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Table · dataset · 2026

Super-Nyquist freq. in Kepler delta Scuti stars

Listed in IVOA Registry (Virtual Observatory)

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.

Description

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.

The full set of extracted frequencies is provided as reference material for future asteroseismic studies.

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Stated by source
Optical
Provenance · 1 source records, 8 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/710/a24514 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:opticalsource · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0