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<ri:Resource created="2021-01-18T13:36:35Z" 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>Effective temperatures of low-mass stars</title><shortName>J/ApJ/879/105</shortName><identifier>ivo://CDS.VizieR/J/ApJ/879/105</identifier><altIdentifier>doi:10.26093/cds/vizier.18790105</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lopez-Valdivia R.</name></creator><creator><name>Mace G.N.</name></creator><creator><name>Sokal K.R.</name></creator><creator><name>Hussaini M.</name></creator><creator><name>Kidder B.T.,Mann A.W.</name></creator><creator><name>Gosnell N.M.</name></creator><creator><name>Oh H.</name></creator><creator><name>Kesseli A.Y.</name></creator><creator><name>Muirhead P.S.,Johns-Krull C.M.</name></creator><creator><name>Jaffe D.T.</name></creator><date role="Updated">2021-06-18T13:48:34Z</date><date role="Created">2021-01-18T13:36:35Z</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>effective-temperature</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>k-stars</subject><description>High-resolution, near-infrared spectra will be the primary tool for finding and characterizing Earth-like planets around low-mass stars. Yet, the properties of exoplanets cannot be precisely determined without accurate and precise measurements of the host star. Spectra obtained with the Immersion Grating Infrared Spectrometer simultaneously provide diagnostics for most stellar parameters, but the first step in any analysis is the determination of the effective temperature. Here we report the calibration of high-resolution H-band spectra to accurately determine the effective temperature for stars between 4000 and 3000K (~K8-M5) using absorption line-depths of FeI, OH, and Al I. The field star sample used here contains 254 K and M stars with temperatures derived using BT-Settl synthetic spectra. We use 106 stars with precise temperatures in the literature to calibrate our method, with typical errors of about 140K, and systematic uncertainties less than ~120K. For the broadest applicability, we present Teff-line-depth-ratio relationships, which we test on 12 members of the TW Hydrae Association and at spectral resolving powers between ~10000 and 120000. These ratios offer a simple but accurate measure of effective temperatures in cool stars that are distance and reddening independent.</description><source format="bibcode">2019ApJ...879..105L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/879/105</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/VI/39">VI/39 : Model Atmospheres (Kurucz, 1979)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/119">III/119 : Spectral classifications of proper motion stars (Bidelman+ 1985)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/123">III/123 : Dwarf K and M stars of small proper motion (Stephenson 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/150">III/150 : Perkins Revised MK Types for the Cooler Stars (Keenan+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/182">III/182 : HDE Charts: positions, proper motions (Nesterov+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/266">III/266 : Revised First Byurakan Survey of late-type stars (Gigoyan+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/336">II/336 : AAVSO Photometric All Sky Survey (APASS) DR9 (Henden+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/390/491">J/A+A/390/491 : DENIS new nearby stars (Reyle+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/2048">J/AJ/126/2048 : NStars project: the Northern Sample. 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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>SpT</name><description>Spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>r_SpT</name><description>[1/50] Simbad reference for SpT (see refs.dat file)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>rmag</name><description>[6.6/16.3]? APASS r band 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>T(r-J)</name><description>[2801/4594]? The (r-J) color temperature</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>vsini</name><description>[7/53]? 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Line-depth of peak</description><ucd>phot.flux.density;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_LD(peak)</name><description>[0.001/0.02]? Error in LD(peak)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>LD(Al)</name><description>[0.051/0.46]? Line-depth of Al</description><ucd>phot.flux.density;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_LD(Al)</name><description>[0.001/0.02]? 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