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<ri:Resource created="2016-12-02T08:02:04Z" 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>H{alpha}-activity in the SARG binary survey</title><shortName>J/A+A/596/A76</shortName><identifier>ivo://CDS.VizieR/J/A+A/596/A76</identifier><altIdentifier>doi:10.26093/cds/vizier.35960076</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sissa E.</name></creator><creator><name>Gratton R.</name></creator><creator><name>Desidera S.</name></creator><creator><name>Martinez Fiorenzano A.F.,Bonfanti A.</name></creator><creator><name>Carolo E.</name></creator><creator><name>Vassallo D.</name></creator><creator><name>Claudi R.U.</name></creator><creator><name>Endl M.</name></creator><creator><name>Cosentino R.</name></creator><date role="Updated">2018-03-20T13:23:06Z</date><date role="Created">2016-12-02T08:02:04Z</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>radial-velocity</subject><subject>spectroscopy</subject><description>Stellar activity influences radial velocity (RV) measurements and can also mimic the presence of orbiting planets. As part of the search for planets around the components of wide binaries performed with the SARG High Resolution Spectrograph at the TNG, it was discovered that HD 200466A shows strong variation in RV that is well correlated with the activity index based on H{alpha}. We used SARG to study the H{alpha} line variations in each component of the binaries and a few bright stars to test the capability of the H{alpha} index of revealing the rotation period or activity cycle. We also analysed the relations between the average activity level and other physical properties of the stars. We finally tried to reveal signals in the RVs that are due to the activity. At least in some cases the variation in the observed RVs is due to the stellar activity. 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