<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2000-06-29T23:02:27Z" 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>Young low-mass stars and brown dwarfs in IC 348</title><shortName>J/ApJ/525/466</shortName><identifier>ivo://CDS.VizieR/J/ApJ/525/466</identifier><altIdentifier>doi:10.26093/cds/vizier.15250466</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Luhman K.L.</name></creator><date role="Updated">2000-06-29T23:02:53Z</date><date role="Created">2000-06-29T23:02:27Z</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>infrared-photometry</subject><subject>spectroscopy</subject><subject>late-type-stars</subject><subject>open-star-clusters</subject><description>I present new results from a continuing program to identify and characterize the low-mass stellar and substellar populations in the young cluster IC 348 (0.5 - 10 Myr). Optical spectroscopy has revealed young objects with spectral types as late as M8.25. The intrinsic J-H and H-K colors of these sources are dwarflike, whereas the R-I and I-J colors appear intermediate between the colors of dwarfs and giants. Furthermore, the spectra from 6500 to 9500 {AA} are reproduced well with averages of standard dwarf and giant spectra, suggesting that such averages should be used in the classification of young late-type sources.</description><source format="bibcode">1999ApJ...525..466L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/525/466</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></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/525/466</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/525/466</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/525/466</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/525/466</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/525/466</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/525/466</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/525/466/table1 (Data for low-mass sources in IC 348)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/525/466/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/525/466/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/525/466/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>56.1752083</ra><dec>32.1495556</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/1539</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/525/466?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/525/466/table1</name><description>Data for low-mass sources in IC 348</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>Identification number of IC 348 source</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>f_ID</name><description>[g] Indicates IR photometry includes a companion while the optical data resolve the two sources.</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description></column><column><name>DEJ2000</name><description>Declination (J2000)</description></column><column><name>SpIR</name><description>Spectral type from IR measurements</description><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>SpOpt</name><description>Spectral type from optical measurements</description><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>EqW</name><description>? Equivalent width of H{alpha}</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_EqW</name><description>? Error in EqW</description><unit>nm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_EqW</name><description>[?] Indicates an uncertain EqW measurement</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>r_SpType</name><description>Reference for SpType</description><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>SpType</name><description>Adopted spectral type</description><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Teff</name><description>Effective temperature (1)</description><unit>K</unit><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Extinc</name><description>Extinction in the J band</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Lbol</name><description>Bolometric luminosity</description><unit>solLum</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>(R-I)H</name><description>? (R-I) color from Herbig (1998ApJ...497..736H)</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ImagH</name><description>? I band magnitude from Herbig 1998</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_R-I</name><description>Limit value for R-I</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>R-I</name><description>? (R-I) color from this work</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Imag</name><description>? I band magnitude from this work</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>(J-H)LL</name><description>? (J-H) color from Lada &amp; Lada (1995AJ....109.1682L)</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>(H-K)LL</name><description>? (H-k) color from Lada &amp; Lada 1995</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>KmagLL</name><description>? K band color from Lada &amp; Lada 1995</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>(J-H)L</name><description>? (J-H) color from Luhman et al (1998ApJ...508..347L)</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>(H-K)L</name><description>? (H-k) color from Luhman et al 1998</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>KmagL</name><description>? K band color from Luhman et al 1998</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>