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<ri:Resource created="2005-11-24T20:34:23Z" 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>X-ray properties of NGC 300. I.</title><shortName>J/A+A/443/103</shortName><identifier>ivo://CDS.VizieR/J/A+A/443/103</identifier><altIdentifier>doi:10.26093/cds/vizier.34430103</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Carpano S.</name></creator><creator><name>Wilms J.</name></creator><creator><name>Schirmer M.</name></creator><creator><name>Kendziorra E.</name></creator><date role="Updated">2005-11-24T19:34:37Z</date><date role="Created">2005-11-24T20:34:23Z</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>x-ray-sources</subject><subject>astronomical-object-identification</subject><subject>visible-astronomy</subject><subject>photographic-photometry</subject><description>X-ray properties of NGC 300 point sources, extracted from 66ks of XMM-Newton data taken in 2000 December and 2001 January. A total of 163 sources were detected in the energy range of 0.3-6kev. We report on the global properties of the sources detected inside the D_25_ optical disk, such as the hardness ratio and X-ray fluxes, and on the properties of their optical counterparts found in B, V, and R images from the 2.2m MPG/ESO telescope. 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