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<ri:Resource created="2023-09-15T07:16:05Z" 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>Cataclysmic variables in the Gaia era</title><shortName>J/AJ/165/163</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/163</identifier><altIdentifier>doi:10.26093/cds/vizier.51650163</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Canbay R.</name></creator><creator><name>Bilir S.</name></creator><creator><name>Ozdonmez A.</name></creator><creator><name>Ak T.</name></creator><date role="Updated">2025-02-06T20:08:44Z</date><date role="Created">2023-09-15T07:16:05Z</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>variable-stars</subject><subject>proper-motions</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><description>The spatial distribution, Galactic model parameters, and luminosity function of cataclysmic variables (CVs) are established using reestimated trigonometric parallaxes from Gaia DR3. The data sample of 1587 CVs in this study is claimed to be suitable for Galactic model parameter estimation as the distances are based on trigonometric parallaxes, and the Gaia DR3 photometric completeness limits were taken into account when the sample was created. According to the analysis, the scale height of all CVs increases from 248{+/-}2 to 430{+/-}4pc toward shorter periods near the lower limit of the period gap and suddenly drops to 300{+/-}2pc for the shortest orbital period CVs. The exponential scale heights of all CVs and the magnetic systems are found to be 375{+/-}2 and 281{+/-}3pc, respectively, considerably larger than those suggested in previous observational studies. The local spatial density of all CVs and the magnetic systems in the sample are 6.8_-1.1_^+1.3^x10^-6^ and 2.1_-0.4_^+0.5^x10^-6^/pc^3^, respectively. Our measurements strengthen the 1-2 order of magnitude discrepancy between the CV spatial densities predicted by population synthesis models and observations. It is likely that this discrepancy is due to objects undetected by CV surveys, such as systems with very low M{sun} and ones in the period gap. A comparison of the luminosity function of white dwarfs with the luminosity function of all CVs in this study show that 500 times the luminosity function of CVs fits very well to the luminosity function of white dwarfs. We conclude that the estimations and data sample in this study can be confidently used for further analyses of CVs.</description><source format="bibcode">2023AJ....165..163C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/163</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/cb">B/cb : Cataclysmic Binaries, LMXBs, and related objects (Ritter+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/gcvs">B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/110">V/110 : Catalog of Cataclysmic Variables (Downes+ 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/113">V/113 : Cataclysmic Binaries, LMXBs, and related objects (Ritter+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/123">V/123 : Catalog of Cataclysmic Variables (Downes+ 2001-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/312/93">J/A+A/312/93 : Cataclysmic variable systemic-velocity (van Paradijs+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/355/307">J/MNRAS/355/307 : SA114 Ug'r'i'Z photometry (Karaali+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/453/635">J/A+A/453/635 : Modelling Galactic Interstellar Extinction (Marshall+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/463/1053">J/A+A/463/1053 : Differential photometry of WX Cet (Sterken+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/185">J/AJ/134/185 : Cataclysmic variables from SDSS-DR5 (Szkody+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/NewA/13.133">J/other/NewA/13.133 : 2MASS photometry of cataclysmic variables (Ak+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/175/191">J/ApJS/175/191 : Variables from 2MASS calibration fields (Plavchan+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/122/1285">J/PASP/122/1285 : Radial-velocities 20 cataclysmic var. 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xsi:type="vs:VOTableType">int</dataType></column><column><name>Ref</name><description>[1/82]? References</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>Sequential identifier used in this work</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Star Name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="39*">char</dataType></column><column><name>RAJ2000</name><description>[0/23] Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Group</name><description>Object Group; magnetic (mCV) or non-magnetic (non-mCVs)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>Porb</name><description>[0.002/5.8]? Orbital Period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Gmag</name><description>[8.01/18.6] Gaia DR3 G-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Gmag</name><description>[-0.02/0.2] Uncertainty in Gmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>plx</name><description>[0.1/45.7] trigonometric parallax, Gaia DR3</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_plx</name><description>[0.01/0.8] Uncertainty in plx</description><unit>mas</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/165/163/refs</name><description>References used</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ref</name><description>[1/82] Reference number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Author</name><description>Main author</description><ucd>meta.bib.author</ucd><dataType xsi:type="vs:VOTableType" arraysize="30*">char</dataType></column><column><name>BIB</name><description>BIBcode</description><ucd>meta.bib.bibcode</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Cat.</name><description>Catalog in Vizier</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column></table></schema></tableset></ri:Resource>