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<ri:Resource created="2018-08-30T10:00:51Z" status="active" updated="2025-06-13T15:25:00Z" version="1.2" 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/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>Vanadium transitions in the spectrum of Arcturus</title><shortName>J/ApJS/234/25</shortName><identifier>ivo://CDS.VizieR/J/ApJS/234/25</identifier><altIdentifier>doi:10.26093/cds/vizier.22340025</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wood M.P.</name></creator><creator><name>Sneden C.</name></creator><creator><name>Lawler J.E.</name></creator><creator><name>Den Hartog E.A.</name></creator><creator><name>Cowan J.J.</name></creator><creator><name>Nave G.</name></creator><date role="Updated">2018-10-22T07:58:30Z</date><date role="Created">2018-08-30T10:00:51Z</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>atomic-physics</subject><subject>chemical-abundances</subject><subject>giant-stars</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><subject>infrared-astronomy</subject><description>We derive a new abundance for vanadium in the bright, mildly metal-poor red giant Arcturus. This star has an excellent high-resolution spectral atlas and well-understood atmospheric parameters, and it displays a rich set of neutral vanadium lines that are available for abundance extraction. We employ a newly recorded set of laboratory FTS spectra to investigate any potential discrepancies in previously reported V I log(gf) values near 900nm. These new spectra support our earlier laboratory transition data and the calibration method utilized in that study. We then perform a synthetic spectrum analysis of weak V I features in Arcturus, deriving log{epsilon}(V)=3.54+/-0.01 ({sigma}=0.04) from 55 lines. There are no significant abundance trends with wavelength, line strength, or lower excitation energy.</description><source format="bibcode">2018ApJS..234...25W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/234/25</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/pastel">B/pastel : The PASTEL catalogue (Soubiran+, 2016-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/124">III/124 : Spectrophotometry of 60 stars (Kiehling, 1987)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/111/445">J/ApJS/111/445 : Spectra of normal stars in the K band (Wallace+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/129/237">J/A+AS/129/237 : G and K dwarfs abundances (Feltzing+ 1998)</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>lambda</name><description>[554.4/908.6] Wavelength</description><unit>nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Elower</name><description>[0.01/2.4] Lower energy level</description><unit>eV</unit><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggf</name><description>[-3.7/-0.1] log(gf) from Lawler+ 2014, J/ApJS/215/20</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loge</name><description>[3.4/3.7] log{epsilon} from Lawler+ 2014, J/ApJS/215/20</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggf2</name><description>[-3.5/-0.8]? log(gf) from Holmes+, 2016, J/ApJS/224/35</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>loge2</name><description>[3.3/3.8]? log{epsilon} from Holmes+, 2016, J/ApJS/224/35</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJS/234/25/table3</name><description>Hyperfine Structure (HFS) line component patterns</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>WaveNum</name><description>[10918.1/41621] Center-of-Gravity Wavenumber (1)</description><unit>cm**-1</unit><ucd>em.wavenumber</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>lamAir</name><description>[240.1/915.7] Center-of-Gravity Air Wavelength (1)</description><unit>nm</unit><ucd>em.wl;phys.atmol.transition</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Fupp</name><description>[0/11] Component upper level F or total angular momentum (2)</description><ucd>phys.atmol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Flow</name><description>[0/10] Component lower level F or total angular momentum (2)</description><ucd>phys.atmol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CWaveR</name><description>[-0.5/0.4] Component offset Wavenumber with respect to Center-of-gravity Wavenumber (2)</description><unit>cm**-1</unit><ucd>stat.fit.omc;phys.energy</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>CWave</name><description>[-20.7/26.2] Component offset Wavelength with respect to Center-of-gravity Wavelength (2)</description><unit>pm</unit><ucd>stat.fit.omc;phys.energy</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Str</name><description>[0/0.4] Component strength (2)(3)</description><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>