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<ri:Resource created="2017-08-29T07:38:47Z" 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>2007.5 to 2010.4 HST astrometry of HD 202206</title><shortName>J/AJ/153/258</shortName><identifier>ivo://CDS.VizieR/J/AJ/153/258</identifier><altIdentifier>doi:10.26093/cds/vizier.51530258</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Benedict G.F.</name></creator><creator><name>Harrison T.E.</name></creator><date role="Updated">2017-09-04T07:53:41Z</date><date role="Created">2017-08-29T07:38:47Z</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>solar-system-planets</subject><subject>astrometry</subject><subject>parallax</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><subject>Wide-band photometry</subject><subject>proper-motions</subject><subject>stellar-spectral-types</subject><description>Using Hubble Space Telescope Fine Guidance Sensor astrometry and previously published radial velocity measures, we explore the exoplanetary system HD202206. Our modeling results in a parallax, {pi}_abs_=21.96+/-0.12 milliseconds of arc, a mass for HD202206B of M_B_=0.089_-0.006_^+0.007M_{Sun}_, and a mass for HD202206c of M_c_=17.9_-1.8_^+2.9^M_Jup_. HD202206 is a nearly face-on G + M binary orbited by a brown dwarf. 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