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<ri:Resource created="2017-01-12T15:11:47Z" 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>SFR for WISE + SDSS spectroscopic galaxies</title><shortName>J/ApJS/219/8</shortName><identifier>ivo://CDS.VizieR/J/ApJS/219/8</identifier><altIdentifier>doi:10.26093/cds/vizier.22190008</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chang Y.-Y.</name></creator><creator><name>van der Wel A.</name></creator><creator><name>da Cunha E.</name></creator><creator><name>Rix H.-W.</name></creator><date role="Updated">2017-06-01T08:49:40Z</date><date role="Created">2017-01-12T15:11:47Z</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>spectroscopy</subject><subject>redshifted</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><subject>spectral-energy-distribution</subject><description>We combine Sloan Digitital Sky Survey (SDSS) and WISE photometry for the full SDSS spectroscopic galaxy sample, creating spectral energy distributions (SEDs) that cover {lambda}=0.4-22{mu}m for an unprecedentedly large and comprehensive sample of 858365 present-epoch galaxies. Using MAGPHYS (da Cunha+ 2008MNRAS.388.1595D), we then simultaneously and consistently model both the attenuated stellar SED and the dust emission at 12 and 22{mu}m, producing robust new calibrations for monochromatic mid-IR star formation rate (SFR) proxies. These modeling results provide the first mid-IR-based view of the bimodality in star formation activity among galaxies, exhibiting the sequence of star-forming galaxies ("main sequence") with a slope of dlogSFR/dlogM_*_=0.80 and a scatter of 0.39dex. We find that these new SFRs along the SF main sequence are systematically lower by a factor of 1.4 than those derived from optical spectroscopy. We show that for most present-day galaxies, the 0.4-22{mu}m SED fits can exquisitely predict the fluxes measured by Herschel at much longer wavelengths. Our analysis also illustrates that the majority of stars in the present-day universe are formed in luminous galaxies (~L*) in and around the "green valley" of the color-luminosity plane. We make publicly available the matched photometry catalog and SED modeling results.</description><source format="bibcode">2015ApJS..219....8C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/219/8</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/V/139">V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/196/11">J/ApJS/196/11 : Bulge+disk decompositions of SDSS galaxies (Simard+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/415/2336">J/MNRAS/415/2336 : Herschel-ATLAS Science Demonstration Catalog (Rigby+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/692/556">J/ApJ/692/556 : Star forming galaxy templates (Rieke+, 2009)</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/ApJS/219/8</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/219/8</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/219/8</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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WISE/W1-band flux after corrections</description><unit>Jy</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_flux-w1</name><description>? Uncertainty in flux-w1</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>flux-w2</name><description>? WISE/W2-band flux after corrections</description><unit>Jy</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_flux-w2</name><description>? Uncertainty in flux-w2</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>flux-w3</name><description>? WISE/W3-band flux after corrections</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_flux-w3</name><description>? Uncertainty in flux-w3</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_flux-w4</name><description>? Uncertainty in flux-w4</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>extin-u</name><description>[0.01/5.7] Galactic extinction correction for u-band</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>extin-g</name><description>[0.009/4.5] Galactic extinction correction for g-band</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>extin-r</name><description>[0.006/3.1] Galactic extinction correction for r-band</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>extin-i</name><description>[0.005/2.3] Galactic extinction correction for i-band</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>extin-z</name><description>[0.003/1.7] Galactic extinction correction for z-band</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Sp</name><description>Interactive spectrum from SDSS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>lmass2.5</name><description>? log stellar mass; 2.5th percentile</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lmass16</name><description>? log stellar mass; 16th percentile</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lmass50</name><description>? log stellar mass; 50th percentile</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lmass84</name><description>? log stellar mass; 84th percentile</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lmass97.5</name><description>[7/13]? log stellar mass; 97.5th percentile</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lsfr2.5</name><description>? log SFR; 2.5th percentile</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lsfr16</name><description>? log SFR; 16th percentile</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lsfr50</name><description>? log SFR; 50th percentile</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lsfr84</name><description>? log SFR; 84th percentile</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lsfr97.5</name><description>[-5/3]? log SFR; 97.5th percentile</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lssfr2.5</name><description>? log specific SFR; 2.5th percentile</description><unit>log(yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lssfr16</name><description>? log specific SFR; 16th percentile</description><unit>log(yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lssfr50</name><description>? log specific SFR; 50th percentile</description><unit>log(yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lssfr84</name><description>? log specific SFR; 84th percentile</description><unit>log(yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lssfr97.5</name><description>[-18/-7]? log specific SFR; 97.5th percentile</description><unit>log(yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lDust2.5</name><description>? log Dust luminosity; 2.5th percentile</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lDust16</name><description>? log Dust luminosity; 16th percentile</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lDust50</name><description>? log Dust luminosity; 50th percentile</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lDust84</name><description>? log Dust luminosity; 84th percentile</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lDust97.5</name><description>[7/13]? log Dust luminosity; 97.5th percentile</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mu2.5</name><description>? Dust attenuation parameter; 2.5th percentile (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mu16</name><description>? Dust attenuation parameter; 16th percentile (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mu50</name><description>? Dust attenuation parameter; 50th percentile (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mu84</name><description>? Dust attenuation parameter; 84th percentile (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mu97.5</name><description>? Dust attenuation parameter; 97.5th percentile (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>tauv2.5</name><description>? Dust attenuation parameter; 2.5th percentile (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>tauv16</name><description>? Dust attenuation parameter; 16th percentile (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>tauv50</name><description>? Dust attenuation parameter; 50th percentile (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>tauv84</name><description>? Dust attenuation parameter; 84th percentile (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>tauv97.5</name><description>[0.002/6]? Dust attenuation parameter; 97.5th percentile (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>vmax</name><description>? Maximum volume for LMASS_50</description><unit>Mpc**3</unit><ucd>meta.bib.volume</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>lrest-u</name><description>[-10.6/13.5]? Rest-frame u-band Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>lrest-g</name><description>[-11.2/14.3]? Rest-frame g-band Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>lrest-r</name><description>[-11.9/13.7]? Rest-frame r-band Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>lrest-i</name><description>[-8.8/15.1]? Rest-frame i-band Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>lrest-z</name><description>[-7.5/17.6]? Rest-frame z-band Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>lrest-w1</name><description>[-7.2/12.4]? Rest-frame W1-band Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity;em.IR</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>lrest-w2</name><description>[-7.5/12]? Rest-frame W2-band Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity;em.IR</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>lrest-w3</name><description>[-7.5/12.5]? Rest-frame W3-band Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>lrest-w4</name><description>[-6.5/16.4]? Rest-frame W4-band Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>flagW</name><description>[0/2]? WISE flag (1 = single match) (4)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>flagW1</name><description>[0/2]? WISE W1 filter detection flag (5)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>flagW2</name><description>[0/2]? WISE W2 filter detection flag (5)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>flagW3</name><description>[0/2]? WISE W3 filter detection flag (5)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>flagW4</name><description>[0/2]? WISE W4 filter detection flag (5)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>flagChi2</name><description>[0/1]? Best-fit model flag (1=chi^2^&lt;3) (6)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>flag</name><description>[0/1]? Flag (1=good fit) (7)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>DR9</name><description>Display data from the SDSS-DR9 photometric catalog (V/139)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>