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<ri:Resource created="2023-03-22T08:33:42Z" 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>"Super-deblended" dust emission in gal. II. COSMOS</title><shortName>J/ApJ/864/56</shortName><identifier>ivo://CDS.VizieR/J/ApJ/864/56</identifier><altIdentifier>doi:10.26093/cds/vizier.18640056</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jin S.</name></creator><creator><name>Daddi E.</name></creator><creator><name>Liu D.</name></creator><creator><name>Smolcic V.</name></creator><creator><name>Schinnerer E.</name></creator><creator><name>Calabro A.</name></creator><creator><name>Gu Q.,Delhaize J.</name></creator><creator><name>Delvecchio I.</name></creator><creator><name>Gao Y.</name></creator><creator><name>Salvato M.</name></creator><creator><name>Puglisi A.</name></creator><creator><name>Dickinson M.,Bertoldi F.</name></creator><creator><name>Sargent M.</name></creator><creator><name>Novak M.</name></creator><creator><name>Magdis G.</name></creator><creator><name>Aretxaga I.</name></creator><creator><name>Wilson G.W.,Capak P.</name></creator><date role="Updated">2023-11-03T11:11:24Z</date><date role="Created">2023-03-22T08:33:42Z</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><subject>millimeter-astronomy</subject><subject>photometry</subject><subject>submillimeter-astronomy</subject><subject>galaxies</subject><subject>redshifted</subject><subject>active-galactic-nuclei</subject><subject>surveys</subject><description>We present a "super-deblended" far-infrared (FIR) to (sub)millimeter photometric catalog in the Cosmic Evolution Survey (COSMOS), prepared with the method recently developed by Liu+ 2018 (J/ApJ/853/172), with key adaptations. We obtain point-spread function fitting photometry at fixed prior positions including 88,008 galaxies detected in VLA 1.4, 3GHz, and/or MIPS 24{mu}m images. By adding a specifically carved mass-selected sample (with an evolving stellar mass limit), a highly complete prior sample of 194428 galaxies is achieved for deblending FIR/(sub)mm images. We performed "active" removal of nonrelevant priors at FIR/(sub)mm bands using spectral energy distribution fitting and redshift information. In order to cope with the shallower COSMOS data, we subtract from the maps the flux of faint nonfitted priors and explicitly account for the uncertainty of this step. The resulting photometry (including data from Spitzer, Herschel, SCUBA2, AzTEC, MAMBO, and NSF's Karl G. Jansky Very Large Array at 3 and 1.4GHz) displays well-behaved quasi-Gaussian uncertainties calibrated from Monte Carlo simulations and tailored to observables (crowding, residual maps). Comparison to ALMA photometry for hundreds of sources provides a remarkable validation of the technique. We detect 11220 galaxies over the 100-1200{mu}m range extending to z_phot_~7. We conservatively selected a sample of 85 z&gt;4 high-redshift candidates significantly detected in the FIR/(sub)mm, often with secure radio and/or Spitzer/IRAC counterparts. This provides a chance to investigate the first generation of vigorous starburst galaxies (SFRs~1000M_{sun}_/yr).</description><source format="bibcode">2018ApJ...864...56J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/864/56</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/VII/250">VII/250 : The 2dF Galaxy Redshift Survey (2dFGRS) (2dFGRS Team, 1998-2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/95">VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/103">VIII/103 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/373">II/373 : The fourth UltraVISTA data release (DR4) (Moneti+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/554/803">J/ApJ/554/803 : New VLA Sky Survey (NVSS) Cat of IRAS 2Jy Galaxies (Yun+ 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/644/100">J/ApJ/644/100 : SDSS quasars in the COSMOS field (Prescott+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/172/70">J/ApJS/172/70 : zCOSMOS-bright catalog (Lilly+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/172/383">J/ApJS/172/383 : AGN candidates in the COSMOS field (Trump+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/218">J/ApJS/184/218 : The zCOSMOS 10k-bright spectroscopic sample (Lilly+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/709/572">J/ApJ/709/572 : COSMOS 70um sources (Kartaltepe+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/188/178">J/ApJS/188/178 : VLA 1.4GHz observations of GOODS-North field (Morrison+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/188/384">J/ApJS/188/384 : The VLA-COSMOS survey. 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Super-deblended Herschel/SPIRE 350um flux</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.750-1500GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F350</name><description>[1.2/13956]? Error in F350 (DF350) (9)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F500</name><description>[0/96]? Super-deblended Herschel/SPIRE 500um flux</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.400-750GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F500</name><description>[0.7/9627]? Error in F500 (DF500) (9)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F850</name><description>[0/19.4]? Super-deblended JCMT/SCUBA2 850um flux</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.200-400GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F850</name><description>[0.4/1427]? Error in F850 (DF850) (9)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F1100</name><description>[0.9/637]? Error in F1100 (DF1100) (9)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F1200</name><description>[0/7]? Super-deblended IRAM/MAMBO 1.2mm flux</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.200-400GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F1200</name><description>[0.4/11]? Error in F1200 (DF1200) (9)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F10cm</name><description>[0/25.2]? Super-deblended VLA 3GHz flux</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F10cm</name><description>[0.002/210]? Error in F10cm (DF10CM)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>S17</name><description>[0/1] Flag of whether the original 10cm photometry is from Smolcic+ (2017, J/A+A/602/A1) (SMOLCIC)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>F10cmC1p5</name><description>[0/2451]? Super-deblended flux in 1.5" convolved 3GHz image (F10CM_1ARC5)</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F10cmC1p5</name><description>[0.002/1e+10]? Error in F10cm_1arc5 (DF10CM_1ARC5)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F10cmC2</name><description>[0/19.4]? Super-deblended flux in 2" convolved 3GHz image (F10CM_2ARC)</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F10cmC2</name><description>[0.005/1e+10]? Error in F10cm_2arc (DF10CM_2ARC)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XF3000</name><description>[0/28]? Error in xf3000 (XE3000)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F20cm</name><description>[0/1.1e+7]? Super-deblended VLA 1.4GHz flux</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_F20cm</name><description>[0.003/1e+8]? Error in F20cm (DF20CM)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>XLAGN</name><description>[0/8868]? Super-deblended SED best-fit AGN luminosity (XFAGN)</description><unit>1e+10solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_XLAGN</name><description>[0/8868]? Error in xfAGN (XEAGN)</description><unit>1e+10solLum</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>XLTot</name><description>[0/49530]? Super-deblended SED fit Total luminosity (XFTOT)</description><unit>1e+10solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XLTot</name><description>[0/739065]? Super-deblend. SED fit Total luminosity error (XETOT)</description><unit>1e+10solLum</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>XF70</name><description>[0/803]? Super-deblended SED predicted flux density at 70um</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.60-100um;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XF70</name><description>[7.8e-5/154]? Error in xf70 (XE70)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>XF100</name><description>[0/1016]? Super-deblended SED predicted flux density at 100um</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.60-100um;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XF100</name><description>[0/126]? Error in xf100 (XE100)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>XF160</name><description>[0/977]? Super-deblended SED predicted flux density at 160um</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.1500-3000GHz;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XF160</name><description>[3.5e-5/49]? Error in xf160 (XE160)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>XF250</name><description>[0/457]? Super-deblended SED predicted flux density at 250um</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.750-1500GHz;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XF250</name><description>[1e-5/114]? Error in xf250 (XE250)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>XF350</name><description>[0/192]? Super-deblended SED predicted flux density at 350um</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.750-1500GHz;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XF350</name><description>[4e-6/158]? Error in xf350 (XE350)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>XF500</name><description>[0/286]? Super-deblended SED predicted flux density at 500um</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.400-750GHz;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XF500</name><description>[1e-6/273]? Error in xf500 (XE500)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>XF850</name><description>[0/353]? Super-deblended SED predicted flux density at 850um</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.200-400GHz;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XF850</name><description>[0/350]? Error in xf850 (XE850)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>XF1100</name><description>[0/291]? Super-deblended SED predicted flux density at 1.1mm</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.200-400GHz;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XF1100</name><description>[0/290]? Error in xf1100 (XE1100)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XF1200</name><description>[0/262]? Error in xf1200 (XE1200)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>XF2000</name><description>[0/90]? Super-deblended SED predicted flux density at 2mm</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.100-200GHz;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XF2000</name><description>[0/90]? Error in xf2000 (XE2000)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>XF3000</name><description>[-000017/28]? Super-deblended SED predicted flux density at 3mm</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.50-100GHz;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>XF10CM</name><description>[0/1.8]? Super-deblended SED predicted flux density at 10cm</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.1500-3000MHz;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XF10CM</name><description>[0/0.5]? Error in xf10cm (XE10CM)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>XF20CM</name><description>[0/3.1]? Super-deblended SED predicted flux density at 20cm</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.750-1500MHz;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_XF20CM</name><description>[0/0.8]? Error in xf20cm (XE20CM)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Ubest</name><description>[2.2/101]? Super-deblended SED best-fit dust template's mean interstellar radiation field strength (10)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Chi2</name><description>[0/1045]? Super-deblended SED chi-sq. of fitted data points (CHI2_MIN)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Chi2Star</name><description>[0/171]? Super-deblended SED chi-sq. of fitted data points for stellar component of the SED (S_CHI2_MIN)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Chi2Dust</name><description>[0/1030]? Super-deblended SED chi-sq. of fitted data points for dust component of the SED (R_CHI2_MIN)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FIR</name><description>[0/1] Super-deblended SED fitting's Type_FIR flag (TYPE_FIR) (11)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cl</name><description>[-1/1]? Super-deblended SED fitting's Type_SED flag (TYPE_SED) (12)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>AGN</name><description>[0/1] Super-deblended SED fitting's Type_SED flag (TYPE_AGN) (13)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>L16</name><description>Display data from COSMOS2015 (Laigle+ 2016, J/ApJS/224/24) within 0.5"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>