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<ri:Resource created="2024-04-22T07:27:20Z" 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-Keck Survey. XVI. 8 systems Radial velocity</title><shortName>J/AJ/166/153</shortName><identifier>ivo://CDS.VizieR/J/AJ/166/153</identifier><altIdentifier>doi:10.26093/cds/vizier.51660153</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Murphy J.M.</name></creator><creator><name>Batalha N.M.</name></creator><creator><name>Scarsdale N.</name></creator><creator><name>Isaacson H.</name></creator><creator><name>Ciardi D.R.,Gonzales E.J.</name></creator><creator><name>Giacalone S.</name></creator><creator><name>Twicken J.D.</name></creator><creator><name>Dattilo A.</name></creator><creator><name>Fetherolf T.,Rubenzahl R.A.</name></creator><creator><name>Crossfield I.J.M.</name></creator><creator><name>Dressing C.D.</name></creator><creator><name>Fulton B.</name></creator><creator><name>Howard A.W.,Huber D.</name></creator><creator><name>Kane S.R.</name></creator><creator><name>Petigura E.A.</name></creator><creator><name>Robertson P.</name></creator><creator><name>Roy A.</name></creator><creator><name>Weiss L.M.,Beard C.</name></creator><creator><name>Chontos A.</name></creator><creator><name>Dai F.</name></creator><creator><name>Rice M.</name></creator><creator><name>Van Zandt J.</name></creator><creator><name>Lubin J.</name></creator><creator><name>Blunt S.,Polanski A.S.</name></creator><creator><name>Behmard A.</name></creator><creator><name>Dalba P.A.</name></creator><creator><name>Hill M.L.</name></creator><creator><name>Rosenthal L.J.,Brinkman C.L.</name></creator><creator><name>Mayo A.W.</name></creator><creator><name>Turtelboom E.V.</name></creator><creator><name>Angelo I.</name></creator><creator><name>Mocnik T.,MacDougall M.G.</name></creator><creator><name>Pidhorodetska D.</name></creator><creator><name>Tyler D.</name></creator><creator><name>Kosiarek M.R.</name></creator><creator><name>Holcomb R.,Louden E.M.</name></creator><creator><name>Hirsch L.A.</name></creator><creator><name>Gilbert E.A.</name></creator><creator><name>Anderson J.</name></creator><creator><name>Valenti J.A.</name></creator><date role="Updated">2025-05-05T20:07:51Z</date><date role="Created">2024-04-22T07:27:20Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><description>With JWST's successful deployment and unexpectedly high fuel reserves, measuring the masses of sub-Neptunes transiting bright, nearby stars will soon become the bottleneck for characterizing the atmospheres of small exoplanets via transmission spectroscopy. Using a carefully curated target list and observations from more than 2yr of APF-Levy and Keck-HIRES Doppler monitoring, the TESS-Keck Survey is working toward alleviating this pressure. Here we present mass measurements for 11 transiting planets in eight systems that are particularly suited to atmospheric follow-up with JWST. We also report the discovery and confirmation of a temperate super-Jovian-mass planet on a moderately eccentric orbit. The sample of eight host stars, which includes one subgiant, spans early-K to late-F spectral types (Teff=5200-6200K). We homogeneously derive planet parameters using a joint photometry and radial velocity modeling framework, discuss the planets possible bulk compositions, and comment on their prospects for atmospheric characterization.</description><source format="bibcode">2023AJ....166..153M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/153</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/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/453/635">J/A+A/453/635 : Modelling Galactic Interstellar Extinction (Marshall+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/687/1264">J/ApJ/687/1264 : Age estimation for solar-type dwarfs (Mamajek+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/725/875">J/ApJ/725/875 : Chromospheric activity for CPS stars (Isaacson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/204/24">J/ApJS/204/24 : Kepler planetary candidates. 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