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<ri:Resource created="2012-12-14T10:12:32Z" 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>Gas and stellar metallicities in HII galaxies</title><shortName>J/MNRAS/421/398</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/421/398</identifier><altIdentifier>doi:10.26093/cds/vizier.74210398</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Westera P.</name></creator><creator><name>Cuisinier F.</name></creator><creator><name>Curty D.</name></creator><creator><name>Buser R.</name></creator><date role="Updated">2024-07-17T20:15:29Z</date><date role="Created">2012-12-14T10:12:32Z</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>galaxies</subject><subject>spectroscopy</subject><subject>h-ii-regions</subject><description>We examine the gas and stellar metallicities in a sample of HII galaxies from the Sloan Digital Sky Survey, which possibly contains the largest homogeneous sample of HII galaxy spectra to date. We eliminated all spectra with an insufficient signal-to-noise ratio, without strong emission lines and without the [OII] {lambda}3727{AA} line, which is necessary for the determination of the gas metallicity. This excludes galaxies with redshift ~&lt;0.033. 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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>MJD</name><description>MJD SDSS spectroscopic ID</description><unit>d</unit><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Plate</name><description>Plate SDSS spectroscopic ID</description><unit>d</unit><ucd>meta.id;pos.parallax.spect;instr.plate</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Fiber</name><description>Fiber SDSS spectroscopic ID</description><ucd>meta.id;pos.parallax.spect</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>I(Hb)</name><description>H{beta} 4861{AA} intensity (in 10^-15^erg.cm^-2^.s^-1^)</description><unit>aW.m**-2</unit><ucd>phot.flux;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>I(Ha)</name><description>Flux ratio of H{alpha} 6563{AA} (1)</description><ucd>spect.line.intensity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>I([OII])</name><description>Flux ratio of [OII] 3727{AA} (1)</description><ucd>spect.line.intensity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S/N</name><description>Signal-to-noise ratio for [OII]</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>I([OIII]1)</name><description>Flux ratio of [OIII] 4959{AA} (1)</description><ucd>spect.line.intensity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>I([OIII]2)</name><description>Flux ratio of [OIII] 5007{AA} (1)</description><ucd>spect.line.intensity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>I([NII]1)</name><description>Flux ratio of [NII] 6548{AA} (1)</description><ucd>spect.line.intensity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>I([NII]2)</name><description>Flux ratio of [NII] 6584{AA} (1)</description><ucd>spect.line.intensity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E(B-V)</name><description>Internal redenning</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[O/H]P</name><description>Gas metallicity [O/H]_P_</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mtot</name><description>Total stellar mass</description><unit>1e+09solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sloan</name><description>Display the SDSS data for this galaxy</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Positions from SDSS DR7 (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from SDSS DR7 (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>