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Table 2

1.34 GHz source counts as derived from our survey.

ΔS (mJy) (1) 〈S〉 (mJy) (2) Ns (3) dN/dS S2.5 (sr−1 Jy1.5) (4) σ (5) σ+ (6) Sys (7) Sys+ (8) dNuncorr/dSS2.5 (sr−1Jy1.5) (9)
0.019 − 0.027 0.023 207 2.89 0.20 0.21 0.27 0.16 0.82
0.027 − 0.038 0.032 297 3.79 0.22 0.23 0.43 0.26 2.38
0.038 − 0.054 0.045 279 4.69 0.28 0.30 0.28 0.48 3.9
0.054 − 0.077 0.065 209 5.64 0.39 0.42 0.44 0.63 5.03
0.077 − 0.109 0.091 121 5.32 0.48 0.53 0.37 0.61 4.89
0.109 − 0.154 0.129 73 5.48 0.64 0.72 0.37 0.66 5.05
0.154 − 0.217 0.183 40 4.94 0.78 0.91 0.19 0.67 5.53
0.217 − 0.307 0.258 21 4.34 0.95 1.15 0.34 0.50 3.99
0.307 − 0.435 0.365 15 5.21 1.34 1.69 1.29 0.63 3.91
0.435 − 0.615 0.517 12 7.14 2.06 2.66 0.36 1.80 8.93
0.615 − 1.229 0.869 8 5.02 1.78 2.40 0.98 0.58 4.04
1.229 − 2.459 1.739 7 12.68 4.79 6.60 0.67 1.96 12.9
2.459 − 4.918 3.477 6 30.03 12.26 17.27 5.78 3.66 24.25
4.918 − 19.670 9.835 3 34.82 18.92 33.89 2.17 4.87 34.29
19.670 − 78.680 39.340 2 177.1 114.2 233.8 100.2 21.77 76.89

Notes. (1) Flux density interval. (2) Geometric mean of the flux density. (3) Number of sources detected. (4) Differential counts normalized to a non-evolving Euclidean model. (5) and (6) Poissonian errors on the normalized counts. (7) and (8) Systematic errors, accounting for different modeling of resolution and Eddington bias corrections (see Sects. 3.5 and 3.6 for more details). (9) Normalized differential counts before applying the corrections for the visibility function and for the systematic effects discussed in Sect. 3.

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