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<ri:Resource created="2022-04-11T07:16:54Z" 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>Multiwavelength study in M33 star clusters</title><shortName>J/AJ/163/16</shortName><identifier>ivo://CDS.VizieR/J/AJ/163/16</identifier><altIdentifier>doi:10.26093/cds/vizier.51630016</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Moeller C.</name></creator><creator><name>Calzetti D.</name></creator><date role="Updated">2022-09-30T22:24:37Z</date><date role="Created">2022-04-11T07:16:54Z</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>open-star-clusters</subject><subject>stellar-ages</subject><subject>stellar-masses</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>We combine archival images for the nearby galaxy M33 (Triangulum Galaxy) from the ultraviolet (UV) to the infrared to derive ages, masses, and extinctions for the young star cluster population, and compare our physical parameters with published ones. Our goal is to test the robustness of clusters ages and masses, and possibly improve on existing ones both by expanding the wavelength range of the spectral-energy distribution (SED) fits and by using more recent population synthesis models. The rationale for this experiment is to verify the sensitivity of the clusters physical parameters to observational setups and model choices that span those commonly found in the literature. We derive the physical parameters of 137 clusters, using SEDs measured in eight UV-to-I bands, including H{alpha}, from GALEX and ground-based images. We also add the 24{mu}m image from the Spitzer Space Telescope to help break some age degeneracies. We find that our derived cluster ages show significant differences with earlier determinations, while the masses remain relatively insensitive to the fitting approach adopted. We also highlight an already known difficulty in recovering old, low-extinction clusters, as SED-fitting codes tend to prefer younger, higher extinction solutions when the extinction is a free parameter. We publish updated ages, masses, and extinctions, with uncertainties for all sample star clusters, together with their photometry. Given the proximity of M33, this represents an important population to secure for the study of star formation and cluster evolution in spirals.</description><source format="bibcode">2022AJ....163...16M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/163/16</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/141/371">J/A+AS/141/371 : Low-mass stars evolut. tracks &amp; isochrones (Girardi+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/633/871">J/ApJ/633/871 : Positions and photometry of HII knots in M51 (Calzetti+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/2478">J/AJ/131/2478 : M31 and M33 UBVRI photometry (Massey+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/2474">J/AJ/134/2474 : H{alpha} emission-line stars 7 dwarfs galaxies (Massey+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/658/1006">J/ApJ/658/1006 : Radial profiles for 161 face-on spirals (Munoz-Mateos+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/447">J/AJ/134/447 : Catalog of star cluster candidates in M 33 (Sarajedini+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/178/247">J/ApJS/178/247 : H{alpha} and [NII] survey in local 11 Mpc (Kennicutt+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/706/553">J/ApJ/706/553 : Fluxes in nearby star-forming galaxies (Boquien+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/517">J/ApJ/703/517 : The Spitzer Local Volume Legacy: IR photometry (Dale+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/534/A96">J/A+A/534/A96 : Spitzer photometry of YSC in M33 (Sharma+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/812/147">J/ApJ/812/147 : Slug analysis star clusters in NGC628 &amp; 7793 (Krumholz+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/824/71">J/ApJ/824/71 : Compact star clusters in M51 with HST (Chandar+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/841/92">J/ApJ/841/92 : Young massive star clusters in 2 LEGUS galaxies (Ryon+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/889/154">J/ApJ/889/154 : LEGUS &amp; Ha-LEGUS obs. NGC4449 star clusters (Whitmore+, 2020)</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/AJ/163/16</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/163/16</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/163/16</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/163/16</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/163/16</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/163/16</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/163/16/table6 (Derived and literature physical properties of the M33 star clusters)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/163/16/table6?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/163/16/table6?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/163/16/table6?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>23.178875</ra><dec>30.5940556</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/163/16/table3 (*Photometric measurements of the M33 star clusters)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/163/16/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/163/16/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/163/16/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>23.178875</ra><dec>30.5940556</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/163/16/table4 (Clusters excluded from analysis)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/163/16/table4?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/163/16/table4?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/163/16/table4?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>23.3075</ra><dec>30.4843333</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/2154-2155 2241</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/163/16?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/163/16/table6</name><description>Derived and literature physical properties of the M33 star clusters</description><column><name>Comm</name><description>? 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