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.
Standard AL

Magnitude 17.5 22.5 27.5 32.5 17.5 22.5 27.5 32.5

$\langle N_{\rm WD}\rangle$ $0\pm1$ $0\pm1$ $0\pm1$ $0\pm1$ $0\pm1$ $0\pm1$ $0\pm 0$ $0\pm 0$

$\langle m \rangle$ $(M/M_{\hbox{$\odot$ }})$ 0.324 0.228 0.119 0.092 0.747 0.622 - -

$\langle\mu\rangle$ $(^{\prime\prime}~{\rm yr}^{-1})$ 0.018 0.011 0.006 0.005 0.010 0.002 - -

$\langle d\rangle$ (kpc) 2.89 4.88 8.27 10.20 5.15 17.59 - -

$\langle V_{\rm tan}\rangle$ $({\rm km~s}^{-1})$ 242 244 254 235 246 180 - -

$\langle\hat{t}_{\rm E}\rangle$ (d) 41.2 48.5 41.3 43.3 98.2 158.0 - -

$\langle \tau/\tau_0\rangle$ 0.130 0.118 0.096 0.070 0.091 0.125 - -

**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.
	Standard	AL
Magnitude	17.5	22.5	27.5	32.5	17.5	22.5	27.5	32.5
$\langle N_{\rm WD}\rangle$	$0\pm1$	$0\pm1$	$0\pm1$	$0\pm1$	$0\pm1$	$0\pm1$	$0\pm 0$	$0\pm 0$
$\langle m \rangle$ $(M/M_{\hbox{$\odot$ }})$	0.324	0.228	0.119	0.092	0.747	0.622	-	-
$\langle\mu\rangle$ $(^{\prime\prime}~{\rm yr}^{-1})$	0.018	0.011	0.006	0.005	0.010	0.002	-	-
$\langle d\rangle$ (kpc)	2.89	4.88	8.27	10.20	5.15	17.59	-	-
$\langle V_{\rm tan}\rangle$ $({\rm km~s}^{-1})$	242	244	254	235	246	180	-	-
$\langle\hat{t}_{\rm E}\rangle$ (d)	41.2	48.5	41.3	43.3	98.2	158.0	-	-
$\langle \tau/\tau_0\rangle$	0.130	0.118	0.096	0.070	0.091	0.125	-	-

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