Table 4: Standard error on our magnitudes as a function of the limiting magnitudes.
$m_{\rm lim}$ $\sigma(I)$ n $\sigma(J)$ n $\sigma(K_{\rm s})$ n

10.00 - - 0.09 143 0.11 470

11.00 0.10 14 0.08 685 0.13 1766

12.00 0.10 67 0.09 2804 0.16 5517

13.00 0.11 240 0.10 9703 0.20 13790

14.00 0.12 461 0.12 25470 0.25 21943

15.00 0.14 586 0.15 48439 0.26 22959

16.00 0.14 586 0.16 53750 0.26 22961

**Table 4:** Standard error on our magnitudes as a function of the limiting magnitudes.
$m_{\rm lim}$	$\sigma(I)$	n	$\sigma(J)$	n	$\sigma(K_{\rm s})$	n
10.00	-	-	0.09	143	0.11	470
11.00	0.10	14	0.08	685	0.13	1766
12.00	0.10	67	0.09	2804	0.16	5517
13.00	0.11	240	0.10	9703	0.20	13790
14.00	0.12	461	0.12	25470	0.25	21943
15.00	0.14	586	0.15	48439	0.26	22959
16.00	0.14	586	0.16	53750	0.26	22961

Source LaTeX | All tables | In the text

	1 Introduction
	2 First reduction process and checking
	3 Recognition and photometry of galaxies
	4 Mean of different determinations
	5 Magnitudes and diameters
	6 Comparison with independent surveys
	7 Influence of flags
	8 The catalog of raw data
	References