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<ri:Resource created="2026-02-25T15:54:10Z" status="active" updated="2026-02-25T14:59:58Z" 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>Chemical abundances of Cet II brightest star</title><shortName>J/ApJ/959/141</shortName><identifier>ivo://CDS.VizieR/J/ApJ/959/141</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Webber K.B.</name></creator><creator><name>Hansen T.T.</name></creator><creator><name>Marshall J.L.</name></creator><creator><name>Simon J.D.</name></creator><creator><name>Pace A.B.,Mutlu-Pakdil B.</name></creator><creator><name>Drlica-Wagner A.</name></creator><creator><name>Martinez-Vazquez C.E.</name></creator><creator><name>Aguena M.,Allam S.S.</name></creator><creator><name>Alves O.</name></creator><creator><name>Bertin E.</name></creator><creator><name>Brooks D.</name></creator><creator><name>Carnero Rosell A.,Carretero J.</name></creator><creator><name>da Costa L.N.</name></creator><creator><name>De Vicente J.</name></creator><creator><name>Doel P.</name></creator><creator><name>Ferrero I.,Friedel D.</name></creator><creator><name>Frieman J.</name></creator><creator><name>Garcia-Bellido J.</name></creator><creator><name>Giannini G.</name></creator><creator><name>Gruen D.,Gruendl R.A.</name></creator><creator><name>Hinton S.R.</name></creator><creator><name>Hollowood D.L.</name></creator><creator><name>Honscheid K.</name></creator><creator><name>Kuehn K.,Mena-Fernandez J.</name></creator><creator><name>Menanteau F.</name></creator><creator><name>Miquel R.</name></creator><creator><name>Ogando R.L.C.</name></creator><creator><name>Pereira M.E.S.,Pieres A.</name></creator><creator><name>Plazas Malagon A.A.</name></creator><creator><name>Sanchez E.</name></creator><creator><name>Santiago B.</name></creator><creator><name>Smith J.A.,Smith M.</name></creator><creator><name>Suchyta E.</name></creator><creator><name>Tarle G.</name></creator><creator><name>To C.</name></creator><creator><name>Weaverdyck N.</name></creator><creator><name>Yanny B.</name></creator><date role="Updated">2026-02-25T14:59:58Z</date><date role="Created">2026-02-25T15:54:10Z</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>dwarf-galaxies</subject><subject>line-intensities</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-photometry</subject><subject>broad-band-photometry</subject><subject>radial-velocity</subject><description>We present a detailed chemical abundance analysis of the brightest star in the ultrafaint dwarf (UFD) galaxy candidate Cetus II from high-resolution Magellan/MIKE spectra. For this star, DES_J011740.53-173053, abundances or upper limits of 18 elements from carbon to europium are derived. Its chemical abundances generally follow those of other UFD galaxy stars, with a slight enhancement of the {alpha}-elements (Mg, Si, and Ca) and low neutron-capture element (Sr, Ba, and Eu) abundances supporting the classification of Cetus II as a likely UFD. The star exhibits lower Sc, Ti, and V abundances than Milky Way (MW) halo stars with similar metallicity. This signature is consistent with yields from a supernova originating from a star with a mass of ~11.2M_{sun}_. In addition, the star has a potassium abundance of [K/Fe]=0.81, which is somewhat higher than the K abundances of MW halo stars with similar metallicity, a signature that is also present in a number of UFD galaxies. A comparison including globular clusters and stellar stream stars suggests that high K is a specific characteristic of some UFD galaxy stars and can thus be used to help classify objects as UFD galaxies.</description><source format="bibcode">2023ApJ...959..141W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/959/141</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/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/416/1117">J/A+A/416/1117 : Abundances in the early Galaxy (Cayrel+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/439/129">J/A+A/439/129 : HERES II. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column><column><name>ID</name><description>Abbreviated ID used in the paper</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</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>gmag0</name><description>[16.443] Dereddened DES g-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rmag0</name><description>[15.716] Dereddened DES r-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>imag0</name><description>[15.818] Dereddened DES i-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zmag0</name><description>[16.014] Dereddened DES z-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HJD</name><description>Heliocentric Julian Date at the beginning of the exposure</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ExpTime</name><description>Exposure times</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>S/N</name><description>[15/21] Signal-to-noise ratio per pixel at 4500{AA}</description><ucd>stat.snr;instr.pixel</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HRV</name><description>[-81.9/-81.38] Heliocentric radial velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_HRV</name><description>[0.51/0.52] HRV uncertainty</description><unit>km/s</unit><ucd>stat.error;spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/959/141/table2</name><description>Data for atomic lines used in analysis and individual line EW measurements</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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