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<ri:Resource created="2017-07-07T12:27:34Z" 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>WISE reduced proper motions and spectral types</title><shortName>J/ApJ/787/126</shortName><identifier>ivo://CDS.VizieR/J/ApJ/787/126</identifier><altIdentifier>doi:10.26093/cds/vizier.17870126</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Luhman K.L.</name></creator><creator><name>Sheppard S.S.</name></creator><date role="Updated">2017-10-04T07:40:24Z</date><date role="Created">2017-07-07T12:27:34Z</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>dwarf-stars</subject><subject>infrared-photometry</subject><subject>proper-motions</subject><subject>stellar-spectral-types</subject><description>We present an analysis of high proper motion objects that we have found in a recent study and in this work with multi-epoch astrometry from the Wide-field Infrared Survey Explorer (WISE). Using photometry and proper motions from the Two Micron All-Sky Survey and WISE, we have identified the members of this sample that are likely to be late-type, nearby, or metal-poor. We have performed optical and near-infrared spectroscopy on 41 objects, from which we measure spectral types that range from M4-T2.5. This sample includes 11 blue L dwarfs and 5 subdwarfs; the latter were also classified as such in the recent study by Kirkpatrick and coworkers. Based on their spectral types and photometry, several of our spectroscopic targets may have distances of &lt;20 pc with the closest at ~12 pc. The tangential velocities implied by the spectrophotometric distances and proper motions indicate that four of the five subdwarfs are probably members of the Galactic halo while several other objects, including the early-T dwarf WISE J210529.08-623558.7, may belong to the thick disk.</description><source format="bibcode">2014ApJ...787..126L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/787/126</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/123/3409">J/AJ/123/3409 : SDSS M, L, and T dwarfs (Hawley+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/3553">J/AJ/127/3553 : JHK photometry and spectroscopy for L and T dwarfs</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/148">J/AJ/144/148 : Infrared photometry of brown dwarf and Hyper-LIRG</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/781/4">J/ApJ/781/4 : Photometry of high proper motion objects from WISE</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/783/122">J/ApJ/783/122 : AllWISE motion survey (Kirkpatrick+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/454/4054">J/MNRAS/454/4054 : High proper motion sources from WISE (Beamin+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/817/112">J/ApJ/817/112 : 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