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<ri:Resource created="2019-07-05T12:12:32Z" 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>GALEX spectral database correction with IUE SEDs</title><shortName>J/AJ/157/107</shortName><identifier>ivo://CDS.VizieR/J/AJ/157/107</identifier><altIdentifier>doi:10.26093/cds/vizier.51570107</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bohlin R.C.</name></creator><creator><name>Bianchi L.</name></creator><date role="Updated">2019-07-26T12:38:28Z</date><date role="Created">2019-07-05T12:12:32Z</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>white-dwarf-stars</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><description>The CALSPEC database of absolute spectral energy distributions (SEDs) from the Hubble Space Telescope is based on pure hydrogen model atmosphere calculations for three unreddened white dwarf stars and represents the current UV flux calibration standard with a precision approaching 1% for well observed stars. Following our previous work to correct International Ultraviolet Explorer (IUE) fluxes, this paper provides an average correction for the Galaxy Evolution Explorer (GALEX) spectral database that places GALEX fluxes on the current CALSPEC scale. Our correction is derived by comparing GALEX spectroscopic flux distributions with CALSPEC and corrected IUE SEDs. This recalibration is relevant for any project based on GALEX archival spectroscopic data, e.g., UV or multi-wavelength analyses, correlating GALEX spectra with other existing or future databases, and planning of new observations. The recalibration will be applied to our planned catalog of corrected GALEX SEDs.</description><source format="bibcode">2019AJ....157..107B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/157/107</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/ApJS/119/207">J/ApJS/119/207 : IUE echelle spectra of hot white dwarfs (Holberg+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/147/145">J/ApJS/147/145 : IUE low-dispersion spectra of white dwarfs (Holberg+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/596/A49">J/A+A/596/A49 : Synthetic GALEX photometry for IUE sources</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/162">J/AJ/155/162 : Comparison of IUE and CALSPEC SEDs for 6 WDs (Bohlin+, 2018)</relatedResource><relatedResource>http://archive.stsci.edu/prepds/galex-fluxcal/ : Online version of this paper</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/AJ/157/107</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/157/107</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/157/107</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/157/107</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/157/107</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/157/107</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/157/107/table2 (Spectra used for the IUE/GALEX comparison)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/157/107/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/157/107/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/157/107/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>12.515417</ra><dec>-52.137778</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/326 17094 19097 19141 19145 23101 23468 23476 23545 25742 26808 27863 28026 28538 32956 32958 33955 34975</spatial><spectral>8.591892718685687e-19 1.2907379771320717e-18</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/157/107?format=ascii</footprint><waveband>UV</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/157/107/table2</name><description>Spectra used for the IUE/GALEX comparison</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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