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<ri:Resource created="2016-11-10T09:42:07Z" 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>Pan-STARRS 1: occurrence in the Kepler field</title><shortName>J/MNRAS/455/4212</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/455/4212</identifier><altIdentifier>doi:10.26093/cds/vizier.74554212</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Deacon N.R.</name></creator><creator><name>Kraus A.L.</name></creator><creator><name>Mann A.W.</name></creator><creator><name>Magnier E.A.</name></creator><creator><name>Chambers K.C.,Wainscoat R.J.</name></creator><creator><name>Tonry J.L.</name></creator><creator><name>Kaiser N.</name></creator><creator><name>Waters C.</name></creator><creator><name>Flewelling H.,Hodapp K.W.</name></creator><creator><name>Burgett W.S.</name></creator><date role="Updated">2024-08-15T20:17:04Z</date><date role="Created">2016-11-10T09:42:07Z</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>multiple-stars</subject><subject>solar-system-planets</subject><subject>proper-motions</subject><description>The NASA Kepler mission has revolutionized time-domain astronomy and has massively expanded the number of known extrasolar planets. However, the effect of wide multiplicity on exoplanet occurrence has not been tested with this data set. We present a sample of 401 wide multiple systems containing at least one Kepler target star. Our method uses Pan-STARRS 1 and archival data to produce an accurate proper motion catalogue of the Kepler field. Combined with Pan-STARRS 1 SED fits and archival proper motions for bright stars, we use a newly developed probabilistic algorithm to identify likely wide binary pairs which are not chance associations. As byproducts of this we present stellar SED templates in the Pan-STARRS 1 photometric system and conversions from this system to Kepler magnitudes. We find that Kepler target stars in our binary sample with separations above 6arcsec are no more or less likely to be identified as confirmed or candidate planet hosts than a weighted comparison sample of Kepler targets of similar brightness and spectral type. Therefore we find no evidence that binaries with projected separations greater than 3000au affect the occurrence rate of planets with P&lt;300d around FGK stars.</description><source format="bibcode">2016MNRAS.455.4212D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/455/4212</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/317">I/317 : The PPMXL Catalog (Roeser+ 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/322">I/322 : UCAC4 Catalogue (Zacharias+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/728/117">J/ApJ/728/117 : Kepler planetary candidates. 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Reduced {chi}^2^</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></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>KIC</name><description>Kepler identification number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right ascension (Eq=J2000, Ep=2013.0)</description><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Declination (Eq=J2000, Ep=2013.0)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>pmRA</name><description>Proper motion along RA (pmRA*cosDE)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmRA</name><description>rms uncertainty on pmRA</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmDE</name><description>Proper motion along DE</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmDE</name><description>rms uncertainty on pmDE</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>o_pmRA</name><description>Number of measurements for proper motions</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>gP1mag</name><description>? Pan-STARRS 1 g magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_gP1mag</name><description>? rms uncertainty on gP1mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>rP1mag</name><description>Pan-STARRS 1 r magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_rP1mag</name><description>? rms uncertainty on rP1mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>iP1mag</name><description>? Pan-STARRS 1i magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_iP1mag</name><description>? rms uncertainty on iP1mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>zP1mag</name><description>? Pan-STARRS 1 z magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_zP1mag</name><description>? rms uncertainty on zP1mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>yP1mag</name><description>? Pan-STARRS 1 y magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_yP1mag</name><description>? rms uncertainty on yP1mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>n_chi2r</name><description>[I] I for Infinity</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>n3PS1</name><description>Number of objects within 3 arcsec in Pan-STARRS 1</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n6PS1</name><description>Number of objects within 6 arcsec in Pan-STARRS 1</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n3USNO</name><description>Number of objects within 3 arcsec in USNO</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n6USNO</name><description>Number of objects within 6 arcsec in USNO</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>flag</name><description>[false true] if this object passes the 'good' proper motion test previously set out in the text</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>visual</name><description>[false true] Objects of Interest KOI which have passed or failed our visual proper motion inspection</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column></table><table><name>J/MNRAS/455/4212/table2</name><description>White dwarf candidates selected from their reduced proper motion diagram position</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>KIC</name><description>Kepler Identification number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>OName</name><description>Other name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="24*">char</dataType></column><column><name>Class</name><description>Literature classification</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>r_Class</name><description>? 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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>KIC1</name><description>KIC number of the primary</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n_KIC1</name><description>[cd] Note on KIC1 (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>pmRA1</name><description>Primary proper motion along RA, pmRAi*cosDE</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmRA1</name><description>rms uncertainty on pmRA1</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_pmRA1</name><description>[ab] Reference for proper motion (2)</description><ucd>meta.ref;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>pmDE1</name><description>Primary proper motion along DE</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmDE1</name><description>rms uncertainty on pmDE1</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SpType1</name><description>Primary spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>e_SpType1</name><description>rms uncertainty on SpType1</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MOD1</name><description>Primary distance modulus</description><unit>mag</unit><ucd>phot.mag.distMod</ucd><dataType 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Primary rotational period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Prot1</name><description>? rms uncertainty on Prot (2)</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pbin</name><description>[0.8/1] Binary probability</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r</name><description>Separation between primary and secondary stars in arcsec</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rAU</name><description>? Separation between primary and secondary stars in AU</description><unit>AU</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>KIC2</name><description>? Secondary Kepler identification number if exist</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>KOI2</name><description>Secondary KOI name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>RA2</name><description>Secondary right ascension (Eq=J2000, Ep=2013.0)</description><ucd>pos.eq.ra</ucd></column><column><name>DE2</name><description>Secondary declination (Eq=J2000, Ep=2013.0)</description><ucd>pos.eq.dec</ucd></column><column><name>pmRA2</name><description>Secondary proper motion along RA (pmRA*cosDE)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmRA2</name><description>rms uncertainty on pmRA2</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmDE2</name><description>Secondary proper motion along DE</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmDE2</name><description>rms uncertainty on pmDE2</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_pmRA2</name><description>Reference for proper motion (1)</description><ucd>meta.ref;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>MOD2</name><description>Secondary distance modulus</description><unit>mag</unit><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_MOD2</name><description>rms uncertainty on MOD2</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SpType2</name><description>Secondary spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>r_SpType2</name><description>Reference for SpType (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Prot2</name><description>? Secondary rotation period (2)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Prot2</name><description>? rms uncertainty on Prot2</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>