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<ri:Resource created="2007-02-12T15:27:09Z" 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>Effective temperatures of 215 FGK giants</title><shortName>J/MNRAS/371/879</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/371/879</identifier><altIdentifier>doi:10.26093/cds/vizier.73710879</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kovtyukh V.V.</name></creator><creator><name>Soubiran C.</name></creator><creator><name>Bienayme O.</name></creator><creator><name>Mishenina T.V.</name></creator><creator><name>Belik S.I.</name></creator><date role="Updated">2024-07-03T20:14:11Z</date><date role="Created">2007-02-12T15:27:09Z</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>giant-stars</subject><subject>effective-temperature</subject><description>We present precise effective temperatures (Teff) of 215 FGK giants determined using the method of line-depth ratios. For each star, we have measured the line depths and equivalent widths of a large number of spectral lines of low and high excitation potentials and established ~100 relations between Teff and their ratios. Starting with an initial value Teff, the relations are then self-calibrated by an iterative process. Our final estimates have been compared with very accurate (1 per cent) published temperatures and show a good agreement. Using our calibrations, we derive precise temperatures for 215 giants with near-solar metallicity, from high-resolution (R=42000) and high signal-to-noise ratio (S/N=100250) echelle spectra, obtained with the ELODIE spectrometer at the Observatoire de Haute Provence (OHP).</description><source format="bibcode">2006MNRAS.371..879K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/371/879</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/A+AS/129/505">J/A+AS/129/505 : Teff by Infrared Flux Method (Blackwell+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/339/858">J/A+A/339/858 : Calibration of stellar parameters (Di Benedetto 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/626/446">J/ApJ/626/446 : Effective temperature scale of FGK stars (Ramirez+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AN/321/277">J/AN/321/277 : MK-class III giants temperatures (Strassmeier+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/218">III/218 : ELODIE archive (Prugniel+, 2001)</relatedResource><relatedResource>http://atlas.obs-hp.fr/elodie/ : the ELODIE archive</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/MNRAS/371/879</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/371/879</mirrorURL><mirrorURL 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(Effective temperatures of the programme stars)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/371/879/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/371/879/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/371/879/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>4.1418367</ra><dec>8.2401564</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/140 166 210 327 341 377 428 915 1249 1819 1960 1998 2014 2202 2229 2324 2433 2440 2541 2828 3026 3094 3146 3335 3418 3619 3755 4051 4090 4226 4444 4559 4574 4794 4969 4985 5059 5245 5286 5530 5587 5589 5789 5815 5950 5983 6120 6166 6203 6334 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