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<ri:Resource created="2014-01-30T09:55:15Z" 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>Star-forming galaxies in AKARI Deep Field-South</title><shortName>J/A+A/562/A15</shortName><identifier>ivo://CDS.VizieR/J/A+A/562/A15</identifier><altIdentifier>doi:10.26093/cds/vizier.35620015</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Malek K.</name></creator><creator><name>Pollo A.</name></creator><creator><name>Takeuchi T.T.</name></creator><creator><name>Buat V.</name></creator><creator><name>Burgarella D.</name></creator><creator><name>Malkan M.,Giovannoli E.</name></creator><creator><name>Kurek A.</name></creator><creator><name>Matsuura S.</name></creator><date role="Updated">2017-10-09T13:33:56Z</date><date role="Created">2014-01-30T09:55:15Z</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>surveys</subject><subject>galaxies</subject><subject>infrared-sources</subject><subject>spectral-energy-distribution</subject><description>The main aim of this work is the characterization of physical properties of galaxies detected in the far infrared (FIR) in the AKARI Deep Field-South (ADF-S) survey. Starting from a catalog of the brightest 1000 ADF-S sources in the WIDE-S (90um) AKARI band, we constructed a subsample of galaxies with spectral coverage from the ultraviolet to the far-infrared. Then, we analyzed the multiwavelength properties of this 90um-selected sample of galaxies. For galaxies without known spectroscopic redshifts we computed photometric redshifts using codes Le PHARE and CIGALE, tested these photometric redshifts using spectroscopic redshifts, and compared the performances of both codes. To test the reliability of parameters obtained by fitting Spectral Energy Distributions, a mock catalogue has been generated. We built a large multiwavelength catalog of more than 500 ADF-S galaxies. We successfully fitted Spectral Energy Distributions of 186 galaxies with {chi}^2^&lt;4, and analyzed the output parameters of the fits. We conclude that our sample consists mostly of nearby actively star-forming galaxies, and all our galaxies have a relatively high metallicity. We estimated photometric redshifts for 113 galaxies from the whole ADF-S sample. Comparing the performance of Le PHARE and CIGALE, we found that CIGALE gives more reliable redshift estimates for our galaxies, which implies that including the IR photometry allows for substantial improvement of photometric redshift estimation.</description><source format="bibcode">2014A&amp;A...562A..15M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/562/A15</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/115">VII/115 : Surface Photometry of ESO-Uppsala Galaxies (Lauberts+ 1989)</relatedResource><relatedResource 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ivo-id="ivo://CDS.VizieR/J/MNRAS/411/373">J/MNRAS/411/373 : Catalog of AKARI Deep Field South (Clements+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/427/1830">J/MNRAS/427/1830 : 20cm survey of the AKARI SEP (ATCA-ADFS) (White+, 2012)</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/A+A/562/A15</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/562/A15</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/562/A15</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/562/A15</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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Flux density at 0.1um GALEX band (Dale et al., 2007ApJ...655..863D)</description><unit>mJy</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_FUV</name><description>? rms uncertainty on 0.1um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NUV</name><description>? Flux density at 0.2um GALEX band (Dale et al., 2007ApJ...655..863D)</description><unit>mJy</unit><ucd>phot.mag;em.UV</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_NUV</name><description>? rms uncertainty on 0.2um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FUV1</name><description>? Flux density at 0.1um GALEX band (measured by co-authors)</description><unit>mJy</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_FUV1</name><description>? rms uncertainty on 0.1um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NUV1</name><description>? Flux density at 0.2um GALEX band (measured by co-authors)</description><unit>mJy</unit><ucd>phot.mag;em.UV</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_NUV1</name><description>? rms uncertainty on 0.2um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Bj</name><description>? Flux density at 0.4um APM band (Maddox et al., 1990MNRAS.243..692M)</description><unit>mJy</unit><ucd>phot.flux.density;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Bj</name><description>? rms uncertainty on 0.4um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B</name><description>? Flux density at 0.4um (2)</description><unit>mJy</unit><ucd>phot.flux.density;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_B</name><description>? rms uncertainty on 0.4um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>R</name><description>? Flux density at 0.6um (3)</description><unit>mJy</unit><ucd>phot.flux.density;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>J</name><description>? Flux density at 1.2um (4)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_J</name><description>? rms uncertainty on 1.2um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Jtot</name><description>? Flux density at 1.2um (5)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Jtot</name><description>? rms uncertainty on 1.2um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>H</name><description>? Flux density at 1.7um (4)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_H</name><description>? rms uncertainty on 1.7um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Htot</name><description>? 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