<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2025-01-17T12:37:49Z" status="active" updated="2025-09-30T20:07:43Z" 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>Single vs mult. planet syst. radius distribution</title><shortName>J/AJ/168/92</shortName><identifier>ivo://CDS.VizieR/J/AJ/168/92</identifier><altIdentifier>doi:10.26093/cds/vizier.51680092</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Liberles B.T.</name></creator><creator><name>Dittmann J.A.</name></creator><creator><name>Elardo S.M.</name></creator><creator><name>Ballard S.</name></creator><date role="Updated">2025-09-30T20:07:43Z</date><date role="Created">2025-01-17T12:37:49Z</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>multiple-stars</subject><subject>exoplanets</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>trigonometric-parallax</subject><subject>stellar-radii</subject><subject>stellar-masses</subject><description>Previous work has established the enhanced occurrence of compact systems of multiple small exoplanets around metal-poor stars. Understanding the origin of this effect in the planet formation process is a topic of ongoing research. Here we consider the radii of planets residing in systems of multiple transiting planets, compared to those residing in single-transiting systems, with a particular focus on late-type host stars. We investigate whether the two radius distributions are consistent with being drawn from the same underlying planetary population. We construct a planetary sample of 290 planets around late K and M dwarfs containing 149 planets from single-transiting planetary systems and 141 planets from multi-transiting compact multiple planetary systems (54 compact multiples). We performed a two-sample Kolmogorov-Smirnov test, Mann-Whitney U test, and Anderson-Darling k-sampling test on the radius distributions of our two samples. We find statistical evidence (p&lt;0.0026) that planets in compact multiple systems are larger, on average, than their single-transiting counterparts for planets with R_p_&lt;6R_{Earth}_. We determine that the offset cannot be explained by detection bias. We investigate whether this effect could be explained via more efficient outgassing of a secondary atmosphere in compact multiple systems due to the stress and strain forces of interplanetary tides on planetary interiors. We find that this effect is insufficient to explain our observations without significant enrichment in H_2_O compared to Earth-like bulk composition.</description><source format="bibcode">2024AJ....168...92L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/168/92</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</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/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/622/1102">J/ApJ/622/1102 : The planet-metallicity correlation. (Fischer+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/112">J/AJ/142/112 : KIC photometric calibration (Brown+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/197/8">J/ApJS/197/8 : Kepler's candidate mult. transiting planets (Lissauer+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/767/95">J/ApJ/767/95 : Stellar parameters of smallest KIC stars (Dressing+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/790/146">J/ApJ/790/146 : Planets in Kepler's multi-transiting systems (Fabrycky+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/787/47">J/ApJ/787/47 : 106 Kepler ultra-short-period planets (Sanchis-Ojeda+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/814/130">J/ApJ/814/130 : Planet occurrence rates calculated for KOIs (Mulders+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/158">J/AJ/152/158 : Final Kepler transiting planet search (DR25) (Twicken+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/109">J/AJ/154/109 : California-Kepler Survey (CKS). III. Radii (Fulton+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/229/30">J/ApJS/229/30 : Revised properties of Q1-17 Kepler targets (Mathur+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/48">J/AJ/155/48 : California-Kepler Survey. V. Masses &amp; radii (Weiss+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/158/109">J/AJ/158/109 : Occurrence rates of planets orbiting FGK stars (Hsu+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/160/253">J/AJ/160/253 : IR photometry of late-type dwarfs in Kepler Field (Lu+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/203">J/AJ/161/203 : A sample of M or K-dwarfs from KIC and Gaia (Anderson+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/650/A201">J/A+A/650/A201 : 10 parsec sample in the Gaia era first update (Reyle+, 2021)</relatedResource><relatedResource>http://exoplanetarchive.ipac.caltech.edu/ : NASA Exoplanet Archive homepage</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/168/92</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/168/92</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/168/92</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/168/92</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/168/92</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/168/92</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/168/92/table1 (Stellar Parameters)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/168/92/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/168/92/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/168/92/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>285.2871108</ra><dec>41.8611578</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/3733 3736 3741-3743 3778 3782 3785 6/14578-14579 14581 14584-14585 14588 14591 14734 14752-14753 14756-14757 14759 14762-14764 14766 14768 14770-14773 14775-14776 14778-14779 14781-14782 14794 14816 14818-14819 14824-14826 14830 14915 14917 14919-14921 14925 14930-14931 14937 14939 14942 14948 14950 14954 14957-14959 14962-14963 15040-15041 15044 15057 15060-15061 15104-15105 15107-15109 15111 15116 15118-15119 15121-15122 15126-15127 15132-15134 15137-15138 15145 15147-15149 15151 15155-15158 15160 15168-15169 15171-15172 15174</spatial><spectral>8.650015785639275e-20 4.621782916333392e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/168/92?