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<ri:Resource created="2013-12-19T08:28:49Z" 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>Line list for solar-type stars</title><shortName>J/A+A/561/A21</shortName><identifier>ivo://CDS.VizieR/J/A+A/561/A21</identifier><altIdentifier>doi:10.26093/cds/vizier.35610021</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sousa S.G.</name></creator><creator><name>Santos N.C.</name></creator><creator><name>Adibekyan V.</name></creator><creator><name>Delgado-Mena E.</name></creator><creator><name>Tabernero H.M.,Gonzalez Hernandez J.I.</name></creator><creator><name>Montes D.</name></creator><creator><name>Smiljanic R.</name></creator><creator><name>Korn A.J.</name></creator><creator><name>Bergemann M.,Soubiran C.</name></creator><creator><name>Mikolatis S.</name></creator><date role="Updated">2014-06-22T16:08:58Z</date><date role="Created">2013-12-19T08:28:49Z</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>metallicity</subject><subject>atomic-physics</subject><description>The homogenization of the stellar parameters is an important goal for large observational spectroscopic surveys, but it is very difficult to achieve it because of the diversity of the spectroscopic analysis methods used within a survey, such as spectrum synthesis and the equivalent width method. To solve this problem, constraints to the spectroscopic analysis can be set, such as the use of a common line-list. We present a procedure for selecting the best spectral lines from a given input line-list, which then allows us to derive accurate stellar parameters with the equivalent width method.</description><source format="bibcode">2014A&amp;A...561A..21S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/561/A21</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/A+A/458/873">J/A+A/458/873 : Metal-rich solar-type stars stellar parameters (Sousa+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/497/563">J/A+A/497/563 : Chemical abundances of 451 stars (Neves+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/512/A13">J/A+A/512/A13 : EW-Teff calibration for solar-type stars (Sousa+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/526/A99">J/A+A/526/A99 : Metal-poor solar-type stars spectroscopy &amp; masses</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/544/A106">J/A+A/544/A106 : p-mode frequencies of the solar twin 18 Sco (Bazot+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/555/A150">J/A+A/555/A150 : Cool solar-type stars precise parameters (Tsantaki+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/720/1592">J/ApJ/720/1592 : Abundances of solar analogs with planets (Hernandez+, 2010)</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/561/A21</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/561/A21</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/561/A21</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/561/A21</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/561/A21</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/561/A21</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"/></coverage><tableset><schema><name>default</name><table><name>J/A+A/561/A21/table2</name><description>Atomic parameters of the spectral lines</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>lambda</name><description>[4808/6610] Central wavelength {lambda} ({AA})</description><unit>0.1nm</unit><ucd>em.wl.central</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EP</name><description>Excitation potential</description><unit>eV</unit><ucd>phys.atmol.excitation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggf</name><description>Oscilator strength</description><ucd>phys.atmol.collStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>El</name><description>Element and ionisation (FeI or FeII)</description><ucd>phys.atmol.element;phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column></table></schema></tableset></ri:Resource>