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<ri:Resource created="2024-04-08T09:29:28Z" status="active" updated="2025-07-18T20:13:13Z" 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>Open cluster nondegenerate stars analysis</title><shortName>J/ApJ/929/29</shortName><identifier>ivo://CDS.VizieR/J/ApJ/929/29</identifier><altIdentifier>doi:10.26093/cds/vizier.19290029</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gutierrez C.M.</name></creator><creator><name>Ramos-Chernenko N.</name></creator><date role="Updated">2025-07-18T20:13:13Z</date><date role="Created">2024-04-08T09:29:28Z</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>radial-velocity</subject><subject>open-star-clusters</subject><subject>visible-astronomy</subject><description>A key observational prediction of Einstein's Equivalence Principle is that light undergoes redshift when it escapes from a gravitational field. Although astrophysics provides a wide variety of physical conditions in which this redshift should be significant, until very recently the observational evidence for this gravitational effect was limited to the light emitted by the Sun and white dwarfs. Gaia-DR2 astrometric and kinematic data, in combination with other spectroscopic observations, provides a test bench to validate such predictions in statistical terms. The aim of this paper is to analyze several thousand main-sequence and giant stars in open clusters (OCs) in order to measure the gravitational redshift effect. Observationally, a spectral shift will depend on the stellar mass-to-radius ratio as expected from the theoretical estimation of relativity. After the analysis, the obtained correlation coefficient between theoretical predictions and observations for 28 (51) OCs is a=0.977+/-0.218 (0.899+/-0.137). The result has proven to be statistically robust and with little dependence on the details of the methodology or sample selection criteria. This study represents one of the more extensive validations of a fundamental prediction of gravity theories.</description><source format="bibcode">2022ApJ...929...29G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/929/29</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/349">I/349 : StarHorse, Gaia DR2 photo-astrometric distances (Anders+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/322/460">J/A+A/322/460 : NGC 3680 photometry and radial velocities (Nordstrom+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/381/446">J/A+A/381/446 : Astrometric Radial Velocities. III. (Madsen+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/526/A127">J/A+A/526/A127 : Velocities of M67 MS and giant stars (Pasquini+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/550/A103">J/A+A/550/A103 : Model 1D (LHD) and 3D (CO5BOLD) sp. (Allende Prieto+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/619/A155">J/A+A/619/A155 : Open cluster kinematics with Gaia DR2 (Soubiran+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/627/A119">J/A+A/627/A119 : Extended halo of NGC 2682 (M 67) (Carrera+ 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/483/5026">J/MNRAS/483/5026 : Radial velocities of Hyades stars (Leao+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/633/A99">J/A+A/633/A99 : Gaia DR2 open clusters in the MW. 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