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<ri:Resource created="2018-09-10T07:44:29Z" 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>NIR photometry of 77 RR Lyrae stars</title><shortName>J/AJ/154/263</shortName><identifier>ivo://CDS.VizieR/J/AJ/154/263</identifier><altIdentifier>doi:10.26093/cds/vizier.51540263</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Karczmarek P.</name></creator><creator><name>Pietrzynski G.</name></creator><creator><name>Gorski M.</name></creator><creator><name>Gieren W.</name></creator><creator><name>Bersier D.</name></creator><date role="Updated">2018-10-22T07:48:27Z</date><date role="Created">2018-09-10T07:44:29Z</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>galaxies</subject><subject>variable-stars</subject><subject>infrared-photometry</subject><description>We have obtained single-phase near-infrared (NIR) magnitudes in the J and K bands for 77 RR Lyrae (RRL) stars in the Fornax Dwarf Spheroidal Galaxy. We have used different theoretical and empirical NIR period-luminosity-metallicity calibrations for RRL stars to derive their absolute magnitudes, and found a true, reddening-corrected distance modulus of 20.818+/-0.015(statistical)+/-0.116(systematic) mag. This value is in excellent agreement with the results obtained within the Araucaria Project from the NIR photometry of red clump stars (20.858+/-0.013 mag), the tip of the red giant branch (20.84+/-0.04+/-0.14 mag), as well as with other independent distance determinations to this galaxy. The effect of metallicity and reddening is substantially reduced in the NIR domain, making this method a robust tool for accurate distance determination at the 5% level. This precision is expected to reach the level of 3% once the zero points of distance calibrations are refined thanks to the Gaia mission. NIR period-luminosity-metallicity relations of RRL stars are particularly useful for distance determinations to galaxies and globular clusters up to 300 kpc, that lack young standard candles, like Cepheids.</description><source format="bibcode">2017AJ....154..263K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/154/263</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/AJ/123/840">J/AJ/123/840 : VI photometry of variable stars in Fornax (Bersier+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/345/747">J/MNRAS/345/747 : RR Lyrae in 4 Fornax globular clusters (Mackey+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/685/947">J/ApJ/685/947 : SX Phe stars in Fornax. II. (Poretti+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/701/1323">J/ApJ/701/1323 : Variable stars in Fornax dSph. III. 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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>FBW</name><description>Star identifier (FBW JHHMMSS.s+DDMMSS) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>Field</name><description>HAWK-I field</description><ucd>meta.id;obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>RAJ2000</name><description>Hour of Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Per</name><description>[0.33563/0.6754] Pulsational period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RRtype</name><description>[ab c] Type of RR Lyrae star (1)</description><ucd>meta.code;src.var</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Jmag</name><description>[19.989/20.755] HAWK-I apparent magnitude in J-band</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Jmag</name><description>[0.011/0.031] Uncertainty in Jmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ksmag</name><description>[19.806/20.499] HAWK-I apparent magnitude in K_s_-band</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Ksmag</name><description>[0.027/0.055] Uncertainty in Ksmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>JD-J</name><description>Julian date of J-band exposure</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>JD-Ks</name><description>Julian date of K_s_-band exposure</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>