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<ri:Resource created="2019-02-25T07:20:15Z" status="active" updated="2026-01-20T12:11:15Z" 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>DustPedia metallicities and HI masses</title><shortName>J/A+A/623/A5</shortName><identifier>ivo://CDS.VizieR/J/A+A/623/A5</identifier><altIdentifier>doi:10.26093/cds/vizier.36230005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>De Vis P.</name></creator><creator><name>Jones A.</name></creator><creator><name>Viaene S.</name></creator><creator><name>Casasola V.</name></creator><creator><name>Clark C.J.R.</name></creator><creator><name>Baes M.,Bianchi S.</name></creator><creator><name>Cassara L. P.</name></creator><creator><name>Davies J.I.</name></creator><creator><name>De Looze I.</name></creator><creator><name>Galametz M.,Galliano F.</name></creator><creator><name>Lianou S.</name></creator><creator><name>Madden S.</name></creator><creator><name>Manilla-Robles A.</name></creator><creator><name>Mosenkov A.V.,Nersesian A.</name></creator><creator><name>Roychowdhury S.</name></creator><creator><name>Xilouris E.M.</name></creator><creator><name>Ysard N.</name></creator><date role="Updated">2026-01-20T12:11:15Z</date><date role="Created">2019-02-25T07:20:15Z</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>chemical-abundances</subject><subject>narrow-band-photometry</subject><subject>atomic-spectroscopy</subject><subject>galaxies</subject><subject>h-i-line-emission</subject><subject>spectroscopy</subject><subject>interstellar-medium</subject><description>Observations of evolution in the dust-to-metal ratio allow to constrain the dominant dust processing mechanisms. In this work, we present a study of the dust-to-metal and dust-to-gas ratios in a subsample of ~500 DustPedia galaxies. Using literature and MUSE emission line fluxes, we derive gas-phase metallicities (oxygen abundances) for over 10000 individual regions and determine characteristic metallicities for each galaxy. We study how the relative dust, gas and metal contents of galaxies evolve by using metallicity and gas fraction as proxies for evolutionary state. The global oxygen abundance and nitrogen-to-oxygen ratio are found to increase monotonically as galaxies evolve. Additionally, unevolved galaxies (gas fraction &gt;60%, metallicity 12+log(O/H)&lt;8.2) have dust-to-metal ratios that are about a factor of 2.1 lower (factor of 6 lower for galaxies with gas fraction &gt;80%) than the typical dust-to-metal ratio (Md/MZ~0.214) for more evolved sources. However, for high gas fractions, the scatter is larger due to larger observational uncertainties as well as a potential dependence of the dust grain growth timescale and supernova dust yield on local conditions and star formation histories. We find chemical evolution models with a strong contribution from dust grain growth describe these observations reasonably well. The dust-to-metal ratio is also found to be lower for low stellar masses and high specific star formation rates (with the exception of some sources undergoing a starburst). Finally, the metallicity gradient correlates weakly with the HI-to-stellar mass ratio, the effective radius and the dust-to-stellar mass ratio, but not with stellar mass.</description><source format="bibcode">2019A&amp;A...623A...5D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/623/A5</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+A/609/A37">J/A+A/609/A37 : 875 nearby galaxies multiwavelength photometry (Clark+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/620/A112">J/A+A/620/A112 : Template SED of DustPedia galaxies 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Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></column><column><name>CHB</name><description>Balmer decrement</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>12+logOHPG16S</name><description>? Resolved metallicity using the Pilyugin &amp; Grebel (2016MNRAS.457.3678P) S calibration</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHPG16S</name><description>? Downwards uncertainty on 12+logOHPG16S</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHPG16S</name><description>? Upwards uncertainty on 12+logOHPG16S</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>12+logOHPG16R</name><description>? Resolved metallicity using the Pilyugin &amp; Grebel (2016MNRAS.457.3678P) R calibration</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHPG16R</name><description>? Downwards uncertainty on 12+logOHPG16R</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHPG16R</name><description>? Upwards uncertainty on 12+logOHPG16R</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>12+logOHN2</name><description>? Resolved metallicity using the Pettini &amp; Pagel (2004MNRAS.348L..59P) N2 calibration</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHN2</name><description>? Downwards uncertainty on 12+logOHN2</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHN2</name><description>? Upwards uncertainty on 12+logOHN2</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>12+logOHO3N2</name><description>? Resolved metallicity using the Pettini &amp; Pagel (2004MNRAS.348L..59P) O3N2 calibration</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHO3N2</name><description>? Downwards uncertainty on 12+logOHO3N2</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHO3N2</name><description>? Upwards uncertainty on 12+logOHO3N2</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>12+logOHIZI</name><description>? Resolved metallicity using the Bayesian-based IZI tool (Blanc et al. 2015ApJ...798...99B)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHIZI</name><description>? Downwards uncertainty on 12+logOHIZI</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHIZI</name><description>? Upwards uncertainty on 12+logOHIZI</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>IZIchi2</name><description>? Chi-squared for the IZI fit</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>12+logOHKK04</name><description>? Resolved metallicity using the Kobulnicky &amp; Kewley (2004ApJ...617..240K) calibration</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHKK04</name><description>? Downwards uncertainty on 12+logOHKK04</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHKK04</name><description>? Upwards uncertainty on 12+logOHKK04</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>12+logOHT04</name><description>? Resolved metallicity using the Tremonti et al. (2004ApJ...617..240K) calibration</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHT04</name><description>? Downwards uncertainty on 12+logOHT04</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHT04</name><description>? Upwards uncertainty on 12+logOHT04</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logNOPG16</name><description>? Resolved N/O ratio using Pilyugin &amp; Grebel (2016MNRAS.457.3678P)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_logNOPG16</name><description>? Downwards uncertainty on logNOPG16</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_logNOPG16</name><description>? Upwards uncertainty on logNOPG16</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>r/r25</name><description>? Deprojected radius of the region divided by the B-band isophotal radius r25</description><ucd>phys.size.radius;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>r/app</name><description>? Deprojected radius of the region divided by the photometry aperture radius</description><ucd>phys.size.radius;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Ref</name><description>Reference