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<ri:Resource created="2021-08-16T10:04:13Z" 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>NUV and FUV measurements of planet host stars</title><shortName>J/ApJ/890/23</shortName><identifier>ivo://CDS.VizieR/J/ApJ/890/23</identifier><altIdentifier>doi:10.26093/cds/vizier.18900023</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Loyd R.O.P.</name></creator><creator><name>Shkolnik E.L.</name></creator><creator><name>Schneider A.C.</name></creator><creator><name>Richey-Yowell T.</name></creator><creator><name>Barman T.S.,Peacock S.</name></creator><creator><name>Pagano I.</name></creator><date role="Updated">2021-09-29T13:33:22Z</date><date role="Created">2021-08-16T10:04:13Z</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>stellar-masses</subject><subject>ultraviolet-photometry</subject><subject>stellar-radii</subject><description>We search for evidence of the cause of the exoplanet radius gap, i.e., the dearth of planets with radii near 1.8R_{Earth}_. If the cause were photoevaporation, the radius gap should trend with proxies for the early-life high-energy emission of the planet-hosting stars. If, alternatively, the cause were core-powered mass loss, no such trends should exist. Critically, spurious trends between the radius gap and stellar properties arise from an underlying correlation with instellation. After accounting for this underlying correlation, we find that no trends remain between the radius gap and stellar mass or present-day stellar activity as measured by near-UV emission. We dismiss the nondetection of a radius gap trend with near-UV emission because present-day near-UV emission is unlikely to trace early-life high-energy emission, but we provide a catalog of Galaxy Evolution Explorer near-UV and far-UV emission measurements for general use. We interpret the nondetection of a radius gap trend with stellar mass by simulating photoevaporation with mass-dependent evolution of stellar high-energy emission. The simulation produces an undetectable trend between the radius gap and stellar mass under realistic sources of error. We conclude that no evidence, from this analysis or others in the literature, currently exists that clearly favors either photoevaporation or core-powered mass loss as the primary cause of the exoplanet radius gap. However, repeating this analysis once the body of well-characterized &lt;4R_{Earth}_ planets has roughly doubled could confirm or rule out photoevaporation.</description><source format="bibcode">2020ApJ...890...23L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/890/23</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/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/335">II/335 : Revised catalog of GALEX UV sources (GUVcat_AIS GR6+7) (Bianchi+ 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/785">J/AJ/135/785 : SDSS-DR5 low-mass star spectroscopic sample (West+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/422/2024">J/MNRAS/422/2024 : X-ray-age relation &amp; exoplanet evaporation (Jackson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/766/9">J/ApJ/766/9 : GALEX observations of exoplanet host stars (Shkolnik, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/780/159">J/ApJ/780/159 : Rotation-mass-ages of old field stars (Epstein+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/148/64">J/AJ/148/64 : HAZMAT. I. FUV &amp; NUV in early M stars (Shkolnik+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/109">J/AJ/154/109 : California-Kepler Survey. III. Planet radii (Fulton+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/848/34">J/ApJ/848/34 : CATalog of Stellar Unified Properties (Hinkel+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/122">J/AJ/155/122 : HAZMAT. III. Low-mass stars GALEX photometry (Schneider+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/264">J/AJ/156/264 : CKS. VII. Planet radius gap (Fulton+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/872/17">J/ApJ/872/17 : HAZMAT. V. UV &amp; X evolution of K stars (Richey-Yowell+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/875/29">J/ApJ/875/29 : Spectroscopic analysis of the CKS sample. I. (Martinez+, 2019)</relatedResource><relatedResource>http://archive.stsci.edu/galexView/ : GalexView home page</relatedResource><relatedResource>http://exoplanetarchive.ipac.caltech.edu/ : NASA exoplanet archive</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/890/23</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/890/23</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/890/23</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/890/23</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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Lower uncertainty in NUV (1)</description><unit>mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_NUV</name><description>[9.6e-16/1.5e-12]? Upper uncertainty in NUV (1)</description><unit>mW.m**-2</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_NUV</name><description>[-1/1]? Limit flag on NUV (2)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>NUVp</name><description>[1e-7/2.9e+10]? NUV band flux at planet (1)</description><unit>mW.m**-2</unit><ucd>phot.flux;em.UV</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_NUVp</name><description>[3.3e-7/2.6e+9]? Lower uncertainty in NUVp (1)</description><unit>mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_NUVp</name><description>[3.3e-7/2.6e+9]? Upper uncertainty in NUVp (1)</description><unit>mW.m**-2</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_NUVp</name><description>[-1/1]? Limit flag on NUVp (2)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>ExNUV</name><description>Excess NUV band flux at planet (1)(3)</description><unit>mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>e_ExNUV</name><description>Lower uncertainty in ExNUV (1)</description><unit>mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>E_ExNUV</name><description>Upper uncertainty in ExNUV (1)</description><unit>mW.m**-2</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>FUV</name><description>[8.4e-17/2.5e-10]? 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Upper limit flag on FUVp (2)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>ExFUV</name><description>Excess FUV band flux at planet (values between -9.1e+97 and 5e+09) (1)(3)</description><unit>mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>e_ExFUV</name><description>Lower uncertainty in ExFUV (1)</description><unit>mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>E_ExFUV</name><description>Upper uncertainty in ExFUV (1)</description><unit>mW.m**-2</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>l_ExFUV</name><description>[1]? Upper limit flag on ExFUV (2)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Per</name><description>[0.09/7.3e+6]? Orbital period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Per</name><description>[1e-8/3.6e+6]? Lower uncertainty in Per</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Per</name><description>[1e-8/3.6e+6]? Upper uncertainty in Per</description><unit>d</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_Per</name><description>[-1]? Lower limit flag on Per (2)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>r_Per</name><description>Bibcode reference for Per</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>S</name><description>[1.97e-6/636430]? Instellation (4)</description><unit>Earth</unit><ucd>phot.flux.bol</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_S</name><description>[1.2e-7/86461]? Lower uncertainty in S</description><unit>Earth</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_S</name><description>[1.2e-7/86461]? Upper uncertainty in S</description><unit>Earth</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>r_S</name><description>Bibcode reference for S</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Mass</name><description>[0.01/23.6]? 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>[0.002/97.1]? Lower uncertainty in Mass</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Mass</name><description>[0.002/97.1]? Upper uncertainty in Mass</description><unit>solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_Mass</name><description>Bibcode reference for Mass</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>L*</name><description>[-6.1/6.1] Log stellar luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_L*</name><description>[0/1] Lower uncertainty in L*</description><unit>log(solLum)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_L*</name><description>[0/1.5] Upper uncertainty in L*</description><unit>log(solLum)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_L*</name><description>Bibcode reference for L*</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Rp</name><description>[0.2/96.1]? Planet radius</description><unit>Earth</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Rp</name><description>[0.008/54.6]? Lower uncertainty in Rp</description><unit>Earth</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Rp</name><description>[0.008/54.6]? Lower uncertainty in Rp</description><unit>Earth</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_Rp</name><description>[-1/1]? Limit flag on Rp (2)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>r_Rp</name><description>Bibcode reference for Rp</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>b</name><description>[0/1] Transit impact parameter; unitless (5)</description><ucd>src.impactParam</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_b</name><description>[0/0.76] Lower uncertainty in b</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_b</name><description>[0/0.7] Lower uncertainty in b</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_b</name><description>[1]? Upper limit flag on b (2)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>logg</name><description>[0/5.52] Log stellar surface gravity (5)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logg</name><description>[0/3.6] Lower uncertainty in logg</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_logg</name><description>[0/0.6] Lower uncertainty in logg</description><unit>log(cm.s**-2)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>_RA</name><description>Position from SIMBAD host star (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position from SIMBAD host star (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>