<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2018-02-05T12:18:52Z" 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>Metallicity evolution of COSMOS BCD sample</title><shortName>J/ApJ/819/73</shortName><identifier>ivo://CDS.VizieR/J/ApJ/819/73</identifier><altIdentifier>doi:10.26093/cds/vizier.18190073</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lian J.</name></creator><creator><name>Hu N.</name></creator><creator><name>Fang G.</name></creator><creator><name>Ye C.</name></creator><creator><name>Kong X.</name></creator><date role="Updated">2018-07-02T15:17:07Z</date><date role="Created">2018-02-05T12:18:52Z</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>line-intensities</subject><subject>redshifted</subject><subject>extinction</subject><subject>chemical-abundances</subject><description>We present oxygen abundance measurements for 74 blue compact dwarf (BCD) galaxies in the redshift range of [0.2, 0.5] using the strong-line method. The spectra of these objects are taken using Hectospec on the Multiple Mirror Telescope. More than half of these BCDs had dust attenuation corrected using the Balmer decrement method. For comparison, we also selected a sample of 2023 local BCDs from the Sloan Digital Sky Survey (SDSS) database. Based on the local and intermediate-z BCD samples, we investigated the cosmic evolution of the metallicity, star formation rate (SFR), and D_n_(4000) index. Compared with local BCDs, the intermediate-z BCDs had a systematically higher R23 ratio but a similar O32 ratio. Interestingly, no significant deviation in the mass-metallicity (MZ) relation was found between the intermediate-z and local BCDs. Besides the metallicity, the intermediate-z BCDs also exhibited an SFR distribution that was consistent with local BCDs, suggesting a weak dependence on redshift. The intermediate-z BCDs seemed to be younger than the local BCDs with lower D_n_(4000) index values. The insignificant deviation in the mass-metallicity and mass-SFR relations between intermediate-z and local BCDs indicates that the relations between the global parameters of low-mass compact galaxies may be universal. These results from low-mass compact galaxies could be used to place important observational constraints on galaxy formation and evolution models.</description><source format="bibcode">2016ApJ...819...73L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/819/73</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/ApJS/147/29">J/ApJS/147/29 : BRHalpha data of blue compact dwarf galaxies</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/429/115">J/A+A/429/115 : JHK' photometry of Blue Compact Dwarf Galaxies (Noeske+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/434/887">J/A+A/434/887 : HI data of blue compact dwarf galaxies (Huchtmeier+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/156/345">J/ApJS/156/345 : Surface photometry of BCD galaxies (Gil de Paz+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/206/8">J/ApJS/206/8 : COSMOS/UltraVISTA Ks-selected catalogs v4.1 (Muzzin+, 2013)</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/ApJ/819/73</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/819/73</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/819/73</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/819/73</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/819/73</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/819/73</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/819/73/table1 (Emission Line Measurements of COSMOS BCD Sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/819/73/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/819/73/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/819/73/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>149.9057917</ra><dec>2.0846667</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/6814</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/819/73?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJ/819/73/table1</name><description>Emission Line Measurements of COSMOS BCD Sample</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="29*">char</dataType></column><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>ID</name><description>[1/74] Source identification number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>F3727</name><description>Flux of [OII]{lambda}3727 line (in 10^-18^erg/s/cm^2^)</description><unit>1e-21W.m**-2</unit><ucd>phot.flux;spect.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F3727</name><description>Uncertainty in F3727</description><unit>1e-21W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FHg</name><description>? H{gamma} line flux</description><unit>1e-21W.m**-2</unit><ucd>phot.flux;em.line.Hgamma;spect.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_FHg</name><description>? Uncertainty in FHg</description><unit>1e-21W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FHb</name><description>H{beta} line flux</description><unit>1e-21W.m**-2</unit><ucd>phot.flux;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_FHb</name><description>Uncertainty in FHb</description><unit>1e-21W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EW(Hb)</name><description>Equivalent width of H{beta} ({AA})</description><unit>0.1nm</unit><ucd>spect.line.eqWidth;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F4959</name><description>Flux of [OIII]{lambda}4959 line (in 10^-18^erg/s/cm^2^)</description><unit>1e-21W.m**-2</unit><ucd>phot.flux;em.line.OIII;spect.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F4959</name><description>Uncertainty in F4959</description><unit>1e-21W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F5007</name><description>Flux of [OIII]{lambda}5007 line (in 10^-18^erg/s/cm^2^)</description><unit>1e-21W.m**-2</unit><ucd>phot.flux;em.line.OIII;spect.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F5007</name><description>Uncertainty in F5007</description><unit>1e-21W.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>COSMOS</name><description>Display the data from Muzzin et al. (2013, Cat. J/ApJS/206/8)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/ApJ/819/73/table2</name><description>Physical Properties of COSMOS BCD Sample</description><column><name>z</name><description>Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>12+log(O/H)</name><description>Oxygen abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_Av</name><description>[s] Note on Av (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><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>ID</name><description>[1/74] Source identification number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Av</name><description>Dust extinction</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>Log of stellar mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_12+log(O/H)</name><description>Uncertainty in 12+log(O/H)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(SFR)</name><description>Log of star formation rate (2)</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log(SFR)</name><description>Uncertainty in log(SFR)</description><unit>log(solMass.yr**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dn(4000)</name><description>? D_n_(4000) index (3)</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>