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<ri:Resource created="2016-06-24T12:18:01Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Kepler light curve of the EB star KIC 9532219</title><shortName>J/ApJ/820/1</shortName><identifier>ivo://CDS.VizieR/J/ApJ/820/1</identifier><altIdentifier>doi:10.26093/cds/vizier.18200001</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lee J.W.</name></creator><creator><name>Hong K.</name></creator><creator><name>Koo J.-R.</name></creator><creator><name>Park J.-H.</name></creator><date role="Updated">2017-07-04T07:08:21Z</date><date role="Created">2016-06-24T12:18:01Z</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>photometry</subject><subject>variable-stars</subject><description>KIC 9532219 is a W UMa-type eclipsing binary with an orbital period of 0.1981549days that is below the short-period limit (~0.22days) of the period distribution for contact binaries. The Kepler light curve of the system exhibits striking changes in both eclipse depths and light maxima. Applying third-body and spot effects, the light-curve synthesis indicates that the eclipsing pair is currently in a marginal contact stage with a mass ratio of q=1.20, an orbital inclination of i=66.0{deg}, a temperature difference of T_1_-T_2_=172K, and a third light of l_3_=75.9%. To understand the light variations with time, we divided up the light curve into 312 segments and analyzed them separately. The results reveal that variation of eclipse depth is primarily caused by changing amounts of contamination due to the nearby star KIC 9532228 between the Kepler Quarters and that the variable O'Connell effect originates from the starspot activity on the less massive primary component. Based on our light-curve timings, a period study of KIC 9532219 indicates that the orbital period has varied as a combination of a downward parabola and a light-travel-time (LTT) effect due to a third body, which has a period of 1196 days and a minimum mass of 0.0892M_{sun}_ in an orbit of eccentricity 0.150. The parabolic variation could be a small part of a second LTT orbit due to a fourth component in a wider orbit, instead of either mass transfer or angular momentum loss.</description><source format="bibcode">2016ApJ...820....1L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/820/1</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>related-to</relationshipType><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/AJ/149/197">J/AJ/149/197 : Minima of 10 Kepler eclipsing binaries (Zasche+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/93">J/AJ/149/93 : Eclipse timings of KIC 5621294 (Lee+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/452/3561">J/MNRAS/452/3561 : Kepler eclipsing binary stars. K2 (LaCourse+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/437/3473">J/MNRAS/437/3473 : Temperatures of Kepler eclipsing binaries (Armstrong+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/126/914">J/PASP/126/914 : Kepler eclipsing binary stars. V. (Conroy+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/2">J/ApJS/211/2 : Revised properties of Q1-16 Kepler targets (Huber+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/148/37">J/AJ/148/37 : Long-term photometric behavior of V404 Lyr (Lee+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/45">J/AJ/147/45 : Kepler mission IV. 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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>BJD</name><description>Barycentric Julian Date of observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>lambda</name><description>[53.1/310.8] Longitude of spot center</description><unit>deg</unit><ucd>pos.galactic.lon</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rs</name><description>[10.7/16] Angular radius</description><unit>deg</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ts</name><description>[0.8/1] Spot temperature factor (1)</description><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>i</name><description>[64.6/68] Orbital inclination</description><unit>deg</unit><ucd>src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>T1</name><description>[5158/5225] Primary's effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Omega1</name><description>[4.06/4.09] Primary's potential</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>q</name><description>[1.19/1.21] Mass ratio</description><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l1</name><description>[0.10/0.15] Primary's light contribution</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l3</name><description>[0.7/0.8] Third light contribution</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/820/1/table1</name><description>Light levels of KIC 9532219 at four characteristic phases</description><column><name>e_maxI</name><description>[0/0.03] Uncertainty in maxI</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</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>BJD</name><description>Mean Barycentric Julian Date of observation (1)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>minI</name><description>[16.17/16.2] Kepler magnitude at phase 0.0</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_minI</name><description>[0/0.03] Uncertainty in minI</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>maxI</name><description>[16.1/16.11] Kepler magnitude at phase 0.25</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>minII</name><description>[16.16/16.2] Kepler magnitude at phase 0.5</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_minII</name><description>[0/0.03] Uncertainty in minI</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>maxII</name><description>[16.1/16.11] Kepler magnitude at phase 0.75</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_maxII</name><description>[0/0.03] Uncertainty in maxII</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>