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<ri:Resource created="2020-04-09T07:42:31Z" 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>Spectroscopically identified CVs from LAMOST survey. I.</title><shortName>J/AJ/159/43</shortName><identifier>ivo://CDS.VizieR/J/AJ/159/43</identifier><altIdentifier>doi:10.26093/cds/vizier.51590043</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hou W.</name></creator><creator><name>Luo A.-L.</name></creator><creator><name>Li Y.-B.</name></creator><creator><name>Qin Li</name></creator><date role="Updated">2020-04-16T13:22:09Z</date><date role="Created">2020-04-09T07:42:31Z</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>novae</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>am-stars</subject><description>A sample of cataclysmic variables (CVs) is presented including spectroscopically identified 380 spectra of 245 objects, of which 58 CV candidates are new discoveries. The BaggingTopPush and the Random Forest algorithms are applied to the Fifth Data Release (DR5) of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) to retrieve CVs with strong emission lines and with broad absorption lines respectively. Based on spectroscopic classification, 134 dwarf novae, 41 nova-like variables, and 19 magnetic CVs are identified from the sample. In addition, 89 high-inclination systems and 33 CVs showing companion stars are recognized and discussed for their distinct spectral characteristics. Comparisons between CVs from LAMOST and from published catalogs are made in spatial and magnitude distribution, and the difference of their locus in the Gaia color-absolute magnitude diagram (CaMD) are also investigated. More interestingly, for two dwarf novae observed through LAMOST and SDSS in different epochs, their spectra both in quiescence phase and during outburst are exhibited.</description><source format="bibcode">2020AJ....159...43H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/159/43</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/vsx">B/vsx : AAVSO International Variable Star Index VSX (Watson+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/gcvs">B/gcvs : General Catalogue of Variable Stars (Samus+, 2017)</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/V/164">V/164 : LAMOST DR5 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/565/511">J/ApJ/565/511 : Cataclysmic variables in the 2MASS 2IDR (Hoard+, 2002)</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/AJ/142/181">J/AJ/142/181 : CVs from SDSS. VIII. The final year (Szkody+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/81">J/AJ/144/81 : Spectrosc. &amp; phot. of CV candidates (Thorstensen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/421/2414">J/MNRAS/421/2414 : Faint cataclysmic variables from SDSS (Woudt+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/443/3174">J/MNRAS/443/3174 : 72 faint CV candidates in CRTS (Breedt+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/441/1186">J/MNRAS/441/1186 : Cataclysmic variables from CRTS (Drake+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/65/313">J/AcA/65/313 : Thousand new dwarf novae from the OGLE Survey (Mroz+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/456/4441">J/MNRAS/456/4441 : Outburst catalogue cataclysmic variables (Coppejans+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/465/4968">J/MNRAS/465/4968 : Cataclysmic variables observations (Hardy+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/RAA/18.68">J/other/RAA/18.68 : Cataclysmic variables from LAMOST DR3 (Han+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/234/31">J/ApJS/234/31 : Carbon stars from LAMOST using machine learning (Li+, 2018)</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/AJ/159/43</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/159/43</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/159/43</mirrorURL></interface></capability><capability><interface 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>f_LAMOST</name><description>[*] Flag on LAMOST, indicate the newly discovered CV spectra (71 occurrences)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>LAMOST</name><description>LAMOST designation (JHHMMSS.ss+DDMMSS.s)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>OName</name><description>? Previous identifications of known CVs</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="29*">char</dataType></column><column><name>RAJ2000</name><description>[3/356] Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-8.6/58.1] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>MJD</name><description>[55859/57912] Local modified Julian Date of observation, (JD-2400000.5)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Type</name><description>Subtypes of CVs (1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>Type-lit</name><description>Literature subtypes of CVs</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>CN</name><description>[y/n] CIII/NIII emission line detection; y=yes (119 occurrences), n=no (261 occurrences)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>FeII</name><description>[y/n] Fe II emission line detection; y=yes (127 occurrences), n=no (253 occurrences)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Ha</name><description>[S/D] S=Single-peak (291 occurrences) or D=Double-peak (89 occurrences) H{alpha} line</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Hb/HeII</name><description>[-9999.0/9999.0] Ratio, H{beta}/HeII 4686A (2)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>HeII/Hb</name><description>[-9999.0/9999.0] Ratio, HeII 4686A/H{beta} (2)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>