If we put the data we've analyzed before into Hickory, we get
the results shown in Table 1
is the
within-population inbreeding coefficient,
,
is
the Bayesian analog of Weir and Cockerham's
,6 and
is the Bayesian analog of Nei's
.
Hickory allows you to select from three models when running the data with codominant markers:
As a result, we can use DIC comparisons among the models to determine
whether we have evidence for inbreeding within populations (
versus
) or for genetic differentiation among populations
(
versus
). If we do that with these
data we get the results shown in Table 2.
The
has a much larger DIC than the full model, a difference of
more than 20 units. Thus, we have strong evidence for inbreeding in
these populations of Isotoma petraea.7 The
model also has a DIC
substantially larger than the DIC for the full model, a difference of
more than 10 units. Thus, we also have good evidence for genetic
differentiation among these populations.8
If we ask Hickory to keep log files of our analyses, we can also
compare the estimates of
for the full and
models. The posterior means are 0.52 and 0.55, respectively, so they
seem pretty similar. But we can do better than that. Since we have the
full posterior distribution for
in both models, we can pick points
at random from each, take their difference, and construct a 95%
credible interval. Doing that we find that the 95% credible interval
for
is (-0.29, 0.24), meaning we have
no evidence that the estimates are different. That may be a little
surprising, since we strong evidence that
in
these data, but it's also good news. It means that our estimate of
within-population inbreeding is not much affected by the amount of
differentiation among populations.9 What may be more
surprising is that the estimates for
with and without
inbreeding are also very similar: 0.19 versus 0.22,
respectively. Moreover, the 95% credible interval for
is (-0.38, 0.33). Thus,
even though we have strong evidence that
, our estimate of
is not strongly affected by what we think about
in
these data.
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One more thing we can do is to look at the posterior distribution of our parameter estimates and at the sample trace.10 (Figure 2). The result of an MCMC analysis, like the ones here or the ones in WinBUGS, is a large number of individual points. We can either fit a distribution to those points and display the results (the black lines in the figures), or we can use a non-parametric, kernel density estimate (the blue lines in the figures). The sample traces below show the values the chain took on at each point in the sampling process, and you can see that the values bounced around, which is good.
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It's also useful to look back and think about the different ways we've used the data from Isotoma petraea (Table 3). Several things become apparent from looking at this table: