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<ri:Resource created="2015-09-15T08:22:02Z" 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>G0-G3 main-sequence stars with V&lt;15</title><shortName>J/MNRAS/444/2251</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/444/2251</identifier><altIdentifier>doi:10.26093/cds/vizier.74442251</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lopez-Valdivia R.</name></creator><creator><name>Bertone E.</name></creator><creator><name>Chavez M.</name></creator><creator><name>Tapia-Schiavon C.,Hernandez-Aguila J.B.</name></creator><creator><name>Valdes J.R.</name></creator><creator><name>Chavushyan V.</name></creator><date role="Updated">2024-08-10T20:18:41Z</date><date role="Created">2015-09-15T08:22:02Z</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>g-stars</subject><subject>dwarf-stars</subject><subject>effective-temperature</subject><subject>chemical-abundances</subject><description>The basic stellar atmospheric parameters (effective temperature, surface gravity and global metallicity) were determined simultaneously for a sample of 233 stars, limited in magnitude (V&lt;15), with spectral types between G0 and G3 and luminosity class V (main sequence). The analysis was based on spectroscopic observations collected at the Observatorio Astrofisico Guillermo Haro and using a set of Lick-like indices defined in the spectral range 3800-4800{AA}. An extensive set of indices computed in a grid of theoretical spectra was used as a comparison tool in order to determine the photospheric parameters. The method was validated by matching the results from spectra of the asteroids Vesta and Ceres with the Sun parameters. 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