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Home All issues Volume 508 / No 1 (December II 2009) A&A, 508 1 (2009) 457-465 Full HTML
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Table 4:

Spearman correlation.
Class $\rho$ $P_{\rm r}$ n
Centaurs      
S vs. i -0.00451293 0.98495 20
S vs. e 0.430989 0.0578041 20
S vs. a 0.0691989 0.771903 20
S vs. H 0.398494 0.0818076 20
S vs. q -0.0910117 0.702757 20
Classicals      
S vs. i -0.641537 0.000176407 29
S vs. e -0.510963 0.00461781 29
S vs. a -0.109633 0.571303 29
S vs. H -0.0892836 0.64510 29
S vs. q 0.430648 0.0196961 29
Resonants      
S vs. i -0.393407 0.164032 14
S vs e 0.767033 0.00136768 14
S vs. a 0.560440 0.0371045 14
S vs. H 0.382838 0.176678 14
S vs. q 0.142857 0.626118 14
SDOs      
S vs. i -0.542857 0.265703 6
S vs e -0.885714 0.0188455 6
S vs. a -0.657143 0.156175 6
S vs. H 0.0857143 0.871743 6
S vs. q -0.0857143 0.871743 6
Detached Objs      
S vs. i -0.200000 0.800000 4
S vs. e 0.00000 1.00000 4
S vs. a -0.400000 0.600000 4
S vs. H 0.800000 0.200000 4
S vs. q -0.400000 0.600000 4

Spearman correlation results of the spectral slope S, orbital parameters (inclination i, eccentricity e, semimajor axis a, perihelion q), and absolute magnitude H. $\rho$ is the Spearman rank correlation, $P_{\rm r}$ is the significance level, and n the number of objectsused in the statistical analysis. Strongest correlations are in bold.

Source LaTeX | All tables | In the text

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