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<ri:Resource created="2018-07-12T14:57:52Z" 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>Spectroscopic and photometric analysis of WDs</title><shortName>J/ApJ/848/11</shortName><identifier>ivo://CDS.VizieR/J/ApJ/848/11</identifier><altIdentifier>doi:10.26093/cds/vizier.18480011</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bedard A.</name></creator><creator><name>Bergeron P.</name></creator><creator><name>Fontaine G.</name></creator><date role="Updated">2018-09-26T14:38:21Z</date><date role="Created">2018-07-12T14:57:52Z</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>stellar-spectral-types</subject><subject>effective-temperature</subject><subject>stellar-radii</subject><subject>stellar-masses</subject><subject>stellar-distance</subject><description>We present a detailed spectroscopic and photometric analysis of 219 DA and DB white dwarfs for which trigonometric parallax measurements are available. Our aim is to compare the physical parameters derived from the spectroscopic and photometric techniques, and then to test the theoretical mass-radius relation for white dwarfs using these results. The agreement between spectroscopic and photometric parameters is found to be excellent, especially for effective temperatures, showing that our model atmospheres and fitting procedures provide an accurate, internally consistent analysis. The values of surface gravity and solid angle obtained, respectively, from spectroscopy and photometry, are combined with parallax measurements in various ways to study the validity of the mass-radius relation from an empirical point of view. After a thorough examination of our results, we find that 73% and 92% of the white dwarfs are consistent within 1{sigma} and 2{sigma} confidence levels, respectively, with the predictions of the mass-radius relation, thus providing strong support to the theory of stellar degeneracy. Our analysis also allows us to identify 15 stars that are better interpreted in terms of unresolved double degenerate binaries. Atmospheric parameters for both components in these binary systems are obtained using a novel approach. We further identify a few white dwarfs that are possibly composed of an iron core rather than a carbon/oxygen core, since they are consistent with Fe-core evolutionary models.</description><source format="bibcode">2017ApJ...848...11B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/848/11</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/B/wd">B/wd : Spectroscopically identified white dwarfs (McCook+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/32">J/AJ/154/32 : Solar neighborhood. XXXIX. 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ivo-id="ivo://CDS.VizieR/J/MNRAS/403/1949">J/MNRAS/403/1949 : UBV(RcIc)JHK photometry of HIP nearby stars (Koen+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/712/585">J/ApJ/712/585 : Apparent velocity measurements of DA WDs (Falcon+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/441">J/A+A/505/441 : UVES/VLT spectra of white dwarfs (Koester+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/1239">J/AJ/135/1239 : Spectral distances to DA white dwarfs (Holberg+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/470/1079">J/A+A/470/1079 : UVES/VLT spectroscopy of white dwarfs (Voss+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/663/1291">J/ApJ/663/1291 : DZ stars in SDSS DR4 (Dufour+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/657/1013">J/ApJ/657/1013 : IR photometry of 2MASS/Spitzer white dwarfs (Tremblay+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/252">J/AJ/134/252 : New nearby white dwarf systems (Subasavage+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/1221">J/AJ/132/1221 : VJHK and SDSS photometry of DA white dwarfs (Holberg+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/161/394">J/ApJS/161/394 : Low-luminosity companions to white dwarfs (Farihi+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/156/47">J/ApJS/156/47 : DA white dwarfs from the Palomar Green Survey (Liebert+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/631/1100">J/ApJ/631/1100 : Atmospheric parameters of DA white dwarfs (Gianninas+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/133/413">J/ApJS/133/413 : BVRIJHK photometry of cool white dwarfs (Bergeron+, 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