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J/A+A/328/83        Globular clusters luminosity function   (Chabrier+ 1997)

Determination of the globular cluster and halo stellar mass functions and stellar and brown dwarf densities Chabrier G., Mera D. <Astron. Astrophys. 328, 83 (1997)> =1997A&A...328...83C (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, globular ; Magnitudes ; Stars, M-type Keywords: stars: low-mass, brown dwarfs - stars: luminosity function, mass function - Galaxy : stellar content - cosmology : dark matter Description: 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. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tables 40 234 Bolometric luminosity function
Byte-by-byte Description of file: tables
Bytes Format Units Label Explanations
1- 8 A8 --- Name Globular cluster name 10- 11 A2 --- Ref References to the observational paper (1) 13- 16 A4 --- n_mag HST magnitude band (I814, V555 or V606) 18- 24 F7.4 mag mag Magnitude in band specified by n_mag 26- 32 F7.4 mag Mbol Bolometric magnitude 34- 40 F7.4 [ct/mag] log(LF) Luminosity function (stellar density as a function of bolometric magnitude) in log scale
Note (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)
Acknowledgements: Dominique Mera
(End) Patricia Bauer [CDS] 14-Oct-1997
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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