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<ri:Resource created="2015-11-16T14:58:31Z" 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>ALESS survey: SMGs in the ECDF-S data</title><shortName>J/ApJ/806/110</shortName><identifier>ivo://CDS.VizieR/J/ApJ/806/110</identifier><altIdentifier>doi:10.26093/cds/vizier.18060110</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>da Cunha E.</name></creator><creator><name>Walter F.</name></creator><creator><name>Smail I.R.</name></creator><creator><name>Swinbank A.M.</name></creator><creator><name>Simpson J.M.,Decarli R.</name></creator><creator><name>Hodge J.A.</name></creator><creator><name>Weiss A.</name></creator><creator><name>van der Werf P.P.</name></creator><creator><name>Bertoldi F.,Chapman S.C.</name></creator><creator><name>Cox P.</name></creator><creator><name>Danielson A.L.R.</name></creator><creator><name>Dannerbauer H.</name></creator><creator><name>Greve T.R.,Ivison R.J.</name></creator><creator><name>Karim A.</name></creator><creator><name>Thomson A.</name></creator><date role="Updated">2017-10-18T08:25:10Z</date><date role="Created">2015-11-16T14:58:31Z</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>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>redshifted</subject><description>The ALESS survey has followed up on a sample of 122 sub-millimeter sources in the Extended Chandra Deep Field South at 870{mu}m with the Atacama Large Millimeter Array (ALMA), allowing us to pinpoint the positions of sub-millimeter galaxies (SMGs) to ~0.3" and to find their precise counterparts at different wavelengths. This enabled the first compilation of the multi-wavelength spectral energy distributions (SEDs) of a statistically reliable survey of SMGs. In this paper, we present a new calibration of the magphys SED modeling code that is optimized to fit these ultraviolet-to-radio SEDs of z&gt;1 star-forming galaxies using an energy balance technique to connect the emission from stellar populations, dust attenuation, and dust emission in a physically consistent way. 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