ADF-S 24-μm number counts. Columns give upper, lower and average flux density for each bin, the observed number of sources in this flux density range, the completeness correction factor for this flux density, the Euclidean normalized corrected counts and the log of these normalized counts. Two errors are given for the counts. The first of these is the Poisson error and the second is the LSS error estimated through a counts-in-cells analysis. The LSS error is given as 0 where there are too few sources in the field to permit the counts-in-cells analysis. The two faintest data points correspond to the 80 and 50 per cent completeness levels of the catalogue, respectively.
Upper (mJy) | Lower (mJy) | Average flux density (mJy) | Observation number | Completeness | Counts (gal sr−1 Jy1.5) | log[(dN/dS)S2.5] |
1000.0 | 180.0 | 590.0 | 1 | 1.001 65 | 918 ± 918 ± 0 | 2.96a |
180.0 | 100.0 | 140.0 | 4 | 1.003 45 | 1034 ± 516 ± 0 | 3.01a |
100.0 | 64.0 | 82.0 | 6 | 1.003 69 | 905 ± 369 ± 0 | 2.96a |
64.0 | 32.0 | 48.0 | 11 | 1.003 82 | 489 ± 148 ± 391 | 2.69a |
32.0 | 20.0 | 26.0 | 26 | 1.003 91 | 666 ± 131 ± 266 | 2.82a |
20.0 | 15.0 | 17.5 | 18 | 1.003 95 | 411 ± 97 ± 82 | 2.61a |
15.0 | 10.0 | 12.5 | 61 | 1.003 97 | 601 ± 77 ± 120 | 2.78a |
10.0 | 8.0 | 9.0 | 42 | 1.003 98 | 455 ± 70 ± 228 | 2.66a |
8.0 | 7.0 | 7.5 | 26 | 1.003 99 | 357 ± 70 ± 193 | 2.55a |
7.0 | 6.0 | 6.5 | 69 | 1.003 99 | 662 ± 80 ± 345 | 2.82a |
6.0 | 5.0 | 5.5 | 91 | 1.003 99 | 576 ± 60 ± 207 | 2.76a |
5.0 | 4.0 | 4.5 | 174 | 1.004 00 | 667 ± 51 ± 160 | 2.82a |
4.0 | 3.0 | 3.5 | 290 | 1.005 50 | 593 ± 35 ± 83 | 2.77a |
3.0 | 2.6 | 2.8 | 226 | 1.008 20 | 664 ± 44 ± 173 | 2.82a |
2.6 | 2.3 | 2.45 | 193 | 1.010 30 | 542 ± 40 ± 141 | 2.73a |
2.3 | 2.0 | 2.15 | 189 | 1.012 10 | 384 ± 28 ± 38 | 2.58 |
2.0 | 1.6 | 1.80 | 444 | 1.016 20 | 436 ± 21 ± 44 | 2.64 |
1.6 | 1.3 | 1.45 | 650 | 1.021 80 | 498 ± 20 ± 40 | 2.70 |
1.3 | 1.0 | 1.15 | 1405 | 1.026 60 | 606 ± 16 ± 61 | 2.78 |
1.0 | 0.8 | 0.90 | 1907 | 1.031 00 | 671 ± 15 ± 54 | 2.82 |
0.8 | 0.6 | 0.70 | 4274 | 1.035 00 | 806 ± 12 ± 8 | 2.91 |
0.6 | 0.5 | 0.55 | 4179 | 1.047 00 | 872 ± 13 ± 35 | 2.94 |
0.5 | 0.40 | 0.45 | 7424 | 1.062 50 | 952 ± 11 ± 48 | 2.98 |
0.4 | 0.35 | 0.375 | 5785 | 1.136 00 | 1006 ± 13 ± 30 | 3.00 |
0.35 | 0.32 | 0.335 | 4424 | 1.240 00 | 1051 ± 16 ± 84 | 3.02 |
0.32 | 0.25 | 0.285 | 8140 | 2.091 50 | 937 ± 10 ± 56 | 2.97 |
Upper (mJy) | Lower (mJy) | Average flux density (mJy) | Observation number | Completeness | Counts (gal sr−1 Jy1.5) | log[(dN/dS)S2.5] |
1000.0 | 180.0 | 590.0 | 1 | 1.001 65 | 918 ± 918 ± 0 | 2.96a |
180.0 | 100.0 | 140.0 | 4 | 1.003 45 | 1034 ± 516 ± 0 | 3.01a |
100.0 | 64.0 | 82.0 | 6 | 1.003 69 | 905 ± 369 ± 0 | 2.96a |
64.0 | 32.0 | 48.0 | 11 | 1.003 82 | 489 ± 148 ± 391 | 2.69a |
32.0 | 20.0 | 26.0 | 26 | 1.003 91 | 666 ± 131 ± 266 | 2.82a |
