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Table 2.

Statistical tests of neighbouring galaxy properties.

log(M/M) log(P1.4 GHz)


10.7 11.2 11.6 22.3 24.0 25.7






KS MWU KS MWU KS MWU KS MWU KS MWU KS MWU
u − r N-HERG vs N-LERG < 10−3 < 10−3 < 10−3 < 10−3 0.05 0.08 < 10−3 < 10−3 < 10−3 < 10−3 < 10−3 < 10−3
N-LERG vs N-CSL 0.02 0.05 < 10−3 < 10−3 < 10−3 < 10−3
N-HERG vs N-CSH 0.26 0.37 0.29 0.59 0.73 0.50

Mr N-HERG vs N-LERG 0.10 0.04 < 10−3 < 10−3 0.49 0.18 < 10−3 < 10−3 < 10−3 < 10−3 < 10−3 < 10−3
N-LERG vs N-CSL 0.04 0.11 < 10−3 < 10−3 < 10−3 < 10−3
N-HERG vs N-CSH 0.31 0.49 0.30 0.09 0.03 0.02

Notes. Results of the KS and MWU statistical tests comparing the distributions of neighbouring galaxy properties around different AGN types. The upper half of the table presents the test results for the u − r colour distribution, while the lower half corresponds to the Mr absolute magnitude distribution. Each pair of columns shows the p values from the KS and MWU tests in separate columns. Columns are divided into three bins of stellar mass (left) and three bins of radio luminosity (right). Low p values indicate statistically significant differences between the distributions being compared. For details, see Section 4.2.

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