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<ri:Resource created="2019-10-14T14:22:07Z" 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>Low-mass stars from the first two TESS sectors</title><shortName>J/AJ/158/81</shortName><identifier>ivo://CDS.VizieR/J/AJ/158/81</identifier><altIdentifier>doi:10.26093/cds/vizier.51580081</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cloutier R.</name></creator><date role="Updated">2022-12-14T08:32:49Z</date><date role="Created">2019-10-14T14:22:07Z</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>photometry</subject><subject>visible-astronomy</subject><subject>infrared-photometry</subject><subject>trigonometric-parallax</subject><subject>stellar-distance</subject><subject>stellar-radii</subject><subject>effective-temperature</subject><subject>stellar-masses</subject><subject>exoplanets</subject><description>Continuous data releases throughout the Transiting Exoplanet Survey Satellite (TESS) primary mission will provide unique opportunities for the exoplanet community at large to contribute to maximizing TESS's scientific return via the discovery and validation of transiting planets. This paper introduces our independent pipeline for the detection of periodic transit events along with the results of its inaugural application to the recently released 2 minute light curves of low-mass stars from the first two TESS sectors. The stellar parameters within our sample are refined using precise parallax measurements from the Gaia DR2 (Cat. I/345), which reduce the number of low-mass stars in our sample relative to those listed in the TESS Input Catalog. In lieu of the follow-up observations required to confirm or refute the planetary nature of transit-like signals, a validation of transit-like events flagged by our pipeline is performed statistically. The resulting vetted catalog contains eight probable blended eclipsing binaries, eight known TOIs, plus seven new planet candidates (PCs) smaller than 4 Earth radii. This work demonstrates the ability of our pipeline to detect sub-Neptune-sized PCs, which to date represent some of the most attractive targets for future atmospheric characterization via transmission or thermal emission spectroscopy and for radial velocity efforts aimed at the completion of the TESS level one requirement to deliver 50 planets smaller than 4 Earth radii with measured masses.</description><source format="bibcode">2019AJ....158...81C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/158/81</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</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/ApJS/216/7">J/ApJS/216/7 : Planets Around Low-Mass Stars (PALMS). IV. (Bowler+, 2015)</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/AJ/156/102">J/AJ/156/102 : The TESS Input Catalog and Candidate Target List</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><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/157/113">J/AJ/157/113 : TESS M-dwarf exoplanetary systems (Ballard, 2019)</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/158/81</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/158/81</mirrorURL><mirrorURL title="VizieR 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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>TIC</name><description>[2733611/471016669] TESS Input Catalog identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">long</dataType></column><column><name>Tmag</name><description>[7.019/15.82] Apparent TESS magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GBPmag</name><description>[7.098/15.862] Apparent Gaia blue passband magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_GBPmag</name><description>[0/0.065] Uncertainty in GBPmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GRPmag</name><description>[9.179/19.383] Apparent Gaia red passband magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_GRPmag</name><description>[0/0.065] Uncertainty in GRPmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Jmag</name><description>[5.669/13.801] Apparent 2MASS 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>[0.017/0.056] Uncertainty in Jmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hmag</name><description>[5.108/13.293] Apparent 2MASS 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>[0.017/0.069] Uncertainty in 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xsi:type="vs:VOTableType">float</dataType></column><column><name>e_plx</name><description>[0.012/1.307] Uncertainty in plx</description><unit>mas</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>[7.673/279.33] Distance from plx</description><unit>pc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Dist</name><description>[0.002/8.9] Uncertainty in Dist</description><unit>pc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>KsMag</name><description>[5.001/8.877] Absolute 2MASS K_S_ band magnitude</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>e_KsMag</name><description>[0.016/0.165] Uncertainty in KsMag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R*</name><description>[0.1506/0.6114] Stellar radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_R*</name><description>[0.0045/0.0324] Uncertainty in R*</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[2737/4042] Stellar effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>[49/70] Uncertainty in Teff</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>M*</name><description>[0.1192/0.6347] Stellar mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_M*</name><description>[0.0015/0.0308] Uncertainty in M*</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(g)</name><description>[4.668/5.158] Log stellar surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log(g)</name><description>[0.026/0.061] Uncertainty in log(g)</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>