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<ri:Resource created="2019-07-05T11:59:07Z" 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>TESS M-dwarf exoplanetary systems</title><shortName>J/AJ/157/113</shortName><identifier>ivo://CDS.VizieR/J/AJ/157/113</identifier><altIdentifier>doi:10.26093/cds/vizier.51570113</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ballard S.</name></creator><date role="Updated">2019-07-31T05:43:35Z</date><date role="Created">2019-07-05T11:59:07Z</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>dwarf-stars</subject><subject>m-stars</subject><subject>exoplanets</subject><subject>stellar-distance</subject><subject>effective-temperature</subject><subject>stellar-masses</subject><subject>stellar-radii</subject><subject>astronomical-models</subject><description>We present a study of the M-dwarf exoplanetary systems forthcoming from NASA's TESS mission. While the mission's footprint is too complex to be characterized by a single detection completeness, we extract ensemble completeness functions that recover the planet detections from previous work for stars between 3200 and 4000 K. We employ these completeness functions, together with a dual- population planet occurrence model that includes compact multiple planetary systems, to infer anew the planet yield. We predict both the number of M-dwarf planets likely from TESS and their system architectures. We report four main findings. First, TESS will likely detect more planets orbiting M dwarfs that previously predicted. Around stars with effective temperatures between 3200 and 4000 K, we predict that TESS will find 1274+/-241 planets orbiting 1026+/-182 stars, a 1.2-fold increase over previous predictions. Second, TESS will find two or more transiting planets around 20% of these host stars, a number similar to the multiplicity yield of NASA's Kepler mission. Third, TESS light curves in which one or more planets are detected will often contain transits of additional planets below the detection threshold of TESS. Among a typical set of 200 TESS hosts to one or more detected planets, 93+/-17 transiting planets will be missed. Transit follow-up efforts with the photometric sensitivity to detect an Earth or larger around a mid-M dwarf, even with very modest period completeness, will readily result in additional planet discoveries. Fourth, the strong preference of TESS for systems of compact multiples indicates that TESS planets will be dynamically cooler on average than Kepler planets, with 90% of TESS planets residing in orbits with e&lt;0.15. We include both (1) a predicted sample of planets detected by TESS orbiting stars between 3200 and 4000 K, including additional nontransiting planets, or transiting and undetected planets orbiting the same star and (2) sample completeness functions for use by the community.</description><source format="bibcode">2019AJ....157..113B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/157/113</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/J/ApJ/757/112">J/ApJ/757/112 : Stellar diameters. II. K and M-stars (Boyajian+, 2012)</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/807/45">J/ApJ/807/45 : Potentially habitable planets orbiting M dwarfs</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/809/77">J/ApJ/809/77 : Transiting Exoplanet Survey Satellite (TESS) (Sullivan+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/825/19">J/ApJ/825/19 : Mass-radius relationship for planets with Rp&lt;4</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/180">J/AJ/155/180 : A catalog of cool dwarf targets for the TESS (Muirhead+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/239/2">J/ApJS/239/2 : Simulated exoplanets from TESS list of targets (Barclay+, 2018)</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/157/113</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/157/113</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/157/113</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/157/113</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/157/113</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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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>Star</name><description>[1/952] Star identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Pl</name><description>[1/8] Planet identifier</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Teff</name><description>[3210/3990] Star surface effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Vmag</name><description>[9.7/19.2] V-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Kmag</name><description>[5.5/14.5] K-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>[4.9/323.5] System distance</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RAJ2000</name><description>[0.48/359.8] Star Right Ascension in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-88.2/88.73] Star Declination in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Per</name><description>[0.8/199.98] Orbital period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>[5.4/579.2] Orbital semi-major axis</description><unit>solRad</unit><ucd>phys.angSize.smajAxis</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>i</name><description>[-28.7/29.12] Inclination</description><unit>deg</unit><ucd>src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M*</name><description>[0.07/16.1] Star mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R*</name><description>[0.5/3.9] Star radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Omega</name><description>[0.1/359.9] Longitude of the node {Omega}</description><unit>deg</unit><ucd>src.orbital.node</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e</name><description>[0.009/0.624] Eccentricity</description><ucd>src.orbital.eccentricity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hill</name><description>[4.765/63.88] Hill spacing quantity {Delta} (1)</description><ucd>phys.size;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Trans</name><description>[0/1]? 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