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<ri:Resource created="2022-01-17T13:22:34Z" status="active" updated="2025-09-09T14:15:11Z" 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>Times of maxima for 23 delta Scuti stars</title><shortName>J/PASP/133/H4201</shortName><identifier>ivo://CDS.VizieR/J/PASP/133/H4201</identifier><altIdentifier>doi:10.26093/cds/vizier.61343201</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Poro A.</name></creator><creator><name>Paki E.</name></creator><creator><name>Mazhari G.</name></creator><creator><name>Sarabi S.</name></creator><creator><name>Kahraman Alicavus F.,Ahangarani Farahani F.</name></creator><creator><name>Guilani H.</name></creator><creator><name>Popov A.A.</name></creator><creator><name>Zubareva A.M.,Zarei Jalalabadi B.</name></creator><creator><name>Nourmohammad M.</name></creator><creator><name>Davoudi F.</name></creator><creator><name>Sabaghpour Arani Z.,Ghalee A.</name></creator><date role="Updated">2025-09-09T14:15:11Z</date><date role="Created">2022-01-17T13:22:34Z</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>ccd-photometry</subject><subject>ephemerides</subject><description>The multi-color CCD photometric study of 27 delta Scuti stars is presented. By using approximately three years of photometric observations, we obtained the times of maxima and magnitude changes during the observation time interval for each star. The ephemeris of our delta Scuti star was calculated based on the Markov Chain Monte Carlo (MCMC) method using the observed times of maxima and the period of star' oscillations. We used the Gaia EDR3 parallaxes to calculate the luminosities and also the absolute magnitudes of these delta Scuti stars. The fundamental physical parameters of all studied stars, such as mass and radius, were estimated. We determined the pulsation modes of the stars based on the pulsation constants. Moreover, the period-luminosity relation of delta Scuti stars was investigated and discussed. Then, by using a machine learning classification, new P-L relations for fundamental and overtone modes are presented.</description><source format="bibcode">2021PASP..133h4201P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/133/H4201</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/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASP/133/H4201</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASP/133/H4201</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASP/133/H4201</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/PASP/133/H4201</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/PASP/133/H4201</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/PASP/133/H4201</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/PASP/133/H4201/table2 (The Coordinates, magnitude, and distance of our delta Scuti stars (from: Gaia EDR3))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/PASP/133/H4201/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/PASP/133/H4201/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PASP/133/H4201/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>306.26949064028054</ra><dec>50.449410231653395</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/15489-15491 15496-15497</spatial><spectral>1.9867573869263685e-19 3.916500758235022e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/PASP/133/H4201?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/PASP/133/H4201/table2</name><description>The Coordinates, magnitude, and distance of our delta Scuti stars (from: Gaia EDR3)</description><column><name>_RA.icrs</name><description>Right ascension (ICRS) at Epoch=J2016. 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Distance</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Dist</name><description>? rms uncertainty on Dist</description><unit>pc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FileName</name><description>Name of the file with times of maximum in subdirectory tm</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column></table></schema></tableset></ri:Resource>