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.
Standard AL

Magnitude 17.5 22.5 27.5 32.5 17.5 22.5 27.5 32.5

$\langle N_{\rm WD}\rangle$ $0\pm1$ $0\pm1$ $0\pm1$ $0\pm1$ $3\pm2$ $2\pm1$ $1\pm1$ $0\pm1$

$\langle m \rangle$ $(M/M_{\hbox{$\odot$ }})$ 0.421 0.411 0.427 0.443 0.638 0.636 0.640 0.684

$\langle\mu\rangle$ $(^{\prime\prime}~{\rm yr}^{-1})$ 0.020 0.017 0.008 0.004 0.036 0.025 0.011 0.003

$\langle {\rm d}\rangle$ (kpc) 2.48 3.79 6.62 13.08 1.39 2.15 5.13 19.6

$\langle V_{\rm tan}\rangle$ $({\rm km~s}^{-1})$ 240 247 262 241 240 252 263 261

$\langle\hat{t}_{\rm E}\rangle$ (d) 41.2 49.3 63.3 82.8 34.7 46.6 76.4 126.8

$\langle \tau/\tau_0\rangle$ 0.283 0.214 0.139 0.055 0.302 0.204 0.140 0.129

**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.
	Standard	AL
Magnitude	17.5	22.5	27.5	32.5	17.5	22.5	27.5	32.5
$\langle N_{\rm WD}\rangle$	$0\pm1$	$0\pm1$	$0\pm1$	$0\pm1$	$3\pm2$	$2\pm1$	$1\pm1$	$0\pm1$
$\langle m \rangle$ $(M/M_{\hbox{$\odot$ }})$	0.421	0.411	0.427	0.443	0.638	0.636	0.640	0.684
$\langle\mu\rangle$ $(^{\prime\prime}~{\rm yr}^{-1})$	0.020	0.017	0.008	0.004	0.036	0.025	0.011	0.003
$\langle {\rm d}\rangle$ (kpc)	2.48	3.79	6.62	13.08	1.39	2.15	5.13	19.6
$\langle V_{\rm tan}\rangle$ $({\rm km~s}^{-1})$	240	247	262	241	240	252	263	261
$\langle\hat{t}_{\rm E}\rangle$ (d)	41.2	49.3	63.3	82.8	34.7	46.6	76.4	126.8
$\langle \tau/\tau_0\rangle$	0.283	0.214	0.139	0.055	0.302	0.204	0.140	0.129

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