Table 2.
Best-fit values of the parameterised angular two-point correlation, the clustering length, and medium sample redshift.
Smin | A | γ − 1 | wΩ | χ2/d.o.f. | N | r0(ϵ = γ − 3) | r0(ϵ = 0) | r0(ϵ = γ − 1) | zmedian |
---|---|---|---|---|---|---|---|---|---|
[mJy] | ( × 10−3) | ( × 10−3) | [h−1Mpc] | [h−1Mpc] | [h−1Mpc] | ||||
1 | 1.9 | 5.78 | 40 599 | 10.9 ± 2.8 | 14.2 ± 2.5 | 15.8 ± 2.9 | 0.92 | ||
2 | 1.2 | 2.70 | 19 719 | 10.1 ± 2.6 | 13.3 ± 2.1 | 15.1 ± 2.5 | 0.96 | ||
4 | 3.0 | 2.34 | 11 269 | 9.5 ± 2.8 | 16.0 ± 3.1 | 18.3 ± 3.9 | 0.99 | ||
8 | 1.4 | 1.86 | 3430 | 13.3 ± 5.2 | 17.6 ± 6.1 | 20.8 ± 7.4 | 0.99 |
Notes. The angular two-point correlation is parameterised as w(θ) = A(θ/1 deg)1 − γ. We report A and γ, as well as the integral constraint (wΩ) for the LoTSS-DR1 value-added source catalogue after appropriate masking (mask 1) in the fit range 0.2 deg ≤θ ≤ 2 deg and for four flux density thresholds. The corresponding clustering length r0 is shown for ϵ = γ − 3, ϵ = 0 and ϵ = γ − 1. The best-fit values for A and γ for 1, 2 and 4 mJy were already reported in Siewert et al. (2020). All reported uncertainties are 68% confidence intervals. We also report the median of the weighted posterior redshift distribution at the corresponding flux threshold, respectively.
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