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<ri:Resource created="2026-06-08T12:19:17Z" status="active" updated="2026-06-15T00:00:00Z" 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>SMASTES. II. KVN obs. SiO masers from S-type AGB stars</title><shortName>J/AJ/170/266</shortName><identifier>ivo://CDS.VizieR/J/AJ/170/266</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Son S.-M.</name></creator><creator><name>Cho S.-H.</name></creator><creator><name>Kim J.</name></creator><creator><name>Baek H.</name></creator><creator><name>Yoon D.-H.</name></creator><creator><name>Suh K.-W.</name></creator><date role="Updated">2026-06-08T11:26:41Z</date><date role="Created">2026-06-08T12:19:17Z</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>astrophysical-masers</subject><subject>radio-astronomy</subject><subject>interstellar-masers</subject><subject>late-type-stars</subject><subject>giant-stars</subject><subject>very-long-baseline-interferometry</subject><subject>radio-sources</subject><subject>interferometry</subject><subject>morgan-keenan-classification</subject><subject>radial-velocity</subject><subject>molecular-physics</subject><subject>co-line-emission</subject><description>We present the observational results of Simultaneous Multi-mAser Survey Toward Evolved Stars (SMASTES) II for 150 S-type asymptotic giant branch stars. Observations have been performed from 2023 September to 2024 March using the upgraded wide four-band (22/43/86/129GHz) receiving system of the Korean VLBI Network. For simultaneous observations, 19 molecular lines of H_2_O and multitransitions of SiO masers including several thermal lines were set up together. H_2_O maser was not detected from any stars among 150 S-type stars. For SiO v=1: J=1-0, J=2-1, and J=3-2 masers were detected from nine, thirteen, and six stars, respectively. For SiO v=2: J=1-0, J=2-1, and J=3-2 masers were detected from five, two, and two stars, respectively. In particular, for v=1: J=1-0, J=2-1, and J=3-2 masers were all detected from five stars. For SiO v=0: J=1-0, J=2-1, and J=3-2 lines in ground vibrational state were detected from five, six, and seven stars, respectively, including the 29SiO v=0: J=1-0 and J=2-1 lines. For SiO v=0: J=1-0, J=2-1, and J=3-2 lines were detected in more stars at higher rotational transition lines. The carbon-bearing molecule HCN was detected from four stars. Based on these observational results, we perform statistical analyses on detection rates of maser and thermal lines, maser properties, and kinematics comparing with the results of M-type stars (SMASTES I). The characteristics of maser properties are investigated in the IRAS two-color diagram in relation to the evolutionary stage.</description><source format="bibcode">2025AJ....170..266S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/170/266</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/J/A+AS/129/363">J/A+AS/129/363 : IRAS flux densities of S stars (Jorissen+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/129">J/AJ/144/129 : Properties of 83 known stellar SiO maser sources (Cho+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/601/A10">J/A+A/601/A10 : A grid of MARCS model atmospheres for S stars (Van Eck+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/617/A132">J/A+A/617/A132 : Abundances and distributions of CS and SiS (Danilovich+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/158/22">J/AJ/158/22 : New IR study of intrinsic &amp; extrinsic S-type stars (Chen+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/642/A20">J/A+A/642/A20 : W Aql APEX spectrum (De Beck+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/653/A53">J/A+A/653/A53 : DEATHSTAR. II. The S-type (Andriantsaralaza+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/931/133">J/ApJ/931/133 : S-type stars from LAMOST MRS DR9 with Gaia DR2 (Chen+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/660/A94">J/A+A/660/A94 : Observational properties of ATOMIUM project (Gottlieb+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/692/A86">J/A+A/692/A86 : Millimetre observations of chi Cygni (Hoai+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/681/A50">J/A+A/681/A50 : ATOMIUM. Molecular inventory (Wallstrom+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/170/84">J/AJ/170/84 : SMASTES.I. KVN obs. 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