Table 2
Results of luminosity distribution comparisons using the DA test.
| Galaxy pairs | DA p-value | Comp | DA p-valuecut | Comp |
|---|---|---|---|---|
| LMC vs SMC | 0.14 | Y | >0.25 | Y |
| LMC vs M31 | <0.01 | N | 0.22 | Y |
| LMC vs M33 L10 | 0.04 | N | 0.14 | Y |
| LMC vs M33 G17 | <0.01 | N | 0.05 | Y |
| SMC vs M31 | <0.01 | N | >0.25 | Y |
| SMC vs M33 L10 | 0.02 | N | >0.25 | Y |
| SMC vs M33 G17 | >0.25 | Y | 0.19 | Y |
| M31 vs M33 L10 | <0.01 | N | 0.14 | Y |
| M31 vs M33 G17 | <0.01 | N | 0.10 | Y |
Notes. The first column shows the galaxy pair considered for the test. The second column shows the results, in p-values, considering the entire catalogue of SNRs in both galaxies. The third column summarises if the two distribution are likely draw from the same underling (Y) or not (N). The last two columns show the test results, including only luminosities larger than 1.7 × 1035ergs−1.
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