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<ri:Resource created="2012-08-09T08:18:51Z" 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>Optical identification of 1RXS J180431.1-273932</title><shortName>J/A+A/544/A114</shortName><identifier>ivo://CDS.VizieR/J/A+A/544/A114</identifier><altIdentifier>doi:10.26093/cds/vizier.35440114</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Masetti N.</name></creator><creator><name>Nucita A.A.</name></creator><creator><name>Parisi P.</name></creator><date role="Updated">2017-06-01T08:52:49Z</date><date role="Created">2012-08-09T08:18:51Z</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>cataclysmic-variable-stars</subject><description>The X-ray source 1RXS J180431.1-273932 has been proposed as a new member of the symbiotic X-ray binary (SyXB) class of systems, which are composed of a late-type giant that loses matter to an extremely compact object, most likely a neutron star. In this paper, we present an optical campaign of imaging plus spectroscopy on selected candidate counterparts of this object. 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