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<ri:Resource created="2021-07-15T09:04:13Z" 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>Predicted positions of {beta}Pictoris b and c</title><shortName>J/AJ/161/179</shortName><identifier>ivo://CDS.VizieR/J/AJ/161/179</identifier><altIdentifier>doi:10.26093/cds/vizier.51610179</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brandt G.M.</name></creator><creator><name>Brandt T.D.</name></creator><creator><name>Dupuy T.J.</name></creator><creator><name>Li Y.</name></creator><creator><name>Michalik D.</name></creator><date role="Updated">2022-01-17T12:30:15Z</date><date role="Created">2021-07-15T09:04:13Z</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>astrometry</subject><subject>infrared-astronomy</subject><description>We present a comprehensive orbital analysis to the exoplanets {beta}Pictoris b and c that resolves previously reported tensions between the dynamical and evolutionary mass constraints on {beta}Picb. We use the Markov Chain Monte Carlo orbit code orvara to fit 15years of radial velocities and relative astrometry (including recent GRAVITY measurements), absolute astrometry from Hipparcos and Gaia, and a single relative radial velocity measurement between {beta}Pic A and b. We measure model-independent masses of 9.3_-2.5_^+2.6^M_Jup_ for {beta}Picb and 8.3{+/-}1.0M_Jup_ for {beta}Picc. These masses are robust to modest changes to the input data selection. We find a well-constrained eccentricity of 0.119{+/-}0.008 for {beta}Picb, and an eccentricity of 0.21_-0.09_^+0.16^ for {beta}Picc, with the two orbital planes aligned to within ~0.5{deg}. Both planets' masses are within ~1{sigma} of the predictions of hot-start evolutionary models and exclude cold starts. We validate our approach on N-body synthetic data integrated using REBOUND. We show that orvara can account for three-body effects in the {beta}Pic system down to a level ~5 times smaller than the GRAVITY uncertainties. Systematics in the masses and orbital parameters from orvara's approximate treatment of multiplanet orbits are a factor of ~5 smaller than the uncertainties we derive here. Future GRAVITY observations will improve the constraints on {beta}Picc's mass and (especially) eccentricity, but improved constraints on the mass of {beta}Picb will likely require years of additional radial velocity monitoring and improved precision from future Gaia data releases.</description><source format="bibcode">2021AJ....161..179B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/161/179</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/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/542/A18">J/A+A/542/A18 : {beta}Pic Harps radial velocity data (Lagrange+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/745/174">J/ApJ/745/174 : Evolutionary models young gas-giant planets (Spiegel+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/758/56">J/ApJ/758/56 : Young M dwarfs within 25pc. II. Kinematics (Shkolnik+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/454/593">J/MNRAS/454/593 : Young moving groups in solar neighbourhood (Bell+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/607/A25">J/A+A/607/A25 : beta Pic HARPS spectrum (Vidal-Madjar+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/18">J/AJ/156/18 : APOGEE DR14:Binary comps evolved stars (Price-Whelan+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/625/L13">J/A+A/625/L13 : TESS light curve of beta Pictoris (Zieba+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/627/A28">J/A+A/627/A28 : beta Pic BRITE, bRing, SMEI light curves (Zwintz+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/633/A110">J/A+A/633/A110 : K band spectrum of beta Pictoris b (GRAVITY+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/648/A15">J/A+A/648/A15 : beta Pictoris photometry (Kenworthy+, 2021)</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/161/179</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/161/179</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/161/179</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/161/179</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/161/179</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/161/179</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>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/161/179/table2</name><description>Predicted positions of {beta}Pic b</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>MJD</name><description>[59213/61028] Modified Julian Date, JD-2400000.5</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dRA</name><description>[211/305] Offset in Right Ascension</description><unit>mas</unit><ucd>pos.eq.ra;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dDE</name><description>[351/488] Offset in Declination</description><unit>mas</unit><ucd>pos.eq.dec;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dRA</name><description>[0.33/6.67] Uncertainty in dRA</description><unit>mas</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dDE</name><description>[0.54/10.9] Uncertainty in dDE</description><unit>mas</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rhoad</name><description>[0.95/1] Correlation coefficient between RA and DE</description><ucd>stat.correlation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sep</name><description>[410/576] Separation</description><unit>mas</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Sep</name><description>[0.13/12.8] Uncertainty in Sep</description><unit>mas</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/161/179/table3</name><description>Predicted positions of {beta}Pic c</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>MJD</name><description>[59213/61028] Modified Julian Date, JD-2400000.5</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dRA</name><description>[-78.2/56.8] Offset in Right Ascension</description><unit>mas</unit><ucd>pos.eq.ra;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dDE</name><description>[-129/94.9] Offset in Declination</description><unit>mas</unit><ucd>pos.eq.dec;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dRA</name><description>[0.93/20.2] Uncertainty in dRA</description><unit>mas</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dDE</name><description>[1.18/31.6] Uncertainty in dDE</description><unit>mas</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rhoad</name><description>[0.34/1] Correlation coefficient between RA and DE</description><ucd>stat.correlation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sep</name><description>[1.59/151] Separation</description><unit>mas</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Sep</name><description>[1.28/37.4] Uncertainty in Sep</description><unit>mas</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>