20.0 | 15.0 | 17.5 | 18 | 1.003 95 | 411 ± 97 ± 82 | 2.61a |
15.0 | 10.0 | 12.5 | 61 | 1.003 97 | 601 ± 77 ± 120 | 2.78a |
10.0 | 8.0 | 9.0 | 42 | 1.003 98 | 455 ± 70 ± 228 | 2.66a |
8.0 | 7.0 | 7.5 | 26 | 1.003 99 | 357 ± 70 ± 193 | 2.55a |
7.0 | 6.0 | 6.5 | 69 | 1.003 99 | 662 ± 80 ± 345 | 2.82a |
6.0 | 5.0 | 5.5 | 91 | 1.003 99 | 576 ± 60 ± 207 | 2.76a |
5.0 | 4.0 | 4.5 | 174 | 1.004 00 | 667 ± 51 ± 160 | 2.82a |
4.0 | 3.0 | 3.5 | 290 | 1.005 50 | 593 ± 35 ± 83 | 2.77a |
3.0 | 2.6 | 2.8 | 226 | 1.008 20 | 664 ± 44 ± 173 | 2.82a |
2.6 | 2.3 | 2.45 | 193 | 1.010 30 | 542 ± 40 ± 141 | 2.73a |
2.3 | 2.0 | 2.15 | 189 | 1.012 10 | 384 ± 28 ± 38 | 2.58 |
2.0 | 1.6 | 1.80 | 444 | 1.016 20 | 436 ± 21 ± 44 | 2.64 |
1.6 | 1.3 | 1.45 | 650 | 1.021 80 | 498 ± 20 ± 40 | 2.70 |
1.3 | 1.0 | 1.15 | 1405 | 1.026 60 | 606 ± 16 ± 61 | 2.78 |
1.0 | 0.8 | 0.90 | 1907 | 1.031 00 | 671 ± 15 ± 54 | 2.82 |
0.8 | 0.6 | 0.70 | 4274 | 1.035 00 | 806 ± 12 ± 8 | 2.91 |
0.6 | 0.5 | 0.55 | 4179 | 1.047 00 | 872 ± 13 ± 35 | 2.94 |
0.5 | 0.40 | 0.45 | 7424 | 1.062 50 | 952 ± 11 ± 48 | 2.98 |
0.4 | 0.35 | 0.375 | 5785 | 1.136 00 | 1006 ± 13 ± 30 | 3.00 |
0.35 | 0.32 | 0.335 | 4424 | 1.240 00 | 1051 ± 16 ± 84 | 3.02 |
0.32 | 0.25 | 0.285 | 8140 | 2.091 50 | 937 ± 10 ± 56 | 2.97 |
aIndicates flux range where the cluster galaxies are likely to have increased the counts significantly above the field value.
ADF-S 24-μm number counts. Columns give upper, lower and average flux density for each bin, the observed number of sources in this flux density range, the completeness correction factor for this flux density, the Euclidean normalized corrected counts and the log of these normalized counts. Two errors are given for the counts. The first of these is the Poisson error and the second is the LSS error estimated through a counts-in-cells analysis. The LSS error is given as 0 where there are too few sources in the field to permit the counts-in-cells analysis. The two faintest data points correspond to the 80 and 50 per cent completeness levels of the catalogue, respectively.
Upper (mJy) | Lower (mJy) | Average flux density (mJy) | Observation number | Completeness | Counts (gal sr−1 Jy1.5) | log[(dN/dS)S2.5] |
1000.0 | 180.0 | 590.0 | 1 | 1.001 65 | 918 ± 918 ± 0 | 2.96a |
180.0 | 100.0 | 140.0 | 4 | 1.003 45 | 1034 ± 516 ± 0 | 3.01a |
100.0 | 64.0 | 82.0 | 6 | 1.003 69 | 905 ± 369 ± 0 | 2.96a |
64.0 | 32.0 | 48.0 | 11 | 1.003 82 | 489 ± 148 ± 391 | 2.69a |
32.0 | 20.0 | 26.0 | 26 | 1.003 91 | 666 ± 131 ± 266 | 2.82a |
20.0 | 15.0 | 17.5 | 18 | 1.003 95 | 411 ± 97 ± 82 | 2.61a |
15.0 | 10.0 | 12.5 | 61 | 1.003 97 | 601 ± 77 ± 120 | 2.78a |
10.0 | 8.0 | 9.0 | 42 | 1.003 98 | 455 ± 70 ± 228 | 2.66a |
8.0 | 7.0 | 7.5 | 26 | 1.003 99 | 357 ± 70 ± 193 | 2.55a |
7.0 | 6.0 | 6.5 | 69 | 1.003 99 | 662 ± 80 ± 345 | 2.82a |
