J/ApJ/626/L15ivo://CDS.VizieR/J/ApJ/626/L15doi:10.26093/cds/vizier.16269015CDSHunt L.K.Maiolino R.2017-06-20T13:15:58Z2007-03-16T10:31:12ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxiesinfrared-sourcesmillimeter-astronomysubmillimeter-astronomyredshiftedThere is growing evidence that some star-forming galaxies at z>1 are characterized by high efficiencies and specific star formation rates. In the local universe, these traits are shared by "active" blue compact dwarf galaxies (BCDs) with compact and dense star-forming regions. The spectral energy distributions (SEDs) of these BCDs are dominated by young massive star clusters, embedded in a cocoon of dust. In this Letter, we incorporate these BCD SEDs as templates for two samples of high-redshift galaxy populations selected at submillimeter wavelengths.2005ApJ...626L..15Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/626/L15CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/ApJ/622/772 : Redshift survey of submillimeter galaxies (Chapman+, 2005)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/626/L15https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/626/L15http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/626/L15https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/626/L15https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/626/L15http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/626/L15GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticalInfraredRadiodefaultJ/ApJ/626/L15/z_photPhotometric redshiftsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintn_Name{bf 1} for redshifts for submillimeter-selected SCUBA sources with VLA and Spitzer data, {bf 1} for redshifts for SCUBA/VLA sourcesmeta.notecharNameSource name (2) (1)meta.id;meta.maincharzspec? Spectroscopic redshift (2)src.redshiftfloatnullable<Res>? Lowest residuals for z=zspec obtained with Templatestat.fit.residualfloatnullableTemplate? Corresponding templatemeta.noteintnullablezII-0.5-30IIZw40 photometric redshift ({alpha}=-0.5 A_V_=30mag) (3)src.redshift.photfloatzII-0.5-20IIZw40 photometric redshift ({alpha}=-0.5 A_V_=20mag) (3)src.redshift.photfloatzII-0.1-30IIZw40 photometric redshift ({alpha}=-0.1 A_V_=30mag) (3)src.redshift.photfloatzII-0.1-20IIZw40 photometric redshift ({alpha}=-0.1 A_V_=20mag) (3)src.redshift.photfloatzNGC-0.1-10NGC5253 photometric redshift ({alpha}=-0.1 A_V_=10mag) (3)src.redshift.photfloatzSBS-0.3-30SBS 0335-052 photometric redshift ({alpha}=-0.3 A_V_=30mag) (3)src.redshift.photfloatzM82M82 photometric redshift (3)src.redshift.photfloatzArp220Arp220 photometric redshift (3)src.redshift.photfloat