Table 4: The same as in Table 3 for lenses located in the M 31 galaxy. In the last three columns we give the calculated pixel event number for the South/North Semisphere and in brackets their ratio.
Model $\langle u_{\rm T} \rangle
_{\phi}$ Bulge Disk M 31 halo M 31 overall Stellar M 31 halo 23

Massive halo
$5.10\times 10^{-2}$ 27.7 27.7 36.1 91.5 31.4/24.0(1.3) 25.3/10.8(2.3) 19.6/5.8(3.4)
Massive bulge   78.6 121.4 18.7 218.7 72.6/127.4(0.6) 11.3/7.4(1.5) 6.0/2.4(2.5)
Massive disk   27.9 162.0 13.9 203.8 85.5/104.5(0.8) 9.2/4.7(1.9) 7.2/2.9(2.5)
Reference   25.9 42.4 28.4 96.7 33.9/34.4(1.0) 19.6/8.9(2.2) 14.9/4.6(3.2)

Reference
$1.4\times 10^{-2}$ 7.1 11.5 7.7 26.3 9.3/9.4(1.0) 5.3/2.4(2.2) 4.0/1.2(3.2)


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