Table C.1
Differential number counts for different populations.
| 150 GHz | ||||
|---|---|---|---|---|
| Flux Bin (mJy) | S2.5dN/dS, sync (Jy1.5sr−1) | S2.5dN/dS, dusty (Jy1.5sr−1) | S2.5dN/dS, dusty-cut (Jy1.5sr−1) | Effective Area (deg2) |
| 8 – 12 | 0.30 ± 0.10 | 0.15 ± 0.05 | 0.08 ± 0.03 | 299 |
| 12 – 16 | 1.50 ± 0.20 | 0.21 ± 0.08 | 0.14 ± 0.07 | 453 |
| 16 – 22 | 2.90 ± 0.40 | 0.10 ± 0.07 | 0.10 ± 0.07 | 555 |
| 22 – 32 | 4.30 ± 0.50 | 0.13 ± 0.09 | 593 | |
| 32 – 46 | 5.30 ± 0.80 | 595 | ||
| 46 – 80 | 5.20 ± 0.90 | 595 | ||
| 80 – 120 | 9.20 ± 2.00 | 595 | ||
| 120 – 240 | 7.00 ± 2.10 | 595 | ||
| 240 – 800 | 7.70 ± 3.80 | 595 | ||
| 800 – 1750 | 21.30 ± 15.10 | 595 | ||
| 220 GHz | ||||
| Flux Bin | S2.5dN/dS, sync | S2.5dN/dS, dusty | S2.5dN/dS, dusty-cut | Effective Area |
| (mJy) | (Jy1.5sr−1) | (Jy1.5sr−1) | (Jy1.5sr−1) | (deg2) |
| 10-14 | 2.1 ± 0.2 | 3.2 ± 0.3 | 2.8 ± 0.2 | 138 |
| 14 – 19 | 2.1 ± 0.3 | 2.1 ± 0.3 | 1.7 ± 0.3 | 330 |
| 19 – 27 | 2.3 ± 0.4 | 1.7 ± 0.3 | 0.5 ± 0.2 | 490 |
| 27 – 37 | 4.0 ± 0.6 | 1.2 ± 0.4 | 0.6 ± 0.3 | 585 |
| 37 – 51 | 2.9 ± 0.7 | 1.1 ± 0.4 | 0.6 ± 0.3 | 595 |
| 51 -70 | 4.2 ± 1.1 | 0.8 ± 0.5 | 0.5 ± 0.4 | 595 |
| 70 – 120 | 5.2 ± 1.3 | 0.9 ± 0.5 | 595 | |
| 120 – 200 | 5.6 ± 2.0 | 595 | ||
| 200 – 700 | 6.0 ± 3.0 | 595 | ||
| 700 – 1700 | 8.7 ± 8.7 | 595 | ||
| 280 GHz | ||||
| Flux Bin | S2.5dN/dS, sync | S2.5dN/dS, dusty | S2.5dN/dS, dusty-cut | Effective Area |
| (mJy) | (Jy1.5sr−1) | (Jy1.5sr−1) | (Jy1.5sr−1) | (deg2) |
| 20.0 – 24.0 | 2.4 ± 0.5 | 12.8 ± 1.2 | 11.2 ± 1.1 | 105 |
| 24.0 – 32.0 | 2.1 ± 0.5 | 5.0 ± 0.7 | 4.1 ± 0.6 | 222 |
| 32.0 – 55.0 | 2.8 ± 0.5 | 2.8 ± 0.5 | 1.5 ± 0.4 | 468 |
| 55.0 – 92.0 | 4.1 ± 1.0 | 2.9 ± 0.8 | 1.7 ± 0.6 | 545 |
| 92.0 – 160.0 | 5.0 ± 1.6 | 1.5 ± 0.9 | 1.5 ± 0.9 | 546 |
| 160.0 – 600.0 | 6.1 ± 2.7 | 546 | ||
| 600.0 – 1400.0 | 7.5 ± 7.5 | 546 | ||
Notes. The dusty-cut sample does not include sources with IRAS counterparts, effectively removing nearby luminous infrared galaxies. These number counts come from a combination of three fields: coaddL, coaddR and s2 excluding the coaddL patch. The fields encompass an area of 160, 147 and 288 sq deg, respectively; thus the full area is 595 sq deg (except for 280 GHz where the s2 field is smaller by 49 sq deg). The effective area of each flux bin is proportional to the completeness value at the center of the bin. This entry is only informative since the calculation is done using individual fluxes from sources.
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