Table 2: Differential number counts in the SWAN fields. The raw number of detected galaxies is reported in (2). In (3) the corrected number counts ( $\textrm {N}\ \textrm {mag}^{-1}\ \textrm {deg}^{-2}$) for the whole sample are shown, while (4) and (5) separate late-type and early-type counts, respectively.

Mag($K_{\rm s}$)		 $n_{\rm raw}$ $N_{\rm tot}$ Late-type Early-type
(1) (2) (3) (4) (5)

14		 3 7e + 02 2e + 02 5e + 02
15 8 1.9e + 03 5e + 02 1.4e + 03
16 8 1.8e + 03 1.4e + 03 4e + 02
17 19 4e + 03 1.4e + 03 3.0e + 03
18 62 1.5e + 04 4.9e + 03 9e + 03
19 69 1.6e + 04 9e + 03 7.8e + 03
20 96 2.8e + 04 2.0e + 04 8.7e + 03
21 67 4.8e + 04 4.1e + 04 6.8e + 03
22 35 9.8 + 04 9.3e + 04 4.4e + 04


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