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<ri:Resource created="2024-06-10T09:17:02Z" status="active" updated="2025-06-13T15:25:00Z" 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>Asteroseismic study of TESS mission's DSCTs</title><shortName>J/MNRAS/505/1476</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/505/1476</identifier><altIdentifier>doi:10.26093/cds/vizier.75051476</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hasanzadeh A.</name></creator><creator><name>Safari H.</name></creator><creator><name>Ghasemi H.</name></creator><date role="Updated">2024-11-06T20:33:53Z</date><date role="Created">2024-06-10T09:17:02Z</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>photometry</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>standard-stars</subject><description>We investigate the relationship between the asteroseismic indices and the physical quantities of 438 {delta} Scuti (DSCT) stars observed by the Transiting Exoplanet Survey Satellite (TESS) mission at 26 sectors. We study the scaling relations of stellar parameters (effective temperature, surface gravity, density, etc.) and asteroseismic indices such as fundamental frequency, large frequency separation ({Delta}{nu}), frequency of the highest peak in the spectrum, and the peak of the envelope of oscillation mode ({nu}_max_) for DSCT targets. Using an empirical relation and a 2D autocorrelation method, we determine the large frequency separation for targets. We obtain a highly positive correlation between the fundamental radial pressure mode and the large separation for one- third of targets. We find a scaling relation between the large separation and {nu}_max_ as {Delta}{nu}= 0.49{nu}_max_^{0.68}^, which is similar to that of the solar-like and red giant stars. We show a strong positive correlation between the effective temperature and {nu}_max_ (Pearson correlation R = 0.65). We also obtain a very strong positive correlation (R = 0.86) between the effective temperature multiplying by the surface gravity and {nu}_max_.</description><source format="bibcode">2021MNRAS.505.1476H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/505/1476</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/A+A/534/A125">J/A+A/534/A125 : Variability of A- and F-stars from Kepler (Uytterhoeven+ 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/68">J/AJ/149/68 : A-F type variable stars from Kepler (Bradley+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/236/42">J/ApJS/236/42 : Asteroseismology of ~16000 Kepler red giants (Yu+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/638/A59">J/A+A/638/A59 : delta Scuti stars with TESS (Barcelo Forteza+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/164">V/164 : LAMOST DR5 catalogs (Luo+, 2019)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>TIC</name><description>Tess Input Catalog identifier (TIC) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>Sector</name><description>Sky mapped sectors surveyed by TESS mission which divides the sky into 26 sectors (Sector) (1)</description><ucd>obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Teff</name><description>Effective temperature (Teff) (1)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>? 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Mean error on R (R_error) (1)</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logg</name><description>Surface gravity in log scale (logg) (1)</description><unit>log(cm.s**-2)</unit><ucd>instr.scale</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logg</name><description>? Mean error on log(g) (logg_error) (1)</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>L</name><description>Stellar luminosity (L) (1)</description><unit>solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_L</name><description>? Mean error on L (L_error) (1)</description><unit>solLum</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>rho</name><description>Stellar density in solar scale (rho) (1)</description><unit>Sun</unit><ucd>phys.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>nuf</name><description>? Fundamental frequency (nuf) (2)</description><unit>d**-1</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>nu(Amax)</name><description>The frequency related to the highest peak amplitude of the DSCT star spectrum (nuAmax) (3)</description><unit>d**-1</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>numax</name><description>The peak of the envelope of oscillation mode (numax) (4)</description><unit>d**-1</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dnu</name><description>The large frequency separation (Deltanu) (5)</description><unit>d**-1</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>