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<ri:Resource created="2000-10-29T18:50:38Z" 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>YSOs in the l=+45 ISOGAL field</title><shortName>J/A+A/362/199</shortName><identifier>ivo://CDS.VizieR/J/A+A/362/199</identifier><altIdentifier>doi:10.26093/cds/vizier.33620199</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Felli M.</name></creator><creator><name>Comoretto G.</name></creator><creator><name>Testi L.</name></creator><creator><name>Omont A.</name></creator><creator/><creator><name>Schuller F.</name></creator><date role="Updated">2000-10-29T17:51:43Z</date><date role="Created">2000-10-29T18:50:38Z</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>young-stellar-objects</subject><subject>infrared-sources</subject><subject>infrared-photometry</subject><description>The 7 and 15{mu}m observations of the Galaxy obtained by the ISOGAL program offer an unique possibility to investigate and separate the different populations of stars in the Galactic Plane, in particular to study the population of low flux density YSOs which could not be detected with IRAS.</description><source 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