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<ri:Resource created="2017-10-04T13:16:20Z" 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>KIC 11401845 eclipse timings</title><shortName>J/ApJ/835/189</shortName><identifier>ivo://CDS.VizieR/J/ApJ/835/189</identifier><altIdentifier>doi:10.26093/cds/vizier.18350189</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lee J.W.</name></creator><creator><name>Hong K.</name></creator><creator><name>Kim S.-L.</name></creator><creator><name>Koo J.-R.</name></creator><date role="Updated">2017-11-06T13:56:55Z</date><date role="Created">2017-10-04T13:16:20Z</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>eclipsing-binary-stars</subject><subject>photometry</subject><description>We report the Kepler photometry of KIC 11401845 displaying multiperiodic pulsations, superimposed on binary effects. Light-curve synthesis shows that the binary star is a short-period detached system with a very low mass ratio of q=0.070 and filling factors of F_1_=45% and F_2_=99%. Multiple-frequency analyses were applied to the light residuals after subtracting the synthetic eclipsing curve from the observed data. We detected 23 frequencies with signal-to-noise ratios larger than 4.0, of which the orbital harmonics (f_4_, f_6_, f_9_, f_15_) in the low-frequency domain may originate from tidally excited modes. For the high frequencies of 13.7-23.8day^-1^, the period ratios and pulsation constants are in the ranges of P_pul_/P_orb_=0.020-0.034 and Q=0.018-0.031days, respectively. These values and the position on the Hertzsprung-Russell diagram demonstrate that the primary component is a {delta} Sct pulsating star. We examined the eclipse timing variation of KIC 11401845 from the pulsation-subtracted data and found a delay of 56+/-17s in the arrival times of the secondary eclipses relative to the primary eclipses. A possible explanation of the time shift may be some combination of a light-travel-time delay of about 34s and a very small eccentricity of e.cos{omega}&lt;0.0002. This result represents the first measurement of the Romer delay in noncompact binaries.</description><source format="bibcode">2017ApJ...835..189L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/835/189</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/106/2096">J/AJ/106/2096 : Limb-darkening coefficients in binaries (Van Hamme 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/373/435">J/MNRAS/373/435 : Angular momentum evolution of Algol binaries</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/A+ARV/18.67">J/other/A+ARV/18.67 : Accurate masses and radii of normal stars (Torres+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/753/101">J/ApJ/753/101 : Kepler eclipse timings of KIC 9472174 (Barlow+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/557/A79">J/A+A/557/A79 : Spectra of KIC10661783 (Lehmann+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/104">J/AJ/147/104 : Photometry and velocities of 1SWASP J093010A and B (Koo+, 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/ApJ/812/46">J/ApJ/812/46 : Transit metric for Q1-Q17 Kepler candidates (Thompson+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/68">J/AJ/151/68 : Kepler Mission. 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Eclipsing binaries in DR3 (Kirk+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/833/170">J/ApJ/833/170 : Spots parameters for LCs of the EB star KIC 6048106 (Lee, 2016)</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/ApJ/835/189</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/835/189</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/835/189</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/835/189</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/835/189</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/835/189</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/835/189/table3</name><description>Eclipse timings measured from both datasets including and removing the pulsations</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>O-BJD</name><description>Observed Barycentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_O-BJD</name><description>[0.0001/0.003] Error in O-BJD</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>O-(O-C1)</name><description>[-0.0009/0.002] The (O-C) residual for observed data</description><unit>d</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Epoch</name><description>Epoch</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Min</name><description>Minimum type ("I": orbital phase 0.0 or "II": orbital phase 0.5)</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>PS-BJD</name><description>Pulsation-Subtracted Barycentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_PS-BJD</name><description>[0.0001/0.0008] Error in PS-BJD</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>PS-(O-C2)</name><description>[-0.0008/0.0008] The (O-C) residual for Pulsation-Subtracted data</description><unit>d</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>