Table 2
Differential and cumulative source number counts at 1.2 mm in GOODS-N and COSMOS.
GOODS-N | COSMOS | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
S | <N> | dN/dS | Rdif | Smin | N(>S) | Rcum | S | <N> | dN/dS | Rdif | Smin | N(>S) | Rcum |
mJy | deg−2mJy−1 | mJy | deg−2 | mJy | deg−2 mJy−1 | mJy | deg−2 | ||||||
0.66 | 10.9 | ![]() |
0.76 | 0.60 | ![]() |
0.71 | 1.75 | 24.2 | ![]() |
0 68 | 1.57 | ![]() |
0.70 |
0.81 | 13.6 | ![]() |
0.72 | 0.73 | ![]() |
0.69 | 2.12 | 31.3 | ![]() |
0 71 | 1.92 | ![]() |
0.72 |
0.98 | 14.6 | ![]() |
0.71 | 0.88 | ![]() |
0.68 | 2.57 | 31.4 | ![]() |
0 72 | 2.32 | ![]() |
0.72 |
1.19 | 13.1 | ![]() |
0.66 | 1.07 | ![]() |
0.66 | 3.12 | 24.3 | ![]() |
0 73 | 2.82 | ![]() |
0.72 |
1.44 | 11.4 | ![]() |
0.64 | 1.30 | ![]() |
0.66 | 3.79 | 15.2 | ![]() |
0 69 | 3.42 | ![]() |
0.71 |
1.75 | 8.8 | ![]() |
0.66 | 1.58 | ![]() |
0.67 | 4.59 | 5.6 | ![]() |
0 72 | 4.15 | ![]() |
0.74 |
2.12 | 8.9 | ![]() |
0.72 | 1.92 | ![]() |
0.69 | 5.58 | 2.5 | ![]() |
0 72 | 5.04 | ![]() |
0.76 |
2.57 | 6.9 | ![]() |
0.66 | 2.32 | ![]() |
0.66 | 6.76 | 3.4 | ![]() |
0 71 | 6.11 | ![]() |
0.83 |
3.12 | 3.5 | ![]() |
0.67 | 2.82 | ![]() |
0.66 | 8.21 | 1.5 | ![]() |
1.19 | 7.42 | ![]() |
0.95 |
Notes. The columns S and Smin refer to the midpoint and the lower bound flux of the flux bins used to compute the number counts. The differential and cumulative number counts are dN/dS and N(> S). Rdif and Rcum represent the source-to-galaxy counts correction factor (see Sect. 4.3). The average number of sources within each differential flux bin among the 100 Monte Carlo realizations is presented in column <N> of each field and array (see Sect. 4.1).
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