For each class of MBOSS, we compute the average color indexes.
Table 3 lists the average colors of the various
classes of objects together with the square root of their variances
(which will become equivalent to the standard deviation for large
samples with a normal distribution). These values are of
practical interest, for instance when preparing observations of an
object whose colors are not known.
Figure 4 displays the average populations' colors in a set of color-color diagrams.
It is customary to visually compare distributions of objects using their histograms, i.e. the number of objects if given bins. Such histograms are displayed in Fig. 5. However, one has to be extremely careful in working with such plots: the size of the bin has a strong influence on the shape of the final histogram. Indeed, binning the data is equivalent to smoothing the data with a window equal to the bin size. Structures in the distribution that have a size similar to or smaller than the bin will be masked in the histogram, an effect that can create dangerously convincing - but wrong - artifacts.
A better way to represent a distribution is its Cumulative Probability
Function (CPF). If one of the sample is
x1, x2, ... , xn(e.g. the V-R color indexes of n Centaurs), the corresponding CPF
F(x) is the fraction of the sample whose value is smaller than
x. The CPF always has a typical "S'' shape, with
,
and F increases by step at each xi till it reaches a value of 1
when x is larger than all the xi. The advantage of the CPF is
that no information is lost with respect to the original
distribution. While its use is not as instinctive as that of the
histogram, it is a worthwhile exercise to train ones eye to use
them. The CPFs are also displayed in Fig. 5
Copyright ESO 2002