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<ri:Resource created="2012-01-20T07:48:01Z" status="active" updated="2025-09-29T20:17:54Z" 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>Colour indices of selected OB stars</title><shortName>J/AN/333/60</shortName><identifier>ivo://CDS.VizieR/J/AN/333/60</identifier><altIdentifier>doi:10.26093/cds/vizier.113330060</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Krelowski J.</name></creator><creator><name>Strobel A.</name></creator><date role="Updated">2025-09-29T20:17:54Z</date><date role="Created">2012-01-20T07:48:01Z</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>ob-stars</subject><subject>ultraviolet-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>infrared-photometry</subject><description>We have applied the method of investigating extinction curves using statistically meaningful samples that was proposed by us 25 years ago. The extensive data sets of the ANS (Astronomical Netherlands Satellite) and 2MASS (Two Micron All Sky Survey) were used, together with UBV photometry to create average extinction curves for samples of OB stars. Our results demonstrate that in the vast majority of cases the extinction curves are very close to the mean galactic extinction curve. Only a few objects were found to be obviously discrepant from the average. 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