All Tables

Table 1: The different IMFs used in this paper.
Table 2: Summary of the results obtained for the simulation of microlenses towards the LMC for an age of the halo of 14 Gyr, different model IMFs, and several magnitude cuts.
Table 3: Summary results of the microlensing events towards the LMC for a limiting magnitude of $m_{\rm V}=17.5~{\rm mag}$ and different halo ages and IMFs.
Table 4: Summary of the HDF results. The authors, the selection criteria and number of objects are indicated.
Table 5: Summary of the results for the HDF obtained with our Monte Carlo simulator for the different proposed IMFs.
Table 6: Summary of the results for the EROS experiment obtained with our Monte Carlo simulator for the different proposed IMFs.
Table 7: Summary of the results obtained for the microlensing events towards the LMC when the density profile of Navarro et al. (1997) is adopted. See text for more details.
Table 8: Summary of the results obtained for a limiting magnitude of $m_{\rm V}=17.5^{\rm mag}$ and diferent values of the LMC distance and the tangential velocity.