<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2019-09-20T14:03:42Z" status="active" updated="2025-06-13T15:25:00Z" 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>Abundances of 3 bright extremely metal-poor giants</title><shortName>J/ApJ/864/43</shortName><identifier>ivo://CDS.VizieR/J/ApJ/864/43</identifier><altIdentifier>doi:10.26093/cds/vizier.18640043</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cain M.</name></creator><creator><name>Frebel A.</name></creator><creator><name>Gull M.</name></creator><creator><name>Ji A.P.</name></creator><creator><name>Placco V.M.</name></creator><creator><name>Beers T.C.</name></creator><creator><name>Melendez J.,Ezzeddine R.</name></creator><creator><name>Casey A.R.</name></creator><creator><name>Hansen T.T.</name></creator><creator><name>Roederer I.U.</name></creator><creator><name>Sakari C.</name></creator><date role="Updated">2020-04-30T07:23:48Z</date><date role="Created">2019-09-20T14:03:42Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>chemical-abundances</subject><subject>giant-stars</subject><subject>halo-stars</subject><subject>line-intensities</subject><description>We present detailed chemical abundances of three new bright (V~11), extremely metal-poor ([Fe/H]~-3.0), r-process-enhanced halo red giants based on high-resolution, high-S/N Magellan/MIKE spectra. We measured abundances for 20-25 neutron-capture elements in each of our stars. J1432-4125 is among the most r-process-rich r-II stars, with [Eu/Fe]=+1.44+/-0.11. J2005-3057 is an r-I star with [Eu/Fe]=+0.94+/-0.07. J0858-0809 has [Eu/Fe]=+0.23+/-0.05 and exhibits a carbon abundance corrected for an evolutionary status of [C/Fe]_corr_=+0.76, thus adding to the small number of known carbon-enhanced r-process stars. All three stars show remarkable agreement with the scaled solar r-process pattern for elements above Ba, consistent with enrichment of the birth gas cloud by a neutron star merger. The abundances for Sr, Y, and Zr, however, deviate from the scaled solar pattern. This indicates that more than one distinct r-process site might be responsible for the observed neutron-capture element abundance pattern. Thorium was detected in J1432-4125 and J2005-3057. Age estimates for J1432-4125 and J2005-3057 were adopted from one of two sets of initial production ratios each by assuming the stars are old. This yielded individual ages of 12+/-6Gyr and 10+/-6Gyr, respectively.</description><source format="bibcode">2018ApJ...864...43C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/864/43</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/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/279">III/279 : RAVE 5th data release (Kunder+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/439/129">J/A+A/439/129 : HERES II. Spectroscopic analysis (Barklem+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/655/492">J/ApJ/655/492 : Equivalent widths of 26 metal-poor stars (Aoki+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/80">J/ApJS/182/80 : Rare earth abundances (Sneden+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/175">J/AJ/141/175 : Abundances in M15 RGB/RHB stars (Sobeck+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/769/57">J/ApJ/769/57 : Equivalent widths of metal-poor stars (Frebel+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/762/26">J/ApJ/762/26 : Most metal-poor stars. II. Galactic halo stars (Yong+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/794/58">J/ApJ/794/58 : Metal-poor stars in the Galaxy thick disk (Beers+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/215/23">J/ApJS/215/23 : FeI branching fractions (Den Hartog+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/571/A47">J/A+A/571/A47 : Linelist of CH in stellar atmospheres (Masseron+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/797/21">J/ApJ/797/21 : Carbon-enhanced metal-poor stars (Placco+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/441/3127">J/MNRAS/441/3127 : FeI oscillator strengths for Gaia-ESO (Ruffoni+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/214/26">J/ApJS/214/26 : Line lists for CN isotopes transitions (Sneden+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/830/93">J/ApJ/830/93 : Ret II brightest red giant member abundances (Ji+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/817/53">J/ApJ/817/53 : Fe-group abundance analysis in HD84937 (Sneden+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/835/81">J/ApJ/835/81 : Bright metal-poor stars from HES Survey. II. (Beers+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/847/142">J/ApJ/847/142 : Ultra-metal-poor stars LTE &amp; NLTE abund. (Ezzeddine+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/838/44">J/ApJ/838/44 : Abundances of Tuc III brightest members (Hansen+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/607/A91">J/A+A/607/A91 : CS 29497-004 abundances (Hill+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/844/18">J/ApJ/844/18 : RAVE J203843.2-002333 high-res. spectroscopy (Placco+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/838/11">J/ApJ/838/11 : Member stars in the MW satellite Tucana III (Simon+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/612/A90">J/A+A/612/A90 : Inelastic Fe+H collision data (Barklem, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/858/92">J/ApJ/858/92 : RPA Southern Pilot Search of 107 Stars (Hansen+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/256">J/AJ/155/256 : Spectroscopy of RAVE metal-poor stars (Placco+, 2018)</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/864/43</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/864/43</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/864/43</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/864/43</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/864/43</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/864/43</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/864/43/stars (Stellar parameters and observation details (Tables 1 and 2))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/864/43/stars?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/864/43/stars?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/864/43/stars?