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<ri:Resource created="2015-03-05T06:37:19Z" 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>GAPS V: Global analysis of the XO-2 system</title><shortName>J/A+A/575/A111</shortName><identifier>ivo://CDS.VizieR/J/A+A/575/A111</identifier><altIdentifier>doi:10.26093/cds/vizier.35750111</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Damasso M.</name></creator><creator><name>Biazzo K.</name></creator><creator><name>Bonomo A.S.</name></creator><creator><name>Desidera S.</name></creator><creator><name>Lanza A.F.</name></creator><creator><name>Nascimbeni V.,Esposito M.</name></creator><creator><name>Scandariato G.</name></creator><creator><name>Sozzetti A.</name></creator><creator><name>Cosentino R.</name></creator><creator><name>Gratton R.,Malavolta L.</name></creator><creator><name>Rainer M.</name></creator><creator><name>Gandolfi D.</name></creator><creator><name>Poretti E.</name></creator><creator><name>Zanmar Sanchez R.,Ribas I.</name></creator><creator><name>Santos N.</name></creator><creator><name>Affer L.</name></creator><creator><name>Andreuzzi G.</name></creator><creator><name>Barbieri M.</name></creator><creator><name>Bedin L.R.,Benatti S.</name></creator><creator><name>Bernagozzi A.</name></creator><creator><name>Bertolini E.</name></creator><creator><name>Bonavita M.</name></creator><creator><name>Borsa F.</name></creator><creator><name>Borsato L.,Boschin W.</name></creator><creator><name>Calcidese P.</name></creator><creator><name>Carbognani A.</name></creator><creator><name>Cenadelli D.</name></creator><creator><name>Christille J.M.,Claudi R.U.</name></creator><creator><name>Covino E.</name></creator><creator><name>Cunial A.</name></creator><creator><name>Giacobbe P.</name></creator><creator><name>Granata V.</name></creator><creator><name>Harutyunyan A.,Lattanzi M.G.</name></creator><creator><name>Leto G.</name></creator><creator><name>Libralato M.</name></creator><creator><name>Lodato G.</name></creator><creator><name>Lorenzi V.</name></creator><creator><name>Mancini L.,Martinez Fiorenzano A.F.</name></creator><creator><name>Marzari F.</name></creator><creator><name>Masiero S.</name></creator><creator><name>Micela G.</name></creator><creator><name>Molinari E.,Molinaro M.</name></creator><creator><name>Munari U.</name></creator><creator><name>Murabito S.</name></creator><creator><name>Pagano I.</name></creator><creator><name>Pedani M.</name></creator><creator><name>Piotto G.,Rosenberg A.</name></creator><creator><name>Silvotti R.</name></creator><creator><name>Southworth J.</name></creator><date role="Updated">2017-06-20T13:17:24Z</date><date role="Created">2015-03-05T06:37:19Z</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>photometry</subject><subject>radial-velocity</subject><description>XO-2 is the first confirmed wide stellar binary system where the almost twin components XO-2N and XO-2S have planets, and it is a peculiar laboratory in which to investigate the diversity of planetary systems. This stimulated a detailed characterization study of the stellar and planetary components based on new observations. We collected high-resolution spectra with the HARPS-N spectrograph and multi-band light curves. Spectral analysis led to an accurate determination of the stellar atmospheric parameters and characterization of the stellar activity, and high-precision radial velocities of XO-2N were measured. We collected 14 transit light curves of XO-2Nb used to improve the transit parameters. Photometry provided accurate magnitude differences between the stars and a measure of their rotation periods.</description><source format="bibcode">2015A&amp;A...575A.111D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/575/A111</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/J/A+A/527/A85">J/A+A/527/A85 : Light curves of HAT-P-3b and HAT-P-14b (Nascimbeni+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/554/A28">J/A+A/554/A28 : Qatar-1 differential light curve (Covino+, 2013)</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/A+A/575/A111</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/575/A111</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/575/A111</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/575/A111</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/575/A111</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/575/A111</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></coverage><tableset><schema><name>default</name><table><name>J/A+A/575/A111/xo2ntra</name><description>Transit light curves of XO-2N collected in R-band, in the framework of the TASTE project, with the facilities described in Table 4 (Fig.8 of paper)</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>BJD</name><description>Barycentric Julian Date (UTC)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dmag</name><description>Differential magnitude in R-band</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_dmag</name><description>Uncertainty associated to differential magnitude</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/A+A/575/A111/xo2sapa</name><description>*Light-curve of the star XO-2S collected by the APACHE survey in I-band (Fig. 7 in the paper)</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>Heliocentric Julian Date (HJD-2456000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dmag</name><description>Differential magnitude in I-band</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dmag</name><description>Uncertainty associated to differential magnitude</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/575/A111/xo2napa</name><description>*Light-curve of the star XO-2N collected by the APACHE survey in I-band (Fig. 6 in the paper)</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>Heliocentric Julian Date (HJD-2456000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dmag</name><description>Differential magnitude in I-band</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dmag</name><description>Uncertainty associated to differential magnitude</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/575/A111/table7</name><description>Radial velocities of the star XO-2N as measured by the HARPS-N spectrograph</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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