Table 5: Standard error on total magnitudes as a function of the flag. The first two lines give the result when there is no flag but for actual error limited to either 0.2 mag or 0.9 mag.
${\rm Flag}$ $\sigma(I)$ n $\sigma(J)$ n $\sigma(K_{\rm s})$ n

no flag 0.14 606 0.15 48439 0.25 21943

(a.e. $\leq$ 0.2)

no flag 0.15 713 0.16 148350 0.27 85380

(a.e. $\leq$ 0.9)

$f_{\rm zp}$ 0.14 44 0.16 4291 0.26 1679

$f_{\rm qlt}$ 0.14 61 0.16 4595 0.30 2782

$f_{\rm edge}$ 0.12 14 0.17 294 0.25 354

f_* 0.24 91 0.28 4249 0.36 3776

**Table 5:** Standard error on total magnitudes as a function of the flag. The first two lines give the result when there is no flag but for actual error limited to either 0.2 mag or 0.9 mag.
${\rm Flag}$	$\sigma(I)$	n	$\sigma(J)$	n	$\sigma(K_{\rm s})$	n
no flag	0.14	606	0.15	48439	0.25	21943
(a.e. $\leq$ 0.2)
no flag	0.15	713	0.16	148350	0.27	85380
(a.e. $\leq$ 0.9)
$f_{\rm zp}$	0.14	44	0.16	4291	0.26	1679
$f_{\rm qlt}$	0.14	61	0.16	4595	0.30	2782
$f_{\rm edge}$	0.12	14	0.17	294	0.25	354
f_*	0.24	91	0.28	4249	0.36	3776

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