for the lines, in refs.dat file</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="45*">char</dataType></column></table><table><name>J/A+A/623/A5/dp-mg</name><description>Global metallicities and metal masses for each galaxy</description><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>Name</name><description>Galaxy name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>z</name><description>Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SF</name><description>Number of SF-classified regions for this galaxy</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AGN</name><description>Number of AGN-classified regions for this galaxy</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Comp</name><description>Number of composite-classified regions for this galaxy</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>12+logOHPG16S</name><description>? Global metallicity using the Pilyugin &amp; Grebel (2016MNRAS.457.3678P) S calibration</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHPG16S</name><description>? Downwards uncertainty on 12+logOHPG16S</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHPG16S</name><description>? Upwards uncertainty on 12+logOHPG16S</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MzPG16S</name><description>? Mass of metals for the Pilyugin &amp; Grebel (2016MNRAS.457.3678P) S calibration</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_MzPG16S</name><description>? Downwards uncertainty on MzPG16S</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_MzPG16S</name><description>? Upwards uncertainty on MzPG16S</description><unit>log(solMass)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>12+logOHPG16R</name><description>? Global metallicity using the Pilyugin &amp; Grebel (2016MNRAS.457.3678P) R calibration</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHPG16R</name><description>? Downwards uncertainty on 12+logOHPG16R</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHPG16R</name><description>? Upwards uncertainty on 12+logOHPG16R</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MzPG16R</name><description>? Mass of metals for the Pilyugin &amp; Grebel (2016MNRAS.457.3678P) R calibration</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_MzPG16R</name><description>? Downwards uncertainty on Mz_PG16R</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_MzPG16R</name><description>? Upwards uncertainty on MzPG16R</description><unit>log(solMass)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>12+logOHN2</name><description>? Global metallicity using the Pettini &amp; Pagel (2004MNRAS.348L..59P) N2 calibration</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHN2</name><description>? Downwards uncertainty on 12+logOHN2</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHN2</name><description>? Upwards uncertainty on 12+logOHN2</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MzN2</name><description>? Mass of metals for the Pettini &amp; Pagel (2004MNRAS.348L..59P) N2 calibration</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_MzN2</name><description>? Downwards uncertainty on MzN2</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_MzN2</name><description>? Upwards uncertainty on MzN2</description><unit>log(solMass)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>12+logOHO3N2</name><description>? Global metallicity using the Pettini &amp; Pagel (2004MNRAS.348L..59P) O3N2 calibration</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHO3N2</name><description>? Downwards uncertainty on 12+logOHO3N2</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHO3N2</name><description>? Upwards uncertainty on 12+logOHO3N2</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MzO3N2</name><description>? Mass of metals for the Pettini &amp; Pagel (2004MNRAS.348L..59P) O3N2 calibration</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_MzO3N2</name><description>? Downwards uncertainty on MzO3N2</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_MzO3N2</name><description>? Upwards uncertainty on MzO3N2</description><unit>log(solMass)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>12+logOHIZI</name><description>? Global metallicity using the Bayesian-based IZI tool (Blanc et al. 2015ApJ...798...99B)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHIZI</name><description>? Downwards uncertainty on 12+logOHIZI</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHIZI</name><description>? Upwards uncertainty on 12+logOHIZI</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MzIZI</name><description>? Mass of metals for the Bayesian-based IZI tool</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_MzIZI</name><description>? Downwards uncertainty on Mz_IZI</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_MzIZI</name><description>? Upwards uncertainty on Mz_IZI</description><unit>log(solMass)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>12+logOHKK04</name><description>? Global metallicity using the Kobulnicky &amp; Kewley (2004ApJ...617..240K) calibration</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHKK04</name><description>? Downwards uncertainty on 12+logOHKK04</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHKK04</name><description>? Upwards uncertainty on 12+logOHKK04</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MzK04</name><description>? Mass of metals for the Kobulnicky &amp; Kewley (2004ApJ...617..240K) calibration</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_MzK04</name><description>? Downwards uncertainty on MzK04</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_MzK04</name><description>? Upwards uncertainty on MzK04</description><unit>log(solMass)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>12+logOHT04</name><description>? Global metallicity using the Tremonti et al. (2004ApJ...613..898T) calibration</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_12+logOHT04</name><description>? Downwards uncertainty on 12+logOH_T04</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_12+logOHT04</name><description>? Upwards uncertainty on 12+logOH_T04</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>MzT04</name><description>? Mass of metals for the Tremonti et al. (2004ApJ...613..898T) calibration</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_MzT04</name><description>? Downwards uncertainty on MzT04</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_MzT04</name><description>? Upwards uncertainty on MzT04</description><unit>log(solMass)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logNOPG16</name><description>? Global N/O ratio using Pilyugin &amp; Grebel (2016MNRAS.457.3678P)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_logNOPG16</name><description>? Downwards uncertainty on logNOPG16</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_logNOPG16</name><description>? Upwards uncertainty on logNOPG16</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table><table><name>J/A+A/623/A5/refs</name><description>References</description><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>Com</name><description>Comments</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="74*">char</dataType></column><column><name>Ref</name><description>Reference code</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>BibCode</name><description>BibCode</description><ucd>meta.bib.bibcode</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Aut</name><description>Author's name</description><ucd>meta.bib.author</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column></table></schema></tableset></ri:Resource>