Astronomy & Astrophysics

Table 1: List of fields observed. See text for more details.
Table 2: For each field for J-band data this table lists $\rm mag_{\rm comp}$ , i.e. the center of the 0.5 mag bin where 90% of point-like sources are retrieved, $\rm mag_{\rm {lim}}$ i.e. the center of the 0.5 mag bin where 50% of sources are retrieved, and $m_{\rm {cont} < 10\%}$ , i.e. is the center of the 0.5 mag bin where contamination by spurious sources is below 10%. See text for more details.
Table 3: As for Table 2 but for K-band data. See text for more details.
Table 4: Columns 2 to 5 show, for each of our fields, the raw differential number counts per half magnitude bin. Column 6 show our raw total number densities (number 0.5 mag^-1 deg^-2). Column 7 shows our total, differential galaxy densities, corrected for star contamination and Column 8 is their $1\sigma$ error bar, obtained from the variance of the counts among the different fields.
Table 5: As in Table 4, but for K-band counts.
Table 6: Observed $\omega (\theta )$ amplitudes A, in units of 10^-4 at $1\deg$ , together with their $1\sigma$ error bars, for each of our fields and for the total sample. For each field the number of objects used in the analysis down to the K magnitude faint limits shown in the first column is also listed.