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/168/92/table1</name><description>Stellar Parameters</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>Gaia</name><description>Gaia DR3 source identifier</description><ucd>meta.id;meta.main</ucd></column><column><name>plx</name><description>[0.88/15]? Gaia DR3 parallax</description><unit>mas</unit><ucd>pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Positions from SIMBAD (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from SIMBAD (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>NEA</name><description>Display data from the NASA Exoplanet Archive (http://exoplanetarchive.ipac.caltech.edu)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>RAdeg</name><description>[280.3/300.4] Gaia DR3 right ascension (ICRS) at Epoch=2016.0</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>e_RAdeg</name><description>[0.01/1] Uncertainty in RAdeg</description><unit>mas</unit><ucd>stat.error;pos.eq.ra;meta.main</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DEdeg</name><description>[37.5/51.5] Gaia DR3 declination (ICRS) at Epoch=2016.0</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>e_DEdeg</name><description>[0.01/1] Uncertainty in DEdeg</description><unit>mas</unit><ucd>stat.error;pos.eq.dec;meta.main</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_plx</name><description>[0.01/0.5]? Uncertainty in plx</description><unit>mas</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Gflux</name><description>[2206/195025] Gaia DR3 apparent broad band flux; electrons/s</description><unit>ct/s</unit><ucd>phot.flux.density;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Gflux</name><description>[1.7/78.2] Uncertainty in Gflux</description><unit>ct/s</unit><ucd>stat.error;phot.flux.density;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gmag</name><description>[12.46/17.33] Gaia DR3 apparent broad band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BPflux</name><description>[540/60133] Gaia DR3 apparent blue band flux; electrons/s</description><unit>ct/s</unit><ucd>phot.flux;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_BPflux</name><description>[7/106] Uncertainty in BPflux</description><unit>ct/s</unit><ucd>stat.error;phot.flux;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BPmag</name><description>[13.39/18.51] Gaia DR3 apparent blue band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RPflux</name><description>[1934/197399] Gaia DR3 apparent red band flux; electrons/s</description><unit>ct/s</unit><ucd>phot.flux;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_RPflux</name><description>[8.6/220.1] Uncertainty in Rflux</description><unit>ct/s</unit><ucd>stat.error;phot.flux;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RPmag</name><description>[11.51/16.54] Gaia DR3 apparent red band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[3283/6067]? Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Teff</name><description>[3273/5948]? Lower uncertainty in Teff</description><unit>K</unit><ucd>stat.error;stat.min;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Teff</name><description>[3309/6212]? Upper uncertainty in Teff</description><unit>K</unit><ucd>stat.error;stat.max;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Jmag</name><description>[10.29/14.84] 2MASS apparent J band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Jmag</name><description>[0.019/0.05] Uncertainty in Jmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hmag</name><description>[9.68/14.23] 2MASS apparent H band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Hmag</name><description>[0.015/0.06] Uncertainty in Hmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ksmag</name><description>[9.50/13.89] 2MASS apparent Ks band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Ksmag</name><description>[0/0.07] Uncertainty in Ksmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>gmag</name><description>[13.81/18.7] Apparent g band magnitude (Sloan)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_gmag</name><description>[0.025] Uncertainty in gmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rmag</name><description>[12.77/17.47] Apparent r band magnitude (Sloan)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_rmag</name><description>[0.02] Uncertainty in rmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>imag</name><description>[12.45/16.97] Apparent i band magnitude (Sloan)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_imag</name><description>[0.02] Uncertainty in imag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>KIC</name><description>Kepler Input Catalog Identifier</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>Np</name><description>Number of planets for this star (link to Table 4)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Rad</name><description>[0.20/0.82] Stellar radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Rad</name><description>[0.004/0.05]? Upper uncertainty in Rad</description><unit>solRad</unit><ucd>stat.error;stat.max;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Rad</name><description>[0.005/0.05]? Lower uncertainty in Rad</description><unit>solRad</unit><ucd>stat.error;stat.min;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Mass</name><description>[0.18/0.78]? Stellar mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Mass</name><description>[0/0.06]? Upper uncertainty in Mass</description><unit>solMass</unit><ucd>stat.error;stat.max;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Mass</name><description>[0/0.06]? Lower uncertainty in Mass</description><unit>solMass</unit><ucd>stat.error;stat.min;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>2M</name><description>Display the 2MASS data (II/246) within 3"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="28*">char</dataType><flag>nullable</flag></column></table><table><name>J/AJ/168/92/table4</name><description>Planet Parameters</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 Input Catalog Identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Type</name><description>Type of planetary system (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Rp</name><description>[0.38/29.65] Planetary radius value</description><unit>(6.3781x10+6m)</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rp</name><description>[0.001/186] Relative percent uncertainty in Rp</description><unit>%</unit><ucd>stat.error;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Per</name><description>[0/628.2] Orbital period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>