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<ri:Resource created="2025-09-19T15:51:08Z" status="active" updated="2026-08-03T07:31:43Z" 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>Variability of {delta} Scuti stars with TESS LC</title><shortName>J/MNRAS/516/2080</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/516/2080</identifier><altIdentifier>doi:10.26093/cds/vizier/bg-g4-210</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Barac N.</name></creator><creator><name>Bedding T.R.</name></creator><creator><name>Murphy S.J.</name></creator><creator><name>Hey D.R.</name></creator><date role="Updated">2026-08-03T07:31:43Z</date><date role="Created">2025-09-19T15:51:08Z</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>variable-stars</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>stellar-distance</subject><subject>extinction</subject><description>We have used NASA's TESS mission to study catalogued {delta} Scuti stars. We examined TESS light curves for 434 stars, including many for which few previous observations exist. We found that 62 are not {delta} Scuti pulsators, with most instead showing variability from binarity. For the 372 {delta} Scuti stars, we provide a catalogue of the period and amplitude of the dominant pulsation mode. Using Gaia DR3 parallaxes, we place the stars in the period-luminosity (P-L) diagram and confirm previous findings that most stars lie on a ridge that corresponds to pulsation in the fundamental radial mode, and that many others fall on a second ridge that is a factor two shorter in period. This second ridge is seen more clearly than before, thanks to the revised periods and distances. We demonstrate the value of the P-L diagram in distinguishing {delta} Scuti stars from short-period RR Lyrae stars, and we find several new examples of high-frequency {delta} Scuti stars with regular sequences of overtone modes, including XX Pyx and 29 Cyg. Finally, we revisit the sample of {delta} Scuti stars observed by Kepler and show that they follow a tight period-density relation, with a pulsation constant for the fundamental mode of Q = 0.0315 d.</description><source format="bibcode">2022MNRAS.516.2080B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/516/2080</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/491/3586">J/MNRAS/491/3586 : 611 {gamma} Doradus stars Kepler data (Li+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/477/907">J/A+A/477/907 : Beta Cephei stars in the ASAS-3 data. I. (Pigulski+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/144/469">J/A+AS/144/469 : Delta Scuti stars (Rodriguez+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/145/132">J/AJ/145/132 : New catalog of 1578 {delta} Scuti stars (Chang+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/45">J/AJ/155/45 : Metal-rich RRc stars in the Carnegie RR Lyrae Survey</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/258/8">J/ApJS/258/8 : LCs of RR Lyrae stars from TESS (Molnar+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/133/H4201">J/PASP/133/H4201 : Times of maxima for 23 delta Scuti stars (Poro+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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