<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2012-02-02T15:05:33Z" status="active" updated="2026-05-19T14:24:40Z" 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>The orbit of S2 star around Sgr A*</title><shortName>J/ApJ/707/L114</shortName><identifier>ivo://CDS.VizieR/J/ApJ/707/L114</identifier><altIdentifier>doi:10.26093/cds/vizier.17079114</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gillessen S.</name></creator><creator><name>Eisenhauer F.</name></creator><creator><name>Fritz T.K.</name></creator><creator><name>Bartko H.</name></creator><creator><name>Dodds-Eden K.,Pfuhl O.</name></creator><creator><name>Ott T.</name></creator><creator><name>Genzel R.</name></creator><date role="Updated">2026-05-19T14:24:40Z</date><date role="Created">2012-02-02T15:05:33Z</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>astrometry</subject><subject>radial-velocity</subject><subject>milky-way-galaxy</subject><subject>multiple-stars</subject><description>Two recent papers (Ghez et al. 2008ApJ...689.1044G; Gillessen et al. 2009ApJ...692.1075G) have estimated the mass of and the distance to the massive black hole (MBH) in the center of the Milky Way using stellar orbits. The two astrometric data sets are independent and yielded consistent results, even though the measured positions do not match when simply overplotting the two sets. In this Letter, we show that the two sets can be brought to excellent agreement with each other when we allow for a small offset in the definition of the reference frame of the two data sets. The required offsets in the coordinates and velocities of the origin of the reference frames are consistent with the uncertainties given in Ghez et al. The so-combined data set allows for a moderate improvement of the statistical errors of the mass of and the distance to Sgr A*, but the overall accuracies of these numbers are dominated by systematic errors and the long-term calibration of the reference frame.</description><source format="bibcode">2009ApJ...707L.114G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/707/L114</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/V/55">V/55 : A catalogue of high-velocity stars (Roman, 1955)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/186">J/ApJ/699/186 : VLA observations of the Galactic center (Zhao+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/697/1741">J/ApJ/697/1741 : Warped disks of YSOs in Galactic center (Bartko+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/681/1254">J/ApJ/681/1254 : Radial velocities of stars in the Galactic Center (Zhu+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/659/1241">J/ApJ/659/1241 : Stellar variability in Galactic Center (Rafelski+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/3399">J/AJ/127/3399 : Sgr A* variability at cm wavelengths (Herrnstein+, 2004)</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/ApJ/707/L114</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/707/L114</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/707/L114</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/707/L114</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/707/L114</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/707/L114</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/ApJ/707/L114/table1</name><description>Orbital data for S2 used in this work</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>Ep.A</name><description>Year of the astrometric observation</description><unit>yr</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>oRA</name><description>Offset in Right Ascension relative to SgrA*</description><unit>mas</unit><ucd>pos.eq.ra;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_oRA</name><description>Uncertainty in oRA</description><unit>mas</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>oDE</name><description>Offset in Declination relative to SgrA*</description><unit>mas</unit><ucd>pos.eq.dec;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_oDE</name><description>Uncertainty in oDE</description><unit>mas</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tel.A</name><description>Telescope used in astrometric observation</description><ucd>meta.id;instr.tel</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Ep.V</name><description>? Year of the radial velocity observation</description><unit>yr</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>VLSR</name><description>? Local Standard of Rest Velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_VLSR</name><description>? Uncertainty in VLSR</description><unit>km/s</unit><ucd>stat.error;phys.veloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Tel.V</name><description>Telescope used in radial velocity observation (VLT or Keck)</description><ucd>meta.id;instr.tel</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column></table></schema></tableset></ri:Resource>