Table 3: The exponent $\alpha$ from equation (5), for a flattened halo with an axis ratio of c/a=0.6, and for c/a=1.0 (no flattening). The numbers in brackets are the corresponding $\chi ^2$ values.
CADIS field $\alpha(c/a=0.6)$ $\alpha(c/a=1.0)$

1 h $2.36\pm0.14(1.37)$ $2.8\pm0.16 (1.05)$

9 h $0.44\pm0.08(13.99)$ $0.5\pm0.1 (13.68)$

13 h $1.50\pm0.09(3.13)$ $1.98\pm0.09 (1.54)$

16 h $2.84\pm0.14(3.24)$ $3.52\pm0.18 (1.65)$

23 h $2.98\pm0.18(11.81)$ $3.68\pm0.22 (7.01)$

**Table 3:** The exponent $\alpha$ from equation (5), for a flattened halo with an axis ratio of c/a=0.6, and for c/a=1.0 (no flattening). The numbers in brackets are the corresponding $\chi ^2$ values.
CADIS field	$\alpha(c/a=0.6)$	$\alpha(c/a=1.0)$
1 h	$2.36\pm0.14(1.37)$	$2.8\pm0.16 (1.05)$
9 h	$0.44\pm0.08(13.99)$	$0.5\pm0.1 (13.68)$
13 h	$1.50\pm0.09(3.13)$	$1.98\pm0.09 (1.54)$
16 h	$2.84\pm0.14(3.24)$	$3.52\pm0.18 (1.65)$
23 h	$2.98\pm0.18(11.81)$	$3.68\pm0.22 (7.01)$

Source LaTeX | All tables | In the text

	1 Introduction
	2 The Calar Alto Deep Imaging Survey
	3 The stellar density distribution
	4 Star counts - a direct measurement
	5 A Monte Carlo model of the Milky Way
	6 Summary and discussion
	References