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<ri:Resource created="2008-08-26T08:53:20Z" 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>RR Lyrae in Northern Sky Variability Survey</title><shortName>J/AJ/132/1202</shortName><identifier>ivo://CDS.VizieR/J/AJ/132/1202</identifier><altIdentifier>doi:10.26093/cds/vizier.51321202</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kinemuchi K.</name></creator><creator><name>Smith H.A.</name></creator><creator><name>Wozniak P.R.</name></creator><creator><name>McKay T.A.</name></creator><date role="Updated">2018-01-05T08:55:49Z</date><date role="Created">2008-08-26T08:53:20Z</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>surveys</subject><subject>variable-stars</subject><subject>photometry</subject><subject>metallicity</subject><description>We use data from the Northern Sky Variability Survey (NSVS), obtained from the first-generation Robotic Optical Transient Search Experiment (ROTSE-I), to identify and study RR Lyrae variable stars in the solar neighborhood. We initially identified 1197 RRab (RR0) candidate stars brighter than the ROTSE median magnitude V=14. Periods, amplitudes, and mean V magnitudes are determined for a subset of 1188 RRab stars with well-defined light curves. Metallicities are determined for 589 stars by the Fourier parameter method and by the relationship between period, amplitude, and [Fe/H]. We comment on the difficulties of clearly classifying RRc (RR1) variables in the NSVS data set. Distances to the RRab stars are calculated using an adopted luminosity-metallicity relation with corrections for interstellar extinction. The 589 RRab stars in our final sample are used to study the properties of the RRab population within 5kpc of the Sun. The Bailey diagram of period versus amplitude shows that the largest component of this sample belongs to Oosterhoff type I. Metal-rich ([Fe/H]&gt;-1) RRab stars appear to be associated with the Galactic disk. Our metal-rich RRab sample may include a thin-disk, as well as a thick-disk population, although the uncertainties are too large to establish this. There is some evidence among the metal-rich RRab stars for a decline in scale height with increasing [Fe/H], as was found by Layden. The distribution of RRab stars with -1&lt;[Fe/H]&lt;-1.25 indicates that within this metallicity range the RRab stars are a mixture of stars belonging to halo and disk populations.</description><source format="bibcode">2006AJ....132.1202K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/132/1202</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/119/1901">J/AJ/119/1901 : ROTSE all-sky surveys for variable stars (Akerlof+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/2965">J/AJ/128/2965 : Red variables in the NSVS (Williams+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/312/111">J/A+A/312/111 : [Fe/H] from RR Lyrae light curves (Jurcsik+, 1996)</relatedResource><relatedResource>http://skydot.lanl.gov : NSVS database</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/AJ/132/1202</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/132/1202</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/132/1202</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/132/1202</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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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>NSVS</name><description>Northern Sky Variability Survey ID number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>n_NSVS</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Per</name><description>Period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Vamp</name><description>ROTSE amplitude, scaled to Johnson V band</description><unit>mag</unit><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmag</name><description>Mean intensity-weighted V band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/132/1202/table3</name><description>Photometric Metallicity of NSVS RRab Stars</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NSVS</name><description>Northern Sky Variability Survey ID number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Fe/H]AP</name><description>The Sandage (2004AJ....128..858S) [Fe/H] value</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Fe/H]AP</name><description>The 1{sigma} uncertainty in [Fe/H]AP</description><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]JK</name><description>? The Jurcsik &amp; Kovacs (1996, Cat. &lt;J/A+A/312/111&gt;) [Fe/H] value</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Fe/H]JK</name><description>? 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