In a qualitative sense, this result is to be expected for the following
reasons: given that, after any folding process, absolute errors will inevitably
exist in the estimated position of the dynamical centre of any given galaxy,
then there will be absolute errors of similar magnitudes in the pre-hole cutting and
post-hole cutting estimates of
.
Since the pre-hole cutting estimate of
is less than the post-hole cutting
estimate of
,
it follows that the corresponding percentage
errors in the pre-hole cutting estimates of
will be greater than those in the post-hole
cutting estimates of
.
Consequently, given that
correlations exist in the first place,
these correlations must automatically increase through the hole-cutting process.
The real significance of the foregoing results is therefore not that the
correlations increase at all through the hole-cutting
process, but is rather that the magnitude of this increase acts potentially as an
uncalibrated statistical measure for the magnitude of the original absolute
errors in the estimated positions of the dynamical centres taken over the whole sample.
Thus, we might expect that relatively large changes in
correlations through the hole-cutting process will indicate the presence of
relatively large errors in the estimates of
over the set of
folding solutions, and vice-versa.
These considerations play a significant part in the developments from Sect. 8
onwards.
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