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<ri:Resource created="2007-11-03T22:03:56Z" 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>L_IR_-T_dust_ relation in galaxies</title><shortName>J/A+A/462/81</shortName><identifier>ivo://CDS.VizieR/J/A+A/462/81</identifier><altIdentifier>doi:10.26093/cds/vizier.34620081</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chanial P.</name></creator><creator><name>Flores H.</name></creator><creator><name>Guiderdoni B.</name></creator><creator><name>Elbaz D.</name></creator><creator><name>Hammer F.</name></creator><creator><name>Vigroux L.</name></creator><date role="Updated">2017-07-11T13:08:40Z</date><date role="Created">2007-11-03T22:03:56Z</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>radio-galaxies</subject><subject>galaxies</subject><subject>infrared-sources</subject><subject>effective-temperature</subject><description>IRAS observations show the existence of a correlation between the infrared luminosity L_IR_ and dust temperature T_d_ in star-forming galaxies, in which larger L_IR_ leads to higher dust temperature. The L_IR_-T_d_ relation is commonly seen as reflecting the increase in dust temperature in galaxies with higher star formation rate (SFR). Even though the correlation shows a significant amount of dispersion, a unique relation has been commonly used to construct spectral energy distributions (SEDs) of galaxies in distant universe studies, such as source number counting or photometric redshift determination. 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