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<ri:Resource created="2018-12-10T16:29:45Z" 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 galaxies. I.</title><shortName>J/ApJ/853/172</shortName><identifier>ivo://CDS.VizieR/J/ApJ/853/172</identifier><altIdentifier>doi:10.26093/cds/vizier.18530172</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Liu D.</name></creator><creator><name>Daddi E.</name></creator><creator><name>Dickinson M.</name></creator><creator><name>Owen F.</name></creator><creator><name>Pannella M.</name></creator><creator><name>Sargent M.,Bethermin M.</name></creator><creator><name>Magdis G.</name></creator><creator><name>Gao Yu</name></creator><creator><name>Shu X.</name></creator><creator><name>Wang T.</name></creator><creator><name>Jin S.</name></creator><creator><name>Inami H.</name></creator><date role="Updated">2018-12-11T13:47:26Z</date><date role="Created">2018-12-10T16:29:45Z</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>photometry</subject><subject>infrared-photometry</subject><subject>spectral-energy-distribution</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>surveys</subject><subject>redshifted</subject><description>We present a new technique to measure multi-wavelength "super-deblended" photometry from highly confused images, which we apply to Herschel and ground-based far-infrared (FIR) and (sub-)millimeter (mm) data in the northern field of the Great Observatories Origins Deep Survey (GOODS-N). There are two key novelties. First, starting with a large database of deep Spitzer 24{mu}m and VLA 20cm detections that are used to define prior positions for fitting the FIR/submm data, we perform an active selection of useful priors independently at each frequency band, moving from less to more confused bands. Exploiting knowledge of redshift and all available photometry, we identify hopelessly faint priors that we remove from the fitting pool. This approach significantly reduces blending degeneracies and allows reliable photometry to be obtained for galaxies in FIR+mm bands. Second, we obtain well-behaved, nearly Gaussian flux density uncertainties, individually tailored to all fitted priors for each band. This is done by exploiting extensive simulations that allow us to calibrate the conversion of formal fitting uncertainties to realistic uncertainties, depending on directly measurable quantities. We achieve deeper detection limits with high fidelity measurements and uncertainties at FIR+mm bands. As an illustration of the utility of these measurements, we identify 70 galaxies with z&gt;=3 and reliable FIR+mm detections. We present new constraints on the cosmic star formation rate density at 3&lt;z&lt;6, finding a significant contribution from z&gt;=3 dusty galaxies that are missed by optical-to-near-infrared color selection. Photometric measurements for 3306 priors, including more than 1000 FIR+mm detections, are released publicly with our catalog.</description><source format="bibcode">2018ApJ...853..172L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/853/172</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/261">II/261 : GOODS initial results (Giavalisco+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/471/L5">J/ApJ/471/L5 : Redshift clustering in the Hubble Deep Field (Cohen+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/481/673">J/ApJ/481/673 : HDF flanking fields and related data (Lowenthal+, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/519/1">J/ApJ/519/1 : Lyman-break galaxies at z {&gt;~} 4 (Steidel+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/538/29">J/ApJ/538/29 : HDF-N Caltech faint galaxy redshift survey. 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luminosity</description><unit>1e+10solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.AGN</name><description>[0/2292] Error in SED_AGN</description><unit>1e+10solLum</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.TOT</name><description>[0.001/3265] Super-deblended SED best-fit total luminosity</description><unit>1e+10solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.TOT</name><description>[0/2453] Error in SED.TOT</description><unit>1e+10solLum</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.70</name><description>[0.002/46.2] Super-deblended SED predicted 70um flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.30-60um</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.70</name><description>[0.0004/12.5] Error in SED.70</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.100</name><description>[0.002/76] Super-deblended SED predicted 100um flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.60-100um</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.100</name><description>[0.0006/25] Error in SED.100</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.160</name><description>[0.001/95] Super-deblended SED predicted 160um flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.1500-3000GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.160</name><description>[0.0006/60] Error in SED.160</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.250</name><description>[0.0006/72] Super-deblended SED predicted 250um flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.750-1500GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.250</name><description>[0.0002/72] Error in SED.250</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.350</name><description>[0.0002/51] Super-deblended SED predicted 350um flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.750-1500GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.350</name><description>[0.0001/51] Error in SED.350</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.500</name><description>[0.0001/33] Super-deblended SED predicted 500um flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.400-750GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.500</name><description>[4.5e-05/25] Error in SED.500</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.850</name><description>[2e-05/17] Super-deblended SED predicted 850um flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.200-400GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.850</name><description>[8.8e-06/7] Error in SED.850</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.1160</name><description>[4e-06/8.1] Super-deblended SED predicted 1160um flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.200-400GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.1160</name><description>[3.2e-06/4] Error in SED.1160</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.1200</name><description>[3e-06/7.4] Super-deblended SED predicted 1200um flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.200-400GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.1200</name><description>[2.9e-06/3.2] Error in SED.1200</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.1250</name><description>[2.5e-06/6.6] Super-deblended SED predicted 1250um flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.200-400GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.1250</name><description>[2.5e-06/3] Error in SED.1250</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.2000</name><description>[-1.5e-08/1.6] Super-deblended SED predicted 2000um flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.100-200GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.2000</name><description>[1.4e-08/0.9] Error in SED.2000</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.2050</name><description>[-2.2e-09/1.5] Super-deblended SED predicted 2050um flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.100-200GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.2050</name><description>[2e-09/0.8] Error in SED.2050</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.10cm</name><description>[2e-14/0.2] Super-deblended SED predicted 10cm flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.10cm</name><description>[2e-14/0.1] Error in SED.10cm</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SED.20cm</name><description>[2e-14/0.3] Super-deblended SED predicted 20cm flux density</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SED.20cm</name><description>[2e-14/0.2] Error in SED.20cm</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>chi2Tot</name><description>[0/171] Super-deblended SED chi-squ. of fitted data points for whole SED</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>o_chi2Tot</name><description>[3/18] Number of fitted data points in chi2Tot</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>chi2*</name><description>[0/101] Super-deblended SED chi-sq. of fitted data points for stellar component of SED</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>o_chi2*</name><description>[0/6] Number of fitted data points in chi2*</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>chi2D</name><description>[0/134] Super-deblended SED chi-sq. of fitted data points for dust component of the D</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>o_chi2D</name><description>[2/10] Number of fitted data points for chi2D</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>U</name><description>[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></column><column><name>SFR-tot</name><description>[0/1813] Sum of UV-unattenuated SFR and super-deblended SED best-fit dust-obscured SFR</description><unit>solMass/yr</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SFR-Ratio</name><description>[0/1] Ratio of UV-unattenuated and super-deblended SED best-fit dust-obscured SFRs</description><ucd>stat.fit.omc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S14</name><description>Display data from Skelton+, 2014, J/ApJS/214/24, within 1"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Plot</name><description>IR-SED plot of this galaxy</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>