Analysis of $\\delta$ Scuti Components of Binary systems: The Case of KIC 8504570","version":1},"cited_work":{"arxiv_id":"2010.10187","doi":null,"metadata_source":"pith","pith_arxiv_id":"2010.10187","snapshot_observed_at":"2026-08-06T14:45:20.916219Z","title":"Asteroseismic Analysis of $\\delta$ Scuti Components of Binary systems: The Case of KIC 8504570","venue":"astro-ph.SR","work_id":"979f0c02-7442-44e1-9c3f-433006bf61a9","year":2020},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.310826Z"},"links":{"cited_paper":"/paper/2010.10187","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:9eaeec01d07c471c51e7e1323e56385ca22fe3e975efe33356b999337b547b03","observation_id":"f362310f-adf6-4312-af65-2f255d8bf1b0","resolution":{"observed_at":"2026-08-06T14:45:20.919473Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1306.1819","last_updated":"2013-06-07T19:50:44Z","snapshot_observed_at":"2026-08-09T05:54:29.847614Z","submitted_at":"2013-06-07T19:50:44Z","title":"KIC 4544587: an Eccentric, Short Period Binary System with delta Sct Pulsations and Tidally Excited Modes","version":1},"cited_work":{"arxiv_id":"1306.1819","doi":null,"metadata_source":"pith","pith_arxiv_id":"1306.1819","snapshot_observed_at":"2026-08-06T14:45:20.904879Z","title":"KIC 4544587: an Eccentric, Short Period Binary System with delta Sct Pulsations and Tidally Excited Modes","venue":"astro-ph.SR","work_id":"143610f7-8cd2-497e-b122-c0adff6f9339","year":2013},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.313266Z"},"links":{"cited_paper":"/paper/1306.1819","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:f1888f8dc1667a00eb867664b2b881814b5ff798fe742953ae3eff497f375e82","observation_id":"a0316064-89d3-4450-858c-21887e205b89","resolution":{"observed_at":"2026-08-06T14:45:20.908217Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.09915","last_updated":"2020-07-20T07:41:21Z","snapshot_observed_at":"2026-08-06T20:48:37.799803Z","submitted_at":"2020-07-20T07:41:21Z","title":"KIC 12268220: A $\\delta$ Scuti Pulsating Star and an Active Protohelium White Dwarf in an Eclipsing Binary System","version":1},"cited_work":{"arxiv_id":"2007.09915","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.09915","snapshot_observed_at":"2026-08-06T14:45:20.894193Z","title":"KIC 12268220: A $\\delta$ Scuti Pulsating Star and an Active Protohelium White Dwarf in an Eclipsing Binary System","venue":"astro-ph.SR","work_id":"442d6236-afe0-4b97-976f-2f48b1506b07","year":2020},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.316068Z"},"links":{"cited_paper":"/paper/2007.09915","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:19bc3cbfc845d4c7692daeda32c7d0731ffcc4d4e2d6c257a88321b881068608","observation_id":"88e7f82c-e54a-4594-9861-201cd71aa86a","resolution":{"observed_at":"2026-08-06T14:45:20.897295Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1304.1543","last_updated":"2013-04-09T16:23:56Z","snapshot_observed_at":"2026-07-06T03:10:26.639960Z","submitted_at":"2013-04-04T20:00:03Z","title":"Asteroseismology of KIC 11754974: a high-amplitude SX Phe pulsator in a 343-day binary system","version":2},"cited_work":{"arxiv_id":"1304.1543","doi":null,"metadata_source":"pith","pith_arxiv_id":"1304.1543","snapshot_observed_at":"2026-08-06T14:45:20.883219Z","title":"Asteroseismology of KIC 11754974: a high-amplitude SX Phe pulsator in a 343-day binary system","venue":"astro-ph.SR","work_id":"323cdac6-bf5a-4193-8391-88a529dea0f6","year":2013},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.319335Z"},"links":{"cited_paper":"/paper/1304.1543","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:2dadcffb33c72f6bf675e80f506720765a70ef836bc396ee4777d8fc5f63a5b6","observation_id":"d7d6525d-eb6c-47fe-b6d1-9a138fd02f7e","resolution":{"observed_at":"2026-08-06T14:45:20.886173Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09916","last_updated":"2020-04-21T11:33:42Z","snapshot_observed_at":"2026-08-04T06:59:12.828068Z","submitted_at":"2020-04-21T11:33:42Z","title":"KIC 10736223: An Algol-type eclipsing binary just undergone the rapid mass-transfer stage","version":1},"cited_work":{"arxiv_id":"2004.09916","doi":null,"metadata_source":"pith","pith_arxiv_id":"2004.09916","snapshot_observed_at":"2026-08-06T14:45:20.871082Z","title":"KIC 10736223: An Algol-type eclipsing binary just undergone the rapid mass-transfer stage","venue":"astro-ph.SR","work_id":"3779b76c-2dce-46df-bdc4-a4d54b0c97cf","year":2020},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.321890Z"},"links":{"cited_paper":"/paper/2004.09916","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:ad0e0c8f24b0d3bf11a47268e3042d5d9b84effceddc39efdbf8dcffeba30205","observation_id":"f5514d85-0f40-4d47-b986-6eb739422511","resolution":{"observed_at":"2026-08-06T14:45:20.874571Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1210.8432","last_updated":"2012-10-31T18:36:07Z","snapshot_observed_at":"2026-07-06T02:58:55.015492Z","submitted_at":"2012-10-31T18:36:07Z","title":"Low-frequency variations of unknown origin in the Kepler Delta Scuti star KIC 5988140 = HD 188774","version":1},"cited_work":{"arxiv_id":"1210.8432","doi":null,"metadata_source":"pith","pith_arxiv_id":"1210.8432","snapshot_observed_at":"2026-08-06T14:45:20.859122Z","title":"Low-frequency variations of unknown origin in the Kepler Delta Scuti star