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<ri:Resource created="2024-02-23T09:05:07Z" 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>EXPRES. IV. Two Additional Planets Orbiting</title><shortName>J/AJ/166/46</shortName><identifier>ivo://CDS.VizieR/J/AJ/166/46</identifier><altIdentifier>doi:10.26093/cds/vizier.51660046</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brewer J.M.</name></creator><creator><name>Zhao L.L.</name></creator><creator><name>Fischer D.A.</name></creator><creator><name>Roettenbacher R.M.</name></creator><creator><name>Henry G.W.,Llama J.</name></creator><creator><name>Szymkowiak A.E.</name></creator><creator><name>Cabot S.H.C.</name></creator><creator><name>Weiss S.A.</name></creator><creator><name>McCarthy C.</name></creator><date role="Updated">2024-11-06T20:18:44Z</date><date role="Created">2024-02-23T09:05:07Z</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>exoplanets</subject><subject>high-velocity-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><description>Thousands of exoplanet detections have been made over the last 25 years using Doppler observations, transit photometry, direct imaging, and astrometry. Each of these methods is sensitive to different ranges of orbital separations and planetary radii (or masses). This makes it difficult to fully characterize exoplanet architectures and to place our solar system in context with the wealth of discoveries that have been made. Here, we use the EXtreme PREcision Spectrograph to reveal planets in previously undetectable regions of the mass- period parameter space for the star {rho} Coronae Borealis. We add two new planets to the previously known system with one hot Jupiter in a 39day orbit and a warm super-Neptune in a 102day orbit. The new detections include a temperate Neptune planet (Msini~20M{Earth}) in a 281.4day orbit and a hot super-Earth (Msini=3.7M{Earth}) in a 12.95day orbit. This result shows that details of planetary system architectures have been hiding just below our previous detection limits; this signals an exciting era for the next generation of extreme precision spectrographs.</description><source format="bibcode">2023AJ....166...46B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/46</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/III/185">III/185 : Search for Jupiter-Mass Companions (Walker+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/311">I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/457/L99">J/ApJ/457/L99 : 25yr CaII-HK observations of FK nearby stars (Baliunas+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/622/1102">J/ApJ/622/1102 : The planet-metallicity correlation. (Fischer+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/646/505">J/ApJ/646/505 : Catalog of nearby exoplanets (Butler+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Sci/330.653">J/other/Sci/330.653 : Detected planets in the Eta-Earth Survey (Howard+, 2010)</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/ApJ/736/19">J/ApJ/736/19 : Kepler planetary candidates. II. (Borucki+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/776/67">J/ApJ/776/67 : Rotational tracks (van Saders+, 2013)</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/ApJ/795/64">J/ApJ/795/64 : Exoplanet physical parameters (Foreman-Mackey+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/809/8">J/ApJ/809/8 : Terrestrial planet occurrence rates KOI stars (Burke+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/809/25">J/ApJ/809/25 : Stellar &amp; planet properties for K2 candidates (Montet+, 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/ApJ/828/99">J/ApJ/828/99 : Kepler pipeline transit signal. 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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>BMJD</name><description>[58983/60074] Barycentric modified Julian Date; BJD-2400000.5</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RVel</name><description>[-72.2/70.8] Relative 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>[0.2/0.6] Uncertainty in RVel</description><unit>m/s</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/166/46/table5</name><description>APT photometry</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>HJD</name><description>[51557/59027] Heliocentric Julian Date; JD-2400000</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Dmag</name><description>[-1.02/-0.99] The (b+y)/2 differential magnitude</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>TRmag</name><description>[-1.008/-1.003] Trend removed magnitude</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>