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<ri:Resource created="2016-04-20T15:18:45Z" 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>NIR spectroscopy of Galactic WR stars. III</title><shortName>J/MNRAS/452/2858</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/452/2858</identifier><altIdentifier>doi:10.26093/cds/vizier.74522858</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kanarek G.</name></creator><creator><name>Shara M.</name></creator><creator><name>Faherty J.</name></creator><creator><name>Zurek D.</name></creator><creator><name>Moffat A.</name></creator><date role="Updated">2024-08-15T20:14:25Z</date><date role="Created">2016-04-20T15:18:45Z</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>wolf-rayet-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>line-intensities</subject><subject>stellar-spectral-types</subject><description>A new method of image subtraction is applied to images from a J, K, and narrow-band imaging survey of 300 deg2 of the plane of the Galaxy, searching for new Wolf-Rayet (WR) stars. Our survey spans 150{deg} in Galactic longitude and reaches b=+/-1{deg} with respect to the Galactic plane. The survey has a useful limiting magnitude of K=15 over most of the observed Galactic plane, and K=14 (due to severe crowding) within a few degrees of the Galactic Centre. The new image subtraction method described here (better than aperture or even point-spread-function photometry in very crowded fields) detected several thousand emission-line candidates. In 2011 and 2012 June and July, we spectroscopically followed up on 333 candidates with MDM-TIFKAM and Infrared Telescope Facility (IRTF)-SpeX, discovering 89 emission-line sources. These include 49 WR stars, 43 of them previously unidentified, including the most distant known Galactic WR stars, more than doubling the number on the far side of the Milky Way. We also demonstrate our survey's ability to detect very faint planetary nebulae and other NIR emission objects.</description><source format="bibcode">2015MNRAS.452.2858K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/452/2858</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/AJ/143/149">J/AJ/143/149 : NIR spectroscopy of Galactic Wolf-Rayet stars. 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NOMAD B magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vmag</name><description>? NOMAD V magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rmag</name><description>? NOMAD R magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_Jmag</name><description>Limit flag on Jmag</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Jmag</name><description>? 2MASS J magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_Jmag</name><description>[:*+] Uncertainty flag on Jmag (1)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_Hmag</name><description>Limit flag on Hmag</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Hmag</name><description>? 2MASS H magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_Hmag</name><description>[:*+] Uncertainty flag on Hmag (1)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_Ksmag</name><description>Limit flag on Ksmag</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Ksmag</name><description>? 2MASS Ks magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_Ksmag</name><description>[:*+] Uncertainty flag on Ksmag (1)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_W1mag</name><description>Limit flag on W1mag</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>W1mag</name><description>? 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II/246)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/MNRAS/452/2858/table6</name><description>Extinction and distances for confirmed WR stars</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>Name (Field-Object) (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>SpType</name><description>Wolf-Rayet spectral subtype (1)</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Jmag</name><description>? 2MASS J magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Hmag</name><description>? 2MASS H magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ksmag</name><description>? 2MASS Ks magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AKs.J</name><description>? Ks-band extinction from 2MASS J-Ks colour</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AKs.H</name><description>? Ks-band extinction from 2MASS H-Ks colour</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AKs</name><description>? Ks-band extinction from J-Ks colour</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>KsMAG</name><description>? Absolute Ks magnitude (2)</description><unit>mag</unit><ucd>phys.magAbs;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DM</name><description>? Distance modulus</description><unit>mag</unit><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist</name><description>? Heliocentric distance (3)</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RG</name><description>? Galactocentric radius (3)</description><unit>kpc</unit><ucd>pos.distance;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/452/2858/table7</name><description>*Lines in the NIR WR spectrum</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>lambda</name><description>Wavelength</description><unit>um</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Trans</name><description>Transition</description><ucd>meta.id;phys.atmol.transition</ucd></column></table><table><name>J/MNRAS/452/2858/table8</name><description>*Measured equivalent widths for confirmed WN stars between 2.037 and 2.115um</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>Name (Field-Object) (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>SpType</name><description>Wolf-Rayet spectral subtype</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>lcHeII</name><description>? Line center from the Gaussian fit for HeII 2.037um line</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHeII</name><description>? Equivalent width for HeII 2.037um line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMHeII</name><description>? FWHM for HeII 2.037um line</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lcHeI</name><description>? Line center from the Gaussian fit for HeI 2.059um line</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHeI</name><description>? Equivalent width for HeI 2.059um line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMHeI</name><description>? FWHM for HeII 2.037um line</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lcHeIIb</name><description>? Line center from the Gaussian fit for HeII 2.097um + NV 2.100um + CIII 2.104um + NIII 2.104um