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<ri:Resource created="2019-11-04T07:33:31Z" 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>504 F-G dwarfs photometric metallicities</title><shortName>J/other/ApSS/364</shortName><identifier>ivo://CDS.VizieR/J/other/ApSS/364.172</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Celebi M.</name></creator><creator><name>Bilir S.</name></creator><creator><name>Ak S.</name></creator><creator><name>Ak T.</name></creator><creator><name>Bostanci Z.F.</name></creator><creator><name>Yontan T.</name></creator><date role="Updated">2019-11-04T06:34:16Z</date><date role="Created">2019-11-04T07:33:31Z</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>visible-astronomy</subject><subject>Wide-band photometry</subject><subject>metallicity</subject><subject>stellar-distance</subject><description>In this study, photometric metallicity and absolute magnitude calibrations were derived using F-G spectral type main-sequence stars in the Solar neighbourhood with precise spectroscopic, photometric and Gaia astrometric data for UBV photometry. The sample consists of 504 main-sequence stars covering the temperature, surface gravity and colour index intervals 5300&lt;Teff&lt;7300K, logg&gt;4 (cgs) and 0.3&lt;(B-V)0&lt;0.8mag, respectively. Stars with relative trigonometric parallax errors {sigma}_{pi}/{pi}&lt;=0.01 were preferred from Gaia DR2 data for the estimation of their M_V absolute magnitudes. In order to obtain calibrations, (U-B)0 and (B-V)0 colour indices of stars were preferred and a multi-variable second order equation was used. Calibrations are valid for main-sequence stars in the metallicity and absolute magnitude ranges -2&lt;[Fe/H]&lt;0.5dex and 2.5&lt;M_V_&lt;6mag, respectively. The mean value and standard deviation of the differences between original and estimated values for the metal abundance and absolute magnitude are &lt;{Delta}[Fe/H]&gt;=0.00+/-0.11dex and &lt;{Delta}M_V_&gt;=0.00+/-0.22mag, respectively. 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