J/ApJ/675/1319ivo://CDS.VizieR/J/ApJ/675/1319doi:10.26093/cds/vizier.16751319CDSHarayama Y.Eisenhauer F.Martins F.2017-11-29T11:48:33Z2010-09-20T09:09:30ZCDS support team

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

cds-question@unistra.frh-ii-regionsinfrared-photometryWe study the initial mass function (IMF) of one of the most massive Galactic star-forming regions NGC 3603 to answer a fundamental question in current astrophysics: is the IMF universal, or does it vary? Using our very deep, high angular resolution JHKSL' images obtained with NAOS-CONICA at the VLT at ESO, we have successfully revealed the stellar population down to the subsolar mass range in the core of the starburst cluster.2008ApJ...675.1319Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/675/1319CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/AJ/127/1014 : CCD UBVRIHa photometry in NGC 3603 (Sung+, 2004)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/675/1319https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/675/1319http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/675/1319https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/675/1319https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/675/1319http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/675/1319GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/675/1319/table6 (Photometry list)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/675/1319/table6?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/675/1319/table6?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/675/1319/table6?GETtext/xml+votable180.050000true168.7808769-61.26071670.0055555555555555566/379244.925240337479573e-20 1.7798557115773645e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/675/1319?format=asciiInfrareddefaultJ/ApJ/675/1319/table6Photometry listrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNo[1/256] Running identification number <[HEM2008] NNN> in Simbadmeta.id;meta.mainintoRAOffset in Right Ascension (1)arcsecpos.eq.ra;arith.difffloatoDEOffset in Declination (1)arcsecpos.eq.dec;arith.difffloatJmagJ band magnitudemagphot.mag;em.IR.JfloatHmagH band magnitudemagphot.mag;em.IR.HfloatKsmagK_S_ band magnitudemagphot.mag;em.IR.KfloatL'mag? L' band magnitude (2)magphot.mag;em.IR.3-4umfloatnullableSpTypeMK spectral type (3)src.spTypecharf_MDS94[H] H indicates that source is found to have a X-ray counterpart by Moffat et al. (2002ApJ...573..191M)meta.codecharMDS94? Identification in Moffat et al. (1994ApJ...436..183M) (4)meta.idintnullableONameOther names (5)meta.idcharRemRemarks on Moffat names (6)meta.notecharNS03Identification in Nurnberger & Stanke (2003A&A...400..223N) (7)meta.idcharn_NS03Note on NS03 (8)meta.notecharSB04? Identification in Sung & Bessel (2004, Cat. <J/AJ/127/1014>) (9)meta.idintnullablen_SB04"e1" indicates that Stars 21 and 52 together would correspond to 10207meta.notecharSimbadSimbad column added by the CDSchar_RASimbad column added by the CDSdegpos.eq.ra;meta.main_DESimbad column added by the CDSdegpos.eq.dec;meta.main