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<ri:Resource created="2025-11-18T14:22:53Z" status="active" updated="2026-07-02T11:52:22Z" 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>Light curves &amp; y-band magnitudes of RR Lyrae from LOT</title><shortName>J/AJ/169/58</shortName><identifier>ivo://CDS.VizieR/J/AJ/169/58</identifier><altIdentifier>doi:10.26093/cds/vizier/be-59-1t</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ngeow C.-C.</name></creator><creator><name>Cheng C.-Y.</name></creator><date role="Updated">2026-07-02T11:52:22Z</date><date role="Created">2025-11-18T14:22:53Z</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>infrared-photometry</subject><subject>variable-stars</subject><description>We complement the y-band template light curves for RR Lyrae to the well-established template light curves in the ugriz-band, where the latter have been adopted in the astroML/gatspy python package as one of the period-search methods for RR Lyrae. These y-band template light curves were constructed based on the z-band time series data taken from the Sloan Digital Sky Survey (SDSS), the y-band light curves from the Pan-STARRS1 survey, and dedicated y-band observations using the Lulin One-meter Telescope for RR Lyrae located in the SDSS Stripe 82 region. These y-band template light curves, 9 for the ab-type RR Lyrae and 3 for the c-type RR Lyrae, can be applied in conjunction to the ugriz-band template light curves for upcoming sky surveys involving the y-band, such as the Vera C. Rubin Observatory Legacy Survey of Space and Time.</description><source format="bibcode">2025AJ....169...58N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/169/58</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/358">I/358 : Gaia DR3 Part 4. 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