J/A+A/328/83ivo://CDS.VizieR/J/A+A/328/83doi:10.26093/cds/vizier.33280083CDSChabrier G.Mera D.1998-06-12T10:36:33Z1998-06-12T10:36:28ZCDS support team

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

cds-question@unistra.frglobular-star-clustersapparent-magnitudem-starsData of figure 1 of the paper, namely the luminosity function of globular clusters in bolometric magnitude. The original HST magnitude is given, then the corresponding bolometric magnitude and the converted luminosity function. The vertical scale of the LF is arbitrary (it is the scale used on the figure). The conversion between the HST and bolometric magnitudes uses a spline fit of the theoretical models of Baraffe et al. (1997A&A...327.1054B), for the appropriate metallicities. The name of the cluster and of the observational paper main authors are given as a header, followed by the magnitudes description and the data.1997A&A...328...83Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/328/83CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/328/83https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/328/83http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/328/83https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/328/83https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/328/83http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/328/83GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/328/83/tablesBolometric luminosity functionrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameGlobular cluster namemeta.id;meta.maincharRefReferences to the observational paper (1)meta.refcharn_magHST magnitude band (I814, V555 or V606)meta.notecharmagMagnitude in band specified by n_magmagphot.magfloatMbolBolometric magnitudemagphot.mag.bolfloatlog(LF)Luminosity function (stellar density as a function of bolometric magnitude) in log scalelog(count.mag**-1)phys.luminosity.funfloat