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Table 3

Differential source counts of MALS, including corrected counts using RMS coverage, completeness of unresolved sources, and completeness of resolved sources.

S (mJy) Smean (mJy) N Nfalse Sky coverage (sq. deg.) (Jy3/2 sr−1) Corrected RMS coverage (Jy3/2 sr−1) Corrected Completeness (Jy3/2 sr−1) fn SKADS
0.1−0.13 0.11 850 ± 33 4 2.2 0.377 ± 0.015 6.06 ± 0.24 2.90 ± 0.11 0.0
0.13−0.17 0.15 1254 ± 43 11 5.3 0.816 ± 0.028 5.51 ± 0.19 3.93 ± 0.13 0.0
0.17−0.22 0.19 1575 ± 51 13 8.7 1.50 ± 0.05 6.16 ± 0.20 5.23 ± 0.15 0.0
0.22−0.28 0.25 1708 ± 54 12 12.5 2.39 ± 0.076 6.82 ± 0.22 6.47 ± 0.18 0.0
0.28−0.36 0.32 1558 ± 50 20 16.6 3.20 ± 0.10 6.89 ± 0.22 6.91 ± 0.19 0.0
0.36−0.46 0.41 1393 ± 46 22 20.9 4.21 ± 0.14 7.18 ± 0.24 7.58 ± 0.21 0.0
0.46−0.6 0.53 1257 ± 43 19 25.4 5.57 ± 0.19 7.83 ± 0.27 8.76 ± 0.25 0.0
0.6−0.77 0.69 1053 ± 38 15 23.3 6.85 ± 0.25 10.5 ± 0.4 9.67 ± 0.30 0.0
0.77−1 0.89 881 ± 34 16 31.6 8.41 ± 0.33 9.49 ± 0.37 11.1 ± 0.4 0.0
1−1.3 1.1 769 ± 31 10 30.9 10.8 ± 0.5 12.5 ± 0.5 13.4 ± 0.5 0.0
1.3−1.7 1.5 635 ± 28 7 34.4 13.1 ± 0.6 13.6 ± 0.6 15.5 ± 0.6 0.0
1.7−2.2 1.9 503 ± 24 4 35.0 15.2 ± 0.7 15.5 ± 0.8 17.3 ± 0.8 0.0
2.2−2.8 2.5 411 ± 21 7 35.3 18.2 ± 1.0 18.4 ± 1.0 20.3 ± 1.0 0.0
2.8−3.6 3.2 318 ± 18 2 35.5 20.7 ± 1.2 20.8 ± 1.2 22.5 ± 1.3 0.0
3.6−4.6 4.1 307 ± 18 3 35.6 29.3 ± 1.8 29.4 ± 1.8 31.3 ± 1.8 0.01
4.6−6 5.3 232 ± 15 6 35.7 32.5 ± 2.2 32.5 ± 2.2 34.3 ± 2.3 0.02
6−7.7 6.9 199 ± 14 1 35.7 40.9 ± 3.0 40.9 ± 3.0 42.7 ± 3.0 0.07
7.7−10 8.9 160 ± 13 1 35.7 48.3 ± 3.9 48.3 ± 4.0 49.6 ± 4.0 0.11
10−13 11 137 ± 12 1 35.7 60.7 ± 5.3 60.7 ± 5.3 60.7 ± 5.3 0.16
13−17 15 136 ± 11 0 35.7 88.5 ± 7.8 88.5 ± 7.8 88.5 ± 7.8 0.22
17−22 19 84 ± 9 1 35.7 80.2 ± 8.9 80.2 ± 8.9 80.2 ± 8.9 0.32
22−28 25 100 ± 10 0 35.7 140 ± 14 140 ± 14 140 ± 14 0.5
28−36 32 48 ± 6 0 35.7 98.7 ± 14.4 98.7 ± 14.4 98.7 ± 14.4 0.5
36−46 41 50 ± 7 0 35.7 151 ± 22 151 ± 23 151 ± 22 0.47
46−60 53 36 ± 6 0 35.7 160 ± 27 160 ± 27 160 ± 27 0.63
60−77 69 34 ± 5 0 35.7 221 ± 38 221 ± 38 221 ± 38 0.73
77−100 89 24 ± 4 0 35.7 229 ± 47 229 ± 47 229 ± 47 0.82
100−130 110 21 ± 4 0 35.7 294 ± 65 294 ± 65 294 ± 65 0.93
130−170 150 19 ± 4 0 35.7 391 ± 90 391 ± 90 391 ± 90 1.0
170−220 190 13 ± 3 0 35.7 392 ± 109 392 ± 109 392 ± 109 0.67
220−280 250 10 ± 3 0 35.7 443 ± 140 443 ± 140 443 ± 140 0.75
280−360 320 10 ± 3 0 35.7 650 ± 206 650 ± 206 650 ± 206 0.89
360−460 410 9 ± 3 0 35.7 859 ± 287 859 ± 287 859 ± 287 1.9
460−600 530 6 ± 2 0 35.7 841 ± 344 841 ± 344 841 ± 344 0.75
600−770 690 5 ± 2 0 35.7 1030 ± 460 1030 ± 460 1030 ± 460 0.5
770−1000 890 3 ± 1 0 35.7 906 ± 523 906 ± 523 906 ± 523 1.5
1000−1300 1100 4 ± 2 0 35.7 1770 ± 890 1770 ± 890 1770 ± 890 1.2
1300−1700 1500 1 ± 1 0 35.7 650 ± 650 650 ± 650 650 ± 650 0.75
1700−2200 1900 1 ± 1 0 35.7 955 ± 955 955 ± 955 955 ± 955 0.0

Notes. Counts are normalised for the sky area of 35.7 degrees. Raw counts (N) and number of false detections in (Nfalse) per bin are also given. The excess fraction of sources due to separated components fn is also given, based on a separation distance of 6.5″ of FRII sources in SKADS.

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