All Tables

• Table 1: Error budget of distance moduli based on the Main Sequence Fitting Method before and after this paper.
• Table 2: Unevolved bona fide single local subdwarfs.
• Table 3: Reddening estimates for the three globular clusters.
• Table 4: Distances and ages for globular clusters.
• Table 5: Comparison with previous distance determinations using the Main Sequence Fitting method based on Hipparcos parallaxes for the local subdwarfs. Errors quoted are those given in the original papers; they have different meanings from the present error bar.
• Table 6: Comparison between our distance determinations and those from the White Dwarf cooling sequence.
• Table 7: Comparison between various determinations of the luminosity of the horizontal branch (from Cacciari & Clementini 2003).
• Table 8: Model error budget.