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<ri:Resource created="2022-03-09T07:59:55Z" 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>TESS-Keck survey. VI. HIP-97166 radial velocity</title><shortName>J/AJ/162/265</shortName><identifier>ivo://CDS.VizieR/J/AJ/162/265</identifier><altIdentifier>doi:10.26093/cds/vizier.51620265</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Macdougall M.G.</name></creator><creator><name>Petigura E.A.</name></creator><creator><name>Angelo I.</name></creator><creator><name>Lubin J.</name></creator><creator><name>Batalha N.M.,Beard C.</name></creator><creator><name>Behmard A.</name></creator><creator><name>Blunt S.</name></creator><creator><name>Brinkman C.</name></creator><creator><name>Chontos A.</name></creator><creator><name>Crossfield I.J.M.,Dai F.</name></creator><creator><name>Dalba P.A.</name></creator><creator><name>Dressing C.</name></creator><creator><name>Fulton B.</name></creator><creator><name>Giacalone S.</name></creator><creator><name>Hill M.L.,Howard A.W.</name></creator><creator><name>Huber D.</name></creator><creator><name>Isaacson H.</name></creator><creator><name>Kane S.R.</name></creator><creator><name>Mayo A.</name></creator><creator><name>Mocnik T.,Murphy J.M.A.</name></creator><creator><name>Polanski A.</name></creator><creator><name>Rice M.</name></creator><creator><name>Robertson P.</name></creator><creator><name>Rosenthal L.J.</name></creator><creator><name>Roy A.,Rubenzahl R.A.</name></creator><creator><name>Scarsdale N.</name></creator><creator><name>Turtelboom E.</name></creator><creator><name>Van Zandt J.</name></creator><creator><name>Weiss L.M.,Matthews E.</name></creator><creator><name>Jenkins J.M.</name></creator><creator><name>Latham D.W.</name></creator><creator><name>Ricker G.R.</name></creator><creator><name>Seager S.,Vanderspek R.K.</name></creator><creator><name>Winn J.N.</name></creator><creator><name>Brasseur C.E.</name></creator><creator><name>Doty J.</name></creator><creator><name>Fausnaugh M.,Guerrero N.</name></creator><creator><name>Henze C.</name></creator><creator><name>Lund M.B.</name></creator><creator><name>Shporer A.</name></creator><date role="Updated">2025-05-05T20:07:39Z</date><date role="Created">2022-03-09T07:59:55Z</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>k-stars</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>We report the discovery of HIP-97166b (TOI-1255b), a transiting sub-Neptune on a 10.3day orbit around a K0 dwarf 68pc from Earth. This planet was identified in a systematic search of TESS Objects of Interest for planets with eccentric orbits, based on a mismatch between the observed transit duration and the expected duration for a circular orbit. We confirmed the planetary nature of HIP-97166b with ground-based radial-velocity measurements and measured a mass of M_b_=20{+/-}2M{Earth} along with a radius of R_b_=2.7{+/-}0.1R{Earth} from photometry. We detected an additional nontransiting planetary companion with M_c_sini=10{+/-}2M{Earth} on a 16.8day orbit. While the short transit duration of the inner planet initially suggested a high eccentricity, a joint RV-photometry analysis revealed a high impact parameter b=0.84{+/-}0.03 and a moderate eccentricity. Modeling the dynamics with the condition that the system remain stable over &gt;10^5^ orbits yielded eccentricity constraints e_b_=0.16{+/-}0.03 and e_c_&lt;0.25. The eccentricity we find for planet b is above average for the small population of sub-Neptunes with well-measured eccentricities. We explored the plausible formation pathways of this system, proposing an early instability and merger event to explain the high density of the inner planet at 5.3{+/-}0.9g/cc as well as its moderate eccentricity and proximity to a 5:3 mean-motion resonance.</description><source format="bibcode">2021AJ....162..265M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/162/265</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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/787/80">J/ApJ/787/80 : 139 Kepler planets transit time variations (Hadden+, 2014)</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/ApJS/210/20">J/ApJS/210/20 : Small Kepler planets radial velocities (Marcy+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/825/19">J/ApJ/825/19 : Mass-radius relationship planets with Rp&lt;4 (Wolfgang+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/153/142">J/AJ/153/142 : Radial velocities systems hosting sub-Saturns (Petigura+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/107">J/AJ/154/107 : California-Kepler Survey (CKS). I. 1305 stars (Petigura+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/228">J/AJ/154/228 : Properties of transiting planet's host stars (Sandford+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/844/102">J/ApJ/844/102 : KIC star parallaxes from asteroseismology/Gaia (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/48">J/AJ/155/48 : California-Kepler Survey. V. Masses and radii (Weiss+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/18">J/AJ/156/18 : APOGEE DR14:Binary comp. of evolved stars (Price-Whelan+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/264">J/AJ/156/264 : California-Kepler Survey VII. 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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>Obs</name><description>[2020/2021] Year of the observation</description><ucd>time.epoch</ucd></column><column><name>BJD</name><description>[2458978/2459316] Barycentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Tel</name><description>Telescope identifier; APF or HIRES</description><ucd>meta.id;instr.tel</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>RVel</name><description>[-18.8/19.6] Radial velocity</description><unit>m/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RVel</name><description>[0.7/8.1] Uncertainty in RVel</description><unit>m/s</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SHK</name><description>[0.11/0.35] S_HK_ activity index (1)</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_SHK</name><description>[0.001/0.002] Uncertainty in SHK (1)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>