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<ri:Resource created="2015-09-30T09:13:31Z" status="active" updated="2025-05-19T09:50:00Z" 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>Keck+HIRES spectra of HD 80606 and HD 80607</title><shortName>J/A+A/582/A17</shortName><identifier>ivo://CDS.VizieR/J/A+A/582/A17</identifier><altIdentifier>doi:10.26093/cds/vizier.35820017</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Saffe C.</name></creator><creator><name>Flores M.</name></creator><creator><name>Buccino A.</name></creator><date role="Updated">2015-09-30T09:44:10Z</date><date role="Created">2015-09-30T09:13:31Z</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>solar-system-planets</subject><subject>chemical-abundances</subject><subject>spectroscopy</subject><description>We explore the probable chemical signature of planet formation in the remarkable binary system HD 80606/7. The star HD 80606 hosts a giant planet with 4 MJup detected by both transit and radial velocity techniques. We study condensation temperature Tc trends of volatile and refractory element abundances to determine whether there is a depletion of refractories that could be related to the terrestrial planet formation. 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