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<ri:Resource created="2020-09-08T14:49:48Z" status="active" updated="2025-06-13T15:25:00Z" 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>Detached eclipsing binaries with Gaia parallaxes</title><shortName>J/ApJ/872/85</shortName><identifier>ivo://CDS.VizieR/J/ApJ/872/85</identifier><altIdentifier>doi:10.26093/cds/vizier.18720085</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Graczyk D.</name></creator><creator><name>Pietrzynski G.</name></creator><creator><name>Gieren W.</name></creator><creator><name>Storm J.</name></creator><creator><name>Nardetto N.</name></creator><creator><name>Gallenne A.,Maxted P.F.L.</name></creator><creator><name>Kervella P.</name></creator><creator><name>Kolaczkowski Z.</name></creator><creator><name>Konorski P.</name></creator><creator><name>Pilecki B.,Zgirski B.</name></creator><creator><name>Gorski M.</name></creator><creator><name>Suchomska K.</name></creator><creator><name>Karczmarek P.</name></creator><creator><name>Taormina M.,Wielgorski P.</name></creator><creator><name>Narloch W.</name></creator><creator><name>Smolec R.</name></creator><creator><name>Chini R.</name></creator><creator><name>Breuval L.</name></creator><date role="Updated">2020-11-30T07:33:15Z</date><date role="Created">2020-09-08T14:49:48Z</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>eclipsing-binary-stars</subject><subject>astronomical-reference-materials</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><subject>Wide-band photometry</subject><subject>infrared-photometry</subject><subject>stellar-radii</subject><description>Using a sample of 81 Galactic, detached eclipsing binary stars we investigated the global zero-point shift of their parallaxes with the Gaia Data Release 2 (DR2) parallaxes. The stars in the sample lay in a distance range of 0.04-2kpc from the Sun. The photometric parallaxes {omega}_Phot_ of the eclipsing binaries were determined by applying a number of empirical surface brightness-color (SBC) relations calibrated on optical-infrared colors. For each SBC relation we calculated the individual differences d{varpi}_i_=({varpi}_Gaia_-{varpi}_Phot_)_i_ and then we calculated unweighted and weighted means. As the sample covers the whole sky we interpret the weighted means as the global shifts of the Gaia DR2 parallaxes with respect to our eclipsing binary sample. Depending on the choice of the SBC relation the shifts vary from -0.094 to -0.025mas. The weighted mean of the zero-point shift from all colors and calibrations used is d{omega}=-0.054+/-0.024mas. However, the SBC relations based on (B-K) and (V-K) colors, which are the least reddening dependent and have the lowest intrinsic dispersions, give a zero-point shift of d{omega}=-0.031+/-0.011mas in full agreement with results obtained by Lindegren+ (2018A&amp;A...616A...2L) and Arenou+ (2018A&amp;A...616A..17A). Our result confirms the global shift of Gaia DR2 parallaxes of d{omega}=-0.029mas reported by the Gaia team, but we do not confirm the larger zero-point shift reported by a number of follow-up papers.</description><source format="bibcode">2019ApJ...872...85G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/872/85</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/168">II/168 : Homogeneous Means in the UBV System (Mermilliod 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/152">V/152 : The DEBCat detached eclipsing binary catalogue (Southworth, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer- Jones+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/469/355">J/ApJ/469/355 : Teff, B-V and BC relation (Flower, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/324/137">J/A+A/324/137 : Eclipsing binaries with candidate CP stars (North+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/119/1389">J/AJ/119/1389 : The binary star FS Monocerotis (Lacy+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/387/850">J/A+A/387/850 : Radial velocities of eclipsing binaries (Imbert, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1340">J/AJ/128/1340 : The eclipsing binary star V459 Cas (Lacy+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1840">J/AJ/128/1840 : The eclipsing binary star MU Cas (Lacy+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1319">J/AJ/128/1319 : New AY Cam Photometric Observations (Williamon+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/363/529">J/MNRAS/363/529 : uvby, UBV &amp; 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xsi:type="vs:VOTableType">int</dataType></column><column><name>e_T2</name><description>[30/2000] Error on T2</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ref</name><description>Code for a reference (see refs.dat file)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>a</name><description>[6.3/376] Semimajor axis</description><unit>solRad</unit><ucd>phys.angSize.smajAxis</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>q</name><description>[0.49/1.1] Mass ratio</description><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Omega1</name><description>[4/82.6] Dimensionless Roche potential of stellar surface</description><ucd>arith.factor;phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Omega2</name><description>[4.1/84.1] 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radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rad2</name><description>[0.003/0.5] Error on Rad2</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Bmag</name><description>[5.4/14.7] Magnitude in Johnson B filter</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Bmag</name><description>[0.006/0.1] Error on B</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Jmag</name><description>[5/13] Magnitude in Johnson J filter</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Jmag</name><description>[0.01/0.4] Error on J</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hmag</name><description>[4.8/12.5] Magnitude in Johnson H filter</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Hmag</name><description>[0.01/0.07] Error on H</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Kmag</name><description>[4.7/12.5] Magnitude in Johnson K filter</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Kmag</name><description>[0.01/0.04] Error on K</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L21B</name><description>[0.01/1.6] Light ratio of components in B filter</description><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L21V</name><description>[0.02/1.7] Light ratio of components in V filter</description><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L21J</name><description>[0.06/2.5] Light ratio of components in J filter</description><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L21H</name><description>[0.06/3.2] Light ratio of components in H filter</description><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L21K</name><description>[0.06/3.3] Light ratio of components in K filter</description><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>