Table 1: The Galactic coordinates of the five fields investigated so far, and the number of stars per field, $R\leq 23$ .
CADIS field l b $N_{\rm stars}$

1 h $150^\circ$ $-59^\circ$ 200

9 h $175^\circ$ $45^\circ$ 300

13 h $335^\circ$ $60^\circ$ 517

16 h $85^\circ$ $45^\circ$ 390

23 h $90^\circ$ $-43^\circ$ 220

**Table 1:** The Galactic coordinates of the five fields investigated so far, and the number of stars per field, $R\leq 23$ .
CADIS field	l	b	$N_{\rm stars}$
1 h	$150^\circ$	$-59^\circ$	200
9 h	$175^\circ$	$45^\circ$	300
13 h	$335^\circ$	$60^\circ$	517
16 h	$85^\circ$	$45^\circ$	390
23 h	$90^\circ$	$-43^\circ$	220

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