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<ri:Resource created="1999-06-19T21:14:45Z" status="active" updated="2025-06-13T15:25:00Z" 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>10 Lac UV spectral atlas</title><shortName>J/AJ/116/941</shortName><identifier>ivo://CDS.VizieR/J/AJ/116/941</identifier><altIdentifier>doi:10.26093/cds/vizier.51160941</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brandt J.C.</name></creator><creator><name>Heap S.R.</name></creator><creator><name>Beaver E.A.</name></creator><creator><name>Boggess A.</name></creator><creator><name>Carpenter K.G.,Ebbets D.C.</name></creator><creator><name>Hutchings J.B.</name></creator><creator><name>Jura M.</name></creator><creator><name>Leckrone D.S.</name></creator><creator><name>Linsky J.L.,Maran S.P.</name></creator><creator><name>Savage B.D.</name></creator><creator><name>Smith A.M.</name></creator><creator><name>Trafton L.M.</name></creator><creator><name>Walter F.M.,Weymann R.J.</name></creator><creator><name>Snow M.</name></creator><creator><name>Ake T.B.</name></creator><creator><name>Hogen R.H.</name></creator><date role="Updated">2023-04-06T16:50:31Z</date><date role="Created">1999-06-19T21:14:45Z</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>o-stars</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><description>Observations of the narrow-lined O-type star 10 Lacertae taken with the Goddard High Resolution Spectrograph in 1992 November are presented. The spectra cover the wavelength range 1181-1777{AA} with a resolution of 15km/s and signal-to-noise ratio greater than 100:1. Absorption lines arising in the interstellar medium, the photosphere, and the stellar wind are identified and discussed.</description><source format="bibcode">1998AJ....116..941B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/116/941</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/93/211">J/ApJS/93/211 : IUE survey of H I Ly{alpha} absorption. I. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LambLab</name><description>Laboratory wavelength</description><unit>0.1nm</unit><ucd>em.wl;phys.atmol.transition</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LamObs</name><description>? Observed Wavelength</description><unit>0.1nm</unit><ucd>em.wl.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Species</name><description>Species (1)</description><ucd>phys.atmol.element</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>HV</name><description>? 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