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<ri:Resource created="2026-08-10T10:02:38Z" status="active" updated="2026-08-10T09:15:00Z" 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>RR Lyrae stars from Gaia DR3 and ZTF time series</title><shortName>J/ApJS/281/38</shortName><identifier>ivo://CDS.VizieR/J/ApJS/281/38</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhang J.</name></creator><creator><name>Chen X.</name></creator><creator><name>Wang S.</name></creator><creator><name>Wang J.</name></creator><creator><name>Deng L.</name></creator><date role="Updated">2026-08-10T09:15:00Z</date><date role="Created">2026-08-10T10:02:38Z</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>surveys</subject><subject>visible-astronomy</subject><subject>photometry</subject><description>RR Lyrae (RRL) variable stars are cornerstone distance indicators. In particular, double-mode RR Lyrae (RRd) stars enable period-luminosity relations (PLRs) that are less sensitive to metallicity, reducing systematic biases in distance measurements. However, their utility has been limited by a global sample of only ~3000 objects. We develop an automated RRd-screening pipeline and apply it to a crossmatched sample between the Gaia DR3 RRL catalog and Zwicky Transient Facility (ZTF) DR22 time-series photometry. The workflow combines Lomb-Scargle period searches, iterative prewhitening, period-ratio constraints that suppress ~1 day sampling aliases, and amplitude-based quality cuts, enabling large-scale RRd star screening. We produce two ZTF-based catalogs: (i) 39,322 reliable single-mode RRL stars (40.5% of the crossmatched set) and (ii) 969 RRd stars. Among the RRd stars, 614 objects are newly identified, substantially enlarging this previously scarce sample; the catalog achieves an estimated completeness of 47.7%. The PLR derived from the newly discovered RRd stars agrees with the LMC-based relation, though with larger uncertainties. Incorporating these stars will help tighten the RRd PLR and improve distance measurements. Looking ahead, systematic RRd searches with upcoming surveys such as the Legacy Survey of Space and Time and the China Space Station Telescope should further extend high-accuracy distances across the Local Group and strengthen their cosmological applications.</description><source format="bibcode">2025ApJS..281...38Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/281/38</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/II/366">II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/358">I/358 : Gaia DR3 Part 4. Variability (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/64/177">J/AcA/64/177 : VI light curves of Gal. Bulge RR Lyrae (Soszynski+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/219/25">J/ApJS/219/25 : LCs of RR Lyrae stars in M3 (NGC5272) (Jurcsik+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/807/127">J/ApJ/807/127 : Properties of 70 RR Lyrae stars in LMC bar (Muraveva+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/487/5584">J/MNRAS/487/5584 : First-overtone RR Lyrae stars from OGLE (Netzel+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/625/A14">J/A+A/625/A14 : Reclassification of Cepheids in the Gaia DR2 (Ripepi+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/69/321">J/AcA/69/321 : OGLE RR Lyrae stars in Gal. bulge &amp; disk (Soszynski+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/249/18">J/ApJS/249/18 : The ZTF catalog of periodic variable stars (Chen+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/513/1958">J/MNRAS/513/1958 : Study of RR Lyrae stars in MW substructures (Wang+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/NatAs/7.1081">J/other/NatAs/7.1081 : Double-mode RR Lyrae stars data (Chen+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/674/A18">J/A+A/674/A18 : Gaia DR3. 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