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<ri:Resource created="2020-03-19T14:25:56Z" 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>The BAaDE SiO maser survey at 86GHz with ALMA</title><shortName>J/ApJS/244/25</shortName><identifier>ivo://CDS.VizieR/J/ApJS/244/25</identifier><altIdentifier>doi:10.26093/cds/vizier.22440025</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Stroh M.C.</name></creator><creator><name>Pihlstrom Y.M.</name></creator><creator><name>Sjouwerman L.O.</name></creator><creator><name>Lewis M.O.</name></creator><creator><name>Claussen M.J.,Morris M.R.</name></creator><creator><name>Rich R.M.</name></creator><date role="Updated">2022-08-09T14:16:18Z</date><date role="Created">2020-03-19T14:25:56Z</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>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>astrophysical-masers</subject><subject>radio-astronomy</subject><subject>surveys</subject><subject>infrared-sources</subject><description>We report on the first 1432 sources observed using the Atacama Large Millimeter/submillimeter Array, from the Bulge Asymmetries and Dynamical Evolution survey, which aims to obtain tens of thousands of line-of-sight velocities from SiO masers in Asymptotic Giant Branch (AGB) stars in the Milky Way. A 71% detection rate of 86GHz SiO masers is obtained from the infrared color-selected sample and increases to 80% when considering the likely oxygen-rich stars using Midcourse Space Experiment colors isolated in a region where [D]-[E]&lt;=1.38. Based on Galactic distributions, the presence of extended CS emission, and likely kinematic associations, the population of sources with [D]-[E]&gt;1.38 probably consists of young stellar objects, or alternatively, of planetary nebulae. For the SiO detections, we examined whether individual SiO transitions provide comparable stellar line-of-sight velocities and found that any SiO transition is suitable for determining a stellar AGB line-of-sight velocity. Finally, we discuss the relative SiO detection rates and line strengths in the context of current pumping models.</description><source format="bibcode">2019ApJS..244...25S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/244/25</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+, 2006-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/114">V/114 : MSX6C Infrared Point Source Catalog (Egan+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/93/663">J/AJ/93/663 : Carbon stars from IRAS-LRS spectra (Little-Marenin+, 1987)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/90/327">J/A+AS/90/327 : 1612MHz OH survey of IRAS sources (te Lintel Hekkert+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/115/81">J/A+AS/115/81 : A CS(2-1) survey of UC HII regions (Bronfman+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/112/557">J/ApJS/112/557 : Classification of IRAS Sources (Kwok+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/122/79">J/A+AS/122/79 : Galactic Bulge Region OH 1612MHz survey I. 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Line-peak brightness of SiO v=1</description><unit>Jy</unit><ucd>phot.flux.density;em.mm.50-100GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_S-SiO-v1</name><description>[0.008/0.03]? 1-sigma uncertainty in S-SiO-v1</description><unit>Jy</unit><ucd>stat.error;phot.color</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SSiOv1l</name><description>[0.04/0.2]? 5-sigma upper limit on S-SiO-v1 if not detected</description><unit>Jy</unit><ucd>phot.flux.density;em.mm.50-100GHz;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>S-SiO-v2</name><description>[0.06/3.8]? 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Line-peak velocity (LSRK) of CS line</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SiO-avg-vel</name><description>[-266/181]? Average velocity of SiO lines (1)</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>C-avg-vel</name><description>[-106/2]? Average velocity of carbon lines (1)</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>