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<ri:Resource created="2007-04-24T10:57:35Z" 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>Dwarf effective temperatures</title><shortName>J/A+AS/117/227</shortName><identifier>ivo://CDS.VizieR/J/A+AS/117/227</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Alonso A.</name></creator><creator><name>Arribas S.</name></creator><creator><name>Martinez-Roger C.</name></creator><date role="Updated">2017-12-18T07:57:07Z</date><date role="Created">2007-04-24T10:57:35Z</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>subdwarf-stars</subject><subject>effective-temperature</subject><subject>infrared-photometry</subject><description>We have applied the InfraRed Flux Method (IRFM) to a sample of 475 dwarfs and subdwarfs in order to derive their effective temperatures with a mean accuracy of about 1.5%. We have used the new homogeneous grid of theoretical model atmosphere flux distributions developed by Kurucz (1991, 1993) for the application of the IRFM. The atmospheric parameters of the stars cover, roughly, the ranges: 3500K&lt;=T_eff_&lt;=8000K; -3.5&lt;=[Fe/H]&lt;=+0.5; 3.5&lt;=log(g)&lt;=5. The monochromatic infrared fluxes at the continuum, and the bolometric fluxes are derived using recent results, which satisfy the accuracy requirements of the work.</description><source format="bibcode">1996A&amp;AS..117..227A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/117/227</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/A+AS/107/365">J/A+AS/107/365 : Dwarfs and subdwarfs IR photometry (Alonso+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/131/209">J/A+AS/131/209 : Giants JHK(L') photometry (Alonso+ 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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>ID</name><description>Identification (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>n_ID</name><description>Individual note on ID (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logg</name><description>Surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>Metallicity</description><unit>log(Sun)</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FBol</name><description>Bolometric flux (10^-2^erg/cm2/s)</description><unit>1e-05W.m**-2</unit><ucd>phot.flux.bol</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>E(B-V)</name><description>Interestellar redenning</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FJ</name><description>? Monochromatic flux in the band J</description><unit>mW.m**-2</unit><ucd>phot.flux.density;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>qJ</name><description>? q-factor in the band J (7)</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_TJ</name><description>limit flag on TJ</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>TJ</name><description>? Effective temperature derived in the band J</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_TJ</name><description>? rms uncertainty on TJ (4)</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>FH</name><description>? Monochromatic flux in the band H (6)</description><unit>dW.m**-2.nm**-1</unit><ucd>phot.flux.density;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>qH</name><description>? q-factor in the band H (7)</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_TH</name><description>Limit flag on TH</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>TH</name><description>? Effective temperature derived in the band H</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>n_TH</name><description>[]] Note on TH (3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>e_TH</name><description>? rms uncertainty on TH (4)</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>FK</name><description>? Monochromatic flux in the band K (6)</description><unit>dW.m**-2.nm**-1</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>qK</name><description>? q-factor in the band K (7)</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>TK</name><description>? Effective temperature derived in the band K</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_TK</name><description>? rms uncertainty on TK (4)</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Tmean</name><description>? 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