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<ri:Resource created="2012-04-17T12:28:37Z" 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>Oscillations of red giants observed by Kepler</title><shortName>J/A+A/540/A143</shortName><identifier>ivo://CDS.VizieR/J/A+A/540/A143</identifier><altIdentifier>doi:10.26093/cds/vizier.35400143</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mosser B.</name></creator><creator><name>Goupil M.J.</name></creator><creator><name>Belkacem K.</name></creator><creator><name>Michel E.</name></creator><creator><name>Stello D.</name></creator><creator><name>Marques J.P.,Elsworth Y.</name></creator><creator><name>Barban C.</name></creator><creator><name>Beck P.G.</name></creator><creator><name>Bedding T.R.</name></creator><creator><name>De Ridder J.,Garcia R.A.</name></creator><creator><name>Hekker S.</name></creator><creator><name>Kallinger T.</name></creator><creator><name>Samadi R.</name></creator><creator><name>Stumpe M.C.</name></creator><creator><name>Barclay T.,Burke C.J.</name></creator><date role="Updated">2013-06-10T13:26:26Z</date><date role="Created">2012-04-17T12:28:37Z</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>giant-stars</subject><subject>spectroscopy</subject><description>There are now more than 22 months of long-cadence data available for thousands of red giants observed with the Kepler space mission. Consequently, we are able to clearly resolve fine details in their oscillation spectra and see many components of the mixed modes that probe the stellar core. We report for the first time a parametric fit to the pattern of the l=1 mixed modes in red giants, which is a powerful tool to identify gravity-dominated mixed modes. 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