
Wahba (1983) proposes a Bayesian covariance matrix for parameter estimates
by interpreting a smoothing spline as a posterior mean. Nychka (1988) shows that the derived Bayesian posterior confidence limits work well from frequentist viewpoints. The Bayesian posterior
covariance matrix for the parameters is
![\[ \bV _{\bbeta }=(\bX ’\bW \bX +\bS _{\blambda })^{-1}\sigma ^2 \]](images/stathpug_hpgam0193.png)
The posterior distribution for
is thus
![\[ \bbeta |\mb{y} \sim N(\hat{\bbeta },\bV _{\bbeta }) \]](images/stathpug_hpgam0194.png)
For a particular point whose design row is vector
, the prediction is
and the standard error is
. The Bayesian posterior confidence limits are thus
![\[ \left(\mb{x}\hat{\bbeta } \pm z_{\alpha /2} \sqrt {\mb{x}\bV _{\bbeta }\mb{x}’}\right) \]](images/stathpug_hpgam0197.png)
where
is the
quantile of the standard normal distribution.
For the jth spline term, the prediction for the component is formed by
, where
is a row vector of zeros except for columns that correspond to basis expansions of the jth spline term. And the standard error for the component is
.