Table 5: The instantaneous number of events in pixel lensing observations towards the M 31 galaxy for different locations of sources and lenses is shown (for details see text). Numbers in brackets refer to the South Semisphere of M 31. For the MW disk and halo, lenses in the South Semisphere of the MW contribute to roughly one half of the total and so the corresponding event numbers are not given.
Model $\langle u_{\rm T}^{~2} \rangle _{\phi}$ Bulge Disk M 31 halo M 31 overall Stellar M 31 halo 23

Massive halo
$9.56\times 10^{-3}$ 0.74 0.57 2.25 3.56 0.68/0.63(1.08) 1.52/0.73(2.09) 1.16/0.42(2.74)
Massive bulge   2.22 2.87 1.37 6.45 1.74/3.34(0.52) 0.83/0.54(1.55) 0.41/0.17(2.46)
Massive disk   0.74 3.35 0.98 5.07 1.32/2.77(0.48) 0.64/0.34(1.86) 0.49/0.21(2.29)
Reference   0.70 0.90 1.78 3.37 0.69/0.90(0.77) 1.21/0.57(2.11) 0.89/0.31(2.89)

Massive halo
$1.17\times 10^{-3}$ 0.08 0.05 1.34 1.47 0.09/0.05(1.84) 0.95/0.39(2.47) 0.85/0.30(2.82)
Massive bulge   0.20 0.20 0.67 1.08 0.18/0.22(0.82) 0.44/0.23(1.88) 0.32/0.13(2.50)
Massive disk   0.09 0.29 0.58 0.96 0.17/0.21(0.81) 0.39/0.19(2.10) 0.35/0.15(2.32)
Reference   0.08 0.07 1.04 1.19 0.09/0.07(1.32) 0.74/0.29(2.52) 0.66/0.22(2.96)


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