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Table 8:

Correlations and dependence on ``sizes''.
      OWN     OWN+LP     OWN+LP+2MS  
  correlated magnitudes $\rho$ SL(%) n $\rho$ SL(%) n $\rho$ SL(%) n
Classicals B-V vs. q 0.59 95.13 12 0.37 98.24 43 0.40 99.83 64
  B-V vs. q(HR> 6.2)     2 0.28 84.33 27 0.33 93.04 32
  B-V vs. q(HR< 6.2) 0.64 94.37 10 0.52 95.50 16 0.49 99.40 32
  R-I vs. q 0.17 52.53 19 0.32 97.63 50 0.30 98.71 69
  R-I vs. q(HR> 6.2) 0.71 91.98 7 0.57 99.85 31 0.51 99.68 35
  R-I vs. q(HR< 6.2) -0.10 26.38 12 -0.09 30.42 19 0.06 26.99 34
  B-R vs. q 0.55 92.96 12 0.46 99.71 43 0.46 99.98 64
  B-R vs. q(HR> 6.2)     2 0.48 98.58 27 0.47 99.06 32
  B-R vs. q(HR< 6.2) 0.55 90.20 10 0.43 90.37 16 0.49 99.39 32
  R-I vs. e 0.17 54.82 19 -0.21 86.62 50 -0.17 84.83 69
  R-I vs. e(HR> 6.2) 0.14 27.36 7 -0.41 97.68 31 -0.38 97.28 35
  R-I vs. e(HR< 6.2) 0.15 38.26 12 0.13 42.35 19 0.04 19.76 34
  V-R vs. a -0.14 45.84 19 0.18 80.79 52 0.12 69.48 73
  V-R vs. a(HR> 6.2) -0.43 70.62 7 -0.06 26.64 33 -0.02 10.12 38
  V-R vs. a(HR< 6.2) 0.03 7.39 12 0.48 96.01 19 0.21 76.84 35
  B-R vs. a 0.08 21.92 12 0.09 43.80 43 0.14 73.85 64
  B-R vs. a(HR> 6.2)     2 -0.19 67.17 27 -0.11 44.33 32
  B-R vs. a(HR< 6.2) 0.25 54.40 10 0.56 97.04 16 0.29 89.64 32
  V-R vs. $\psi$ 0.20 61.21 19 0.05 27.68 52 0.05 30.00 73
  V-R vs. $\psi$(HR> 6.2) 0.14 27.36 7 0.28 88.87 33 0.35 96.69 38
  V-R vs. $\psi$(HR< 6.2) 0.10 25.46 12 -0.34 84.70 19 -0.28 89.76 35
  B-R vs. $\psi$ 0.20 48.39 12 <0.01 1.44 43 -0.02 14.42 64
  B-R vs. $\psi$(HR> 6.2)     2 0.06 24.44 27 0.19 70.87 32
  B-R vs. $\psi$(HR< 6.2) -0.07 15.85 10 -0.23 62.57 16 -0.32 92.06 32
Hot B-V vs. q 0.29 51.60 7 0.41 94.71 23 0.38 97.96 38
  B-V vs. q(HR> 6.2)     1 0.20 51.87 13 0.31 78.33 17
  B-V vs. q(HR< 6.2) 0.77 91.55 6 0.70 96.35 10 0.39 91.46 21
  R-I vs. q 0.20 45.27 10 0.23 75.89 27 0.19 76.46 40
  R-I vs. q(HR> 6.2) 0.60 70.13 4 0.37 84.55 16 0.20 61.21 19
  R-I vs. q(HR< 6.2) 0.09 15.42 6 <0.01 2.30 11 0.13 45.04 21
  V-R vs. a -0.31 64.62 10 0.19 65.45 27 0.21 82.91 42
  V-R vs. a(HR> 6.2)     4 -0.23 61.99 16 -0.16 51.09 20
  V-R vs. a(HR< 6.2) 0.37 59.38 6 0.67 96.66 11 0.49 97.41 22
  B-R vs. a <0.01 <0.01 7 0.12 41.24 23 0.22 82.46 38
  B-R vs. a(HR> 6.2)     1 -0.13 33.84 13 -0.09 26.85 17
  B-R vs. a(HR< 6.2) 0.60 82.03 6 0.79 98.28 10 0.59 99.15 21
Cold R-I vs. q 0.15 32.86 9 0.25 75.53 23 0.27 84.35 29
  R-I vs. q(HR> 6.2)     3 0.56 96.29 15 0.60 98.06 16
  R-I vs. q(HR< 6.2) -0.14 25.06 6 -0.45 76.86 8 -0.30 69.60 13
  V-R vs. a -0.17 36.26 9 0.35 91.29 25 0.09 38.31 31
  V-R vs. a(HR> 6.2) -0.50 52.05 3 0.41 90.05 17 0.42 91.52 18
  V-R vs. a(HR< 6.2) -0.20 34.53 6 0.17 34.08 8 -0.30 69.60 13
Correlations results of colors versus orbital parameters and versus $\psi$, a measure of the ``average Collisional Energy'' (Opik 1976) for classical objects. We correlate the whole group and two different subgroups of different ``sizes'' with HR> 6.2, and HR< 6.2. OWN means our own data, OWN+LP means our own data merged with the ESO Large Program data (Boehnhardt et al. 2002; Peixinho et al. 2004), OWN+LP+2MS means the OWN+LP data merged with the Meudon Multicolor Survey data (Doressoundiram et al. 2005), $\rho$ = Spearman rank correlation, SL = Significance level, n = Number of objects.

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