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Table 4.

Percentages of paired galaxies with efficient star formation activity and young stellar populations located in the void environment and for matched samples of pairs in walls and fields. Standard errors are included.

Pair restrictions log(SFR/M*)>  − 10.6 Dn(4000)< 1.6
% Void interiors 67.61 ± 0.79% 60.53 ± 0.73%
% Void walls 57.52 ± 0.40% 50.82 ± 0.37%
% Fields 44.67 ± 0.67% 40.08 ± 0.63%

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