J/A+A/497/41ivo://CDS.VizieR/J/A+A/497/41doi:10.26093/cds/vizier.34970041CDSCesetti M.Ivanov V.D.Morelli L.Pizzella A.Buson L.Corsini E.M.,Dalla Bonta E.Stiavelli M.Bertola F.2017-06-13T11:08:16Z2009-05-30T17:18:39ZCDS support team

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

cds-question@unistra.frgalaxiesinfrared-sourcesspectroscopyNear-infrared (hereafter NIR) data may provide complementary information to the traditional optical population synthesis analysis of unresolved stellar populations because the spectral energy distribution of the galaxies in the 1-2.5um range is dominated by different types of stars than at optical wavelengths. Furthermore, NIR data are less affected by dust absorption and hence could constrain the stellar populations in dust-obscured galaxies. We attempt to develop observational constraints on the stellar populations of unresolved stellar systems in the NIR.2009A&A...497...41Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/497/41CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/497/41https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/497/41http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/497/41https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/497/41https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/497/41http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/497/41GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapInfrareddefaultJ/A+A/497/41/table5Average spectrum of the sample galaxiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLambda[14944,24851] Spectrum Wavelengh0.1nmem.wlintFluxAvarage spectrum in arbitrary units and normalized to unity at 22000{AA} (2.2{mu}m)phot.flux;arith.ratiofloatrmsr.m.s. values per Angstroemstat.errorfloat