Table A.1
150 MHz normalized differential radio-source counts as derived from the Lockman Hole final catalogs.
Smin | Smax | ΔS | x | NS | ![]() |
Sys− | Sys+ | c1 | c2 |
---|---|---|---|---|---|---|---|---|---|
0.25 | 0.35 | 0.10 | 0.30 | 6673 | ![]() |
4.56 | 2.82 | 1.12 | 1.34 |
0.35 | 0.50 | 0.15 | 0.42 | 5314 | ![]() |
1.38 | 2.73 | 1.01 | 1.10 |
0.50 | 0.71 | 0.21 | 0.59 | 3545 | ![]() |
0.24 | 2.48 | 1.00 | 1.06 |
0.71 | 1.00 | 0.29 | 0.84 | 2077 | ![]() |
0.02 | 2.09 | 1.00 | 1.04 |
1.00 | 1.41 | 0.41 | 1.19 | 1119 | ![]() |
0.04 | 1.54 | 1.01 | 1.03 |
1.41 | 2.00 | 0.59 | 1.68 | 683 | ![]() |
0.00 | 1.89 | 1.01 | 1.02 |
2.00 | 2.83 | 0.83 | 2.38 | 390 | ![]() |
0.00 | 1.94 | 1.01 | 1.01 |
2.83 | 4.00 | 1.17 | 3.36 | 272 | ![]() |
0.00 | 2.77 | 1.01 | 1.01 |
4.00 | 5.66 | 1.66 | 4.76 | 184 | ![]() |
0.00 | 3.60 | 1.01 | 1.01 |
5.66 | 8.00 | 2.34 | 6.73 | 148 | ![]() |
0.00 | 4.09 | 1.01 | 1.01 |
8.00 | 11.3 | 3.30 | 9.51 | 132 | ![]() |
0.0 | 4.0 | 1.01 | 1.01 |
11.3 | 22.6 | 11.3 | 16.0 | 172 | ![]() |
0.0 | 2.3 | 1.01 | 1.01 |
22.6 | 45.3 | 22.7 | 32.0 | 128 | ![]() |
0.0 | 1.3 | 1.01 | 1.01 |
45.3 | 90.5 | 45.2 | 64.0 | 74 | ![]() |
0.2 | 2.2 | 1.01 | 1.01 |
90.5 | 181 | 90.5 | 128 | 45 | ![]() |
2.5 | 4.2 | 1.01 | 1.01 |
181 | 724 | 543 | 362 | 46 | ![]() |
3 | 15 | 1.01 | 1.01 |
724 | 2896 | 2172 | 1448 | 17 | ![]() |
18 | 86 | 1.00 | 1.00 |
Notes. Columns are as follows: Smin and Smax are the minimum and maximum flux densities (expressed in mJy), respectively; Δ denotes the flux density intervals; x is the geometric mean of Smin and Smax; NS is the number of sources in respective bins; N is the normalized source counts and σ is the Poissonian errors on thenormalized counts; Sys+ and Sys− are the systematic errors, accounting for different modeling of resolution and Eddington bias corrections (see Sects. 4 and 5 for more details); the correction factor c1 represents the weighting applied to the counts to account for resolution and Eddington biases; the correction factor c2 also includes the weighting due to the visibility function.
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