All Tables

• Table 1: Summary of the results obtained for the entire simulated population of microlenses in the direction of the LMC for a halo age of 14 Gyr, different model initial mass functions, and several magnitude cuts.
• Table 2: Summary of the results obtained for the population of red dwarf microlenses towards the LMC for an age of the halo of 14 Gyr, different model initial mass functions, and several magnitude cuts.
• Table 3: Compatibility, as obtained using the Z² statistical test, of the observed MACHO distribution of Einstein crossing times and those of the different simulated populations.
• Table 4: Summary of the results obtained for the simulation of microlenses towards the LMC for the EROS experiment for an age of the halo of 14 Gyr, different model initial mass functions, and several magnitude cuts.