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Table 4.

Lopsidedness p-values for the metrics applied to the ELVES systems.

Host pcentroid pθmax phemisphere ppairwise pMRL pwedge
(1) (2) (3) (4) (5) (6) (7)
M104 0.519 0.912 0.911 0.790 0.805 0.761
NGC0253 0.498 0.480 1.000 0.680 0.586 0.261
NGC0628 0.272 0.379 0.350 0.349 0.314 0.199
NGC0891 0.441 0.397 0.543 0.573 0.665 0.427
NGC1023 0.099 0.608 0.322 0.262 0.240 0.101
NGC1291 0.853 0.516 0.842 0.725 0.702 0.685
NGC1808 0.690 0.113 0.348 0.122 0.112 0.020
NGC2683 0.458 0.874 0.933 0.584 0.514 0.891
NGC2903 0.328 0.589 0.983 0.550 0.655 0.732
NGC3115 0.403 0.254 0.960 0.986 0.991 0.628
NGC3344 0.377 0.607 0.543 0.528 0.560 0.117
NGC3521 0.335 0.202 0.966 0.921 0.911 0.588
NGC3556 0.177 0.228 0.726 0.148 0.144 0.134
NGC4258 0.222 0.722 0.870 0.562 0.530 0.833
NGC4517 0.119 0.021 0.035 0.082 0.137 0.009
NGC4631 0.895 0.883 0.865 0.664 0.621 0.367
NGC4736 0.703 0.321 0.727 0.599 0.556 0.652
NGC4826 0.438 0.813 0.698 0.347 0.366 0.512
NGC5236 0.885 0.934 0.999 0.721 0.725 0.798
NGC5457 0.315 0.124 0.695 0.230 0.217 0.381
NGC6744 0.040 0.013 0.095 0.038 0.035 0.057
Number of statistically significant systems per metric
1 (∼4.7%) 2 (∼9.5%) 1 1 1 2

Notes. Columns: (1) name of the host galaxy, (2–7) p-values for the different metrics: centroid, maximum opening angle, hemisphere, mean pairwise angle, MRL, and wedge. A p-value of 0.05 or lower is considered statistically significant at the 2σ level and highlighted in bold.

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