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<ri:Resource created="2026-06-17T09:24:28Z" status="active" updated="2026-07-07T00:00:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Super-Nyquist freq. in Kepler delta Scuti stars</title><shortName>J/A+A/710/A245</shortName><identifier>ivo://CDS.VizieR/J/A+A/710/A245</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mo Y.</name></creator><creator><name>Zong W.</name></creator><creator><name>Wang X.</name></creator><creator><name>Murphy S.</name></creator><creator><name>Yang Z.</name></creator><creator><name>Fu J.-N.</name></creator><creator><name>Charpinet S.,Ma X.-Y.</name></creator><date role="Updated">2026-06-17T08:26:19Z</date><date role="Created">2026-06-17T09:24:28Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>asteroseismology</subject><subject>variable-stars</subject><subject>visible-astronomy</subject><description>Pressure-mode frequencies in {delta} Scuti stars may exceed the Nyquist limit of Kepler long-cadence photometry and appear as reflected Nyquist aliases at lower frequencies. We performed a systematic survey of 1838 Kepler {delta} Scuti stars using a sliding Lomb-Scargle periodogram analysis, and identified 15265 confirmed super-Nyquist frequencies in 1309 stars among 259883 extracted frequencies. The catalog gives the identified super-Nyquist frequencies, their inferred real frequencies above the Nyquist limit, and the diagnostic quantities used for their classification. 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