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<ri:Resource created="2018-04-03T07:11:48Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Synthetic JWST/MIRI fluxes and magnitudes</title><shortName>J/ApJ/841/15</shortName><identifier>ivo://CDS.VizieR/J/ApJ/841/15</identifier><altIdentifier>doi:10.26093/cds/vizier.18410015</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jones O.C.</name></creator><creator><name>Meixner M.</name></creator><creator><name>Justtanont K.</name></creator><creator><name>Glasse A.</name></creator><date role="Updated">2018-05-16T09:04:50Z</date><date role="Created">2018-04-03T07:11:48Z</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>infrared-photometry</subject><description>The Mid-Infrared Instrument (MIRI) for the James Webb Space Telescope (JWST) will revolutionize our understanding of infrared stellar populations in the Local Volume. Using the rich Spitzer-IRS spectroscopic data set and spectral classifications from the Surveying the Agents of Galaxy Evolution (SAGE)-Spectroscopic survey of more than 1000 objects in the Magellanic Clouds, the Grid of Red Supergiant and Asymptotic Giant Branch Star Model (GRAMS; Sargent+ 2011ApJ...728...93S and Srinivasan+ 2011, J/A+A/532/A54), and the grid of YSO models by Robitaille+ (2006ApJS..167..256R), we calculate the expected flux densities and colors in the MIRI broadband filters for prominent infrared stellar populations. We use these fluxes to explore the JWST/MIRI colors and magnitudes for composite stellar population studies of Local Volume galaxies. MIRI color classification schemes are presented; these diagrams provide a powerful means of identifying young stellar objects, evolved stars, and extragalactic background galaxies in Local Volume galaxies with a high degree of confidence. Finally, we examine which filter combinations are best for selecting populations of sources based on their JWST colors.</description><source format="bibcode">2017ApJ...841...15J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/841/15</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/119/141">J/ApJS/119/141 : Oxygen-rich dust shells IR spectral classif. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Class</name><description>SAGE-Spec classification type (G1)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>F770W</name><description>? JWST/MIRI synthetic F770W fluxes (1)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F770W</name><description>? Uncertainty in F770W</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F1000W</name><description>[0.5/4908]? JWST/MIRI synthetic F1000W fluxes (1)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F1000W</name><description>[0.1/130]? Uncertainty in F1000W</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F1130W</name><description>? JWST/MIRI synthetic F1130W fluxes (1)</description><unit>mJy</unit><ucd>em.IR.8-15um;phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F1130W</name><description>? Uncertainty in F1130W</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F1280W</name><description>? JWST/MIRI synthetic F1280W fluxes (1)</description><unit>mJy</unit><ucd>em.IR.8-15um;phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F1280W</name><description>? Uncertainty in F1280W</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F1500W</name><description>? JWST/MIRI synthetic F1500W fluxes (1)</description><unit>mJy</unit><ucd>em.IR.15-30um;phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F1500W</name><description>? Uncertainty in F1500W</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F1800W</name><description>? JWST/MIRI synthetic F1800W fluxes (1)</description><unit>mJy</unit><ucd>em.IR.15-30um;phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F1800W</name><description>? Uncertainty in F1800W</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F2100W</name><description>? JWST/MIRI synthetic F2100W fluxes (1)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F2100W</name><description>? Uncertainty in F2100W</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F2550W</name><description>[0.4/52919]? JWST/MIRI synthetic F2550W fluxes (1)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F2550W</name><description>[0/2201]? Uncertainty in F2550W</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/841/15/table4</name><description>*Estimated MIRI magnitudes and uncertainties for our LMC and background galaxy sample</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Class</name><description>SAGE-Spec classification type (G1)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>F770Wmag</name><description>[2.7/13]? JWST/MIRI synthetic F770W Vega magnitude (1)</description><unit>mag</unit><ucd>em.IR.4-8um;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F770Wmag</name><description>[0.03/2.4]? Uncertainty in F770W (1)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F1000Wmag</name><description>[2.2/12.2]? 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JWST/MIRI synthetic F1280W Vega magnitude (1)</description><unit>mag</unit><ucd>em.IR.8-15um;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F1280Wmag</name><description>[0.03/1]? Uncertainty in F1280W (1)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F1500Wmag</name><description>[0.3/10.7]? JWST/MIRI synthetic F1500W Vega magnitude (1)</description><unit>mag</unit><ucd>em.IR.15-30um;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F1500Wmag</name><description>[0.03/0.6]? Uncertainty in F1500W (1)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F1800Wmag</name><description>[-0.6/10.5]? JWST/MIRI synthetic F1800W Vega magnitude (1)</description><unit>mag</unit><ucd>em.IR.15-30um;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F1800Wmag</name><description>[0.03/2]? Uncertainty in F1800W (1)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F2100Wmag</name><description>[-1.4/10.4]? JWST/MIRI synthetic F2100W Vega magnitude (1)</description><unit>mag</unit><ucd>em.IR.15-30um;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F2100Wmag</name><description>[0.03/1.7]? Uncertainty in F2100W (1)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F2550Wmag</name><description>[-2.4/10.4]? JWST/MIRI synthetic F2550W Vega magnitude (1)</description><unit>mag</unit><ucd>em.IR.15-30um;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F2550Wmag</name><description>[0.03/1.8]? Uncertainty in F2550W (1)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>