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Table 4

Results from the Kolmogorov–Smirnov test used to compare the families to their corresponding backgrounds.

Family NOBS NBGR DFAM−BGR DCritical Compatible
Juno 26 18 0.3162 0.4998 ✓
Vesta 408 225 0.2626 0.1354 –
Flora 355 587 0.1467 0.1096 –
Hygiea 70 19 0.1504 0.4217 ✓
Eunomia 248 180 0.1341 0.1596 ✓
Themis 161 31 0.1513 0.3197 ✓
Phocaea 32 18 0.2396 0.4802 ✓
Euterpe 15 10 0.3333 0.6654 ✓
Nysa–Polana 356 138 0.1295 0.1635 ✓
Klio 9 59 0.3804 0.5833 ✓
Meliboea 15 25 0.1467 0.5324 ✓
Adeona 40 24 0.5833 0.4209 –
Koronis 151 36 0.1038 0.3023 ✓
Erigone 31 24 0.1640 0.4432 ✓
Maria 96 94 0.1190 0.2365 ✓
Eos 328 174 0.1014 0.1529 ✓
Baptistina 77 52 0.2173 0.2926 ✓
Padua 15 17 0.4980 0.5774 ✓
Ursula 23 70 0.2230 0.3918 ✓
Charis 8 8 0.3750 0.8150 ✓
Alauda 37 13 0.4179 0.5255 ✓
Agnia 16 11 0.6023 0.6384 ✓
Gefion 87 29 0.2874 0.3495 ✓
Rafita 30 14 0.3286 0.5276 ✓
Henan 19 39 0.3563 0.4560 ✓
Mitidika 22 75 0.4982 0.3952 –
Witt 20 17 0.2118 0.5377 ✓

Notes. The limits for the number of observed members (in both family and background) and their corresponding errors are the same as in Sect. 4.1. DFAM−BGR is the distance between the CDFs of the family and its background, and DCritical is the critical distance, as in Table 3.

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