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<ri:Resource created="2026-09-04T15:10:13Z" status="active" updated="2026-09-04T14:18:23Z" 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>Single-lined spectroscopic binaries from LAMOST DR11</title><shortName>J/ApJS/282/55</shortName><identifier>ivo://CDS.VizieR/J/ApJS/282/55</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ye T.</name></creator><creator><name>Chen Y.</name></creator><creator><name>Xia F.</name></creator><creator><name>Fu Y.</name></creator><date role="Updated">2026-09-04T14:18:23Z</date><date role="Created">2026-09-04T15:10:13Z</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>spectroscopic-binary-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>metallicity</subject><subject>orbits</subject><description>A typical single-lined spectroscopic binary (SB1) consists of two stars with almost the same age but markedly different masses and physical properties. SB1s are essential for obtaining the statistical properties of stars and constraining stellar evolutionary models, particularly when orbital parameters are well determined. In this study, we first carry out a data-cleaning step on a sample of LAMOST Medium-Resolution Spectroscopic Survey stars with a sufficient number of observations and perform an F2 test, obtaining 7775 radial velocity variables. After removing false positives and crossmatching with variable and double-lined spectroscopic binary (SB2) catalogs, we exclude known astrophysical variables and SB2s, leaving 6106 SB1 candidates. We estimate initial periods using the Heck-Manfroid-Mersch method combined with Monte Carlo simulations and then fit each source with both an orbital model and a trend model, selecting between them via the Snedecor F-test of nested models. For orbital models, we accept the least-{chi}2 solution if it satisfies F2&lt;3.1, s&gt;10, phase_gap_max&lt;0.3, {sigma}v/K&lt;0.25 and passes the Markov Chain Monte Carlo-based robustness tests. For trend cases, we discard zeroth-order fits and require F2&lt;3.1. In total, we obtain 623 accepted solutions, of which 337 SB1s are new relative to existing catalogs.</description><source format="bibcode">2026ApJS..282...55Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/282/55</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+, 2006-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/sb9">B/sb9 : SB9: 9th Catalog of Spectroscopic Binary Orbits (Pourbaix+ 2004-2014)</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/II/366">II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/357">I/357 : Gaia DR3 Part 3. Non-single stars (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/162">V/162 : LAMOST DR11 catalogs (Luo+, 2026)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/184">J/AJ/140/184 : RAVE double-lined spectroscopic binaries (Matijevic+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/1">J/ApJS/190/1 : A survey of stellar families (Raghavan+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/635/A155">J/A+A/635/A155 : Gaia-ESO Survey SB1 catalogue (Merle+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/638/A145">J/A+A/638/A145 : GALAH survey. FGK binary stars (Traven+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/162/184">J/AJ/162/184 : APOGEE: radial velocities of binaries (Kounkel+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/655/A4">J/A+A/655/A4 : MONOS II. SB1 Orbital review (Trigueros Paez+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/256/14">J/ApJS/256/14 : RVs from LAMOST MRS DR7 stellar spectra (Zhang+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/664/A159">J/A+A/664/A159 : Radial velocities of Galactic SB1s (Mahy+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/258/26">J/ApJS/258/26 : Spectroscopic binaries from LAMOST MRS. I. (Zhang+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/269/41">J/ApJS/269/41 : New SB1s with sp. orbits from LAMOST DR8 LRS (Chen+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/266/18">J/ApJS/266/18 : Double-line spectroscopic binaries from LAMOST (Zheng+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/692/A192">J/A+A/692/A192 : C, SB1, SB2 &amp; SB3 southern O stars rot. rate (Blex+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/527/521">J/MNRAS/527/521 : SB2s in LAMOST-MRS (Kovalev+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/278/46">J/ApJS/278/46 : Orbits of 665 SB2s in Lamost-MRS (Guo+, 2025)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/276/11">J/ApJS/276/11 : Spectroscopic binaries from LAMOST MRS DR9 (Li+, 2025)</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/ApJS/282/55</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/282/55</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/282/55</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/282/55</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/282/55</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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V0=a'-c({Delta}T_m_)^2^/12</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>dVdt</name><description>[-0.12/0.22]? {delta}V/{delta}t=b</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Span</name><description>[88.8/1950] Time span of the observation</description><unit>d</unit><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>d2Vdt2</name><description>[-0.0004/0.003]? {delta}^2^V/{delta}t^2^=2c</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>t0</name><description>? Reference time (TDB)</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>r_t0</name><description>? Reference epoch (J2021.0)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Delta-Tm</name><description>[2075.29/2075.3]? The total time span of the parent sample</description><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Chi2-orb</name><description>[4.42/173.4] Chi_{orbit}^2 calculated from Equation 10</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F2-orb</name><description>[-9.7/3.1] The statistic in Section 4.4</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s</name><description>[10/245]? The significance of the solution (Equation 11)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>GapMax</name><description>[0.07/0.3]? Maximum gap in phase</description><ucd>time.phase;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>sigV/K</name><description>[0.018/0.3]? The ratio between the mean RV uncertainty and the semi-amplitude</description><ucd>stat.fit.omc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>New</name><description>[0/1] Flag on new SB1s (1: 377 occurrences)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>[10.3/348] Right Ascension in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-6.4/56.8] Declination in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Teff</name><description>[4008/8096]? LAMOST LASP effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logg</name><description>[1.3/4.82]? LAMOST LASP surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]</name><description>[-2.5/0.52]? LAMOST LASP metallicity</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Nrv</name><description>[12/57] Number of radial velocity measurements</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Chi2</name><description>[32.89/28880] Model {chi}^2 value, equation 1</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F2</name><description>[3.1/93.4] The F2 statistic; equation 2</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>