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<ri:Resource created="2015-07-03T09:52:48Z" 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>DUSTiNGS. I. The Good Source Catalog</title><shortName>J/ApJS/216/10</shortName><identifier>ivo://CDS.VizieR/J/ApJS/216/10</identifier><altIdentifier>doi:10.26093/cds/vizier.22160010</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Boyer M.L.</name></creator><creator><name>McQuinn K.B.W.</name></creator><creator><name>Barmby P.</name></creator><creator><name>Bonanos A.Z.</name></creator><creator><name>Gehrz R.D.,Gordon K.D.</name></creator><creator><name>Groenewegen M.A.T.</name></creator><creator><name>Lagadec E.</name></creator><creator><name>Lennon D.</name></creator><creator><name>Marengo M.,Meixner M.</name></creator><creator><name>Skillman E.</name></creator><creator><name>Sloan G.C.</name></creator><creator><name>Sonneborn G.</name></creator><creator><name>van Loon J.TH.,Zijlstra A.</name></creator><date role="Updated">2017-06-30T05:48:15Z</date><date role="Created">2015-07-03T09:52:48Z</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>galaxies</subject><subject>infrared-photometry</subject><description>Nearby resolved dwarf galaxies provide excellent opportunities for studying the dust-producing late stages of stellar evolution over a wide range of metallicity (-2.7&lt;~[Fe/H]&lt;~-1.0). Here, we describe DUSTiNGS (DUST in Nearby Galaxies with Spitzer): a 3.6 and 4.5{mu}m post-cryogen Spitzer Space Telescope imaging survey of 50 dwarf galaxies within 1.5Mpc that is designed to identify dust-producing asymptotic giant branch (AGB) stars and massive stars. The survey includes 37 dwarf spheroidal, 8 dwarf irregular, and 5 transition-type galaxies. This near-complete sample allows for the building of statistics on these rare phases of stellar evolution over the full metallicity range. The photometry is &gt;75% complete at the tip of the red giant branch for all targeted galaxies, with the exception of the crowded inner regions of IC 10, NGC 185, and NGC 147. This photometric depth ensures that the majority of the dust-producing stars, including the thermally pulsing AGB stars, are detected in each galaxy. The images map each galaxy to at least twice the half-light radius to ensure that the entire evolved star population is included and to facilitate the statistical subtraction of background and foreground contamination, which is severe at these wavelengths. In this overview, we describe the survey, the data products, and preliminary results. We show evidence for the presence of dust-producing AGB stars in eight of the targeted galaxies, with metallicities as low as [Fe/H]=-1.9, suggesting that dust production occurs even at low metallicity.</description><source format="bibcode">2015ApJS..216...10B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/216/10</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/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/305">II/305 : SAGE LMC and SMC IRAC Source Catalog (IPAC 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/566/A44">J/A+A/566/A44 : gr photometry of Sextans A and Sextans B (Bellazzini+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/778/15">J/ApJ/778/15 : SAGE-SMC III. 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(Riebel+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/4">J/AJ/144/4 : Dwarf galaxies in the Local Group (McConnachie+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/103">J/AJ/142/103 : Cool evolved stars in SAGE-SMC (Boyer+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/88">J/AJ/142/88 : Segue 3 photometric and kinematic data (Fadely+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/193/23">J/ApJS/193/23 : Fundamental stellar parameters in 47 Tucanae (McDonald+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/416">J/AJ/140/416 : IR photometry of massive stars in the SMC (Bonanos+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/712/1259">J/ApJ/712/1259 : LCID project. II. Variables in IC1613 (Bernard+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/506/1277">J/A+A/506/1277 : Magellanic Cloud C/O stars modelisation (Groenewegen+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/697/1993">J/ApJ/697/1993 : Spitzer study of AGB stars. III. (Boyer+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/4810">J/AJ/137/4810 : LMC-SAGE AGB star candidates (Srinivasan+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/3139">J/AJ/137/3139 : LMC SAGE. New variable evolved stars and YSOs (Vijh+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/385/1045">J/MNRAS/385/1045 : JHKsIc photom. of AGB in Phoenix dwarf gal. (Menzies+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/664/850">J/ApJ/664/850 : Spitzer observations of stars in M33 (McQuinn+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/376/313">J/MNRAS/376/313 : Carbon star in Magellanic Cloud (Groenewegen+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/655/212">J/ApJ/655/212 : S3MC IRAC and MIPS photometry (Bolatto+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/2268">J/AJ/132/2268 : SAGE calibration stars (Meixner+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/448/181">J/A+A/448/181 : IR colours of AGB and post-AGB stars (Groenewegen+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/97/729">J/A+AS/97/729 : JHKL'M obs. of O-Rich late-type star (Le Bertre 1993)</relatedResource><relatedResource>http://irsa.ipac.caltech.edu/data/SPITZER/DUSTiNGS/ : NASA/IRSA DUSTiNGS 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Spitzer/IRAC 3.6um magnitude, epoch 2</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[3.6]2</name><description>[0.02/0.3]? 1{sigma} uncertainty in [3.6]2</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[4.5]</name><description>[9.4/21]? Spitzer/IRAC 4.5um magnitude, combined epochs</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[4.5]</name><description>[0.02/0.3]? 1{sigma} uncertainty in [4.5]</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[4.5]1</name><description>[9.8/20.6]? Spitzer/IRAC 4.5um magnitude, epoch 1</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[4.5]1</name><description>[0.03/0.3]? 1{sigma} uncertainty in [4.5]1</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[4.5]2</name><description>[9.4/20.6]? Spitzer/IRAC 4.5um magnitude, epoch 2</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[4.5]2</name><description>[0.03/0.3]? 1{sigma} uncertainty in [4.5]2</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sh3.6</name><description>[-1/0.8]? 3.6um sharpness, combined epochs (1)</description><ucd>src.class.starGalaxy</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sh3.6e1</name><description>[-1/0.8]? 3.6{mu}m sharpness, epoch 1 (1)</description><ucd>src.class.starGalaxy</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sh3.6e2</name><description>[-1/0.8]? 3.6{mu}m sharpness, epoch 2 (1)</description><ucd>src.class.starGalaxy</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sh4.5</name><description>[-1.2/1]? 4.5um sharpness, combined epochs (1)</description><ucd>src.class.starGalaxy</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sh4.5e1</name><description>[-1/1]? 4.5{mu}m sharpness, epoch 1 (1)</description><ucd>src.class.starGalaxy</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sh4.5e2</name><description>[-1/1]? 4.5{mu}m sharpness, epoch 2 (1)</description><ucd>src.class.starGalaxy</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>x3.6</name><description>[0/15]? 3.6um {chi} value, combined epochs (1)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>x3.6e1</name><description>[0/13]? 3.6{mu}m {chi} value, epoch 1 (1)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>x3.6e2</name><description>[0/17]? 3.6{mu}m {chi} value, epoch 2 (1)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>x4.5</name><description>[0/12]? 4.5um {chi} value, combined epochs (1)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>x4.5e1</name><description>[0/12]? 4.5{mu}m {chi} value, epoch 1 (1)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>x4.5e2</name><description>[0/18]? 4.5{mu}m {chi} value, epoch 2 (1)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Im</name><description>Image of the 4 bands from the IRSA server (IPAC)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>