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<ri:Resource created="2013-06-06T09:28:52Z" 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>Photometry of W UMa eclipsing binaries</title><shortName>J/AJ/143/99</shortName><identifier>ivo://CDS.VizieR/J/AJ/143/99</identifier><altIdentifier>doi:10.26093/cds/vizier.51430099</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Terrell D.</name></creator><creator><name>Gross J.</name></creator><creator><name>Cooney W.R.</name></creator><date role="Updated">2017-12-12T14:45:18Z</date><date role="Created">2013-06-06T09:28:52Z</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>eclipsing-binary-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>interstellar-reddening</subject><description>We report on a BVRcIc survey of field W Ursae Majoris (UMa) binary stars and present accurate colors for 606 systems that have been observed on at least three photometric nights from a robotic observatory in southern Arizona. Comparison with earlier photometry for a subset of the systems shows good agreement. We investigate two independent methods of determining the interstellar reddening, although both have limitations that can render them less effective than desired. A subset of 101 systems shows good agreement between the two reddening methods.</description><source format="bibcode">2012AJ....143...99T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/143/99</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/B/gcvs">B/gcvs : General Catalogue of Variable Stars (Samus+ 2007-2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/119">V/119 : Catalogue of field contact binary stars (Pribulla+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/621">J/AJ/131/621 : A catalog of 1022 bright contact binary stars (Gettel+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/357/497">J/MNRAS/357/497 : Kinematics of W UMa-type binaries (Bilir+, 2005)</relatedResource><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/A+A/311/523">J/A+A/311/523 : Photometry of W UMa (Maceroni+, 1996)</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/143/99</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/143/99</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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44635 44664 44772 44929 44945 44963 45003 48562 48942 49127</spatial><spectral>3.322582951404819e-19 3.852589004194616e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/143/99?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/143/99/table1</name><description>The BVRcIc colors of 606 W Ursae Majoris binaries</description><column><name>o_ID</name><description>[3/54] Number of observations</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><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>ID</name><description>Star identification (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType><flag>primary</flag></column><column><name>RAJ2000</name><description>Right ascension in decimal degrees (J2000) (2)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination in decimal degrees (J2000) (2)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Period</name><description>Orbital period of the binary (3)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B-V</name><description>The measured (B-V) color index</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_B-V</name><description>Error in B-V (4)</description><unit>mag</unit><ucd>stat.error;phot.color;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>V-Rc</name><description>The measured (V-Rc) color index</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_V-Rc</name><description>Error in V-Rc (4)</description><unit>mag</unit><ucd>stat.error;phot.color;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rc-Ic</name><description>The measured (Rc-Ic) color index</description><unit>mag</unit><ucd>phot.color;em.opt.R;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rc-Ic</name><description>Error in Rc-Ic (4)</description><unit>mag</unit><ucd>stat.error;phot.color;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>V-Ic</name><description>The (V-Ic) color index (5)</description><unit>mag</unit><ucd>phot.color;em.opt.V;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_V-Ic</name><description>Error in V-Ic (4)</description><unit>mag</unit><ucd>stat.error;phot.color;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmax</name><description>[8.9/13] V magnitude at maximum brightness (3)</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmin</name><description>[9.2/13.8] V magnitude at minimum brightness (3)</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E</name><description>Display the reddening estimates for this variable (table2)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>M</name><description>Cross-matches with Gettel et al., 2006, Cat. J/AJ/131/621, and Pitbulla et al., 2003, Cat. V/119, within 10"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/AJ/143/99/table2</name><description>Reddening estimates for the 101 systems showing a maximum difference of 0.02mag in E(B-V) between the color difference method and the N_H1_ method</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>ID</name><description>Star identification</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>E(B-V)0</name><description>Reddening produced with the Color Difference method</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_E(B-V)0</name><description>Uncertainty on E(B-V)0</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E(B-V)1</name><description>Reddening produced with the N_H1_ method (2)</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>