KIC 5988140 = HD 188774","venue":"astro-ph.SR","work_id":"6b8af566-fcd9-4d3e-9a9a-2d4ba947d9ff","year":2012},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.324615Z"},"links":{"cited_paper":"/paper/1210.8432","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:f793639c25bd224503cd75f54f71f809ccf8338c926426dc97ff3644bddae547","observation_id":"3194e197-5ea7-4ba4-8f26-587a72ed5879","resolution":{"observed_at":"2026-08-06T14:45:20.862689Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ab8ad5","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"A Pre-main-sequence γ Dor-δ Sct Hybrid with Extremely Slow Internal Rotation in a Short-period Eclipsing Binary KIC 9850387 Revealed by Asteroseismology","venue":"The Astrophysical Journal","work_id":"1dfdaf13-9ded-434e-a713-120310b96916","year":2020},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.327159Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:7c8111a55cc8eafbe0b7df1e0019ff7196ff1e6de873e1bff5d2a2692d07c6c4","observation_id":"ad4557ac-900c-46a3-9202-a124b0126e85","resolution":{"observed_at":"2026-08-06T14:45:20.425290Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:45:20.329581Z","title":"Unusual high-frequency oscillations in the Kepler δ Scuti star KIC 4840675","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.329581Z"},"links":{"citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:fca74809877e1ae57e5838eaf95d75ebfff785d54812023deb401476c2fa9e20","observation_id":"0b1edf19-976e-456d-981e-c2f50e648d04","resolution":{"observed_at":"2026-08-06T14:45:20.329581Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.05931","last_updated":"2021-02-11T10:32:55Z","snapshot_observed_at":"2026-08-07T11:16:19.133975Z","submitted_at":"2021-02-11T10:32:55Z","title":"On the pulsations of the $\\delta$ Scuti star of the binary system KIC 6629588","version":1},"cited_work":{"arxiv_id":"2102.05931","doi":null,"metadata_source":"pith","pith_arxiv_id":"2102.05931","snapshot_observed_at":"2026-08-06T14:45:20.749120Z","title":"On the pulsations of the $\\delta$ Scuti star of the binary system KIC 6629588","venue":"astro-ph.SR","work_id":"9c3c26f1-9faf-4411-80fd-884554843773","year":2021},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.332091Z"},"links":{"cited_paper":"/paper/2102.05931","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:c54a54b0208fd0c5942ec2ccb9a0f2cfcdc50d84a3bc4c365a138c3bea0ff521","observation_id":"b8dfd4a5-3782-437b-a39a-3dcee1c270de","resolution":{"observed_at":"2026-08-06T14:45:20.752024Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1202.0105","last_updated":"2012-02-03T16:15:10Z","snapshot_observed_at":"2026-08-07T11:18:35.928945Z","submitted_at":"2012-02-01T06:17:12Z","title":"FM stars: A Fourier view of pulsating binary stars, a new technique for measuring radial velocities photometrically","version":3},"cited_work":{"arxiv_id":"1202.0105","doi":null,"metadata_source":"pith","pith_arxiv_id":"1202.0105","snapshot_observed_at":"2026-08-06T14:45:20.737529Z","title":"FM stars: A Fourier view of pulsating binary stars, a new technique for measuring radial velocities photometrically","venue":"astro-ph.SR","work_id":"bff8ac2f-96ab-4ed9-809d-87b320940ae4","year":2012},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.334554Z"},"links":{"cited_paper":"/paper/1202.0105","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:f0602c50e06e373d6b9669379ba89d9f4184c62338ac9a7d70333e91dc81d1e3","observation_id":"fb4d7664-00ce-490d-a58c-5eeeae45ace8","resolution":{"observed_at":"2026-08-06T14:45:20.741047Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1102.3599","last_updated":"2011-02-17T15:03:29Z","snapshot_observed_at":"2026-08-10T10:57:04.168522Z","submitted_at":"2011-02-17T15:03:29Z","title":"Kepler photometry of KIC 10661783: a binary star with total eclipses and delta Scuti pulsations","version":1},"cited_work":{"arxiv_id":"1102.3599","doi":null,"metadata_source":"pith","pith_arxiv_id":"1102.3599","snapshot_observed_at":"2026-08-06T14:45:20.725523Z","title":"Kepler photometry of KIC 10661783: a binary star with total eclipses and delta Scuti pulsations","venue":"astro-ph.SR","work_id":"43413c02-b7c6-4d76-96eb-3eb5aa2aa335","year":2011},"citing_paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry","version":1},"reference_index":102,"source":"pdf_text","source_observed_at":"2026-08-06T14:45:20.337478Z"},"links":{"cited_paper":"/paper/1102.3599","citing_paper":"/paper/2507.18128"},"observation_digest":"sha256:f27a1b463bc7a5b0ed88d1114372ae293a8ab015d7f885afd0b4dff8f5809844","observation_id":"04bee3a8-e178-457b-b469-36d27b2ddf7f","resolution":{"observed_at":"2026-08-06T14:45:20.729144Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2507.18128","last_updated":"2025-07-24T06:32:04Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-08T04:40:11.212059Z","submitted_at":"2025-07-24T06:32:04Z","title":"Re-examining Super-Nyquist Frequencies of 68 $\\delta$ Scuti Stars Utilizing the Kepler Long Cadence Photometry"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":8,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":45,"verified_exact":47,"verified_fuzzy":0},"total_outbound_references":115},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 100 of 115 outbound references and 0 inbound Pith citation observations for arXiv:2507.18128."}