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>134.524167</ra><dec>-8.154722</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/40898 43367 47955</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/864/43?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/864/43/table3</name><description>Equivalent width and synthesis measurements for J0858-0809, J1432-4125, and J2005-3057</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>Ion</name><description>Element/Ion identifier</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>lambda</name><description>[3329.4/8824.3] Wavelength; Angstrom</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ExPot</name><description>[0/4.5]? Excitation potential</description><unit>eV</unit><ucd>phys.atmol.excitation</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(gf)</name><description>[-9.9/0.8]? log oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EW1</name><description>[1.8/219.4]? Equivalenth width of J0858-0809 (1)</description><unit>1e-13m</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_EW1</name><description>[s] Flag on EW1 (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_loge1</name><description>Limit flag on loge1</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>loge1</name><description>[-3.1/6.5]? log absolute abundance of J0858-0809</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EW2</name><description>[3.5/208.3]? Equivalenth width of J1432-4125 (1)</description><unit>1e-13m</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_EW2</name><description>[s] Flag on EW2 (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_loge2</name><description>Limit flag on loge2</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>loge2</name><description>[-1.7/5.7]? log absolute abundance of J1432-4125</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EW3</name><description>[2.6/250.7]? Equivalenth width of J2005-3057 (1)</description><unit>1e-13m</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_EW3</name><description>[s] Flag on EW3 (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_loge3</name><description>Limit flag on loge3</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>loge3</name><description>[-2.2/6.6]? log absolute abundance of J2005-3057</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/864/43/stars</name><description>Stellar parameters and observation details (Tables 1 and 2)</description><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></column><column><name>Exp2</name><description>? Exposure time of the second observation</description><unit>min</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></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>Name</name><description>Star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Teff1</name><description>[4430/4900] LTE corrected effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg1</name><description>[0.6/1.7] LTE corrected surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vt1</name><description>[1.6/2.3] LTE corrected microturbulent velocity</description><unit>km/s</unit><ucd>phys.veloc.microTurb</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]1</name><description>[-3.2/-2.9] LTE corrected [Fe/H]</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff2</name><description>[4180/4705] LTE uncorrected effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg2</name><description>[0/1.2] LTE uncorrected surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vt2</name><description>[1.5/2.2] LTE uncorrected microturbulent velocity</description><unit>km/s</unit><ucd>phys.veloc.microTurb</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]2</name><description>[-3.4/-3.1] LTE uncorrected [Fe/H]</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff3</name><description>[4300/4850] NLTE effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg3</name><description>[0.9/1.9] NLTE surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vt3</name><description>[1.5/2.2] NLTE microturbulent velocity</description><unit>km/s</unit><ucd>phys.veloc.microTurb</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]3</name><description>[-2.9/-2.8] NLTE [Fe/H]</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff4</name><description>[4599/5334] Effective temperature from medium-resolution spectrum</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg4</name><description>[0.9/2.7] Surface gravity from medium-resolution spectrum</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]4</name><description>[-3.1/-2.9] [Fe/H] from medium-resolution spectrum</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</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>Obs</name><description>Observation date (UT)</description><unit>s</unit><ucd>time.epoch;obs</ucd><flag>nullable</flag></column><column><name>Slit</name><description>Slit</description><unit>arcsec</unit><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Exp</name><description>Exposure time</description><unit>min</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Vmag</name><description>V-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B-V</name><description>B-V color index</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SN4000</name><description>Signal-to-noise ratio per pixel at 4000{AA} (1)</description><ucd>stat.snr;instr.pixel</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SN4500</name><description>Signal-to-noise ratio per pixel at 4500{AA} (1)</description><ucd>stat.snr;instr.pixel</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SN6000</name><description>Signal-to-noise ratio per pixel at 6000{AA} (1)</description><ucd>stat.snr;instr.pixel</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HRV</name><description>Heliocentric velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Obs2</name><description>Second date of observation (UT)</description><unit>s</unit><ucd>time.epoch;obs</ucd><flag>nullable</flag></column><column><name>HRV2</name><description>? Second measure of heliocentric velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Link1</name><description>Display the equivalent widths for this star (link to Table 3)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>