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<ri:Resource created="2024-06-28T07:16:55Z" status="active" updated="2025-05-19T09:50:00Z" 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>Variable stars in the NIR in nearby galaxies. I.</title><shortName>J/AJ/167/247</shortName><identifier>ivo://CDS.VizieR/J/AJ/167/247</identifier><altIdentifier>doi:10.26093/cds/vizier.51670247</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bhardwaj A.</name></creator><creator><name>Rejkuba M.</name></creator><creator><name>Ngeow C.-C.</name></creator><creator><name>Marconi M.</name></creator><creator><name>Ripepi V.,Samantaray A.S.</name></creator><creator><name>Singh H.P.</name></creator><date role="Updated">2024-11-06T20:20:12Z</date><date role="Created">2024-06-28T07:16:55Z</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>dwarf-galaxies</subject><subject>infrared-photometry</subject><subject>variable-stars</subject><description>The Draco Dwarf spheroidal (dSph) galaxy is one of the nearest and the most dark-matter-dominated satellites of the Milky Way. We obtained multiepoch near-infrared (NIR, JHKs) observations of the central region of Draco dSph covering a sky area of ~21x21' using the WIRCam instrument at the 3.6m Canada-France-Hawaii Telescope. Homogeneous JHKs time-series photometry for 212 RR Lyrae (173 fundamental-mode, 24 first-overtone, and 15 mixed-mode variables) and five Anomalous Cepheids in Draco dSph are presented and used to derive their period-luminosity relations at NIR wavelengths for the first- time. The small scatter of ~0.05mag in these empirical relations for RR Lyrae stars is consistent with those in globular clusters and suggests a very small metallicity spread, up to ~0.2dex, among these centrally located variables. Based on empirically calibrated NIR period-luminosity-metallicity relations for RR Lyrae in globular clusters, we determined a distance modulus to Draco dSph of {mu}RRL=19.557{+/-}0.026mag. The calibrated Ks-band period-luminosity relations for Anomalous Cepheids in the Draco dSph and the Large Magellanic Cloud exhibit statistically consistent slopes but systematically different zero points, hinting at possible metallicity dependence of ~-0.3mag/dex. Finally, the apparent magnitudes of the tip of the red-giant branch in I and J bands also agree well with their absolute calibrations with the adopted RR Lyrae distance to Draco. Our recommended ~1.5% precise RR Lyrae distance, DDraco=81.55{+/-}0.98(statistical){+/-}1.17(systematic)kpc, is the most accurate and precise distance to Draco dSph galaxy.</description><source format="bibcode">2024AJ....167..247B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/167/247</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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/3222">J/AJ/124/3222 : VI photometry of Draco and UMi galaxies (Bellazzini+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/861">J/AJ/127/861 : RR Lyrae in Draco dSph (Bonanos+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/421/937">J/A+A/421/937 : Metal abundances of LMC RR Lyrae (Gratton+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/442/165">J/A+A/442/165 : IJKs photom of late-type stars in Draco dSph (Cioni+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/375/831">J/MNRAS/375/831 : Draco MegaCam, INT and HST photometry (Segall+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/1921">J/AJ/136/1921 : Variable stars of Draco dSph (Kinemuchi+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/502/505">J/A+A/502/505 : Ks photometry of LMC RR Lyrae (Borissova+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/4">J/AJ/144/4 : Prop of dwarf galaxies in Local Group (McConnachie+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/779/102">J/ApJ/779/102 : Metallicities of RGB stars in dwarf galaxies (Kirby+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/437/2307">J/MNRAS/437/2307 : LMC anomalous Cepheid Ks light curves (Ripepi+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/448/2717">J/MNRAS/448/2717 : Bayesian analysis resolved stellar spectra (Walker+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/153/204">J/AJ/153/204 : RR Lyrae stars from the PS1 3{pi} survey (Sesar+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/625/A1">J/A+A/625/A1 : RR Lyrae variables NIR light-curve templates (Braga+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/160/220">J/AJ/160/220 : NIR light curve 234 RR Lyrae in Messier 3 (Bhardwaj+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/633/A36">J/A+A/633/A36 : 3D kinematics in the Draco dwarf spheroidal (Massari+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/499/4040">J/MNRAS/499/4040 : RR Lyrae population in Draco dwarf galaxy (Muraveva+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/922/20">J/ApJ/922/20 : CFHT optical &amp; NIR obs. of RR Lyrae in M15 (Bhardwaj+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/253/42">J/ApJS/253/42 : The Araucaria Project; deep NIR phot. 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