6.0 | 5.0 | 5.5 | 91 | 1.003 99 | 576 ± 60 ± 207 | 2.76a |
5.0 | 4.0 | 4.5 | 174 | 1.004 00 | 667 ± 51 ± 160 | 2.82a |
4.0 | 3.0 | 3.5 | 290 | 1.005 50 | 593 ± 35 ± 83 | 2.77a |
3.0 | 2.6 | 2.8 | 226 | 1.008 20 | 664 ± 44 ± 173 | 2.82a |
2.6 | 2.3 | 2.45 | 193 | 1.010 30 | 542 ± 40 ± 141 | 2.73a |
2.3 | 2.0 | 2.15 | 189 | 1.012 10 | 384 ± 28 ± 38 | 2.58 |
2.0 | 1.6 | 1.80 | 444 | 1.016 20 | 436 ± 21 ± 44 | 2.64 |
1.6 | 1.3 | 1.45 | 650 | 1.021 80 | 498 ± 20 ± 40 | 2.70 |
1.3 | 1.0 | 1.15 | 1405 | 1.026 60 | 606 ± 16 ± 61 | 2.78 |
1.0 | 0.8 | 0.90 | 1907 | 1.031 00 | 671 ± 15 ± 54 | 2.82 |
0.8 | 0.6 | 0.70 | 4274 | 1.035 00 | 806 ± 12 ± 8 | 2.91 |
0.6 | 0.5 | 0.55 | 4179 | 1.047 00 | 872 ± 13 ± 35 | 2.94 |
0.5 | 0.40 | 0.45 | 7424 | 1.062 50 | 952 ± 11 ± 48 | 2.98 |
0.4 | 0.35 | 0.375 | 5785 | 1.136 00 | 1006 ± 13 ± 30 | 3.00 |
0.35 | 0.32 | 0.335 | 4424 | 1.240 00 | 1051 ± 16 ± 84 | 3.02 |
0.32 | 0.25 | 0.285 | 8140 | 2.091 50 | 937 ± 10 ± 56 | 2.97 |
Upper (mJy) | Lower (mJy) | Average flux density (mJy) | Observation number | Completeness | Counts (gal sr−1 Jy1.5) | log[(dN/dS)S2.5] |
1000.0 | 180.0 | 590.0 | 1 | 1.001 65 | 918 ± 918 ± 0 | 2.96a |
180.0 | 100.0 | 140.0 | 4 | 1.003 45 | 1034 ± 516 ± 0 | 3.01a |
100.0 | 64.0 | 82.0 | 6 | 1.003 69 | 905 ± 369 ± 0 | 2.96a |
64.0 | 32.0 | 48.0 | 11 | 1.003 82 | 489 ± 148 ± 391 | 2.69a |
32.0 | 20.0 | 26.0 | 26 | 1.003 91 | 666 ± 131 ± 266 | 2.82a |
20.0 | 15.0 | 17.5 | 18 | 1.003 95 | 411 ± 97 ± 82 | 2.61a |
15.0 | 10.0 | 12.5 | 61 | 1.003 97 | 601 ± 77 ± 120 | 2.78a |
10.0 | 8.0 | 9.0 | 42 | 1.003 98 | 455 ± 70 ± 228 | 2.66a |
8.0 | 7.0 | 7.5 | 26 | 1.003 99 | 357 ± 70 ± 193 | 2.55a |
7.0 | 6.0 | 6.5 | 69 | 1.003 99 | 662 ± 80 ± 345 | 2.82a |
6.0 | 5.0 | 5.5 | 91 | 1.003 99 | 576 ± 60 ± 207 | 2.76a |
5.0 | 4.0 | 4.5 | 174 | 1.004 00 | 667 ± 51 ± 160 | 2.82a |
4.0 | 3.0 | 3.5 | 290 | 1.005 50 | 593 ± 35 ± 83 | 2.77a |
3.0 | 2.6 | 2.8 | 226 | 1.008 20 | 664 ± 44 ± 173 | 2.82a |
2.6 | 2.3 | 2.45 | 193 | 1.010 30 | 542 ± 40 ± 141 | 2.73a |
2.3 | 2.0 | 2.15 | 189 | 1.012 10 | 384 ± 28 ± 38 | 2.58 |
2.0 | 1.6 | 1.80 | 444 | 1.016 20 | 436 ± 21 ± 44 | 2.64 |
1.6 | 1.3 | 1.45 | 650 | 1.021 80 | 498 ± 20 ± 40 | 2.70 |
1.3 | 1.0 | 1.15 | 1405 | 1.026 60 | 606 ± 16 ± 61 | 2.78 |
1.0 | 0.8 | 0.90 | 1907 | 1.031 00 | 671 ± 15 ± 54 | 2.82 |
0.8 | 0.6 | 0.70 | 4274 | 1.035 00 | 806 ± 12 ± 8 | 2.91 |
0.6 | 0.5 | 0.55 | 4179 | 1.047 00 | 872 ± 13 ± 35 | 2.94 |
0.5 | 0.40 | 0.45 | 7424 | 1.062 50 | 952 ± 11 ± 48 | 2.98 |
0.4 | 0.35 | 0.375 | 5785 | 1.136 00 | 1006 ± 13 ± 30 | 3.00 |
0.35 | 0.32 | 0.335 | 4424 | 1.240 00 | 1051 ± 16 ± 84 | 3.02 |
0.32 | 0.25 | 0.285 | 8140 | 2.091 50 | 937 ± 10 ± 56 | 2.97 |
aIndicates flux range where the cluster galaxies are likely to have increased the counts significantly above the field value.
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