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<ri:Resource created="2017-02-14T07:16:29Z" 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>RX J0503.9-2854 spectral energy distribution</title><shortName>J/A+A/598/A135</shortName><identifier>ivo://CDS.VizieR/J/A+A/598/A135</identifier><altIdentifier>doi:10.26093/cds/vizier.35980135</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hoyer D.</name></creator><creator><name>Rauch T.</name></creator><creator><name>Werner K.</name></creator><creator><name>Kruk J.W.</name></creator><creator><name>Quinet P.</name></creator><date role="Updated">2017-03-15T07:16:20Z</date><date role="Created">2017-02-14T07:16:29Z</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>spectral-energy-distribution</subject><subject>spectroscopy</subject><description>In the line-of-sight toward the DO-type white dwarf RX J0503.9-2854, the density of the interstellar medium (ISM) is very low, and thus the contamination of the stellar spectrum almost negligible. This allows us to identify many metal lines in a wide wavelength range from the extreme ultraviolet to the near infrared. In previous spectral analyses, many metal lines in the ultraviolet spectrum of RX J0503.9-2854 have been identified. A complete line list of observed and identified lines is presented here. We compared synthetic spectra that had been calculated from model atmospheres in non-local thermodynamical equilibrium, with observations. In total, we identified 1272 lines (279 of them were newly assigned) in the wavelength range from the extreme ultraviolet to the near infrared. 287 lines remain unidentified. A close inspection of the EUV shows that still no good fit to the observed shape of the stellar continuum flux can be achieved although He, C, N, O, Al, Si, P, S, Ca, Sc, Ti, V, Cr, Mn, Fe, Cr, Ni Zn, Ga, Ge, As, Kr, Zr, Mo, Sn, Xe, and Ba are included in the stellar atmosphere models.</description><source format="bibcode">2017A&amp;A...598A.135H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/598/A135</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/598/A135</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/598/A135</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/598/A135</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/598/A135</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/598/A135</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/598/A135</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>X-ray</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/598/A135/tablea4</name><description>Line list for optical spectrum of RX J0503.9-2854</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>El</name><description>Element with ionization stage</description><ucd>phys.atmol.ionStage;phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Lower</name><description>Lower level electron configuration or principal quantum number or energy in cm^-1^</description><ucd>phys.atmol.configuration</ucd></column><column><name>Upper</name><description>Upper level electron configuration or principal quantum number or energy in cm^-1^</description><ucd>phys.atmol.configuration</ucd></column><column><name>f</name><description>? Oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>EWobs</name><description>? Observed equivalent width (if measured)</description><unit>0.1pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>WTh</name><description>? Theoretical wavelength</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>WObs</name><description>? Observed wavelength (if measured)</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RV</name><description>? Radial velocity (if measured)</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Com</name><description>Comments</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="50*">char</dataType></column></table><table><name>J/A+A/598/A135/tablea1</name><description>Line list for EUVE spectrum of RX J0503.9-2854</description><column><name>Com</name><description>Comments</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="50*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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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>El</name><description>Element with ionization stage</description><ucd>phys.atmol.ionStage;phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Lower</name><description>Lower level electron configuration or principal quantum number or energy in cm^-1^</description><ucd>phys.atmol.configuration</ucd></column><column><name>Upper</name><description>Upper level electron configuration or principal quantum number or energy in cm^-1^</description><ucd>phys.atmol.configuration</ucd></column><column><name>f</name><description>? Oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>EWobs</name><description>? 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