<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2026-07-31T09:31:52Z" status="active" updated="2026-07-31T08:41:54Z" 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>HD 4614 RVs from HIRES, APF, Hamilton &amp; NEID</title><shortName>J/AJ/170/270</shortName><identifier>ivo://CDS.VizieR/J/AJ/170/270</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kane S.R.</name></creator><creator><name>Li Z.</name></creator><creator><name>Hill M.L.</name></creator><creator><name>D'Angiolillo S.</name></creator><creator><name>Fulton B.J.</name></creator><creator><name>Howard A.W.</name></creator><date role="Updated">2026-07-31T08:41:54Z</date><date role="Created">2026-07-31T09:31:52Z</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>multiple-stars</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-astronomy</subject><description>Given the vast number of stars that exist within binary systems, it remains important to explore the effect of binary star environments on the formation and evolution of exoplanetary systems. Nearby binaries provide opportunities to characterize their properties and orbits through a combination of radial velocities, astrometry, and direct imaging. Eta Cassiopeiae is a bright, well-known binary system for which recent observations have provided greatly improved stellar masses and orbital parameters. We present additional radial velocity data that are used to perform an injection-recovery analysis for potential planetary signatures. We further provide a detailed dynamical study that explores the viability of planetary orbits throughout the system. Our combined analysis shows that giant planets are significantly ruled out for the system, and indeed no planetary orbits are viable beyond ~8AU of the primary star. However, terrestrial planets may yet exist within the habitable zone where orbits can remain long-term stable. We discuss the implications of these results, highlighting the effect of wide binary companions on giant planet formation, and the consequences for occurrence rates and planetary habitability.</description><source format="bibcode">2025AJ....170..270K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/170/270</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/I/355">I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/716/1336">J/ApJ/716/1336 : Stability analysis of single-planet (Kopparapu+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/746/101">J/ApJ/746/101 : Diameters and temperatures of AFG stars (Boyajian+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/745/19">J/ApJ/745/19 : Binary systems in Taurus-Auriga (Kraus+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/210/5">J/ApJS/210/5 : The twenty-five year Lick planet search (Fischer+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/452/2127">J/MNRAS/452/2127 : Fundamental param. of Kepler stars (Silva Aguirre+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/225/32">J/ApJS/225/32 : Extended abundance analysis of cool stars (Brewer+, 2016)</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/154/184">J/AJ/154/184 : Multiplicity of RV exoplanet host stars (Wittrock+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/264">J/AJ/156/264 : California-Kepler Survey. VII. Planet radius gap (Fulton+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/160/81">J/AJ/160/81 : 20 years of Beta CVn HIRES/APF radial velocities (Kane+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/496/851">J/MNRAS/496/851 : Planet candidates from K2 Campaigns 1-13 (Wittenmyer+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/159/19">J/AJ/159/19 : SOAR TESS survey. I. (Ziegler+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/130">J/AJ/161/130 : List of 100 targets for NEID Earth Twin Survey (Gupta+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/134">J/AJ/161/134 : Survey of stellar &amp; planetary comp. within 25pc (Hirsch+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/255/8">J/ApJS/255/8 : The California Legacy Survey. I. Planet cat. (Rosenthal+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/165/34">J/AJ/165/34 : Habitable Zone Exoplanets from NASA Exoplanet Arch. (Hill+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/165/176">J/AJ/165/176 : Doppler constraints comp. to Sun-like stars (Laliotis+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/272/30">J/ApJS/272/30 : Habitable Worlds Observatory (HWO): 164 targets (Harada+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/167/139">J/AJ/167/139 : HPIC catalog &amp; potential contaminants from Gaia (Tuchow+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/170/52">J/AJ/170/52 : NETS. II. RV &amp; astrometry of 7 star systems (Giovinazzi+, 2025)</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/170/270</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/170/270</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/170/270</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/170/270</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/170/270</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/170/270</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/170/270/table1</name><description>HD 4614 radial velocities</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Inst</name><description>Instrument (1)</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>MJD</name><description>[9969/20846] Modified Barycentric Julian Date; BJD-2440000 (Date)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RVel</name><description>[-71.39/8460.7] Radial velocity</description><unit>m/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RVel</name><description>[0.3/46.15] Uncertainty in RVel</description><unit>m/s</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>