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<ri:Resource created="2023-09-13T15:32:19Z" 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>S-type stars from LAMOST MRS DR9 with Gaia DR2 data</title><shortName>J/ApJ/931/133</shortName><identifier>ivo://CDS.VizieR/J/ApJ/931/133</identifier><altIdentifier>doi:10.26093/cds/vizier.19310133</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chen J.</name></creator><creator><name>Luo A.-L.</name></creator><creator><name>Li Y.-B.</name></creator><creator><name>Chen X.-L.</name></creator><creator><name>Wang R.</name></creator><creator><name>Li S.</name></creator><creator><name>Du B.</name></creator><creator><name>Ma X.-X.</name></creator><date role="Updated">2024-09-09T20:16:54Z</date><date role="Created">2023-09-13T15:32:19Z</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>s-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>surveys</subject><subject>infrared-photometry</subject><subject>chemical-abundances</subject><subject>two-color-diagrams</subject><subject>trigonometric-parallax</subject><subject>absolute-magnitude</subject><description>In this paper, we report on 606 S-type stars identified from Data Release 9 of the LAMOST medium-resolution spectroscopic (MRS) survey; 539 of them are reported for the first time. The discovery of these stars is a three-step process, i.e., selecting with ZrO-band indices greater than 0.25, excluding non-S-type stars with the iterative Support Vector Machine method, and finally retaining stars with absolute bolometric magnitude larger than -7.1. The 606 stars are consistent with the distribution of known S-type stars in the color- magnitude diagram. We estimated the C/Os using the [C/Fe] and [O/Fe] provided by APOGEE and the MARCS model for S-type stars, respectively, and the results of the two methods show that the C/Os of all stars are larger than 0.5. Both the locations on the color-magnitude diagram and C/Os further verify the nature of our S-type sample. Investigating the effect of TiO and atmospheric parameters on ZrO with the sample, we found that log g has a more significant impact on ZrO than Teff and [Fe/H], and both TiO and logg may negatively correlate with ZrO. According to the criterion of Tian+ (2020, J/ApJS/249/22), a total of 238 binary candidates were found by the zero-point-calibrated radial velocities from the officially released catalog of LAMOST MRS and the catalog of Zhang+ 2021, J/ApJS/256/14.</description><source format="bibcode">2022ApJ...931..133C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/931/133</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/156">V/156 : LAMOST DR7 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/400/1413">J/MNRAS/400/1413 : Near-IR spectra of extremely red AGB stars (Wright+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/103">J/AJ/142/103 : Cool evolved stars in SAGE-SMC and SAGE-LMC (Boyer+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/727/53">J/ApJ/727/53 : Red supergiant stars in the LMC. 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(Yang+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/831/20">J/ApJ/831/20 : C/O and Mg/Si for solar neighborhood's stars (Brewer+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/601/A10">J/A+A/601/A10 : MARCS model atmospheres for S stars (Van Eck+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/90">J/AJ/156/90 : APOGEE radial velocity standard stars (Huang+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/858/L7">J/ApJ/858/L7 : Red clump stars selected from LAMOST &amp; APOGEE (Ting+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/475/3633">J/MNRAS/475/3633 : Mass and age of red giant branch stars (Wu+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/158/22">J/AJ/158/22 : IR study of intrinsic &amp; extrinsic S-type stars (Chen+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/629/A91">J/A+A/629/A91 : A source catalog for the SMC (Yang+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/249/22">J/ApJS/249/22 : Radial velocity variable stars from LAMOST DR4 (Tian+, 2020)</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/ApJS/256/43">J/ApJS/256/43 : O-rich and C-rich AGB stars in our Galaxy (Suh, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/267/5">J/ApJS/267/5 : S-type stars from LAMOST MRS DR10 spectra (Chen+, 2023)</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/931/133</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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