lines</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHeIIb</name><description>? Equivalent width for HeII 2.097um + NV 2.100um + CIII 2.104um + NIII 2.104um lines</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMHeIIb</name><description>? FWHM for HeII 2.097um + NV 2.100um + CIII 2.104um + NIII 2.104um lines</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lcCIII</name><description>? Line center from the Gaussian fit for CIII 2.108um + HeI 2.113um + CIII 2.115um + NIII 2.115um lines</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWCIII</name><description>? Equivalent width for CIII 2.108um or HeI 2.113um + CIII 2.115um or NIII 2.115um lines</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMCIII</name><description>? FWHM for CIII 2.108um + HeI 2.113um + CIII 2.115um + NIII 2.115um lines</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/452/2858/table9</name><description>*Measured equivalent widths for confirmed WN stars between 2.148 and 2.217um</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>Name (Field-Object) (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>SpType</name><description>Wolf-Rayet spectral subtype</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>lcHeII</name><description>? Line center from the Gaussian fit for HeII 2.148um line</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHeII</name><description>? Equivalent width for HeII 2.148um line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMHeII</name><description>? FWHM for HeII 2.148um line</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lcHeI</name><description>? Line center from the Gaussian fit for HeI 2.162um + HeII 2.165um + HI 2.166um lines</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHeI</name><description>? Equivalent width for HeI 2.162um + HeII 2.165um + HI 2.166um lines</description><unit>0.1nm</unit><ucd>spect.line.eqWidth;em.line.HI</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMHeI</name><description>? FWHM for HeI 2.162um + HeII 2.165um + HI 2.166um lines</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lcHeIIb</name><description>? Line center from the Gaussian fit for HeII 2.189um line</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHeIIb</name><description>? Equivalent width for HeII 2.189um line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMHeIIb</name><description>? FWHM for HeII 2.189um line</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lcHeIIc</name><description>? Line center from the Gaussian fit for HeII 2.217um line</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHeIIc</name><description>? Equivalent width for HeII 2.217um line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMHeIIc</name><description>? FWHM for HeII 2.217um line</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/452/2858/table10</name><description>*Measured equivalent widths for confirmed WC stars between 2.037 and 2.115um</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>Name (Field-Object) (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>n_Name</name><description>[abc] Note on Name (G2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>SpType</name><description>Wolf-Rayet spectral subtype</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>lcHeII</name><description>? Line center from the Gaussian fit for HeII 2.037um line</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHeII</name><description>? Equivalent width for HeII 2.037um line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMHeII</name><description>? FWHM for HeII 2.037um line</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lcHeI</name><description>? Line center from the Gaussian fit for HeI 2.059um line</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHeI</name><description>? Equivalent width for HeI 2.059um line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMHeI</name><description>? FWHM for HeII 2.037um line</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lcCIV</name><description>? Line center from the Gaussian fit for CIV 2.071um + 2.080um + 2.048um lines</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWCIV</name><description>? Equivalent width for CIV 2.071um + 2.080um + 2.048um lines</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMCIV</name><description>? FWHM for CIV 2.071um + 2.080um + 2.048um lines</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lcCIII</name><description>? Line center from the Gaussian fit for CIII 2.104um + 2.115um lines</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWCIII</name><description>? Equivalent width for CIII 2.104um + 2.115um lines</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMCIII</name><description>? FWHM for CIII 2.104um + 2.115um lines</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/452/2858/table11</name><description>*Measured equivalent widths for confirmed WC stars between 2.139 and 2.217um</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>Name (Field-Object) (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>n_Name</name><description>[abc] Note on Name (G2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>SpType</name><description>Wolf-Rayet spectral subtype</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>lcCIV</name><description>? Line center from the Gaussian fit for CIV 2.139um line</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWCIV</name><description>? Equivalent width for CIV 2.139um line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMCIV</name><description>? FWHM for CIV 2.139um line</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lcHeI</name><description>? Line center from the Gaussian fit for HeI 2.1.62um + HeII 2.165um lines</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHeI</name><description>? Equivalent width for HeI 1.62um + HeII 2.165um lines</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMHeI</name><description>? FWHM for HeI 1.62um + HeII 2.165um lines</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lcHeIIa</name><description>? Line center from the Gaussian fit for HeII 2.189um line</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHeIIa</name><description>? Equivalent width for HeII 2.189um line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMHeIIa</name><description>? FWHM for HeII 2.189um line</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lcHeIIb</name><description>? Line center from the Gaussian fit for HeII 2.217um line</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHeIIb</name><description>? Equivalent width for HeII 2.217um line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FWHMHeIIb</name><description>? FWHM for HeII 2.217um line</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>