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<ri:Resource created="2013-02-13T08:32:26Z" 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>Sydney observatory Galactic survey (SOGS)</title><shortName>J/A+A/469/1221</shortName><identifier>ivo://CDS.VizieR/J/A+A/469/1221</identifier><altIdentifier>doi:10.26093/cds/vizier.34691221</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fresneau A.</name></creator><creator><name>Vaughan A.E.</name></creator><creator><name>Argyle R.W.</name></creator><date role="Updated">2017-07-13T11:09:08Z</date><date role="Created">2013-02-13T08:32:26Z</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>surveys</subject><subject>visible-astronomy</subject><subject>photographic-photometry</subject><description>First Epoch astrometric and radiometric information of a survey in the optical along the Galactic fourth quadrant is archived for further analysis in the time-domain. A photographic survey of 1.9x10^6^ stars down to B-magnitude 14.5+/-0.5 along the galactic meridian l=(330+/-5){deg},-64{deg}&lt;b&lt;-7{deg} and along the galactic equator 272{deg}&lt;l&lt;341{deg},-7{deg}&lt;b&lt;7{deg}, is provided from century old astrographic plates of Sydney Observatory. Stellar candidates to investigate the Galaxy disk kinematics up to a distance of 1kpc from the Sun are tentatively selected. A catalogue of 4.8x10^5^ stars is provided for further investigation of the galactic disk heating by transient spiral wave or by GMC encounter.</description><source format="bibcode">2007A&amp;A...469.1221F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/469/1221</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/2701">J/AJ/130/2701 : Stars in the Sagittarius Rift (Fresneau+, 2005)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface 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