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<ri:Resource created="2008-01-20T17:05:30Z" status="active" updated="2025-09-09T14:12:29Z" 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>Late-type stars toward galactic antirotation</title><shortName>J/PASP/111/1169</shortName><identifier>ivo://CDS.VizieR/J/PASP/111/1169</identifier><altIdentifier>doi:10.26093/cds/vizier.61111169</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Westpfahl D.J.</name></creator><creator><name>Bell D.J.</name></creator><creator><name>Yoss K.M.</name></creator><date role="Updated">2025-09-09T14:12:29Z</date><date role="Created">2008-01-20T17:05:30Z</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>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>morgan-keenan-classification</subject><description>Low-resolution objective-prism spectra (1360{AA}/mm at H{gamma}) of 184 late-type stars in the Galactic antirotation direction have been obtained with the Curtis Schmidt telescope at Cerro Tololo Inter-American Observatory. The stars have been classified into three groups: F6-G2, G3-K0, and K1-M8. Subsequent observations on the BV and DDO systems have been obtained. The correlation between the thin-prism classes and the DDO classes is as expected, with no significant systematic differences of note. A comparison of Guide Star Catalog magnitudes, corrected to V, is also made, with favorable results. 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