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<ri:Resource created="2007-04-30T19:28:22Z" status="active" updated="2026-03-17T20:04:32Z" 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>High-dispersion spectra of nearby F-K stars</title><shortName>J/PASJ/57/13</shortName><identifier>ivo://CDS.VizieR/J/PASJ/57/13</identifier><altIdentifier>doi:10.26093/cds/vizier/bj-1s-d</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Takeda Y.</name></creator><creator><name>Sato B.</name></creator><creator><name>Kambe E.</name></creator><creator><name>Masuda S.</name></creator><creator><name>Izumiura H.</name></creator><creator><name>Watanabe E.,Ohkubo M.</name></creator><creator><name>Yanagisawa K.</name></creator><creator><name>Yasaka Y.</name></creator><creator><name>Honda S.</name></creator><creator><name>Kawanomoto S.</name></creator><creator><name>Aoki W.,Ando H.</name></creator><creator><name>Sadakane K.</name></creator><creator><name>Takada-hidai M.</name></creator><creator><name>Miyama S.M.</name></creator><date role="Updated">2026-03-17T20:04:32Z</date><date role="Created">2007-04-30T19:28:22Z</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>late-type-stars</subject><subject>spectroscopy</subject><description>Towards constructing a system of high-dispersion spectroscopic standard stars with well-established abundances, so that adequate reference stars of similar properties may be found for precise differential abundance studies of any near-solar type stars, we have collected high-resolution (R~70000) echelle spectra for 160 F-K dwarfs and subgiants of the solar neighborhood in three wavelength regions (5000-6200{AA}, 5800-7000{AA}, and 7600-8800{AA}) at Okayama Astrophysical Observatory. 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