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Table 1.

Power-law cross-correlation amplitudes and slopes for the analysed samples.

Inner (0.1 < rp < 1 h−1 Mpc) Outer (1 < rp < 10 h−1 Mpc)

Sample M, P Acc α A cc f $ A_{\mathrm{cc}}^{f} $ Acc α A cc f $ A_{\mathrm{cc}}^{f} $
LERG 11.36 133.1 ± 4.9 −1.08 ± 0.07 114.4 ± 4.95 −0.76 ± 0.08
HERG 11.13 73.6 ± 18.8 −0.94 ± 0.52 75.6 ± 20.4 −0.65 ± 0.6
Control LERG (CSL) 11.33 115.2 ± 2.3 −0.89 ± 0.04 104.3 ± 2.1 −0.79 ± 0.04
Control HERG (CSH) 11.11 64.3 ± 8.2 −0.82 ± 0.27 80.1 ± 9.4 −0.81 ± 0.26
Control HERG (CSHL) 11.17 124.3 ± 52.6 −0.98 ± 0.23 94.2 ± 38.2 −0.71 ± 0.21

LERG M1 10.99 108.2 ± 8.3 −1.04 ± 0.14 104.1 ± 8.06 98.6 ± 8.87 −0.78 ± 0.16 96.6 ± 8.7
LERG M2 11.36 137.7 ± 6.6 −1.10 ± 0.09 140.8 ± 6.80 118.0 ± 6.3 −0.75 ± 0.11 119.8 ± 6.4
LERG M3 11.63 208.2 ± 13.8 −1.10 ± 0.14 212.7 ± 14.1 162.7 ± 12.5 −0.77 ± 0.16 160.9 ± 12.3

HERG M1 10.91 73.2 ± 21.2 −0.91 ± 0.55 70.9 ± 20.5 86.7 ± 27.2 −0.69 ± 0.7 84.0 ± 26.4
HERG M2 11.38 58.1 ± 28.2 −1.42 ± 1.01 92.3 ± 44.7 41.7 ± 25.2 −0.53 ± 1.2 47.1 ± 28.4

LERG P1 23.17 111 ± 5.6 −1.1 ± 0.09 114.1 ± 5.76 103 ± 6.2 −0.75 ± 0.11 104.4 ± 6.3
LERG P2 23.96 183.9 ± 10.5 −1.03 ± 0.11 175.6 ± 10.0 139.9 ± 8.6 −0.79 ± 0.12 135.8 ± 8.3
LERG P3 24.72 213.4 ± 23 −1.05 ± 0.23 209 ± 22.5 153.8 ± 17.4 −0.78 ± 0.23 151.8 ± 17.4
HERG P1 23.27 59.3 ± 23.8 −0.99 ± 0.76 63 ± 25.4 74.6 ± 25.9 −0.59 ± 0.8 79.3 ± 27.6
HERG P2 24.77 99.3 ± 38.9 −0.97 ± 0.79 102.1 ± 40 77.9 ± 38.4 −0.8 ± 1.0 67.7 ± 33.4

Unclass. (UNC) 10.95 68.9 ± 5.2 −0.67 ± 0.14 71.0 ± 5.8 −0.93 ± 0.18
Unclass. AGN (UNC-agn) 11.48 168.1 ± 20.9 −1.08 ± 0.28 150.5 ± 18.7 −0.84 ± 0.23
Unclass. SF (UNC-sf) 10.62 64.7 ± 6.2 −0.64 ± 0.17 68.6 ± 6.5 −0.93 ± 0.19
Unclass. SF-D4 (UNC-sf-D4000) 11.05 81.4 ± 15.6 −0.64 ± 0.36 86.2 ± 15.8 −0.88 ± 0.38

Notes. Power-law cross-correlation amplitudes (Acc) and slopes (α) for the samples analysed in this paper. ⟨M, P⟩ denotes the mean logarithm of stellar mass (or radio power). Accf refers to the cross-correlation amplitude with α fixed to the value of the complete sample before splitting in bins. The results for UNCs are discussed in detail in Appendix A.

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