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<ri:Resource created="2025-02-26T08:58:24Z" status="active" updated="2025-10-13T20:09:28Z" 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>SDSS magnetic white dwarfs rich in hydrogen</title><shortName>J/ApJ/944/56</shortName><identifier>ivo://CDS.VizieR/J/ApJ/944/56</identifier><altIdentifier>doi:10.26093/cds/vizier.19440056</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Amorim L.L.</name></creator><creator><name>Kepler S.O.</name></creator><creator><name>Kulebi B.</name></creator><creator><name>Jordan S.</name></creator><creator><name>Romero A.D.</name></creator><date role="Updated">2025-10-13T20:09:28Z</date><date role="Created">2025-02-26T08:58:24Z</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>magnetic-fields</subject><subject>effective-temperature</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>White dwarfs are excellent research laboratories as they reach temperatures, pressures, and magnetic fields that are unattainable on Earth. To better understand how these three physical parameters interact with each other and with other stellar features, we determined the magnetic field strength for a total of 804 hydrogen-rich white dwarfs (WDs) of which 287 are not in the literature. We fitted the spectra observed with the Sloan Digital Sky Survey using atmospheric models that consider the Zeeman effect due to the magnetic field at each point in the stellar disk. Comparing magnetic and nonmagnetic WDs, the literature already shows that the magnetic ones have on average higher mass than the nonmagnetic. In addition to that, magnetic fields are more common in cooler WDs than in hotter WDs. In consonance, we found that those with higher magnetic field strengths tend to have higher masses, and lower temperatures, for which models indicate the crystallization process has already started. This reinforces the hypothesis that the field is being generated and/or amplified in the cooling process of the white dwarf. Our sample constitutes the largest number of white dwarfs with determined magnetic fields to date.</description><source format="bibcode">2023ApJ...944...56A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/944/56</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/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/306">II/306 : The SDSS Photometric Catalog, Release 8 (Adelman-McCarthy+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/139">V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/734">J/AJ/130/734 : Magnetic WDs from SDSS DR2 and DR3 (Vanlandingham+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/506/1341">J/A+A/506/1341 : Magnetic fields in white dwarfs (Kuelebi+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/429/2934">J/MNRAS/429/2934 : SDSS magnetic white dwarf stars (Kepler+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/480/1547">J/MNRAS/480/1547 : Full Evolutionary Sequences of Massive WDs (Lauffer+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/499/1890">J/MNRAS/499/1890 : Gaia white dwarfs within 40pc. II. (McCleery+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/508/3877">J/MNRAS/508/3877 : Catalogue of white dwarfs in Gaia EDR3 (Gentile+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/935/L12">J/ApJ/935/L12 : Magnetic field measurements of young WDs (Bagnulo+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/518/3055">J/MNRAS/518/3055 : Gaia white dwarfs within 40pc. III (O'Brien+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/682/A5">J/A+A/682/A5 : Gaia white dwarfs Classification (Vincent+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/690/A10">J/A+A/690/A10 : Magnetic fields in featureless WDs (Berdyugin+, 2024)</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/944/56</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/944/56</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/944/56</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/944/56</accessURL><mirrorURL 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