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<ri:Resource created="2025-05-05T13:06:19Z" status="active" updated="2025-06-02T20:09:18Z" 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>The TESS-Keck survey. XXII. TOI-1437</title><shortName>J/AJ/168/135</shortName><identifier>ivo://CDS.VizieR/J/AJ/168/135</identifier><altIdentifier>doi:10.26093/cds/vizier.51680135</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pidhorodetska D.</name></creator><creator><name>Gilbert E.A.</name></creator><creator><name>Kane S.R.</name></creator><creator><name>Barclay T.</name></creator><creator><name>Polanski A.S.,Hill M.L.</name></creator><creator><name>Stassun K.G.</name></creator><creator><name>Giacalone S.</name></creator><creator><name>Ciardi D.R.</name></creator><creator><name>Boyle A.W.,Howell S.B.</name></creator><creator><name>Lillo-Box J.</name></creator><creator><name>MacDougall M.G.</name></creator><creator><name>Fetherolf T.</name></creator><creator><name>Batalha N.M.,Crossfield I.J.M.</name></creator><creator><name>Dressing C.</name></creator><creator><name>Fulton B.</name></creator><creator><name>Howard A.W.</name></creator><creator><name>Huber D.,Isaacson H.</name></creator><creator><name>Petigura E.A.</name></creator><creator><name>Robertson P.</name></creator><creator><name>Weiss L.M.</name></creator><creator><name>Angelo I.</name></creator><creator><name>Beard C.,Behmard A.</name></creator><creator><name>Blunt S.</name></creator><creator><name>Brinkman C.L.</name></creator><creator><name>Chontos A.</name></creator><creator><name>Dai F.</name></creator><creator><name>Dalba P.A.,Holcomb R.</name></creator><creator><name>Lubin J.</name></creator><creator><name>Mayo A.W.</name></creator><creator><name>Murphy J.M.A.</name></creator><creator><name>Rice M.</name></creator><creator><name>Rubenzahl R.,Scarsdale N.</name></creator><creator><name>Turtelboom E.V.</name></creator><creator><name>Tyler D.</name></creator><creator><name>van Zandt J.</name></creator><creator><name>Schwieterman E.W.</name></creator><date role="Updated">2025-06-02T20:09:18Z</date><date role="Created">2025-05-05T13:06:19Z</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>radial-velocity</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-sources</subject><subject>surveys</subject><description>Exoplanet discoveries have revealed a dramatic diversity of planet sizes across a vast array of orbital architectures. Sub-Neptunes are of particular interest; due to their absence in our own solar system, we rely on demographics of exoplanets to better understand their bulk composition and formation scenarios. Here, we present the discovery and characterization of TOI-1437 b, a sub-Neptune with a 18.84 day orbit around a near-solar analog (M*=1.10+/-0.10M_{sun}_, R*=1.17+/-0.12R_{sun}_). The planet was detected using photometric data from the Transiting Exoplanet Survey Satellite (TESS) mission and radial velocity (RV) follow-up observations were carried out as a part of the TESS-Keck Survey using both the HIRES instrument at Keck Observatory and the Levy Spectrograph on the Automated Planet Finder telescope. A combined analysis of these data reveal a planet radius of Rp=2.24+/-0.23R_{Earth}_ and a mass measurement of Mp=9.6+/-3.9M_{Earth}_). TOI-1437 b is one of few (~50) known transiting sub-Neptunes orbiting a solar-mass star that has a RV mass measurement. As the formation pathway of these worlds remains an unanswered question, the precise mass characterization of TOI-1437 b may provide further insight into this class of planet.</description><source format="bibcode">2024AJ....168..135P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/168/135</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/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/356">I/356 : Gaia DR3 Part 2. Extra-galactic (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/357">I/357 : Gaia DR3 Part 3. 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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>BJD</name><description>Barycentric Julian Date; TDB</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RVel</name><description>[-48/31] Relative radial velocity</description><unit>m/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RVel</name><description>[1.2/19] Uncertainty in RVel</description><unit>m/s</unit><ucd>stat.error;phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SHK</name><description>[0.038/0.31] The S_HK_ Value</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_SHK</name><description>[0.001/0.002] Uncertainty in SHK</description><ucd>stat.error;spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Inst</name><description>Instrument ("APF" or "HIRES")</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column></table></schema></tableset></ri:Resource>