Table C.2.

MW tests for differences in the relative frequencies in periphery-sponsored stars in the final 25 periods.

Treatmentn4b0n8b0n4b22n8b22n4b66n8b66
n4b0
n8b00.49
n4b220.000.00
n8b220.020.020.29
n4b660.040.080.070.51
n8b660.000.000.500.530.28
Treatmentn4b0n8b0n4b22n8b22n4b66n8b66
n4b0
n8b00.49
n4b220.000.00
n8b220.020.020.29
n4b660.040.080.070.51
n8b660.000.000.500.530.28

Notes: Entries are p-values coming from Mann–Whitney tests using group averages as the independent unit of observation.

Table C.2.

MW tests for differences in the relative frequencies in periphery-sponsored stars in the final 25 periods.

Treatmentn4b0n8b0n4b22n8b22n4b66n8b66
n4b0
n8b00.49
n4b220.000.00
n8b220.020.020.29
n4b660.040.080.070.51
n8b660.000.000.500.530.28
Treatmentn4b0n8b0n4b22n8b22n4b66n8b66
n4b0
n8b00.49
n4b220.000.00
n8b220.020.020.29
n4b660.040.080.070.51
n8b660.000.000.500.530.28

Notes: Entries are p-values coming from Mann–Whitney tests using group averages as the independent unit of observation.

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