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<ri:Resource created="2020-07-02T12:59:59Z" 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>Velocities and transit times in the Kepler-88 system</title><shortName>J/AJ/159/242</shortName><identifier>ivo://CDS.VizieR/J/AJ/159/242</identifier><altIdentifier>doi:10.26093/cds/vizier.51590242</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Weiss L.M.</name></creator><creator><name>Fabrycky D.C.</name></creator><creator><name>Agol E.</name></creator><creator><name>Mills S.M.</name></creator><creator><name>Howard A.W.</name></creator><creator><name>Isaacson H.,Petigura E.A.</name></creator><creator><name>Fulton B.</name></creator><creator><name>Hirsch L.</name></creator><creator><name>Sinukoff E.</name></creator><date role="Updated">2021-09-13T14:37:47Z</date><date role="Created">2020-07-02T12:59:59Z</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>exoplanets</subject><subject>variable-stars</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>We present the discovery of Kepler-88d (P_d_=1403{+/-}14days, Msin_i_d__=965{+/-}44M_{Earth}_=3.04{+/-}0.13M_J_, e_d_=0.41{+/-}0.03) based on six years of radial velocity (RV) follow-up from the W.M.Keck Observatory High Resolution Echelle Spectrometer spectrograph. Kepler-88 has two previously identified planets. Kepler-88b (KOI-142.01) transits in the NASA Kepler photometry and has very large transit timing variations (TTVs). Nesvorny+, performed a dynamical analysis of the TTVs to uniquely identify the orbital period and mass of the perturbing planet (Kepler-88c), which was later was confirmed with RVs from the Observatoire de Haute-Provence (OHP). To fully explore the architecture of this system, we performed photodynamical modeling on the Kepler photometry combined with the RVs from Keck and OHP and stellar parameters from spectroscopy and Gaia. Planet d is not detectable in the photometry, and long-baseline RVs are needed to ascertain its presence. A photodynamical model simultaneously optimized to fit the RVs and Kepler photometry yields the most precise planet masses and orbital properties yet for b and c: P_b_=10.91647{+/-}0.00014days, M_b_=9.5{+/-}1.2M_{Earth}_, P_c_=22.2649{+/-}0.0007days, and M_c=214.0{+/-}5.3M_{Earth}_. The photodynamical solution also finds that planets b and c have low eccentricites and low mutual inclination, are apsidally anti-aligned, and have conjunctions on the same hemisphere of the star. Continued RV follow-up of systems with small planets will improve our understanding of the link between inner planetary system architectures and giant planets.</description><source format="bibcode">2020AJ....159..242W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/159/242</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/A+A/363/1081">J/A+A/363/1081 : Non-linear limb-darkening law for LTE models (Claret 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/414/351">J/A+A/414/351 : ELODIE survey northern extrasolar planets III (Naef+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/622/1102">J/ApJ/622/1102 : The planet-metallicity correlation. 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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>[1575/4014] Barycentric Julian Date BJD-2454900</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RV</name><description>[-86.7/80.2] Radial velocity (1)</description><unit>m/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RV</name><description>[2.1/16.0] Uncertainty in RV (2)</description><unit>m/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SHK</name><description>[0.1178/0.208]? The Mt. Wilson S_HK_ value</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Inst</name><description>Instrument; HIRES or SOPHIE</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column></table><table><name>J/AJ/159/242/table6</name><description>Kepler-88b transit times and velocities</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>Epoch</name><description>[0/451] Epoch number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>T0</name><description>[55.08/4996] Transit midepoint time; BJD-2454900</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_T0</name><description>[0.0002/0.0344] Uncertainty in T0</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>[0.0016/0.0031] Impact parameter</description><unit>AU</unit><ucd>src.impactParam</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_b</name><description>[0.0001/0.0002] Uncertainty in b</description><unit>AU</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vel</name><description>[0.0507/0.0578] Planet velocity</description><unit>AU/d</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Vel</name><description>[0.0004/0.0005] Uncertainty in Vel</description><unit>AU/d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>