J/A+A/328/83 J/A+A/328/83 Globular clusters luminosity function G Chabrier D Mera Astron. Astrophys. 328 83 1997 1997A&A...328...83C Clusters, globular Magnitudes Stars, M-type dark matter Galaxy: stellar content stars: low-mass, brown dwarfs stars: luminosity function, mass function Data 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.

Name Globular cluster name --- Ref References to the observational paper number=1 MP : De Marchi and Paresce (1995A&A...304..211D) S : Santiago et al. (1996MNRAS.281.1363S) FP : Fusi-Pecci et al. (1996, preprint) E : Elson et al. (1995AJ....110..682E) P : Paresce et al. (1995ApJ...442L..57P) C : Cool et al. (1996ApJ...468..655C) M : Mould (1996PASP..108..682M) --- n_mag HST magnitude band (I814, V555 or V606) --- mag Magnitude in band specified by n_mag mag Mbol Bolometric magnitude mag log(FL) Luminosity function (stellar density as a function of bolometric magnitude) in log scale --- Patricia Bauer CDS 1997Oct14Dominique Mera <dmera@cral.ens-lyon.fr> J_A+A_328_83.xml