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<ri:Resource created="2014-12-17T13:05:25Z" 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>High proper-motion white dwarfs</title><shortName>J/MNRAS/425/1394</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/425/1394</identifier><altIdentifier>doi:10.26093/cds/vizier.74251394</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kawka A.</name></creator><creator><name>Vennes S.</name></creator><date role="Updated">2024-07-18T20:19:03Z</date><date role="Created">2014-12-17T13:05:25Z</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>white-dwarf-stars</subject><subject>proper-motions</subject><subject>photometry</subject><description>We conducted a spectropolarimetric survey of 58 high proper-motion white dwarfs which achieved uncertainties of &gt;~2kG in the H{alpha} line and &gt;~5kG in the upper Balmer line series. The survey aimed at detecting low magnetic fields (&lt;~100kG) and helped identify the new magnetic white dwarfs NLTT2219, with a longitudinal field B_l_=-97kG, and NLTT10480 (B_l_=-212kG). Furthermore, we report the possible identification of a very low-field white dwarf with B_l_=-4.6kG. The observations show that ~~5 per cent of white dwarfs harbour low fields (~10 to ~10^2^kG) and that increased survey sensitivity may help uncover several new magnetic white dwarfs with fields below ~1kG. A series of observations of the high-field white dwarf NLTT12758 revealed changes in polarity occurring within an hour possibly associated with an inclined, fast rotating dipole. Also, the relative strength of the {pi} and {sigma} components in NLTT12758 possibly revealed the effect of a field concentration ('spot'), or, most likely, the presence of a non-magnetic white dwarf companion. Similar observations of NLTT13015 also showed possible polarity variations, but without a clear indication of the time-scale. The survey data also proved useful in constraining the chemical composition, age and kinematics of a sample of cool white dwarfs as well as in constraining the incidence of double degenerates.</description><source format="bibcode">2012MNRAS.425.1394K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/425/1394</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/ApJS/133/413">J/ApJS/133/413 : BVRIJHK photometry of cool white dwarfs (Bergeron+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1825">J/AJ/128/1825 : Photometry 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